[{"type":"journal_article","OA_type":"closed access","status":"public","doi":"10.1007/s10853-024-10582-y","author":[{"first_name":"Saurabh","id":"12d625da-9cb3-11ed-9667-af09d37d3f0a","orcid":"0000-0003-2209-5269","last_name":"Singh","full_name":"Singh, Saurabh"},{"last_name":"Provino","first_name":"A.","full_name":"Provino, A."},{"full_name":"Pallecchi, I.","first_name":"I.","last_name":"Pallecchi"},{"first_name":"F.","last_name":"Caglieris","full_name":"Caglieris, F."},{"first_name":"M.","last_name":"Mödlinger","full_name":"Mödlinger, M."},{"full_name":"Mele, P.","last_name":"Mele","first_name":"P."},{"full_name":"Latronico, G.","first_name":"G.","last_name":"Latronico"},{"full_name":"Takeuchi, T.","last_name":"Takeuchi","first_name":"T."},{"first_name":"P.","last_name":"Manfrinetti","full_name":"Manfrinetti, P."}],"date_created":"2025-03-09T23:01:29Z","year":"2025","quality_controlled":"1","day":"08","title":"The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K)","date_updated":"2025-03-10T06:53:16Z","language":[{"iso":"eng"}],"oa_version":"None","intvolume":" 60","article_number":"100051","abstract":[{"lang":"eng","text":"In the present study, the new ternary rare earth intermetallic compound PrNi6Si6 has been investigated. This work completes the study of the RNi6Si6 series (R = rare earth). While the RNi6Si6 compounds for R = La and Ce adopt the CeNi6Si6-type (tP52, P4/nbm, No. 125), surprisingly PrNi6Si6 crystallizes in the YNi6Si6 prototype (tP52, P − 4b2, No. 117) as do all the heavier lanthanides (but Lu). The YNi6Si6-type and its homolog CeNi6Si6 are two tetragonal ordered derivative of the cubic NaZn13-type structure. Lattice parameters for PrNi6Si6 are a = 7.7846(1) Å, c = 11.2144(1) Å, with a unit cell volume, Vobs = 679.585(5) Å3. The temperature dependence of the inverse magnetic susceptibility χ−1(T) follows the Curie–Weiss law, with calculated values of the effective magnetic moment (µeff) and Weiss temperature (Θpm) of 3.55 μB and − 4.5 K, respectively. While the observed µeff is very close to the theoretical value of 3.58 µB for the free Pr3+ ions, a negative value of the Weiss temperature suggests antiferromagnetic interactions in PrNi6Si6. Magnetization measurements confirm that PrNi₆Si₆ orders antiferromagnetically (AFM) below a Néel temperature (TN) of 9 K. The Ni atoms contribute negligibly to the magnetic properties of this phase. The specific heat of PrNi₆Si₆ is approximately 0.42 J K − 1 g − 1. Measurements of electric and thermal transport reveal that PrNi₆Si₆ exhibits metallic behavior across a wide temperature range of 2–900 K, accompanied by a relatively low thermal conductivity of around 6 W K − 1 m − 1 at room temperature. Such properties, together with its high-temperature refractory behavior, make PrNi₆Si₆ worthy of consideration in technological applications where fairly good electrical conductivity should be accompanied by a limited thermal conductivity."}],"fulldoi":"https://doi.org/10.1007/s10853-024-10582-y","publisher":"Springer Nature","scopus_import":"1","publication":"Journal of Materials Science","_id":"19374","publication_identifier":{"issn":["0022-2461"],"eissn":["1573-4803"]},"date_published":"2025-02-08T00:00:00Z","publication_status":"published","month":"02","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","article_processing_charge":"No","department":[{"_id":"MaIb"}],"volume":60,"citation":{"apa":"Singh, S., Provino, A., Pallecchi, I., Caglieris, F., Mödlinger, M., Mele, P., … Manfrinetti, P. (2025). The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. Springer Nature. https://doi.org/10.1007/s10853-024-10582-y","ista":"Singh S, Provino A, Pallecchi I, Caglieris F, Mödlinger M, Mele P, Latronico G, Takeuchi T, Manfrinetti P. 2025. The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. 60, 100051.","mla":"Singh, Saurabh, et al. “The New PrNi6Si6 Intermetallic: From Crystal Structure to Thermal and Electrical Transport Properties across a Wide Temperature Range (2–900 K).” Journal of Materials Science, vol. 60, 100051, Springer Nature, 2025, doi:10.1007/s10853-024-10582-y.","short":"S. Singh, A. Provino, I. Pallecchi, F. Caglieris, M. Mödlinger, P. Mele, G. Latronico, T. Takeuchi, P. Manfrinetti, Journal of Materials Science 60 (2025).","ieee":"S. Singh et al., “The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K),” Journal of Materials Science, vol. 60. Springer Nature, 2025.","chicago":"Singh, Saurabh, A. Provino, I. Pallecchi, F. Caglieris, M. Mödlinger, P. Mele, G. Latronico, T. Takeuchi, and P. Manfrinetti. “The New PrNi6Si6 Intermetallic: From Crystal Structure to Thermal and Electrical Transport Properties across a Wide Temperature Range (2–900 K).” Journal of Materials Science. Springer Nature, 2025. https://doi.org/10.1007/s10853-024-10582-y.","ama":"Singh S, Provino A, Pallecchi I, et al. The new PrNi6Si6 intermetallic: From crystal structure to thermal and electrical transport properties across a wide temperature range (2–900 K). Journal of Materials Science. 2025;60. doi:10.1007/s10853-024-10582-y"}},{"publication_status":"published","date_published":"2025-03-13T00:00:00Z","month":"03","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","article_processing_charge":"No","department":[{"_id":"GaNo"}],"volume":639,"citation":{"short":"S.P. Pașca, P. Arlotta, H.S. Bateup, J.G. Camp, S. Cappello, F.H. Gage, J.A. Knoblich, A.R. Kriegstein, M.A. Lancaster, G.L. Ming, G. Novarino, H. Okano, M. Parmar, I.H. Park, O. Reiner, H. Song, L. Studer, J. Takahashi, S. Temple, G. Testa, B. Treutlein, F.M. Vaccarino, P. Vanderhaeghen, T. Young-Pearse, Nature 639 (2025) 315–320.","ista":"Pașca SP, Arlotta P, Bateup HS, Camp JG, Cappello S, Gage FH, Knoblich JA, Kriegstein AR, Lancaster MA, Ming GL, Novarino G, Okano H, Parmar M, Park IH, Reiner O, Song H, Studer L, Takahashi J, Temple S, Testa G, Treutlein B, Vaccarino FM, Vanderhaeghen P, Young-Pearse T. 2025. A framework for neural organoids, assembloids and transplantation studies. Nature. 639(8054), 315–320.","apa":"Pașca, S. P., Arlotta, P., Bateup, H. S., Camp, J. G., Cappello, S., Gage, F. H., … Young-Pearse, T. (2025). A framework for neural organoids, assembloids and transplantation studies. Nature. Springer Nature. https://doi.org/10.1038/s41586-024-08487-6","mla":"Pașca, Sergiu P., et al. “A Framework for Neural Organoids, Assembloids and Transplantation Studies.” Nature, vol. 639, no. 8054, Springer Nature, 2025, pp. 315–20, doi:10.1038/s41586-024-08487-6.","ieee":"S. P. Pașca et al., “A framework for neural organoids, assembloids and transplantation studies,” Nature, vol. 639, no. 8054. Springer Nature, pp. 315–320, 2025.","ama":"Pașca SP, Arlotta P, Bateup HS, et al. A framework for neural organoids, assembloids and transplantation studies. Nature. 2025;639(8054):315-320. doi:10.1038/s41586-024-08487-6","chicago":"Pașca, Sergiu P., Paola Arlotta, Helen S. Bateup, J. Gray Camp, Silvia Cappello, Fred H. Gage, Jürgen A. Knoblich, et al. “A Framework for Neural Organoids, Assembloids and Transplantation Studies.” Nature. Springer Nature, 2025. https://doi.org/10.1038/s41586-024-08487-6."},"fulldoi":"https://doi.org/10.1038/s41586-024-08487-6","publisher":"Springer Nature","scopus_import":"1","publication":"Nature","_id":"19444","publication_identifier":{"eissn":["1476-4687"],"issn":["0028-0836"]},"pmid":1,"external_id":{"isi":["001437461900001"],"pmid":["39653126"]},"year":"2025","isi":1,"page":"315-320","quality_controlled":"1","day":"13","date_updated":"2025-09-30T11:13:47Z","title":"A framework for neural organoids, assembloids and transplantation studies","oa_version":"None","language":[{"iso":"eng"}],"intvolume":" 639","abstract":[{"text":"As the field of neural organoids and assembloids expands, there is an emergent need for guidance and advice on designing, conducting and reporting experiments to increase the reproducibility and utility of these models. In this Perspective, we present a framework for the experimental process that encompasses ensuring the quality and integrity of human pluripotent stem cells, characterizing and manipulating neural cells in vitro, transplantation techniques and considerations for modelling human development, evolution and disease. As with all scientific endeavours, we advocate for rigorous experimental designs tailored to explicit scientific questions as well as transparent methodologies and data sharing to provide useful knowledge for current research practices and for developing regulatory standards.","lang":"eng"}],"type":"journal_article","OA_type":"closed access","status":"public","doi":"10.1038/s41586-024-08487-6","author":[{"last_name":"Pașca","first_name":"Sergiu P.","full_name":"Pașca, Sergiu P."},{"full_name":"Arlotta, Paola","first_name":"Paola","last_name":"Arlotta"},{"full_name":"Bateup, Helen S.","last_name":"Bateup","first_name":"Helen S."},{"first_name":"J. Gray","last_name":"Camp","full_name":"Camp, J. Gray"},{"full_name":"Cappello, Silvia","first_name":"Silvia","last_name":"Cappello"},{"first_name":"Fred H.","last_name":"Gage","full_name":"Gage, Fred H."},{"full_name":"Knoblich, Jürgen A.","first_name":"Jürgen A.","last_name":"Knoblich"},{"full_name":"Kriegstein, Arnold R.","first_name":"Arnold R.","last_name":"Kriegstein"},{"last_name":"Lancaster","first_name":"Madeline A.","full_name":"Lancaster, Madeline A."},{"first_name":"Guo Li","last_name":"Ming","full_name":"Ming, Guo Li"},{"id":"3E57A680-F248-11E8-B48F-1D18A9856A87","first_name":"Gaia","orcid":"0000-0002-7673-7178","last_name":"Novarino","full_name":"Novarino, Gaia"},{"full_name":"Okano, Hideyuki","first_name":"Hideyuki","last_name":"Okano"},{"full_name":"Parmar, Malin","last_name":"Parmar","first_name":"Malin"},{"full_name":"Park, In Hyun","first_name":"In Hyun","last_name":"Park"},{"first_name":"Orly","last_name":"Reiner","full_name":"Reiner, Orly"},{"full_name":"Song, Hongjun","last_name":"Song","first_name":"Hongjun"},{"full_name":"Studer, Lorenz","first_name":"Lorenz","last_name":"Studer"},{"first_name":"Jun","last_name":"Takahashi","full_name":"Takahashi, Jun"},{"first_name":"Sally","last_name":"Temple","full_name":"Temple, Sally"},{"full_name":"Testa, Giuseppe","last_name":"Testa","first_name":"Giuseppe"},{"full_name":"Treutlein, Barbara","first_name":"Barbara","last_name":"Treutlein"},{"full_name":"Vaccarino, Flora M.","last_name":"Vaccarino","first_name":"Flora M."},{"full_name":"Vanderhaeghen, Pierre","last_name":"Vanderhaeghen","first_name":"Pierre"},{"full_name":"Young-Pearse, Tracy","last_name":"Young-Pearse","first_name":"Tracy"}],"date_created":"2025-03-23T23:01:27Z","issue":"8054","acknowledgement":"The authors thank members of their laboratories who provided feedback on earlier versions of this manuscript, including A. Jourdon, V. Mariano, T. L. Li, N. Caporale, E. Villa and M. Sutcliffe."},{"oa_version":"Published Version","language":[{"iso":"eng"}],"title":"RUBIES reveals a massive quiescent galaxy at z = 7.3","date_updated":"2026-02-16T12:42:28Z","day":"10","file":[{"date_created":"2025-04-22T09:08:17Z","success":1,"content_type":"application/pdf","checksum":"a1132e0b18bb643f9a32674c6694375a","creator":"dernst","file_id":"19605","access_level":"open_access","date_updated":"2025-04-22T09:08:17Z","file_name":"2025_AstrophysicalJour_Weibel.pdf","relation":"main_file","file_size":1964589}],"DOAJ_listed":"1","abstract":[{"text":"We report the spectroscopic discovery of a massive quiescent galaxy at zspec = 7.29 ± 0.01, just ∼700 Myr after the big bang. RUBIES-UDS-QG-z7 was selected from public JWST/NIRCam and MIRI imaging from the PRIMER survey and observed with JWST/NIRSpec as part of RUBIES. The NIRSpec/PRISM spectrum reveals one of the strongest Balmer breaks observed thus far at z > 6, with no emission lines but tentative Balmer and Ca absorption features, as well as a Lyman break. Simultaneous modeling of the NIRSpec/PRISM spectrum and NIRCam and MIRI photometry (spanning 0.9–18 μm) shows that the galaxy formed a stellar mass of\r\n(math. formular) before z ∼ 8 and ceased forming stars 50–100 Myr prior to the time of observation, resulting in log (sSFR/Gyr- 1) < -1 . We measure a small physical size of (math formular) , which implies a high stellarmass surface density within the effective radius of (math formular) comparable to the highest densities measured in quiescent galaxies at z ∼ 2–5. The 3D stellar-mass density profile of RUBIES-UDS-QG-z7 is remarkably similar to the central densities of local massive ellipticals, suggesting that at least some of their cores may have already been in place at z > 7. The discovery of RUBIES-UDS-QG-z7 has strong implications for galaxy formation models: the estimated number density of quiescent galaxies at z ∼ 7 is >100 × larger than predicted from any model to date, indicating that quiescent galaxies have formed earlier than previously expected. ","lang":"eng"}],"article_number":"11","intvolume":" 983","year":"2025","external_id":{"isi":["001457334900001"],"arxiv":["2409.03829"]},"quality_controlled":"1","isi":1,"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"ddc":["520"],"author":[{"last_name":"Weibel","first_name":"Andrea","full_name":"Weibel, Andrea"},{"full_name":"De Graaff, Anna","last_name":"De Graaff","first_name":"Anna"},{"first_name":"David J.","last_name":"Setton","full_name":"Setton, David J."},{"full_name":"Miller, Tim B.","last_name":"Miller","first_name":"Tim B."},{"full_name":"Oesch, Pascal A.","last_name":"Oesch","first_name":"Pascal A."},{"full_name":"Brammer, Gabriel","first_name":"Gabriel","last_name":"Brammer"},{"last_name":"Lagos","first_name":"Claudia D.P.","full_name":"Lagos, Claudia D.P."},{"last_name":"Whitaker","first_name":"Katherine E.","full_name":"Whitaker, Katherine E."},{"last_name":"Williams","first_name":"Christina C.","full_name":"Williams, Christina C."},{"full_name":"Baggen, Josephine F.W.","last_name":"Baggen","first_name":"Josephine F.W."},{"first_name":"Rachel","last_name":"Bezanson","full_name":"Bezanson, Rachel"},{"full_name":"Boogaard, Leindert A.","last_name":"Boogaard","first_name":"Leindert A."},{"full_name":"Cleri, Nikko J.","first_name":"Nikko J.","last_name":"Cleri"},{"first_name":"Jenny E.","last_name":"Greene","full_name":"Greene, Jenny E."},{"last_name":"Hirschmann","first_name":"Michaela","full_name":"Hirschmann, Michaela"},{"full_name":"Hviding, Raphael E.","last_name":"Hviding","first_name":"Raphael E."},{"full_name":"Kuruvanthodi, Adarsh","first_name":"Adarsh","last_name":"Kuruvanthodi"},{"first_name":"Ivo","last_name":"Labbé","full_name":"Labbé, Ivo"},{"full_name":"Leja, Joel","last_name":"Leja","first_name":"Joel"},{"first_name":"Michael V.","last_name":"Maseda","full_name":"Maseda, Michael V."},{"full_name":"Matthee, Jorryt J","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Mcconachie","first_name":"Ian","full_name":"Mcconachie, Ian"},{"full_name":"Naidu, Rohan P.","first_name":"Rohan P.","last_name":"Naidu"},{"full_name":"Roberts-Borsani, Guido","first_name":"Guido","last_name":"Roberts-Borsani"},{"full_name":"Schaerer, Daniel","last_name":"Schaerer","first_name":"Daniel"},{"last_name":"Suess","first_name":"Katherine A.","full_name":"Suess, Katherine A."},{"full_name":"Valentino, Francesco","last_name":"Valentino","first_name":"Francesco"},{"full_name":"Van Dokkum, Pieter","last_name":"Van Dokkum","first_name":"Pieter"},{"last_name":"Wang","first_name":"Bingjie","full_name":"Wang, Bingjie"}],"acknowledgement":"We thank the PRIMER team for making their imaging data publicly available immediately. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program #4233. Support for program #4233 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. This research was supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team project #562. The Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF140). This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI), under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF), through project grant 200020_207349. Support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. Support for this work for R.P.N. was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A, awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. T.B.M. was supported by a CIERA fellowship.\r\nAll software packages used in this work are publicly available on Github: grizli, msafit, msaexp, Prospector, and sedpy. We acknowledge: astropy (Astropy Collaboration et al. 2013, 2018, 2022), matplotlib (J. D. Hunter 2007), numpy (C. R. Harris et al. 2020), scipy (P. Virtanen et al. 2020), lmfit (M. Newville et al. 2024), eMPT (N. Bonaventura et al. 2023), the jwst pipeline (H. Bushouse et al. 2024), msaexp (G. Brammer 2024a), and grizli (G. Brammer 2024b),.","issue":"1","date_created":"2025-04-20T22:01:28Z","status":"public","file_date_updated":"2025-04-22T09:08:17Z","doi":"10.3847/1538-4357/adab7a","OA_type":"gold","type":"journal_article","department":[{"_id":"JoMa"}],"article_processing_charge":"Yes","citation":{"chicago":"Weibel, Andrea, Anna De Graaff, David J. Setton, Tim B. Miller, Pascal A. Oesch, Gabriel Brammer, Claudia D.P. Lagos, et al. “RUBIES Reveals a Massive Quiescent Galaxy at z = 7.3.” The Astrophysical Journal. IOP Publishing, 2025. https://doi.org/10.3847/1538-4357/adab7a.","ama":"Weibel A, De Graaff A, Setton DJ, et al. RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. 2025;983(1). doi:10.3847/1538-4357/adab7a","ieee":"A. Weibel et al., “RUBIES reveals a massive quiescent galaxy at z = 7.3,” The Astrophysical Journal, vol. 983, no. 1. IOP Publishing, 2025.","short":"A. Weibel, A. De Graaff, D.J. Setton, T.B. Miller, P.A. Oesch, G. Brammer, C.D.P. Lagos, K.E. Whitaker, C.C. Williams, J.F.W. Baggen, R. Bezanson, L.A. Boogaard, N.J. Cleri, J.E. Greene, M. Hirschmann, R.E. Hviding, A. Kuruvanthodi, I. Labbé, J. Leja, M.V. Maseda, J.J. Matthee, I. Mcconachie, R.P. Naidu, G. Roberts-Borsani, D. Schaerer, K.A. Suess, F. Valentino, P. Van Dokkum, B. Wang, The Astrophysical Journal 983 (2025).","apa":"Weibel, A., De Graaff, A., Setton, D. J., Miller, T. B., Oesch, P. A., Brammer, G., … Wang, B. (2025). RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/adab7a","ista":"Weibel A, De Graaff A, Setton DJ, Miller TB, Oesch PA, Brammer G, Lagos CDP, Whitaker KE, Williams CC, Baggen JFW, Bezanson R, Boogaard LA, Cleri NJ, Greene JE, Hirschmann M, Hviding RE, Kuruvanthodi A, Labbé I, Leja J, Maseda MV, Matthee JJ, Mcconachie I, Naidu RP, Roberts-Borsani G, Schaerer D, Suess KA, Valentino F, Van Dokkum P, Wang B. 2025. RUBIES reveals a massive quiescent galaxy at z = 7.3. The Astrophysical Journal. 983(1), 11.","mla":"Weibel, Andrea, et al. “RUBIES Reveals a Massive Quiescent Galaxy at z = 7.3.” The Astrophysical Journal, vol. 983, no. 1, 11, IOP Publishing, 2025, doi:10.3847/1538-4357/adab7a."},"volume":983,"month":"04","publication_status":"published","date_published":"2025-04-10T00:00:00Z","article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","scopus_import":"1","publisher":"IOP Publishing","fulldoi":"https://doi.org/10.3847/1538-4357/adab7a","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"_id":"19596","publication":"The Astrophysical Journal","arxiv":1,"OA_place":"publisher","has_accepted_license":"1","oa":1},{"citation":{"ama":"Hu H, Inayoshi K, Haiman Z, Ho LC, Ohsuga K. The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. 2025;983(2). doi:10.3847/2041-8213/adc680","chicago":"Hu, Haojie, Kohei Inayoshi, Zoltán Haiman, Luis C. Ho, and Ken Ohsuga. “The Convergence of Heavy and Light Seeds to Overmassive Black Holes at Cosmic Dawn.” The Astrophysical Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/adc680.","short":"H. Hu, K. Inayoshi, Z. Haiman, L.C. Ho, K. Ohsuga, The Astrophysical Journal Letters 983 (2025).","apa":"Hu, H., Inayoshi, K., Haiman, Z., Ho, L. C., & Ohsuga, K. (2025). The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/adc680","ista":"Hu H, Inayoshi K, Haiman Z, Ho LC, Ohsuga K. 2025. The convergence of heavy and light seeds to overmassive black holes at cosmic dawn. The Astrophysical Journal Letters. 983(2), L37.","mla":"Hu, Haojie, et al. “The Convergence of Heavy and Light Seeds to Overmassive Black Holes at Cosmic Dawn.” The Astrophysical Journal Letters, vol. 983, no. 2, L37, IOP Publishing, 2025, doi:10.3847/2041-8213/adc680.","ieee":"H. Hu, K. Inayoshi, Z. Haiman, L. C. Ho, and K. Ohsuga, “The convergence of heavy and light seeds to overmassive black holes at cosmic dawn,” The Astrophysical Journal Letters, vol. 983, no. 2. IOP Publishing, 2025."},"volume":983,"department":[{"_id":"ZoHa"}],"article_processing_charge":"Yes","article_type":"letter_note","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"04","publication_status":"published","date_published":"2025-04-20T00:00:00Z","_id":"19638","publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"publication":"The Astrophysical Journal Letters","scopus_import":"1","publisher":"IOP Publishing","fulldoi":"https://doi.org/10.3847/2041-8213/adc680","has_accepted_license":"1","oa":1,"arxiv":1,"OA_place":"publisher","file":[{"relation":"main_file","file_size":3334014,"date_created":"2025-05-05T11:30:34Z","checksum":"1a4fbeeb12e9022873e86c72d230a5ec","success":1,"creator":"dernst","content_type":"application/pdf","file_id":"19655","access_level":"open_access","file_name":"2025_AstrophysicalJourLetters_Hu.pdf","date_updated":"2025-05-05T11:30:34Z"}],"DOAJ_listed":"1","article_number":"L37","abstract":[{"text":"The James Webb Space Telescope has revealed low-luminosity active galactic nuclei at redshifts of z ≳ 4–7, many of which host accreting massive black holes (BHs) with BH-to-galaxy mass (MBH/M⋆) ratios exceeding the local values by more than an order of magnitude. The origin of these overmassive BHs remains unclear but requires potential contributions from heavy seeds and/or episodes of super-Eddington accretion. We present a growth model coupled with dark matter halo assembly to explore the evolution of the MBH/M⋆ ratio under different seeding and feedback scenarios. Given the gas inflow rates in protogalaxies, BHs grow episodically at moderate super-Eddington rates, and the mass ratio increases early on, despite significant mass loss through feedback. Regardless of seeding mechanisms, the mass ratio converges to a universal value ∼0.1–0.3, set by the balance between gas feeding and star formation efficiency in the nucleus. This behavior defines an attractor in the MBH–M⋆ diagram, where overmassive BHs grow more slowly than their hosts, while undermassive seeds experience rapid growth before aligning with the attractor. We derive an analytical expression for the universal mass ratio, linking it to feedback strength and halo growth. The convergence of evolutionary tracks erases seeding information from the mass ratio by z ∼ 4–6. Detecting BHs with ∼105−6 M⊙ at higher redshifts that deviate from the convergence trend would provide key diagnostics of their birth conditions.","lang":"eng"}],"intvolume":" 983","language":[{"iso":"eng"}],"oa_version":"Published Version","title":"The convergence of heavy and light seeds to overmassive black holes at cosmic dawn","date_updated":"2026-02-16T12:44:04Z","day":"20","quality_controlled":"1","isi":1,"year":"2025","external_id":{"arxiv":["2503.03870"],"isi":["001467616800001"]},"acknowledgement":"We thank the anonymous referee for a careful reading of our manuscript and for comments that helped improve this Letter. This work is supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI grant No. 24KF0130. We acknowledge support from the National Natural Science Foundation of China (12073003, 12003003, 11721303, 11991052, 11950410493), and the China Manned Space Project (CMS-CSST-2021-A04 and CMS-CSST-2021-A06). L.C.H. is supported by the National Science Foundation of China (12233001), the National Key R&D Program of China (2022YFF0503401). Z.H. acknowledges support by US NSF grant AST-2006176 and by NASA grant 80NSSC22K0822. Some of the numerical calculation and analysis were performed with the Cray XC50 at the Center for Computational Astrophysics (CfCA) of the National Astronomical Observatory of Japan and with the High-performance Computing Platform of Peking University.","issue":"2","date_created":"2025-05-04T22:02:31Z","tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"ddc":["520"],"author":[{"first_name":"Haojie","last_name":"Hu","full_name":"Hu, Haojie"},{"full_name":"Inayoshi, Kohei","first_name":"Kohei","last_name":"Inayoshi"},{"full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","last_name":"Haiman","orcid":"0000-0003-3633-5403"},{"full_name":"Ho, Luis C.","first_name":"Luis C.","last_name":"Ho"},{"last_name":"Ohsuga","first_name":"Ken","full_name":"Ohsuga, Ken"}],"file_date_updated":"2025-05-05T11:30:34Z","status":"public","doi":"10.3847/2041-8213/adc680","OA_type":"gold","type":"journal_article"},{"date_created":"2025-05-11T22:02:38Z","issue":"2","acknowledgement":"We thank Bjorn Stevens for suggesting the study and for substantial ideas along the way. We also thank Sebastian Rast for helping with the model compilation. This work used resources of the German Climate Computing Center (DKRZ) under project ID mh0066 for our experiments and analysis. Jiawei Bao acknowledges the European Union's Horizon 2020 for funding.Jiawei Bao has been supported by the European Union's Horizon 2020 research and innovation programme under a Marie Skłodowska-Curie grant (grant agreement no. 101034413).\r\nThe article processing charges for this open-access publication were covered by the Max Planck Society.","ddc":["550"],"author":[{"last_name":"Gnanaraj","first_name":"Abisha Mary","full_name":"Gnanaraj, Abisha Mary"},{"id":"bb9a7399-fefd-11ed-be3c-ae648fd1d160","first_name":"Jiawei","last_name":"Bao","full_name":"Bao, Jiawei"},{"full_name":"Schmidt, Hauke","last_name":"Schmidt","first_name":"Hauke"}],"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"type":"journal_article","file_date_updated":"2025-05-12T08:23:10Z","status":"public","doi":"10.5194/wcd-6-489-2025","OA_type":"gold","intvolume":" 6","file":[{"file_size":6500575,"relation":"main_file","file_name":"2025_WeatherClimateDynam_Gnanaraj.pdf","date_updated":"2025-05-12T08:23:10Z","access_level":"open_access","date_created":"2025-05-12T08:23:10Z","file_id":"19680","content_type":"application/pdf","checksum":"2ea68f7e51ee39ccb6886719a83a78ca","creator":"dernst","success":1}],"DOAJ_listed":"1","abstract":[{"lang":"eng","text":"We investigate the effect of changes in the Coriolis force caused by changes in the rotation rate on the top-of-atmosphere (TOA) radiant energy budget of an aquaplanet general circulation model with prescribed sea surface temperatures. We analyse the effective radiative forcing caused by changes from Earth-like rotation to values between 1/32 and 8 times the Earth's rotation rate. The forcing differs by about 60 W m−2 between the fastest and slowest rotation cases, with a monotonically increasing positive forcing for faster-than-Earth-like rotations and a non-monotonically increasing negative forcing for slower rotations. The largest contributions to the forcing are due to changes in, in this order, the shortwave cloud radiative effect (SWCRE) and the clear-sky outgoing longwave radiation (OLR). From the fastest to the slowest rotation, the Hadley cell expands and the troposphere becomes drier, increasing the OLR. This contributes to negative forcing at slower-than-Earth-like rotations and to positive forcing at faster-than-Earth-like rotations. The SWCRE is influenced by changes in the low-level cloudiness within the Hadley cell and the baroclinic regime. With the expansion of the Hadley cell, the area of enhanced tropospheric stability increases, resulting in more low-level clouds, a higher SWCRE, and increased negative forcing. The non-monotonicity results from an intermediate decrease in the SWCRE caused by the disappearance of baroclinic eddies as the Hadley cell reaches global extension. At rotations faster than Earth-like, the decrease in the SWCRE, mainly due to the weakening of baroclinic eddies and storm systems, leads to an increase in positive forcing. In summary, changes in the SWCRE, driven by different circulation responses at slower-than-Earth-like and faster-than-Earth-like rotations, strongly influence the TOA radiant energy budget. These effects, along with a substantial contribution from the clear-sky OLR, could impact the habitability of Earth-like rotating planets."}],"title":"The impact of the rotation rate on an aquaplanet's radiant energy budget: Insights from experiments varying the Coriolis parameter","date_updated":"2025-07-09T08:40:18Z","day":"25","language":[{"iso":"eng"}],"oa_version":"Published Version","page":"489-503","quality_controlled":"1","year":"2025","publication":"Weather and Climate Dynamics","_id":"19662","publication_identifier":{"eissn":["2698-4016"]},"fulldoi":"https://doi.org/10.5194/wcd-6-489-2025","PlanS_conform":"1","publisher":"Copernicus Publications","scopus_import":"1","oa":1,"has_accepted_license":"1","project":[{"name":"IST-BRIDGE: International postdoctoral program","grant_number":"101034413","call_identifier":"H2020","_id":"fc2ed2f7-9c52-11eb-aca3-c01059dda49c"}],"OA_place":"publisher","volume":6,"citation":{"ieee":"A. M. Gnanaraj, J. Bao, and H. Schmidt, “The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter,” Weather and Climate Dynamics, vol. 6, no. 2. Copernicus Publications, pp. 489–503, 2025.","ista":"Gnanaraj AM, Bao J, Schmidt H. 2025. The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. 6(2), 489–503.","apa":"Gnanaraj, A. M., Bao, J., & Schmidt, H. (2025). The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. Copernicus Publications. https://doi.org/10.5194/wcd-6-489-2025","mla":"Gnanaraj, Abisha Mary, et al. “The Impact of the Rotation Rate on an Aquaplanet’s Radiant Energy Budget: Insights from Experiments Varying the Coriolis Parameter.” Weather and Climate Dynamics, vol. 6, no. 2, Copernicus Publications, 2025, pp. 489–503, doi:10.5194/wcd-6-489-2025.","short":"A.M. Gnanaraj, J. Bao, H. Schmidt, Weather and Climate Dynamics 6 (2025) 489–503.","chicago":"Gnanaraj, Abisha Mary, Jiawei Bao, and Hauke Schmidt. “The Impact of the Rotation Rate on an Aquaplanet’s Radiant Energy Budget: Insights from Experiments Varying the Coriolis Parameter.” Weather and Climate Dynamics. Copernicus Publications, 2025. https://doi.org/10.5194/wcd-6-489-2025.","ama":"Gnanaraj AM, Bao J, Schmidt H. The impact of the rotation rate on an aquaplanet’s radiant energy budget: Insights from experiments varying the Coriolis parameter. Weather and Climate Dynamics. 2025;6(2):489-503. doi:10.5194/wcd-6-489-2025"},"ec_funded":1,"department":[{"_id":"CaMu"}],"article_processing_charge":"Yes (via OA deal)","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","date_published":"2025-04-25T00:00:00Z","publication_status":"published","month":"04"},{"citation":{"ama":"Budde C, Hartmanns A, Meggendorfer T, Weininger M, Wienhöft P. Sound statistical model checking for probabilities and expected rewards (experimental reproduction package). 2025. doi:10.5281/ZENODO.14602066","chicago":"Budde, Carlos, Arnd Hartmanns, Tobias Meggendorfer, Maximilian Weininger, and Patrick Wienhöft. “Sound Statistical Model Checking for Probabilities and Expected Rewards (Experimental Reproduction Package).” Zenodo, 2025. https://doi.org/10.5281/ZENODO.14602066.","ieee":"C. Budde, A. Hartmanns, T. Meggendorfer, M. Weininger, and P. Wienhöft, “Sound statistical model checking for probabilities and expected rewards (experimental reproduction package).” Zenodo, 2025.","apa":"Budde, C., Hartmanns, A., Meggendorfer, T., Weininger, M., & Wienhöft, P. (2025). Sound statistical model checking for probabilities and expected rewards (experimental reproduction package). Zenodo. https://doi.org/10.5281/ZENODO.14602066","ista":"Budde C, Hartmanns A, Meggendorfer T, Weininger M, Wienhöft P. 2025. Sound statistical model checking for probabilities and expected rewards (experimental reproduction package), Zenodo, 10.5281/ZENODO.14602066.","mla":"Budde, Carlos, et al. Sound Statistical Model Checking for Probabilities and Expected Rewards (Experimental Reproduction Package). Zenodo, 2025, doi:10.5281/ZENODO.14602066.","short":"C. Budde, A. Hartmanns, T. Meggendorfer, M. Weininger, P. Wienhöft, (2025)."},"abstract":[{"lang":"eng","text":"Artifact to reproduce the experimental results presented in the article \"Sound Statistical Model Checking for Probabilities and Expected Rewards\" by Carlos E. Budde, Arnd Hartmanns, Tobias Meggendorfer, Maximilian Weininger, and Patrick Wienhöft (TACAS 2025).\r\n\r\nThe contents include all data and software (formal models, software tools, Python & bash scripts) used in the experimental evaluation presented in sections 3, 4, and 6 of the article. Detailed instructions on how to reproduce the results are bundled in the artifact."}],"oa_version":"Published Version","date_updated":"2025-06-02T09:45:41Z","title":"Sound statistical model checking for probabilities and expected rewards (experimental reproduction package)","article_processing_charge":"No","day":"07","department":[{"_id":"KrCh"}],"related_material":{"record":[{"status":"public","id":"19742","relation":"used_in_publication"}]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","year":"2025","month":"01","date_published":"2025-01-07T00:00:00Z","_id":"19769","main_file_link":[{"url":"https://doi.org/10.5281/ZENODO.14602066","open_access":"1"}],"date_created":"2025-06-02T09:37:14Z","publisher":"Zenodo","ddc":["000"],"fulldoi":"https://doi.org/10.5281/ZENODO.14602066","author":[{"full_name":"Budde, Carlos","first_name":"Carlos","last_name":"Budde"},{"full_name":"Hartmanns, Arnd","last_name":"Hartmanns","first_name":"Arnd"},{"first_name":"Tobias","id":"b21b0c15-30a2-11eb-80dc-f13ca25802e1","orcid":"0000-0002-1712-2165","last_name":"Meggendorfer","full_name":"Meggendorfer, Tobias"},{"full_name":"Weininger, Maximilian","first_name":"Maximilian","id":"02ab0197-cc70-11ed-ab61-918e71f56881","last_name":"Weininger"},{"full_name":"Wienhöft, Patrick","last_name":"Wienhöft","first_name":"Patrick"}],"oa":1,"doi":"10.5281/ZENODO.14602066","OA_place":"repository","status":"public","OA_type":"green","type":"research_data_reference"},{"article_processing_charge":"Yes","department":[{"_id":"JoMa"}],"citation":{"ieee":"G. Östlin et al., “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm,” Astronomy & Astrophysics, vol. 696. EDP Sciences, 2025.","ista":"Östlin G, Pérez-González PG, Melinder J, Gillman S, Iani E, Costantin L, Boogaard LA, Rinaldi P, Colina L, Nørgaard-Nielsen HU, Dicken D, Greve TR, Wright G, Alonso-Herrero A, Álvarez-Márquez J, Annunziatella M, Bik A, Bosman SEI, Caputi KI, Gomez AC, Eckart A, Garcia-Marin M, Hjorth J, Ilbert O, Jermann I, Kendrew S, Labiano A, Langeroodi D, Le Fevre O, Libralato M, Meyer RA, Moutard T, Peissker F, Pye JP, Tikkanen TV, Topinka M, Walter F, Ward M, Van Der Werf P, Van Dishoeck EF, Güdel M, Henning T, Lagage PO, Ray TP, Vandenbussche B. 2025. MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. Astronomy & Astrophysics. 696, A57.","apa":"Östlin, G., Pérez-González, P. G., Melinder, J., Gillman, S., Iani, E., Costantin, L., … Vandenbussche, B. (2025). MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202451723","mla":"Östlin, Göran, et al. “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey Description and Early Results for the Galaxy Population Detected at 5.6 Μm.” Astronomy & Astrophysics, vol. 696, A57, EDP Sciences, 2025, doi:10.1051/0004-6361/202451723.","short":"G. Östlin, P.G. Pérez-González, J. Melinder, S. Gillman, E. Iani, L. Costantin, L.A. Boogaard, P. Rinaldi, L. Colina, H.U. Nørgaard-Nielsen, D. Dicken, T.R. Greve, G. Wright, A. Alonso-Herrero, J. Álvarez-Márquez, M. Annunziatella, A. Bik, S.E.I. Bosman, K.I. Caputi, A.C. Gomez, A. Eckart, M. Garcia-Marin, J. Hjorth, O. Ilbert, I. Jermann, S. Kendrew, A. Labiano, D. Langeroodi, O. Le Fevre, M. Libralato, R.A. Meyer, T. Moutard, F. Peissker, J.P. Pye, T.V. Tikkanen, M. Topinka, F. Walter, M. Ward, P. Van Der Werf, E.F. Van Dishoeck, M. Güdel, T. Henning, P.O. Lagage, T.P. Ray, B. Vandenbussche, Astronomy & Astrophysics 696 (2025).","ama":"Östlin G, Pérez-González PG, Melinder J, et al. MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm. Astronomy & Astrophysics. 2025;696. doi:10.1051/0004-6361/202451723","chicago":"Östlin, Göran, Pablo G. Pérez-González, Jens Melinder, Steven Gillman, Edoardo Iani, Luca Costantin, Leindert A. Boogaard, et al. “MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey Description and Early Results for the Galaxy Population Detected at 5.6 Μm.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202451723."},"volume":696,"month":"04","date_published":"2025-04-01T00:00:00Z","publication_status":"published","article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publisher":"EDP Sciences","scopus_import":"1","fulldoi":"https://doi.org/10.1051/0004-6361/202451723","publication_identifier":{"eissn":["1432-0746"],"issn":["0004-6361"]},"_id":"19845","publication":"Astronomy & Astrophysics","OA_place":"publisher","arxiv":1,"has_accepted_license":"1","oa":1,"oa_version":"Published Version","language":[{"iso":"eng"}],"day":"01","date_updated":"2026-02-16T12:10:36Z","title":"MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 µm","abstract":[{"lang":"eng","text":"Context. The recently launched James Webb Space Telescope (JWST) is opening new observing windows on the distant Universe. Among JWST’s instruments, the Mid Infrared Instrument (MIRI) offers the unique capability of imaging observations at wavelengths of λ > 5 μm. This enables unique access to the rest frame near-infrared (NIR, λ ≥ 1 μm) emission from galaxies at redshifts of z > 4 and the visual (λ ≳ 5000 Å) rest frame for z > 9. We report here on the guaranteed time observations (GTO), from the MIRI European Consortium, of the Hubble Ultra Deep Field (HUDF), forming the MIRI Deep Imaging Survey (MIDIS), consisting of an on source integration time of ∼41 hours in the MIRI/F560W (5.6 μm) filter. The F560W filter was selected since it would produce the deepest data in terms of AB magnitudes in a given time. To our knowledge, this constitutes the longest single filter exposure obtained with JWST of an extragalactic field as of yet.\r\nAims. The HUDF is one of the most observed extragalactic fields, with extensive multi-wavelength coverage, where (before JWST) galaxies up to z ∼ 7 have been confirmed, and at z > 10 suggested, from HST photometry. We aim to characterise the galaxy population in HUDF at 5.6 μm, enabling studies such as: the rest frame NIR morphologies for galaxies at z ≲ 4.6, probing mature stellar populations and emission lines in z > 6 sources, intrinsically red and dusty galaxies, and active galactic nuclei (AGNs) and their host galaxies at intermediate redshifts.\r\n\r\nMethods. We reduced the MIRI data using the official JWST pipeline, augmented by in-house custom scripts. We measured the noise characteristics of the resulting image. Galaxy photometry was obtained, and photometric redshifts were estimated for sources with available multi-wavelength photometry (and compared to spectroscopic redshifts when available).\r\n\r\nResults. Over the deepest part of our image, the 5σ point source limit is 28.65 mag AB (12.6 nJy), ∼0.35 mag better than predicted by the JWST exposure time calculator. We find ∼2500 sources, the overwhelming majority of which are distant galaxies, but we note that spurious sources likely remain at faint magnitudes due to imperfect cosmic ray rejection in the JWST pipeline. More than 500 galaxies with available spectroscopic redshifts, up to z ≈ 11, have been identified, the majority of which are at z < 6. More than 1000 galaxies have reliable photometric redshift estimates, of which ∼25 are at 6 < z < 12. The point spread function in the F560W filter has a full width at half maximum (FWHM) of ≈0.2″ (corresponding to 1.4 kpc at z = 4), allowing the NIR rest frame morphologies and stellar mass distributions to be resolved for z < 4.5. Moreover, > 100 objects with very red NIRCam vs MIRI (3.6–5.6 μm > 1 mag) colours have been found, suggestive of dusty or old stellar populations at high redshifts.\r\n\r\nConclusions. We conclude that MIDIS surpasses preflight expectations and that deep MIRI imaging has great potential to characterise the galaxy population from cosmic noon to dawn."}],"article_number":"A57","file":[{"relation":"main_file","file_size":15858045,"date_created":"2025-06-23T07:46:01Z","file_id":"19865","content_type":"application/pdf","success":1,"checksum":"67600eba8bda24987a130ac334f10456","creator":"dernst","file_name":"2025_AstronomyAstrophysics_Oestlin.pdf","date_updated":"2025-06-23T07:46:01Z","access_level":"open_access"}],"intvolume":" 696","year":"2025","external_id":{"isi":["001459780300005"],"arxiv":["2411.19686 "]},"quality_controlled":"1","isi":1,"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"author":[{"full_name":"Östlin, Göran","first_name":"Göran","last_name":"Östlin"},{"last_name":"Pérez-González","first_name":"Pablo G.","full_name":"Pérez-González, Pablo G."},{"last_name":"Melinder","first_name":"Jens","full_name":"Melinder, Jens"},{"last_name":"Gillman","first_name":"Steven","full_name":"Gillman, Steven"},{"first_name":"Edoardo","id":"4053390a-6b68-11ef-9828-a3b8adef8d0a","orcid":"0000-0001-8386-3546","last_name":"Iani","full_name":"Iani, Edoardo"},{"last_name":"Costantin","first_name":"Luca","full_name":"Costantin, Luca"},{"full_name":"Boogaard, Leindert A.","last_name":"Boogaard","first_name":"Leindert A."},{"last_name":"Rinaldi","first_name":"Pierluigi","full_name":"Rinaldi, Pierluigi"},{"first_name":"Luis","last_name":"Colina","full_name":"Colina, Luis"},{"full_name":"Nørgaard-Nielsen, Hans Ulrik","last_name":"Nørgaard-Nielsen","first_name":"Hans Ulrik"},{"full_name":"Dicken, Daniel","last_name":"Dicken","first_name":"Daniel"},{"last_name":"Greve","first_name":"Thomas R.","full_name":"Greve, Thomas R."},{"full_name":"Wright, Gillian","first_name":"Gillian","last_name":"Wright"},{"first_name":"Almudena","last_name":"Alonso-Herrero","full_name":"Alonso-Herrero, Almudena"},{"full_name":"Álvarez-Márquez, Javier","last_name":"Álvarez-Márquez","first_name":"Javier"},{"last_name":"Annunziatella","first_name":"Marianna","full_name":"Annunziatella, Marianna"},{"first_name":"Arjan","last_name":"Bik","full_name":"Bik, Arjan"},{"first_name":"Sarah E.I.","last_name":"Bosman","full_name":"Bosman, Sarah E.I."},{"full_name":"Caputi, Karina I.","first_name":"Karina I.","last_name":"Caputi"},{"full_name":"Gomez, Alejandro Crespo","last_name":"Gomez","first_name":"Alejandro Crespo"},{"full_name":"Eckart, Andreas","last_name":"Eckart","first_name":"Andreas"},{"first_name":"Macarena","last_name":"Garcia-Marin","full_name":"Garcia-Marin, Macarena"},{"last_name":"Hjorth","first_name":"Jens","full_name":"Hjorth, Jens"},{"last_name":"Ilbert","first_name":"Olivier","full_name":"Ilbert, Olivier"},{"last_name":"Jermann","first_name":"Iris","full_name":"Jermann, Iris"},{"full_name":"Kendrew, Sarah","last_name":"Kendrew","first_name":"Sarah"},{"first_name":"Alvaro","last_name":"Labiano","full_name":"Labiano, Alvaro"},{"first_name":"Danial","last_name":"Langeroodi","full_name":"Langeroodi, Danial"},{"full_name":"Le Fevre, Olivier","last_name":"Le Fevre","first_name":"Olivier"},{"full_name":"Libralato, Mattia","first_name":"Mattia","last_name":"Libralato"},{"first_name":"Romain A.","last_name":"Meyer","full_name":"Meyer, Romain A."},{"last_name":"Moutard","first_name":"Thibaud","full_name":"Moutard, Thibaud"},{"first_name":"Florian","last_name":"Peissker","full_name":"Peissker, Florian"},{"first_name":"John P.","last_name":"Pye","full_name":"Pye, John P."},{"first_name":"Tuomo V.","last_name":"Tikkanen","full_name":"Tikkanen, Tuomo V."},{"last_name":"Topinka","first_name":"Martin","full_name":"Topinka, Martin"},{"full_name":"Walter, Fabian","last_name":"Walter","first_name":"Fabian"},{"last_name":"Ward","first_name":"Martin","full_name":"Ward, Martin"},{"first_name":"Paul","last_name":"Van Der Werf","full_name":"Van Der Werf, Paul"},{"first_name":"Ewine F.","last_name":"Van Dishoeck","full_name":"Van Dishoeck, Ewine F."},{"full_name":"Güdel, Manuel","first_name":"Manuel","last_name":"Güdel"},{"full_name":"Henning, Thomas","last_name":"Henning","first_name":"Thomas"},{"full_name":"Lagage, Pierre Olivier","last_name":"Lagage","first_name":"Pierre Olivier"},{"first_name":"Tom P.","last_name":"Ray","full_name":"Ray, Tom P."},{"full_name":"Vandenbussche, Bart","first_name":"Bart","last_name":"Vandenbussche"}],"ddc":["520"],"acknowledgement":"We dedicate this paper to the memory of our deceased and much valued MIRI-EC team members Hans Ulrik Nørgaard-Nielsen and Olivier Le Fèvre, both of whom played a central role in defining the MIDIS project. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The work presented is the effort of the entire MIRI team and the enthusiasm within the MIRI partnership is a significant factor in its success. The following National and International Funding Agencies funded and supported the MIRI development: NASA; ESA; Belgian Science Policy Office (BELSPO); Centre Nationale d’Etudes Spatiales (CNES); Danish National Space Centre; Deutsches Zentrum fur Luftund Raumfahrt (DLR); Enterprise Ireland; Ministerio De Economia y Competividad; Netherlands Research School for Astronomy (NOVA); Netherlands Organisation for Scientific Research (NWO); Science and Technology Facilities Council; Swiss Space Office; Swedish National Space Agency (SNSA); and UK Space Agency. MIRI drew on the scientific and technical expertise of the following organizations: Ames Research Center, USA; Airbus Defence and Space, UK; CEAIrfu, Saclay, France; Centre Spatial de Liège, Belgium; Consejo Superior de Investigaciones Cientficas, Spain; Carl Zeiss Optronics, Germany; Chalmers University of Technology, Sweden; Danish Space Research Institute, Denmark; Dublin Institute for Advanced Studies, Ireland; European Space Agency, Netherlands; ETCA, Belgium; ETH Zurich, Switzerland; Goddard Space Flight Center, USA; Institute d’Astrophysique Spatiale, France; Instituto Nacional de Técnica Aeroespacial,Spain; Institute for Astronomy, Edinburgh, UK; Jet Propulsion Laboratory, USA; Laboratoire d’Astrophysique de Marseille (LAM), France; Leiden University, Netherlands; Lockheed Advanced Technology Center (USA); NOVA Opt-IR group at Dwingeloo, Netherlands; Northrop Grumman, USA; Max Planck Institut f ür Astronomie (MPIA), Heidelberg, Germany; Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA), France; Paul Scherrer Institut, Switzerland; Raytheon Vision Systems, USA; RUAG Aerospace, Switzerland; Rutherford Appleton Laboratory (RAL Space), UK; Space Telescope Science Institute, USA; Stockholm University, Sweden; Toegepast- Natuurwetenschappelijk Onderzoek (TNOTPD), Netherlands; UK Astronomy Technology Centre, UK; University College London, UK; University of Amsterdam, Netherlands; University of Arizona, USA; University of Cardiff, UK; University of Cologne, Germany; University of Ghent; University of Groningen, Netherlands; University of Leicester, UK; University of Leuven, Belgium; Utah State University, USA. Additional acknowledgements related to specific grants: G.Ö., J.M. and A.B. acknowledges funding from the Swedish National Space Administration (SNSA). P.G.P.-G. acknowledges support from grant PID2022-139567NB-I00 funded by Spanish Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033, FEDER Una manera de hacer Europa. This work was supported by research grants (VIL16599,VIL54489) from VILLUM FONDEN. L.C. and J.A.-M. acknowledge support by grant PIB2021-127718NB-100 from the Spanish Ministry of Science and Innovation/State Agency of Research MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”. M.A. acknowledges financial support from Comunidad de Madrid under Atracción de Talento grant 2020-T2/TIC-19971. J.P.P. and T.V.T. acknowledge financial support from the UK Science and Technology Facilities Council, and the UK Space Agency. A.A.-H. acknowledges financial support from grant PID2021-124665NB-I00 funded by MCIN/AEI/10.13039/501100011033 and by “ERDF A way of making Europe”. E.I. and K.I.C. acknowledge funding from the Netherlands Research School for Astronomy (NOVA). K.I.C. acknowledges funding from the Dutch Research Council (NWO) through the award of the Vici Grant VI.C.212.036. RAM acknowledges support from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. The paper uses JWST data from programme #1283, obtained from the Barbara Mikulski Archive for Space Telescopes at the Space Telescope Science Institute (STScI). For the purpose of open access, the authors have applied a Creative Commons Attribution (CC BY) licence to the Author Accepted Manuscript version arising from this submission.","date_created":"2025-06-15T22:01:30Z","OA_type":"diamond","file_date_updated":"2025-06-23T07:46:01Z","status":"public","doi":"10.1051/0004-6361/202451723","type":"journal_article"},{"isi":1,"quality_controlled":"1","external_id":{"isi":["001494836700001"],"arxiv":["2407.07004"]},"year":"2025","abstract":[{"lang":"eng","text":"Binding precedents (súmulas vinculantes) constitute a juridical instrument unique to the Brazilian legal system and whose objectives include the protection of the Federal Supreme Court against repetitive demands. Studies of the effectiveness of these instruments in decreasing the Court’s exposure to similar cases, however, indicate that they tend to fail in such a direction, with some of the binding precedents seemingly creating new demands. We empirically assess the legal impact of five binding precedents, 11, 14, 17, 26, and 37, at the highest Court level through their effects on the legal subjects they address. This analysis is only possible through the comparison of the Court’s ruling about the precedents’ themes before they are created, which means that these decisions should be detected through techniques of Similar Case Retrieval, which we tackle from the angle of Case Classification. The contributions of this article are therefore twofold: on the mathematical side, we compare the use of different methods of Natural Language Processing — TF-IDF, LSTM, Longformer, and regex — for Case Classification, whereas on the legal side, we contrast the inefficiency of these binding precedents with a set of hypotheses that may justify their repeated usage. We observe that the TF-IDF models performed slightly better than LSTM and Longformer when compared through common metrics; however, the deep learning models were able to detect certain important legal events that TF-IDF missed. On the legal side, we argue that the reasons for binding precedents to fail in responding to repetitive demand are heterogeneous and case-dependent, making it impossible to single out a specific cause. We identify five main hypotheses, which are found in different combinations in each of the precedents studied."}],"title":"Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification","date_updated":"2026-06-18T08:34:38Z","day":"26","language":[{"iso":"eng"}],"oa_version":"Published Version","type":"journal_article","doi":"10.1007/s10506-025-09458-6","status":"public","OA_type":"hybrid","date_created":"2025-06-15T22:01:31Z","acknowledgement":"Open access funding provided by Institute of Science and Technology (IST Austria).","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1007/s10506-025-09458-6"}],"ddc":["510"],"author":[{"last_name":"Tinarrage","orcid":"0000-0002-1404-1095","first_name":"Raphaël","id":"40ebcc9d-905f-11ef-bf0a-dc475da8a04e","full_name":"Tinarrage, Raphaël"},{"last_name":"Ennes","first_name":"Henrique","full_name":"Ennes, Henrique"},{"first_name":"Lucas","last_name":"Resck","full_name":"Resck, Lucas"},{"full_name":"Gomes, Lucas T.","first_name":"Lucas T.","last_name":"Gomes"},{"last_name":"Ponciano","first_name":"Jean R.","full_name":"Ponciano, Jean R."},{"last_name":"Poco","first_name":"Jorge","full_name":"Poco, Jorge"}],"corr_author":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","date_published":"2025-05-26T00:00:00Z","publication_status":"epub_ahead","month":"05","citation":{"chicago":"Tinarrage, Raphaël, Henrique Ennes, Lucas Resck, Lucas T. Gomes, Jean R. Ponciano, and Jorge Poco. “Empirical Analysis of Binding Precedent Efficiency in Brazilian Supreme Court via Case Classification.” Artificial Intelligence and Law. Springer Nature, 2025. https://doi.org/10.1007/s10506-025-09458-6.","ama":"Tinarrage R, Ennes H, Resck L, Gomes LT, Ponciano JR, Poco J. Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. Artificial Intelligence and Law. 2025. doi:10.1007/s10506-025-09458-6","ieee":"R. Tinarrage, H. Ennes, L. Resck, L. T. Gomes, J. R. Ponciano, and J. Poco, “Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification,” Artificial Intelligence and Law. Springer Nature, 2025.","short":"R. Tinarrage, H. Ennes, L. Resck, L.T. Gomes, J.R. Ponciano, J. Poco, Artificial Intelligence and Law (2025).","mla":"Tinarrage, Raphaël, et al. “Empirical Analysis of Binding Precedent Efficiency in Brazilian Supreme Court via Case Classification.” Artificial Intelligence and Law, Springer Nature, 2025, doi:10.1007/s10506-025-09458-6.","apa":"Tinarrage, R., Ennes, H., Resck, L., Gomes, L. T., Ponciano, J. R., & Poco, J. (2025). Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. Artificial Intelligence and Law. Springer Nature. https://doi.org/10.1007/s10506-025-09458-6","ista":"Tinarrage R, Ennes H, Resck L, Gomes LT, Ponciano JR, Poco J. 2025. Empirical analysis of binding precedent efficiency in Brazilian Supreme Court via case classification. Artificial Intelligence and Law."},"department":[{"_id":"UlWa"}],"article_processing_charge":"Yes (via OA deal)","oa":1,"OA_place":"publisher","arxiv":1,"publication":"Artificial Intelligence and Law","_id":"19848","publication_identifier":{"eissn":["1572-8382"],"issn":["0924-8463"]},"fulldoi":"https://doi.org/10.1007/s10506-025-09458-6","scopus_import":"1","publisher":"Springer Nature"},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_type":"original","date_published":"2025-08-01T00:00:00Z","publication_status":"published","month":"08","volume":541,"citation":{"ieee":"C. A. Pirie et al., “The JWST Emission Line Survey (JELS): An untargeted search for H α emission line galaxies at z > 6 and their physical properties,” Monthly Notices of the Royal Astronomical Society, vol. 541, no. 2. Oxford University Press, pp. 1348–1376, 2025.","ista":"Pirie CA, Best PN, Duncan KJ, Mcleod DJ, Cochrane RK, Clausen M, Dunlop JS, Flury SR, Geach JE, Hale CL, Ibar E, Kondapally R, Li Z, Matthee JJ, Mclure RJ, Ossa-Fuentes L, Patrick AL, Smail I, Sobral D, Stephenson HMO, Stott JP, Swinbank AM. 2025. The JWST Emission Line Survey (JELS): An untargeted search for H α emission line galaxies at z > 6 and their physical properties. Monthly Notices of the Royal Astronomical Society. 541(2), 1348–1376.","apa":"Pirie, C. A., Best, P. N., Duncan, K. J., Mcleod, D. J., Cochrane, R. K., Clausen, M., … Swinbank, A. M. (2025). The JWST Emission Line Survey (JELS): An untargeted search for H α emission line galaxies at z > 6 and their physical properties. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staf1006","mla":"Pirie, C. A., et al. “The JWST Emission Line Survey (JELS): An Untargeted Search for H α Emission Line Galaxies at z > 6 and Their Physical Properties.” Monthly Notices of the Royal Astronomical Society, vol. 541, no. 2, Oxford University Press, 2025, pp. 1348–76, doi:10.1093/mnras/staf1006.","short":"C.A. Pirie, P.N. Best, K.J. Duncan, D.J. Mcleod, R.K. Cochrane, M. Clausen, J.S. Dunlop, S.R. Flury, J.E. Geach, C.L. Hale, E. Ibar, R. Kondapally, Z. Li, J.J. Matthee, R.J. Mclure, L. Ossa-Fuentes, A.L. Patrick, I. Smail, D. Sobral, H.M.O. Stephenson, J.P. Stott, A.M. Swinbank, Monthly Notices of the Royal Astronomical Society 541 (2025) 1348–1376.","ama":"Pirie CA, Best PN, Duncan KJ, et al. The JWST Emission Line Survey (JELS): An untargeted search for H α emission line galaxies at z > 6 and their physical properties. Monthly Notices of the Royal Astronomical Society. 2025;541(2):1348-1376. doi:10.1093/mnras/staf1006","chicago":"Pirie, C. A., P. N. Best, K. J. Duncan, D. J. Mcleod, R. K. Cochrane, M. Clausen, J. S. Dunlop, et al. “The JWST Emission Line Survey (JELS): An Untargeted Search for H α Emission Line Galaxies at z > 6 and Their Physical Properties.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2025. https://doi.org/10.1093/mnras/staf1006."},"department":[{"_id":"JoMa"}],"article_processing_charge":"Yes","oa":1,"has_accepted_license":"1","OA_place":"publisher","arxiv":1,"publication":"Monthly Notices of the Royal Astronomical Society","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"_id":"20027","fulldoi":"https://doi.org/10.1093/mnras/staf1006","scopus_import":"1","PlanS_conform":"1","publisher":"Oxford University Press","page":"1348-1376","isi":1,"quality_controlled":"1","external_id":{"isi":["001527095600001"],"arxiv":["2410.11808"]},"year":"2025","intvolume":" 541","file":[{"access_level":"open_access","file_name":"2025_MonthlyNoticesRAS_Pirie.pdf","date_updated":"2025-07-22T07:19:20Z","date_created":"2025-07-22T07:19:20Z","creator":"dernst","content_type":"application/pdf","success":1,"checksum":"f8708c78016f8917765026502c6b50b6","file_id":"20064","file_size":38102038,"relation":"main_file"}],"DOAJ_listed":"1","abstract":[{"lang":"eng","text":"We present the first results of the JWST Emission Line Survey (JELS). Utilizing the first NIRCam narrow-band imaging at 4.7 μm, over 63 arcmin2 in the PRIMER/COSMOS field, we have identified 609 emission line galaxy candidates. From these, we robustly selected 35 H α star-forming galaxies at z ∼ 6.1, with H α star-formation rates (SFRH α) of ∼ 0.9 − 15 M yr−1.\r\nCombining our unique H α sample with the exquisite panchromatic data in the field, we explored their physical properties and star-formation histories, and compared these to a broad-band selected sample at z ∼ 6 which has offered vital new insights into the nature of high-redshift galaxies. UV-continuum slopes (β) were considerably redder for our H α sample (\u0004β\u0005 ∼ −1.92)\r\ncompared to the broad-band sample (\u0004β\u0005 ∼ −2.35). This was not due to dust attenuation as our H α sample was relatively dustpoor (median AV = 0.23); instead, we argue that the reddened slopes could be due to nebular continuum. We compared SFRH α and the UV-continuum-derived SFRUV to SED-fitted measurements averaged over canonical time-scales of 10 and 100 Myr (SFR10 and SFR100). We found an increase in recent SFR for our sample of H α emitters, particularly at lower stellar masses (< 109 M). We also found that SFRH α strongly traces SFR averaged over 10 Myr time-scales, whereas the UV-continuum overpredicts SFR on 100 Myr time-scales at low stellar masses. These results point to our H α sample undergoing ‘bursty’ star\r\nformation. Our F356W z ∼ 6 sample showed a larger scatter in SFR10/SFR100 across all stellar masses, which has highlighted how narrow-band photometric selections of H α emitters are key to quantifying the burstiness of star-formation activity. "}],"date_updated":"2025-09-30T14:03:40Z","title":"The JWST Emission Line Survey (JELS): An untargeted search for H α emission line galaxies at z > 6 and their physical properties","day":"01","oa_version":"Published Version","language":[{"iso":"eng"}],"type":"journal_article","doi":"10.1093/mnras/staf1006","status":"public","file_date_updated":"2025-07-22T07:19:20Z","OA_type":"gold","date_created":"2025-07-20T22:02:00Z","issue":"2","acknowledgement":"The authors would like to thank Adam Carnall and Joel Leja for their helpful advice with the SED fitting of our sample, Callum Donnan for his advice on the selection techniques of high-redshift\r\ngalaxies, Alice Shapley for discussion around H α SFR calibrations at high-redshift, Fred Jennings for providing insight into the interpretation of SFR ratios, and the anonymous referee for their helpful comments – all of which have greatly improved this paper. Several other authors acknowledge the support of the UK Science and Technology Facilities Council (STFC) via grants ST/W507441/1 (CAP), ST/V000594/1 (DJM, PNB, RK, and RJM), ST/Y000951/1 (PNB and RK) and ST/X001075/1 (AMS and IRS), and through an Ernest Rutherford Fellowship (KJD; grant number ST/W003120/1). RKC was funded by support for programme #02321, provided by\r\nNASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-03127. RKC and CLH are both grateful for support from the Leverhulme Trust via a Leverhulme Early Career Fellowship, and CLH also acknowledges support from the Oxford Hintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze Family\r\nCharitable Foundation. JSD acknowledges the support of the Royal Society via a Royal Society Research Professorship. EI gratefully acknowledge financialsupport from ANID–MILENIO–NCN2024 112 and ANID FONDECYT Regular 1221846. LOF acknowledges by ANID BECAS/DOCTORADO NACIONAL 21220499.","ddc":["520"],"author":[{"first_name":"C. A.","last_name":"Pirie","full_name":"Pirie, C. A."},{"full_name":"Best, P. N.","first_name":"P. N.","last_name":"Best"},{"first_name":"K. J.","last_name":"Duncan","full_name":"Duncan, K. J."},{"full_name":"Mcleod, D. J.","last_name":"Mcleod","first_name":"D. J."},{"full_name":"Cochrane, R. K.","first_name":"R. K.","last_name":"Cochrane"},{"full_name":"Clausen, M.","last_name":"Clausen","first_name":"M."},{"last_name":"Dunlop","first_name":"J. S.","full_name":"Dunlop, J. S."},{"full_name":"Flury, S. R.","first_name":"S. R.","last_name":"Flury"},{"full_name":"Geach, J. E.","last_name":"Geach","first_name":"J. E."},{"last_name":"Hale","first_name":"C. L.","full_name":"Hale, C. L."},{"first_name":"E.","last_name":"Ibar","full_name":"Ibar, E."},{"first_name":"R.","last_name":"Kondapally","full_name":"Kondapally, R."},{"full_name":"Li, Zefeng","first_name":"Zefeng","last_name":"Li"},{"first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","last_name":"Matthee","full_name":"Matthee, Jorryt J"},{"first_name":"R. J.","last_name":"Mclure","full_name":"Mclure, R. J."},{"first_name":"L.","last_name":"Ossa-Fuentes","full_name":"Ossa-Fuentes, L."},{"last_name":"Patrick","first_name":"A. L.","full_name":"Patrick, A. L."},{"first_name":"Ian","last_name":"Smail","full_name":"Smail, Ian"},{"last_name":"Sobral","first_name":"D.","full_name":"Sobral, D."},{"full_name":"Stephenson, H. M.O.","last_name":"Stephenson","first_name":"H. M.O."},{"last_name":"Stott","first_name":"J. P.","full_name":"Stott, J. P."},{"full_name":"Swinbank, A. M.","first_name":"A. M.","last_name":"Swinbank"}],"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"}},{"author":[{"full_name":"Ďurovčíková, Dominika","first_name":"Dominika","last_name":"Ďurovčíková"},{"full_name":"Eilers, Anna Christina","first_name":"Anna Christina","last_name":"Eilers"},{"last_name":"Simcoe","first_name":"Robert A.","full_name":"Simcoe, Robert A."},{"last_name":"Welsh","first_name":"Louise","full_name":"Welsh, Louise"},{"full_name":"Meyer, Romain A.","last_name":"Meyer","first_name":"Romain A."},{"last_name":"Matthee","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"},{"first_name":"Emma V.","last_name":"Ryan-Weber","full_name":"Ryan-Weber, Emma V."},{"full_name":"Yue, Minghao","first_name":"Minghao","last_name":"Yue"},{"first_name":"Harley","last_name":"Katz","full_name":"Katz, Harley"},{"full_name":"Satyavolu, Sindhu","first_name":"Sindhu","last_name":"Satyavolu"},{"last_name":"Becker","first_name":"George","full_name":"Becker, George"},{"full_name":"Davies, Frederick B.","first_name":"Frederick B.","last_name":"Davies"},{"first_name":"Emanuele Paolo","last_name":"Farina","full_name":"Farina, Emanuele Paolo"}],"ddc":["520"],"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2025-07-20T22:02:01Z","acknowledgement":"We thank the referee for the feedback and suggestions that greatly improved the quality of this manuscript. We would like to thank Carlos Contreras, Matías Díaz, Carla Fuentes, Mauricio Martínez, Alberto Pastén, Roger Leiton, Hugo Rivera, and Gabriel Prieto for their help and support during the Magellan/FIRE observations. We would also like to thank Rongmon Bordoloi for helpful discussions. R.A.M. acknowledges support from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. This Letter includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile.\r\nBased on observations collected at the European Southern Observatory under ESO programs 106.215A and 096.A-0418.\r\n\r\nThe HST data presented in this Letter were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. The observations analyzed in this work can be accessed via doi:10.17909/gxmz-zd87.","issue":"2","type":"journal_article","OA_type":"gold","doi":"10.3847/2041-8213/ade71c","file_date_updated":"2025-07-22T08:38:14Z","status":"public","day":"10","title":"An extremely metal-poor Lyα emitter candidate at z = 6 revealed through absorption spectroscopy","date_updated":"2026-02-16T12:44:23Z","language":[{"iso":"eng"}],"oa_version":"Published Version","intvolume":" 987","abstract":[{"lang":"eng","text":"We report the discovery of a Lyα emitter (LAE) candidate in the immediate foreground of the quasar PSO J158-14 at zQSO = 6.0685 at a projected distance ∼29 pkpc that is associated with an extremely metal-poor absorption system. This system was found in archival observations of the quasar field with the Very Large Telescope (VLT)/Multi-Unit Spectroscopic Explorer (MUSE) and was previously missed in searches of absorption systems using quasar absorption line spectroscopy, as it imparts no detectable metal absorption lines on the background quasar spectrum. The detected Lyα emission line at a redshift of zLAE = 6.0323 is well aligned with the outer edge of the quasar’s proximity zone and can plausibly cause its observed damping wing if it is associated with a proximate subdamped Lyα absorption system with a column density of log Nhi/cm^-2 19.7. A >10 hr medium-resolution spectrum of the quasar observed with the Magellan/Folded-port InfraRed Echellette (FIRE) and VLT/X-Shooter spectrographs reveals a metallicity constraint of [Z/H] < −3. Such low metallicity makes this system an extremely metal-poor galaxy candidate and provides an exciting site to study possible signatures of Population III stars."}],"article_number":"L33","DOAJ_listed":"1","file":[{"date_created":"2025-07-22T08:38:14Z","checksum":"75d0c08514209fc6e3078fdec8e815a2","success":1,"creator":"dernst","content_type":"application/pdf","file_id":"20066","access_level":"open_access","date_updated":"2025-07-22T08:38:14Z","file_name":"2025_AstrophysicalJourLetters_Durovcikova.pdf","relation":"main_file","file_size":6453728}],"external_id":{"arxiv":["2505.01499"],"isi":["001524847100001"]},"year":"2025","isi":1,"quality_controlled":"1","fulldoi":"https://doi.org/10.3847/2041-8213/ade71c","publisher":"IOP Publishing","PlanS_conform":"1","scopus_import":"1","publication":"The Astrophysical Journal Letters","publication_identifier":{"eissn":["2041-8213"],"issn":["2041-8205"]},"_id":"20030","arxiv":1,"OA_place":"publisher","oa":1,"has_accepted_license":"1","article_processing_charge":"Yes","department":[{"_id":"JoMa"}],"volume":987,"citation":{"chicago":"Ďurovčíková, Dominika, Anna Christina Eilers, Robert A. Simcoe, Louise Welsh, Romain A. Meyer, Jorryt J Matthee, Emma V. Ryan-Weber, et al. “An Extremely Metal-Poor Lyα Emitter Candidate at z = 6 Revealed through Absorption Spectroscopy.” The Astrophysical Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/ade71c.","ama":"Ďurovčíková D, Eilers AC, Simcoe RA, et al. An extremely metal-poor Lyα emitter candidate at z = 6 revealed through absorption spectroscopy. The Astrophysical Journal Letters. 2025;987(2). doi:10.3847/2041-8213/ade71c","mla":"Ďurovčíková, Dominika, et al. “An Extremely Metal-Poor Lyα Emitter Candidate at z = 6 Revealed through Absorption Spectroscopy.” The Astrophysical Journal Letters, vol. 987, no. 2, L33, IOP Publishing, 2025, doi:10.3847/2041-8213/ade71c.","apa":"Ďurovčíková, D., Eilers, A. C., Simcoe, R. A., Welsh, L., Meyer, R. A., Matthee, J. J., … Farina, E. P. (2025). An extremely metal-poor Lyα emitter candidate at z = 6 revealed through absorption spectroscopy. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ade71c","ista":"Ďurovčíková D, Eilers AC, Simcoe RA, Welsh L, Meyer RA, Matthee JJ, Ryan-Weber EV, Yue M, Katz H, Satyavolu S, Becker G, Davies FB, Farina EP. 2025. An extremely metal-poor Lyα emitter candidate at z = 6 revealed through absorption spectroscopy. The Astrophysical Journal Letters. 987(2), L33.","short":"D. Ďurovčíková, A.C. Eilers, R.A. Simcoe, L. Welsh, R.A. Meyer, J.J. Matthee, E.V. Ryan-Weber, M. Yue, H. Katz, S. Satyavolu, G. Becker, F.B. Davies, E.P. Farina, The Astrophysical Journal Letters 987 (2025).","ieee":"D. Ďurovčíková et al., “An extremely metal-poor Lyα emitter candidate at z = 6 revealed through absorption spectroscopy,” The Astrophysical Journal Letters, vol. 987, no. 2. IOP Publishing, 2025."},"date_published":"2025-07-10T00:00:00Z","publication_status":"published","month":"07","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original"},{"article_processing_charge":"No","department":[{"_id":"MaIb"},{"_id":"LifeSc"}],"citation":{"chicago":"Lee, Seungho, Daniel Balazs, Sharona Horta, Aiswarya Rayaroth Puthiyaveettil, and Maria Ibáñez. “Reaction Precursor-Mediated Formation of Stable Supercrystals in Colloidal Nanocrystal Synthesis: PbTe Case.” In Proceedings of the MATSUS Spring 2025 Conference. Fundació de la comunitat valenciana SCITO, 2025. https://doi.org/10.29363/nanoge.matsusspring.2025.173.","ama":"Lee S, Balazs D, Horta S, Rayaroth Puthiyaveettil A, Ibáñez M. Reaction precursor-mediated formation of stable supercrystals in colloidal nanocrystal synthesis: PbTe case. In: Proceedings of the MATSUS Spring 2025 Conference. Fundació de la comunitat valenciana SCITO; 2025. doi:10.29363/nanoge.matsusspring.2025.173","ieee":"S. Lee, D. Balazs, S. Horta, A. Rayaroth Puthiyaveettil, and M. Ibáñez, “Reaction precursor-mediated formation of stable supercrystals in colloidal nanocrystal synthesis: PbTe case,” in Proceedings of the MATSUS Spring 2025 Conference, Sevilla, Spain, 2025.","short":"S. Lee, D. Balazs, S. Horta, A. Rayaroth Puthiyaveettil, M. Ibáñez, in:, Proceedings of the MATSUS Spring 2025 Conference, Fundació de la comunitat valenciana SCITO, 2025.","mla":"Lee, Seungho, et al. “Reaction Precursor-Mediated Formation of Stable Supercrystals in Colloidal Nanocrystal Synthesis: PbTe Case.” Proceedings of the MATSUS Spring 2025 Conference, 173, Fundació de la comunitat valenciana SCITO, 2025, doi:10.29363/nanoge.matsusspring.2025.173.","ista":"Lee S, Balazs D, Horta S, Rayaroth Puthiyaveettil A, Ibáñez M. 2025. Reaction precursor-mediated formation of stable supercrystals in colloidal nanocrystal synthesis: PbTe case. Proceedings of the MATSUS Spring 2025 Conference. MATSUS: Materials for Sustainable Development Conference, 173.","apa":"Lee, S., Balazs, D., Horta, S., Rayaroth Puthiyaveettil, A., & Ibáñez, M. (2025). Reaction precursor-mediated formation of stable supercrystals in colloidal nanocrystal synthesis: PbTe case. In Proceedings of the MATSUS Spring 2025 Conference. Sevilla, Spain: Fundació de la comunitat valenciana SCITO. https://doi.org/10.29363/nanoge.matsusspring.2025.173"},"month":"03","publication_status":"published","date_published":"2025-03-15T00:00:00Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publisher":"Fundació de la comunitat valenciana SCITO","fulldoi":"https://doi.org/10.29363/nanoge.matsusspring.2025.173","_id":"20055","publication":"Proceedings of the MATSUS Spring 2025 Conference","project":[{"_id":"9B8F7476-BA93-11EA-9121-9846C619BF3A","name":"HighTE: The Werner Siemens Laboratory for the High Throughput Discovery of Semiconductors for Waste Heat Recovery"}],"language":[{"iso":"eng"}],"oa_version":"None","day":"15","title":"Reaction precursor-mediated formation of stable supercrystals in colloidal nanocrystal synthesis: PbTe case","date_updated":"2026-02-19T09:25:57Z","article_number":"173","abstract":[{"text":"Supercrystals represent three-dimensional orderings of colloidal nanocrystals (NCs), showcasing collective properties in photonics, phononics, and electronics applications.1,2 Recent studies have shown that such assemblies are directly produced during nanocrystal reactions.3–6 However, a fundamental understanding of in situ formed supercrystals that withstand typical NC purification processes remains underexplored, which is important for further use. Herein, we report the reaction precursor-mediated formation of stable PbTe supercrystals. Rationalizing the formation of these assemblies through small-angle x-ray scattering (SAXS) measurements, we unveil their formation mechanism. Our findings reveal that the supercrystal formation occurs in the presence of an excess of lead oleates in the crude solution. It should be noted that the formed supercrystals can be stabilized under specific conditions determined by the lead oleate cluster concentration, content of trioctylphosphine telluride (TOP-Te), NC size and the need of an annealing step at mild conditions. Furthermore, this approach allows for the continuous growth of a secondary phase within the supercrystal; for example in the case of PbTe supercrystals, a PbS shell can be grown on each PbTe NC constituent, resulting in core-shell PbTe-PbS supercrystals. Our work elucidates that reaction precursors play an important role in in situ SC formation and stabilization, implying the possibility of applying this knowledge to other NC reactions.","lang":"eng"}],"year":"2025","quality_controlled":"1","corr_author":"1","author":[{"full_name":"Lee, Seungho","orcid":"0000-0002-6962-8598","last_name":"Lee","first_name":"Seungho","id":"BB243B88-D767-11E9-B658-BC13E6697425"},{"full_name":"Balazs, Daniel","first_name":"Daniel","id":"302BADF6-85FC-11EA-9E3B-B9493DDC885E","last_name":"Balazs","orcid":"0000-0001-7597-043X"},{"full_name":"Horta, Sharona","last_name":"Horta","id":"03a7e858-01b1-11ec-8b71-99ae6c4a05bc","first_name":"Sharona"},{"full_name":"Rayaroth Puthiyaveettil, Aiswarya","last_name":"Rayaroth Puthiyaveettil","id":"8aceb01b-8972-11ed-ae7b-d5fe53775add","first_name":"Aiswarya"},{"full_name":"Ibáñez, Maria","first_name":"Maria","id":"43C61214-F248-11E8-B48F-1D18A9856A87","last_name":"Ibáñez","orcid":"0000-0001-5013-2843"}],"acknowledgement":"ISTA and the Werner Siemens Foundation financially supported this work. The Scientific Service Units (SSU) of ISTA supported this research through resources provided by the Electron Microscopy Facility (EMF), NMR Facility and the Lab Support Facility (LSF).","date_created":"2025-07-21T08:33:20Z","OA_type":"closed access","status":"public","doi":"10.29363/nanoge.matsusspring.2025.173","type":"conference","acknowledged_ssus":[{"_id":"EM-Fac"},{"_id":"NMR"},{"_id":"LifeSc"}],"conference":{"end_date":"2025-03-07","location":"Sevilla, Spain","start_date":"2025-03-03","name":"MATSUS: Materials for Sustainable Development Conference"}},{"publication_status":"published","date_published":"2025-10-01T00:00:00Z","month":"10","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","department":[{"_id":"ZoHa"}],"article_processing_charge":"No","volume":9,"citation":{"short":"M. Onoue, X. Ding, J.D. Silverman, Y. Matsuoka, T. Izumi, M.A. Strauss, C. Ward, C.L. Phillips, K. Ito, I.T. Andika, K. Aoki, J. Arita, S. Baba, R. Bieri, S.E.I. Bosman, A.C. Eilers, S. Fujimoto, M. Habouzit, Z. Haiman, M. Imanishi, K. Inayoshi, K. Iwasawa, K. Jahnke, N. Kashikawa, T. Kawaguchi, K. Kohno, C.H. Lee, J. Li, A. Lupi, J. Lyu, T. Nagao, R. Overzier, J.T. Schindler, M. Schramm, M.T. Scoggins, K. Shimasaku, Y. Toba, B. Trakhtenbrot, M. Trebitsch, T. Treu, H. Umehata, B. Venemans, M. Vestergaard, M. Volonteri, F. Walter, F. Wang, J. Yang, H. Zhang, Nature Astronomy 9 (2025) 1541–1552.","mla":"Onoue, Masafusa, et al. “A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z > 6.” Nature Astronomy, vol. 9, Springer Nature, 2025, pp. 1541–52, doi:10.1038/s41550-025-02628-1.","apa":"Onoue, M., Ding, X., Silverman, J. D., Matsuoka, Y., Izumi, T., Strauss, M. A., … Zhang, H. (2025). A post-starburst pathway for the formation of massive galaxies and black holes at z > 6. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-025-02628-1","ista":"Onoue M, Ding X, Silverman JD, Matsuoka Y, Izumi T, Strauss MA, Ward C, Phillips CL, Ito K, Andika IT, Aoki K, Arita J, Baba S, Bieri R, Bosman SEI, Eilers AC, Fujimoto S, Habouzit M, Haiman Z, Imanishi M, Inayoshi K, Iwasawa K, Jahnke K, Kashikawa N, Kawaguchi T, Kohno K, Lee CH, Li J, Lupi A, Lyu J, Nagao T, Overzier R, Schindler JT, Schramm M, Scoggins MT, Shimasaku K, Toba Y, Trakhtenbrot B, Trebitsch M, Treu T, Umehata H, Venemans B, Vestergaard M, Volonteri M, Walter F, Wang F, Yang J, Zhang H. 2025. A post-starburst pathway for the formation of massive galaxies and black holes at z > 6. Nature Astronomy. 9, 1541–1552.","ieee":"M. Onoue et al., “A post-starburst pathway for the formation of massive galaxies and black holes at z > 6,” Nature Astronomy, vol. 9. Springer Nature, pp. 1541–1552, 2025.","chicago":"Onoue, Masafusa, Xuheng Ding, John D. Silverman, Yoshiki Matsuoka, Takuma Izumi, Michael A. Strauss, Charlotte Ward, et al. “A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z > 6.” Nature Astronomy. Springer Nature, 2025. https://doi.org/10.1038/s41550-025-02628-1.","ama":"Onoue M, Ding X, Silverman JD, et al. A post-starburst pathway for the formation of massive galaxies and black holes at z > 6. Nature Astronomy. 2025;9:1541-1552. doi:10.1038/s41550-025-02628-1"},"OA_place":"repository","arxiv":1,"oa":1,"fulldoi":"https://doi.org/10.1038/s41550-025-02628-1","scopus_import":"1","publisher":"Springer Nature","publication":"Nature Astronomy","_id":"20193","publication_identifier":{"eissn":["2397-3366"]},"external_id":{"isi":["001548138600001"],"arxiv":["2409.07113"]},"year":"2025","isi":1,"page":"1541-1552","quality_controlled":"1","day":"01","title":"A post-starburst pathway for the formation of massive galaxies and black holes at z > 6","date_updated":"2025-12-30T13:08:12Z","language":[{"iso":"eng"}],"oa_version":"Preprint","intvolume":" 9","abstract":[{"lang":"eng","text":"Understanding the rapid formation of supermassive black holes in the early Universe requires insights into stellar mass growth in host galaxies. Here we present NIRSpec rest-frame optical spectra and NIRCam imaging from JWST of two galaxies at z > 6, both hosting moderate-luminosity quasars. These galaxies exhibit Balmer absorption lines, like low-redshift post-starburst galaxies. Our analyses of the medium-resolution spectra and multiband photometry show that the bulk of the stellar mass (log(M*/M☉) ≥ 10.6) formed in starburst episodes at redshift 9 and 7. One of the galaxies shows a clear Balmer break and lacks spatially resolved Hα emission. It falls well below the star-formation main sequence at z = 6, indicating quiescence. The other is transitioning to quiescence; together, these massive galaxies are among the most distant post-starburst systems known. The blueshifted wings of the quasar [O iii] emission lines indicate quasar-driven outflow, which possibly influences star formation. Direct stellar velocity dispersion measurements reveal that one galaxy follows the local black hole mass versus σ* relation whereas the other is overmassive. The existence of massive post-starburst galaxies hosting billion-solar-mass black holes in short-lived quasar phases indicates that supermassive black holes and host galaxies played a principal role in each other’s rapid early formation."}],"type":"journal_article","OA_type":"green","status":"public","doi":"10.1038/s41550-025-02628-1","author":[{"first_name":"Masafusa","last_name":"Onoue","full_name":"Onoue, Masafusa"},{"full_name":"Ding, Xuheng","first_name":"Xuheng","last_name":"Ding"},{"last_name":"Silverman","first_name":"John D.","full_name":"Silverman, John D."},{"first_name":"Yoshiki","last_name":"Matsuoka","full_name":"Matsuoka, Yoshiki"},{"first_name":"Takuma","last_name":"Izumi","full_name":"Izumi, Takuma"},{"full_name":"Strauss, Michael A.","last_name":"Strauss","first_name":"Michael A."},{"full_name":"Ward, Charlotte","first_name":"Charlotte","last_name":"Ward"},{"last_name":"Phillips","first_name":"Camryn L.","full_name":"Phillips, Camryn L."},{"full_name":"Ito, Kei","last_name":"Ito","first_name":"Kei"},{"full_name":"Andika, Irham T.","first_name":"Irham T.","last_name":"Andika"},{"first_name":"Kentaro","last_name":"Aoki","full_name":"Aoki, Kentaro"},{"full_name":"Arita, Junya","first_name":"Junya","last_name":"Arita"},{"last_name":"Baba","first_name":"Shunsuke","full_name":"Baba, Shunsuke"},{"first_name":"Rebekka","last_name":"Bieri","full_name":"Bieri, Rebekka"},{"last_name":"Bosman","first_name":"Sarah E.I.","full_name":"Bosman, Sarah E.I."},{"first_name":"Anna Christina","last_name":"Eilers","full_name":"Eilers, Anna Christina"},{"full_name":"Fujimoto, Seiji","first_name":"Seiji","last_name":"Fujimoto"},{"full_name":"Habouzit, Melanie","last_name":"Habouzit","first_name":"Melanie"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","orcid":"0000-0003-3633-5403","last_name":"Haiman","full_name":"Haiman, Zoltán"},{"full_name":"Imanishi, Masatoshi","first_name":"Masatoshi","last_name":"Imanishi"},{"full_name":"Inayoshi, Kohei","last_name":"Inayoshi","first_name":"Kohei"},{"last_name":"Iwasawa","first_name":"Kazushi","full_name":"Iwasawa, Kazushi"},{"first_name":"Knud","last_name":"Jahnke","full_name":"Jahnke, Knud"},{"full_name":"Kashikawa, Nobunari","first_name":"Nobunari","last_name":"Kashikawa"},{"full_name":"Kawaguchi, Toshihiro","first_name":"Toshihiro","last_name":"Kawaguchi"},{"full_name":"Kohno, Kotaro","last_name":"Kohno","first_name":"Kotaro"},{"last_name":"Lee","first_name":"Chien Hsiu","full_name":"Lee, Chien Hsiu"},{"last_name":"Li","first_name":"Junyao","full_name":"Li, Junyao"},{"full_name":"Lupi, Alessandro","first_name":"Alessandro","last_name":"Lupi"},{"first_name":"Jianwei","last_name":"Lyu","full_name":"Lyu, Jianwei"},{"full_name":"Nagao, Tohru","first_name":"Tohru","last_name":"Nagao"},{"last_name":"Overzier","first_name":"Roderik","full_name":"Overzier, Roderik"},{"last_name":"Schindler","first_name":"Jan Torge","full_name":"Schindler, Jan Torge"},{"full_name":"Schramm, Malte","first_name":"Malte","last_name":"Schramm"},{"last_name":"Scoggins","first_name":"Matthew T.","full_name":"Scoggins, Matthew T."},{"full_name":"Shimasaku, Kazuhiro","last_name":"Shimasaku","first_name":"Kazuhiro"},{"last_name":"Toba","first_name":"Yoshiki","full_name":"Toba, Yoshiki"},{"first_name":"Benny","last_name":"Trakhtenbrot","full_name":"Trakhtenbrot, Benny"},{"last_name":"Trebitsch","first_name":"Maxime","full_name":"Trebitsch, Maxime"},{"first_name":"Tommaso","last_name":"Treu","full_name":"Treu, Tommaso"},{"first_name":"Hideki","last_name":"Umehata","full_name":"Umehata, Hideki"},{"last_name":"Venemans","first_name":"Bram","full_name":"Venemans, Bram"},{"full_name":"Vestergaard, Marianne","last_name":"Vestergaard","first_name":"Marianne"},{"first_name":"Marta","last_name":"Volonteri","full_name":"Volonteri, Marta"},{"last_name":"Walter","first_name":"Fabian","full_name":"Walter, Fabian"},{"first_name":"Feige","last_name":"Wang","full_name":"Wang, Feige"},{"full_name":"Yang, Jinyi","last_name":"Yang","first_name":"Jinyi"},{"full_name":"Zhang, Haowen","last_name":"Zhang","first_name":"Haowen"}],"date_created":"2025-08-17T22:01:38Z","main_file_link":[{"url":"https://arxiv.org/abs/2409.07113","open_access":"1"}],"acknowledgement":"We thank A. C. Carnall for supporting our use of Bagpipes. We thank Y. Fu for his help on the use of QSOFitMORE. We thank J. Greene, S. Toft, T. Kakimoto and M. Tanaka for fruitful discussions. This work is based on observations made with the NASA/ESA/CSA JWST. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, under NASA contract NAS 5-03127 for JWST. These observations are associated with programmes GO 1967 and GO 3859. Support for these programmes was provided by NASA through a grant from the Space Telescope Science Institute. This work was supported by World Premier International Research Center Initiative, MEXT, Japan. This work used computing resources at Kavli IPMU. M.O., X.D., J.D.S., Y.M., T.I., K. Ito, K.K. and H.U. are supported by the Japan Society for the Promotion of Science (KAKENHI Grant Numbers JP24K22894, JP22K14071, JP18H01251, JP22H01262, JP21H04494, JP20K14531, JP23K13141, JP17H06130 and JP20H01953). M.O. and K. Inayoshi acknowledge support from the National Natural Science Foundation of China (Grant Numbers 12150410307, 12073003, 11721303, 11991052 and 11950410493). K. Inayoshi acknowledges support from the China Manned Space Project (Grant Numbers CMS-CSST-2021-A04 and CMS-CSST-2021-A06). S.E.I.B. is funded by the Deutsche Forschungsgemeinschaft (German Research Foundation) under Emmy Noether Grant Number BO 5771/1-1. Z.H., T.T. and M.S. acknowledge support from the NSF (Grant Numbers AST-2006176, AST-1907208 and AST-2006177). A.L. acknowledges funding from MUR (Grant Number PRIN 2022935STW). B.T. acknowledges support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant Agreement Number 950533) and from the Israel Science Foundation (Grant Number 1849/19). F. Walter acknowledges support from the ERC (Grant Cosmic_gas). J.-T.S. is supported by the Deutsche Forschungsgemeinschaft (Project Number 518006966). M.T. acknowledges support from the NWO (Grant Number 0.16.VIDI.189.162, ODIN). S.F. acknowledges support from NASA through the NASA Hubble Fellowship (Grant Number HST-HF2-51505.001-A awarded by the Space Telescope Science Institute). K. Iwasawa acknowledges support under Grant Number PID2022-136827NB-C44 funded by MCIN/AEI/10.13039/501100011033 /FEDER, EU. M. Vestergaard gratefully acknowledges financial support from the Independent Research Fund Denmark (Grant Numbers DFF 8021-00130 and 3103-00146). F. Wang acknowledges support from the NSF (Award Number AST-2513040). R.B. is supported by the SNSF through the Ambizione Grant PZ00P2_223532."},{"language":[{"iso":"eng"}],"oa_version":"Published Version","day":"01","date_updated":"2025-09-10T08:14:28Z","title":"An assessment of representing land‐ocean heterogeneity via CAPE relaxation timescale in the Community Atmospheric Model 6 (CAM6)","abstract":[{"text":"The time needed by deep convection to bring the atmosphere back to equilibrium is called convective adjustment timescale or simply adjustment timescale, typically denoted by . In the Community Atmospheric Model|Community Atmosphere Model (CAM), is the convective available potential energy (CAPE) relaxation timescale and is 1 hr, worldwide. Observational evidence suggests that is generally longer than 1 hr. Further, continental and oceanic convection are different in terms of the vigor of updrafts and can have different longevities. So using hour worldwide in CAM has two potential caveats. A longer improves the simulation of the mean climate. However, it does not address the land‐ocean heterogeneity of atmospheric deep convection. We investigate the prescription of two different CAPE relaxation timescales for land ( hr) and ocean ( to 4 hr). It is arguably an extremely crude parameterization of boundary layer control on atmospheric convection. We contrast a suite of 5‐year‐long simulations with two different for land and ocean to having one globally. The choice of longer over ocean is guided by previous studies and inspired by observational pieces of evidence. Nonetheless, to complement our variable experiments, we perform a simulation with hr and hrs. Most importantly, our key findings are immune to the exact values of prescribed and . The CAM model, with two values , improves convective‐stratiform rainfall partitioning and the Madden–Julian oscillation propagation characteristics.","lang":"eng"}],"article_number":"e2025MS005035","DOAJ_listed":"1","file":[{"relation":"main_file","file_size":2143025,"file_id":"20338","success":1,"checksum":"5961d6290432c5ac0e8587ef07f30c9b","content_type":"application/pdf","creator":"dernst","date_created":"2025-09-10T08:12:34Z","file_name":"2025_JAMES_Goswami.pdf","date_updated":"2025-09-10T08:12:34Z","access_level":"open_access"}],"intvolume":" 17","year":"2025","license":"https://creativecommons.org/licenses/by-nc-nd/4.0/","quality_controlled":"1","corr_author":"1","tmp":{"short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode"},"author":[{"orcid":"0000-0001-8602-3083","last_name":"GOSWAMI","first_name":"BIDYUT B","id":"3a4ac09c-6d61-11ec-bf66-884cde66b64b","full_name":"GOSWAMI, BIDYUT B"},{"id":"74c777f4-32da-11ee-b498-874db0835561","first_name":"Andrea","last_name":"Polesello","full_name":"Polesello, Andrea"},{"id":"f978ccb0-3f7f-11eb-b193-b0e2bd13182b","first_name":"Caroline J","last_name":"Muller","orcid":"0000-0001-5836-5350","full_name":"Muller, Caroline J"}],"ddc":["550"],"acknowledgement":"The authors gratefully acknowledge funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (Project CLUSTER, Grant 805041). This research was supported by the Scientific Service Units (SSU) of ISTA through resources provided by Scientific Computing (SciComp). We would like to thank Prof. Courtney Schumacher and Dr. Aaron Funk of Texas A&M University for their help in understanding the TRMM Radar data. The authors are grateful to two anonymous reviewers who helped improve the quality of this paper.","issue":"9","date_created":"2025-09-10T05:36:16Z","OA_type":"gold","status":"public","file_date_updated":"2025-09-10T08:12:34Z","doi":"10.1029/2025ms005035","type":"journal_article","acknowledged_ssus":[{"_id":"ScienComp"}],"article_processing_charge":"Yes","department":[{"_id":"CaMu"}],"ec_funded":1,"citation":{"apa":"GOSWAMI, B. B., Polesello, A., & Muller, C. J. (2025). An assessment of representing land‐ocean heterogeneity via CAPE relaxation timescale in the Community Atmospheric Model 6 (CAM6). Journal of Advances in Modeling Earth Systems. Wiley. https://doi.org/10.1029/2025ms005035","ista":"GOSWAMI BB, Polesello A, Muller CJ. 2025. An assessment of representing land‐ocean heterogeneity via CAPE relaxation timescale in the Community Atmospheric Model 6 (CAM6). Journal of Advances in Modeling Earth Systems. 17(9), e2025MS005035.","mla":"GOSWAMI, BIDYUT B., et al. “An Assessment of Representing Land‐ocean Heterogeneity via CAPE Relaxation Timescale in the Community Atmospheric Model 6 (CAM6).” Journal of Advances in Modeling Earth Systems, vol. 17, no. 9, e2025MS005035, Wiley, 2025, doi:10.1029/2025ms005035.","short":"B.B. GOSWAMI, A. Polesello, C.J. Muller, Journal of Advances in Modeling Earth Systems 17 (2025).","ieee":"B. B. GOSWAMI, A. Polesello, and C. J. Muller, “An assessment of representing land‐ocean heterogeneity via CAPE relaxation timescale in the Community Atmospheric Model 6 (CAM6),” Journal of Advances in Modeling Earth Systems, vol. 17, no. 9. Wiley, 2025.","ama":"GOSWAMI BB, Polesello A, Muller CJ. An assessment of representing land‐ocean heterogeneity via CAPE relaxation timescale in the Community Atmospheric Model 6 (CAM6). Journal of Advances in Modeling Earth Systems. 2025;17(9). doi:10.1029/2025ms005035","chicago":"GOSWAMI, BIDYUT B, Andrea Polesello, and Caroline J Muller. “An Assessment of Representing Land‐ocean Heterogeneity via CAPE Relaxation Timescale in the Community Atmospheric Model 6 (CAM6).” Journal of Advances in Modeling Earth Systems. Wiley, 2025. https://doi.org/10.1029/2025ms005035."},"volume":17,"month":"09","date_published":"2025-09-01T00:00:00Z","publication_status":"published","article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publisher":"Wiley","scopus_import":"1","fulldoi":"https://doi.org/10.1029/2025ms005035","_id":"20319","publication_identifier":{"eissn":["1942-2466"]},"publication":"Journal of Advances in Modeling Earth Systems","OA_place":"publisher","project":[{"call_identifier":"H2020","grant_number":"805041","name":"Organization of CLoUdS, and implications of Tropical cyclones and for the Energetics of the tropics, in current and waRming climate","_id":"629205d8-2b32-11ec-9570-e1356ff73576"}],"has_accepted_license":"1","oa":1},{"publication":"Astronomy & Astrophysics","_id":"20544","publication_identifier":{"issn":["0004-6361"],"eissn":["1432-0746"]},"fulldoi":"https://doi.org/10.1051/0004-6361/202555816","publisher":"EDP Sciences","PlanS_conform":"1","scopus_import":"1","oa":1,"has_accepted_license":"1","OA_place":"publisher","volume":702,"citation":{"ama":"Hviding RE, de Graaff A, Miller TB, et al. RUBIES: A spectroscopic census of little red dots. Astronomy & Astrophysics. 2025;702. doi:10.1051/0004-6361/202555816","chicago":"Hviding, Raphael E., Anna de Graaff, Tim B. Miller, David J. Setton, Jenny E. Greene, Ivo Labbé, Gabriel Brammer, et al. “RUBIES: A Spectroscopic Census of Little Red Dots.” Astronomy & Astrophysics. EDP Sciences, 2025. https://doi.org/10.1051/0004-6361/202555816.","short":"R.E. Hviding, A. de Graaff, T.B. Miller, D.J. Setton, J.E. Greene, I. Labbé, G. Brammer, R. Bezanson, L.A. Boogaard, N.J. Cleri, J. Leja, M.V. Maseda, I. McConachie, J.J. Matthee, R.P. Naidu, P.A. Oesch, B. Wang, K.E. Whitaker, C.C. Williams, Astronomy & Astrophysics 702 (2025).","mla":"Hviding, Raphael E., et al. “RUBIES: A Spectroscopic Census of Little Red Dots.” Astronomy & Astrophysics, vol. 702, A57, EDP Sciences, 2025, doi:10.1051/0004-6361/202555816.","apa":"Hviding, R. E., de Graaff, A., Miller, T. B., Setton, D. J., Greene, J. E., Labbé, I., … Williams, C. C. (2025). RUBIES: A spectroscopic census of little red dots. Astronomy & Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202555816","ista":"Hviding RE, de Graaff A, Miller TB, Setton DJ, Greene JE, Labbé I, Brammer G, Bezanson R, Boogaard LA, Cleri NJ, Leja J, Maseda MV, McConachie I, Matthee JJ, Naidu RP, Oesch PA, Wang B, Whitaker KE, Williams CC. 2025. RUBIES: A spectroscopic census of little red dots. Astronomy & Astrophysics. 702, A57.","ieee":"R. E. Hviding et al., “RUBIES: A spectroscopic census of little red dots,” Astronomy & Astrophysics, vol. 702. EDP Sciences, 2025."},"department":[{"_id":"JoMa"}],"article_processing_charge":"Yes (via OA deal)","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","related_material":{"link":[{"url":"https://doi.org/10.1051/0004-6361/202659153e","relation":"erratum"}]},"article_type":"original","date_published":"2025-10-01T00:00:00Z","publication_status":"published","month":"10","date_created":"2025-10-27T08:17:26Z","acknowledgement":"Open access funding provided by Max Planck Society. We would like to thank the anonymous reviewer for their constructive comments which improved the final manuscript. REH acknowledges support by the German Aerospace Center (DLR) and the Federal Ministry for Economic Affairs and Energy (BMWi) through program 50OR2403 ‘RUBIES’. TBM was supported by a CIERA Postdoctoral Fellowship. This work used computing resources provided by Northwestern University and the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA). This research was supported in part through the computational resources and staff contributions provided for the Quest high performance computing facility at Northwestern University which is jointly supported by the Office of the Provost, the Office for Research, and Northwestern University Information Technology. Support for this work was provided by The Brinson Foundation through a Brinson Prize Fellowship grant. The Cosmic Dawn Center is funded by the Danish National Research Foundation (DNRF) under grant #140. This work has received funding from the Swiss State Secretariat for Education, Research and Innovation (SERI) under contract number MB22.00072, as well as from the Swiss National Science Foundation (SNSF) through project grant 200020_207349. Support for this work for RPN was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. The work of CCW is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The data products presented herein were retrieved from the Dawn JWST Archive (DJA). DJA is an initiative of the Cosmic Dawn Center (DAWN). This work is based in part on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with programs numbers 1345, 1837, 2234, 2279, 2514, 2750, 3990 and 4233. Support for program no. 4233 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127. The authors acknowledge the CEERS, PRIMER, PANORAMIC, and BEACONS teams for developing their observing program with a zero-exclusive-access period. We acknowledge the use of the following software packages which were instrumental in the development of this work: Astropy Astropy Collaboration 2013, 2018, 2022, grizli Brammer 2023a, jax Bradbury et al. 2018, jwst Bushouse et al. 2022, LaTeX Lamport 1994, MatplotlibHunter 2007, msaexp Brammer 2023b, msafit de Graaff et al. 2024, NumPy Oliphant 2006; van der Walt et al. 2011; Harris et al. 2020, NumPyro Phan et al. 2019, photutils Bradley et al. 2024b, pysersic Pasha & Miller 2023, photutils Bradley et al. 2024a, sedpy Johnson 2021, Source-Extractor Bertin & Arnouts 1996, and unite Hviding 2025. This work makes use of color palettes created by Martin Krzywinski designed for colorblindness. The color palettes and more information can be found at http://mkweb.bcgsc.ca/colorblind/","ddc":["520"],"author":[{"full_name":"Hviding, Raphael E.","last_name":"Hviding","first_name":"Raphael E."},{"full_name":"de Graaff, Anna","first_name":"Anna","last_name":"de Graaff"},{"first_name":"Tim B.","last_name":"Miller","full_name":"Miller, Tim B."},{"full_name":"Setton, David J.","first_name":"David J.","last_name":"Setton"},{"first_name":"Jenny E.","last_name":"Greene","full_name":"Greene, Jenny E."},{"last_name":"Labbé","first_name":"Ivo","full_name":"Labbé, Ivo"},{"full_name":"Brammer, Gabriel","first_name":"Gabriel","last_name":"Brammer"},{"full_name":"Bezanson, Rachel","first_name":"Rachel","last_name":"Bezanson"},{"last_name":"Boogaard","first_name":"Leindert A.","full_name":"Boogaard, Leindert A."},{"full_name":"Cleri, Nikko J.","last_name":"Cleri","first_name":"Nikko J."},{"full_name":"Leja, Joel","first_name":"Joel","last_name":"Leja"},{"full_name":"Maseda, Michael V.","first_name":"Michael V.","last_name":"Maseda"},{"first_name":"Ian","last_name":"McConachie","full_name":"McConachie, Ian"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J"},{"full_name":"Naidu, Rohan P.","last_name":"Naidu","first_name":"Rohan P."},{"full_name":"Oesch, Pascal A.","first_name":"Pascal A.","last_name":"Oesch"},{"last_name":"Wang","first_name":"Bingjie","full_name":"Wang, Bingjie"},{"full_name":"Whitaker, Katherine E.","last_name":"Whitaker","first_name":"Katherine E."},{"first_name":"Christina C.","last_name":"Williams","full_name":"Williams, Christina C."}],"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"type":"journal_article","status":"public","doi":"10.1051/0004-6361/202555816","file_date_updated":"2025-10-27T09:16:23Z","OA_type":"hybrid","intvolume":" 702","file":[{"access_level":"open_access","file_name":"2025_AstronomyAstrophysics_Hviding.pdf","date_updated":"2025-10-27T09:16:23Z","date_created":"2025-10-27T09:16:23Z","content_type":"application/pdf","success":1,"creator":"dernst","checksum":"34d6612d80f3f0e79a8f8ac33d9286ae","file_id":"20550","file_size":3885322,"relation":"main_file"}],"article_number":"A57","abstract":[{"text":"The physical nature of little red dots (LRDs), a population of compact red galaxies revealed by JWST, remains unclear. Photometric samples were constructed from varying selection criteria with limited spectroscopic follow-up available to test intrinsic spectral shapes and the prevalence of broad emission lines. We used the RUBIES survey, a large spectroscopic program with wide color-morphology coverage and homogeneous data quality, to systematically analyze the emission-line kinematics, spectral shapes, and morphologies of ∼1500 galaxies at z > 3.1. We identified broad Balmer lines via a novel fitting approach that simultaneously models NIRSpec/PRISM and G395M spectra, yielding 80 broad-line sources with 28 (35%) at z > 6. A large subpopulation naturally emerged from the broad Balmer line sources, with 36 exhibiting v-shaped UV-to-optical continua and a dominant point source component in the rest-optical; we define these as spectroscopic LRDs, constituting the largest such sample to date. Strikingly, the spectroscopic LRD population is largely recovered when either a broad line or rest-optical point source is required in combination with a v-shaped continuum, suggesting an inherent link between these three defining characteristics. We compared the spectroscopic LRD sample to published photometric searches. Although these selections have high accuracy, 80%−95% down to F444W < 26.5, only 50%−80% of the RUBIES LRDs were photometrically identified, depending on the selection criteria used. The remainder were missed due to a mixture of faint rest-UV photometry, comparatively blue rest-optical colors, or highly uncertain photometric redshifts. Our findings highlight that well-selected spectroscopic campaigns are essential for robust LRD identification, while photometric criteria require refinement to capture the full population.","lang":"eng"}],"date_updated":"2026-03-02T09:17:21Z","title":"RUBIES: A spectroscopic census of little red dots","day":"01","language":[{"iso":"eng"}],"oa_version":"Published Version","isi":1,"quality_controlled":"1","external_id":{"isi":["001589731300022"]},"year":"2025"},{"isi":1,"quality_controlled":"1","external_id":{"isi":["001600890100001"],"arxiv":["2507.05381"]},"year":"2025","intvolume":" 993","DOAJ_listed":"1","file":[{"relation":"main_file","file_size":39736710,"checksum":"11d35c1c52c000f8c14bc6de2e9f4b3f","content_type":"application/pdf","success":1,"creator":"dernst","file_id":"20680","date_created":"2025-11-24T13:18:34Z","access_level":"open_access","file_name":"2025_AstrophysicalJour_Yue.pdf","date_updated":"2025-11-24T13:18:34Z"}],"article_number":"L12","abstract":[{"lang":"eng","text":"Ionized proximity zones around luminous quasars provide a unique laboratory to characterize the Lyα emission lines from z > 6 galaxies without significant attenuation from the intergalactic medium (IGM). However, Lyα line measurements for galaxies within high-redshift quasars’ proximity zones have been rare so far. Here we present deep spectroscopic observations obtained with the NIRSpec/Micro-Shutter Assembly (MSA) instrument on the James Webb Space Telescope of galaxies in two z > 6 quasar fields. We measure the Lyα line fluxes for 50 galaxies at 6 < z < 7 with UV absolute magnitude M UV < −19 (median M UV = −19.97), among which 15 are located near the luminous quasars, i.e., within Δv < 2500 km s−1. We find that galaxies near the quasars show significant flux blueward of the systemic Lyα wavelength, and have higher Lyα equivalent width compared to galaxies at similar redshifts that are not located within the quasars’ environment. Our result indicates little or no redshift evolution for the Lyα emitter fraction from z ∼ 6.4 to z ∼ 5. Leveraging the low IGM opacity in the quasars’ vicinity, we evaluate the Lyα escape fraction (f esc Ly α) of high-redshift galaxies. Our analysis suggests that galaxies at 〈z〉 ≈ 6.4 have an average f esc Ly α = 0.14 ± 0.04. This value is consistent with reionization models where the Lyman continuum escape fraction is low ( fescLyC ≲ 0.1 ) for luminous galaxies, and where the most luminous galaxies have only a minor contribution to the total ionizing photon budget. © 2025. The Author(s). Published by the American Astronomical Society."}],"date_updated":"2026-02-16T12:45:16Z","title":"Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars","day":"01","oa_version":"Published Version","language":[{"iso":"eng"}],"type":"journal_article","doi":"10.3847/2041-8213/ae0e0e","status":"public","file_date_updated":"2025-11-24T13:18:34Z","OA_type":"gold","date_created":"2025-11-16T23:01:24Z","acknowledgement":"We thank the referee for valuable comments. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program ID #3117 and #4713. Support for\r\nthis work was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A awarded by the Space Telescope Science Institute, which is operated by the\r\nAssociation of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.","issue":"1","ddc":["520"],"author":[{"full_name":"Yue, Minghao","first_name":"Minghao","last_name":"Yue"},{"last_name":"Eilers","first_name":"Anna Christina","full_name":"Eilers, Anna Christina"},{"last_name":"Matthee","orcid":"0000-0003-2871-127X","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J"},{"first_name":"Rohan P.","last_name":"Naidu","full_name":"Naidu, Rohan P."},{"first_name":"Rongmon","last_name":"Bordoloi","full_name":"Bordoloi, Rongmon"},{"first_name":"Frederick B.","last_name":"Davies","full_name":"Davies, Frederick B."},{"full_name":"Hennawi, Joseph F.","first_name":"Joseph F.","last_name":"Hennawi"},{"last_name":"Kashino","first_name":"Daichi","full_name":"Kashino, Daichi"},{"first_name":"Ruari","last_name":"Mackenzie","full_name":"Mackenzie, Ruari"},{"full_name":"Simcoe, Robert A.","last_name":"Simcoe","first_name":"Robert A."}],"tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","publication_status":"published","date_published":"2025-11-01T00:00:00Z","month":"11","volume":993,"citation":{"chicago":"Yue, Minghao, Anna Christina Eilers, Jorryt J Matthee, Rohan P. Naidu, Rongmon Bordoloi, Frederick B. Davies, Joseph F. Hennawi, Daichi Kashino, Ruari Mackenzie, and Robert A. Simcoe. “Escape Fractions from Unattenuated Lyα Emitters around Luminous z > 6 Quasars.” The Astrophysical Journal Letters. IOP Publishing, 2025. https://doi.org/10.3847/2041-8213/ae0e0e.","ama":"Yue M, Eilers AC, Matthee JJ, et al. Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. 2025;993(1). doi:10.3847/2041-8213/ae0e0e","ieee":"M. Yue et al., “Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars,” The Astrophysical Journal Letters, vol. 993, no. 1. IOP Publishing, 2025.","short":"M. Yue, A.C. Eilers, J.J. Matthee, R.P. Naidu, R. Bordoloi, F.B. Davies, J.F. Hennawi, D. Kashino, R. Mackenzie, R.A. Simcoe, The Astrophysical Journal Letters 993 (2025).","mla":"Yue, Minghao, et al. “Escape Fractions from Unattenuated Lyα Emitters around Luminous z > 6 Quasars.” The Astrophysical Journal Letters, vol. 993, no. 1, L12, IOP Publishing, 2025, doi:10.3847/2041-8213/ae0e0e.","ista":"Yue M, Eilers AC, Matthee JJ, Naidu RP, Bordoloi R, Davies FB, Hennawi JF, Kashino D, Mackenzie R, Simcoe RA. 2025. Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. 993(1), L12.","apa":"Yue, M., Eilers, A. C., Matthee, J. J., Naidu, R. P., Bordoloi, R., Davies, F. B., … Simcoe, R. A. (2025). Escape fractions from unattenuated Lyα emitters around luminous z > 6 quasars. The Astrophysical Journal Letters. IOP Publishing. https://doi.org/10.3847/2041-8213/ae0e0e"},"department":[{"_id":"JoMa"}],"article_processing_charge":"Yes","oa":1,"has_accepted_license":"1","arxiv":1,"OA_place":"publisher","publication":"The Astrophysical Journal Letters","_id":"20649","publication_identifier":{"issn":["2041-8205"],"eissn":["2041-8213"]},"fulldoi":"https://doi.org/10.3847/2041-8213/ae0e0e","PlanS_conform":"1","scopus_import":"1","publisher":"IOP Publishing"},{"article_type":"original","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"12","publication_status":"published","date_published":"2025-12-01T00:00:00Z","citation":{"ama":"Stephenson HMO, Stott JP, Pirie CA, et al. The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. 2025;544(2):1412-1431. doi:10.1093/mnras/staf1725","chicago":"Stephenson, H. M.O., J. P. Stott, C. A. Pirie, K. J. Duncan, D. J. Mcleod, P. N. Best, M. Brinch, et al. “The JWST Emission Line Survey (JELS): The Sizes and Merger Fraction of Star-Forming Galaxies during the Epoch of Reionization.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2025. https://doi.org/10.1093/mnras/staf1725.","ieee":"H. M. O. Stephenson et al., “The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization,” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2. Oxford University Press, pp. 1412–1431, 2025.","short":"H.M.O. Stephenson, J.P. Stott, C.A. Pirie, K.J. Duncan, D.J. Mcleod, P.N. Best, M. Brinch, M. Clausen, R.K. Cochrane, J.S. Dunlop, S.R. Flury, J.E. Geach, C.L. Hale, E. Ibar, Z. Li, J.J. Matthee, R.J. Mclure, L. Ossa-Fuentes, A.L. Patrick, D. Sobral, A.M. Swinbank, Monthly Notices of the Royal Astronomical Society 544 (2025) 1412–1431.","mla":"Stephenson, H. M. O., et al. “The JWST Emission Line Survey (JELS): The Sizes and Merger Fraction of Star-Forming Galaxies during the Epoch of Reionization.” Monthly Notices of the Royal Astronomical Society, vol. 544, no. 2, Oxford University Press, 2025, pp. 1412–31, doi:10.1093/mnras/staf1725.","ista":"Stephenson HMO, Stott JP, Pirie CA, Duncan KJ, Mcleod DJ, Best PN, Brinch M, Clausen M, Cochrane RK, Dunlop JS, Flury SR, Geach JE, Hale CL, Ibar E, Li Z, Matthee JJ, Mclure RJ, Ossa-Fuentes L, Patrick AL, Sobral D, Swinbank AM. 2025. The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. 544(2), 1412–1431.","apa":"Stephenson, H. M. O., Stott, J. P., Pirie, C. A., Duncan, K. J., Mcleod, D. J., Best, P. N., … Swinbank, A. M. (2025). The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/staf1725"},"volume":544,"article_processing_charge":"Yes","department":[{"_id":"JoMa"}],"has_accepted_license":"1","oa":1,"OA_place":"publisher","_id":"20660","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"publication":"Monthly Notices of the Royal Astronomical Society","PlanS_conform":"1","scopus_import":"1","publisher":"Oxford University Press","fulldoi":"https://doi.org/10.1093/mnras/staf1725","quality_controlled":"1","isi":1,"page":"1412-1431","year":"2025","external_id":{"isi":["001611415800001"]},"abstract":[{"lang":"eng","text":"We used observations from the JWST Emission Line Survey (JELS) to measure the half-light radii (re) of 23 Hα-emitting starforming (SF) galaxies at z = 6.1 in the PRIMER/COSMOS field. Galaxy sizes were measured in JWST near-infrared camera observations in rest-frame Hα (tracing recent star formation) with the F466N and F470N narrow-band filters from JELS, and\r\ncompared against rest-R- and V -band (tracing established stellar populations) and near-ultraviolet sizes. We find a size–stellar mass(re − M∗) relationship with a slope that is consistent with literature values at lower redshifts, though offset to lowersizes. We observe a large scatter in re at low stellar mass (M∗ < 10^8.4 Mo) which we believe is the result of bursty star formation histories (SFHs) of SF galaxies at the Epoch of Reionization (EoR). We find that the stellar and ionized gas components are similar in size at z = 6.1. The evidence of already-established stellar components in these Hα emitters (HAEs) indicates previous episodes of star formation have occurred. As such, following other JELS studies finding our HAEs are undergoing a current burst of star formation, we believe our results indicate that SF galaxies at the end of the EoR have already experienced a bursty SFH. From our re − M∗ relationship, we find re,F444W = 0.76 ± 0.46 kpc for fixed stellar mass M∗ = 10^9.25 M, which is in agreement with other observations and simulations of SF galaxies in the literature. We find a close-pair (major) merger fraction of (fmaj. merger =0.44 ± 0.22) fmerger = 0.43 ± 0.11 for galaxy separations d <~ 25 kpc, which is in agreement with other z ≈ 6 studies."}],"DOAJ_listed":"1","file":[{"date_created":"2025-11-24T10:35:15Z","file_id":"20678","creator":"dernst","success":1,"content_type":"application/pdf","checksum":"ddb3f429d2246bbf536efb4b0e52f3a8","date_updated":"2025-11-24T10:35:15Z","file_name":"2025_MonthlyNoticesRAS_Stephenson.pdf","access_level":"open_access","relation":"main_file","file_size":3625308}],"intvolume":" 544","oa_version":"Published Version","language":[{"iso":"eng"}],"day":"01","date_updated":"2025-12-01T15:25:11Z","title":"The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization","OA_type":"gold","status":"public","doi":"10.1093/mnras/staf1725","file_date_updated":"2025-11-24T10:35:15Z","type":"journal_article","issue":"2","acknowledgement":"This work makes use of ASTROPY, 7 a community-developed core PYTHON package for Astronomy (Astropy Collaboration 2013, 2018, 2022), as well as the NUMPY (C. R. Harris et al. 2020) and SCIPY (P.Virtanen et al. 2020) packages(see also T. E. Oliphant 2007). All plots\r\nwere created using the MATPLOTLIB 2D graphics PYTHON package (J. D. Hunter 2007). Conversions between redshift and lookback time in our selected cosmological model were done using the Javascript cosmological calculator from E. L. Wright (2006).8 The authors would like to thank the anonymous referee for their constructive comments and suggestions which have strengthened the analysis of this work and improved the paper. The authors also gratefully acknowledge Ian Smail for providing valuable feedback and helping to guide the science of this paper. This work is based on observations made with the NASA/ESA/CSA James Webb Space\r\nTelescope. The data were obtained from the Mikulski Archive for Space Telescopes9 at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with programs GO no. 2321 (JELS) and GO no. 1837 (PRIMER). The authors acknowledge the PRIMER team for developing their observing program with a zero-exclusive-access period. HMOS acknowledges support from an STFC PhD studentship and the Faculty of Science and Technology at Lancaster University. PNB is grateful for support from the UK STFC\r\nvia grants ST/V000594/1 and ST/Y000951/1. JSD acknowledges the support of the Royal Society via a Royal Society Research Professorship. LOF acknowledges funding by ANID BECAS/DOCTORADO NACIONAL 21220499.CLH acknowledges support from the Oxford\r\nHintze Centre for Astrophysical Surveys which is funded through generous support from the Hintze family charity foundation. EI gratefully acknowledge financial support from ANID – MILENIO –NCN2024 112 and ANID FONDECYT Regular 1221846. For the purpose of open access, the authors have applied a Creative Commons attribution (CC BY) licence to any author accepted manuscript version arising.","date_created":"2025-11-23T23:01:37Z","tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"author":[{"full_name":"Stephenson, H. M.O.","first_name":"H. M.O.","last_name":"Stephenson"},{"last_name":"Stott","first_name":"J. P.","full_name":"Stott, J. P."},{"first_name":"C. A.","last_name":"Pirie","full_name":"Pirie, C. A."},{"first_name":"K. J.","last_name":"Duncan","full_name":"Duncan, K. J."},{"first_name":"D. J.","last_name":"Mcleod","full_name":"Mcleod, D. J."},{"last_name":"Best","first_name":"P. N.","full_name":"Best, P. N."},{"full_name":"Brinch, M.","last_name":"Brinch","first_name":"M."},{"full_name":"Clausen, M.","first_name":"M.","last_name":"Clausen"},{"last_name":"Cochrane","first_name":"R. K.","full_name":"Cochrane, R. K."},{"full_name":"Dunlop, J. S.","last_name":"Dunlop","first_name":"J. S."},{"first_name":"S. R.","last_name":"Flury","full_name":"Flury, S. R."},{"first_name":"J. E.","last_name":"Geach","full_name":"Geach, J. E."},{"first_name":"C. L.","last_name":"Hale","full_name":"Hale, C. L."},{"last_name":"Ibar","first_name":"E.","full_name":"Ibar, E."},{"first_name":"Zefeng","last_name":"Li","full_name":"Li, Zefeng"},{"full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X","last_name":"Matthee","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Mclure","first_name":"R. J.","full_name":"Mclure, R. J."},{"full_name":"Ossa-Fuentes, L.","last_name":"Ossa-Fuentes","first_name":"L."},{"full_name":"Patrick, A. L.","last_name":"Patrick","first_name":"A. L."},{"full_name":"Sobral, D.","first_name":"D.","last_name":"Sobral"},{"first_name":"A. M.","last_name":"Swinbank","full_name":"Swinbank, A. M."}],"ddc":["520"]},{"fulldoi":"https://doi.org/10.5194/mr-6-243-2025","scopus_import":"1","publisher":"Copernicus Publications","PlanS_conform":"1","publication":"Magnetic Resonance","_id":"20664","publication_identifier":{"eissn":["2699-0016"]},"project":[{"_id":"B67AFEDC-15C9-11EA-A837-991A96BB2854","name":"IST Austria Open Access Fund"}],"OA_place":"publisher","oa":1,"has_accepted_license":"1","article_processing_charge":"Yes","department":[{"_id":"JoFi"},{"_id":"GaTk"},{"_id":"JoCs"},{"_id":"EvBe"},{"_id":"TaHa"},{"_id":"GradSch"},{"_id":"GeKa"},{"_id":"PaSc"}],"volume":6,"citation":{"apa":"Kapoor, L., Ruzickova, N., Zivadinovic, P., Leitner, V., Sisak, M. A., Mweka, C. N., … Schanda, P. (2025). Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. Copernicus Publications. https://doi.org/10.5194/mr-6-243-2025","mla":"Kapoor, Lucky, et al. “Quantifying the Carbon Footprint of Conference Travel: The Case of NMR Meetings.” Magnetic Resonance, vol. 6, no. 2, Copernicus Publications, 2025, pp. 243–56, doi:10.5194/mr-6-243-2025.","ista":"Kapoor L, Ruzickova N, Zivadinovic P, Leitner V, Sisak MA, Mweka CN, Dobbelaere JA, Katsaros G, Schanda P. 2025. Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. 6(2), 243–256.","short":"L. Kapoor, N. Ruzickova, P. Zivadinovic, V. Leitner, M.A. Sisak, C.N. Mweka, J.A. Dobbelaere, G. Katsaros, P. Schanda, Magnetic Resonance 6 (2025) 243–256.","ieee":"L. Kapoor et al., “Quantifying the carbon footprint of conference travel: The case of NMR meetings,” Magnetic Resonance, vol. 6, no. 2. Copernicus Publications, pp. 243–256, 2025.","chicago":"Kapoor, Lucky, Natalia Ruzickova, Predrag Zivadinovic, Valentin Leitner, Maria A Sisak, Cecelia N Mweka, Jeroen A Dobbelaere, Georgios Katsaros, and Paul Schanda. “Quantifying the Carbon Footprint of Conference Travel: The Case of NMR Meetings.” Magnetic Resonance. Copernicus Publications, 2025. https://doi.org/10.5194/mr-6-243-2025.","ama":"Kapoor L, Ruzickova N, Zivadinovic P, et al. Quantifying the carbon footprint of conference travel: The case of NMR meetings. Magnetic Resonance. 2025;6(2):243-256. doi:10.5194/mr-6-243-2025"},"publication_status":"published","date_published":"2025-11-10T00:00:00Z","month":"11","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_type":"original","related_material":{"record":[{"status":"public","id":"20242","relation":"research_data"}],"link":[{"url":"https://ista.ac.at/en/news/carbon-footprint-of-conference-travel/","description":"News on ISTA website","relation":"research_data"}]},"author":[{"id":"84b9700b-15b2-11ec-abd3-831089e67615","first_name":"Lucky","orcid":"0000-0001-8319-2148","last_name":"Kapoor","full_name":"Kapoor, Lucky"},{"full_name":"Ruzickova, Natalia","last_name":"Ruzickova","id":"D2761128-D73D-11E9-A1BF-BA0DE6697425","first_name":"Natalia"},{"last_name":"Zivadinovic","first_name":"Predrag","id":"68AA0E5A-AFDA-11E9-9994-141DE6697425","full_name":"Zivadinovic, Predrag"},{"full_name":"Leitner, Valentin","last_name":"Leitner","first_name":"Valentin","id":"4c665ce3-0016-11ec-bea0-e44de7a4fa3d"},{"full_name":"Sisak, Maria A","last_name":"Sisak","id":"44A03D04-AEA4-11E9-B225-EA2DE6697425","first_name":"Maria A"},{"last_name":"Mweka","id":"2a69ab4b-896a-11ed-bdf8-cb8641cf2b21","first_name":"Cecelia N","full_name":"Mweka, Cecelia N"},{"full_name":"Dobbelaere, Jeroen A","id":"c15a5412-de82-11ed-b809-8dc1aa996e40","first_name":"Jeroen A","last_name":"Dobbelaere"},{"first_name":"Georgios","id":"38DB5788-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8342-202X","last_name":"Katsaros","full_name":"Katsaros, Georgios"},{"first_name":"Paul","id":"7B541462-FAF6-11E9-A490-E8DFE5697425","orcid":"0000-0002-9350-7606","last_name":"Schanda","full_name":"Schanda, Paul"}],"ddc":["000"],"corr_author":"1","tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"date_created":"2025-11-23T23:01:39Z","acknowledgement":"First and foremost, we are grateful to the conference organizers who have provided data, either in the form of tables or by pointing us to abstract books. We thank the reviewers and the handling editor (Gottfried Otting) for the careful reading and suggestions. This project emerged from an interactive course about energy and climate, held at IST Austria by Jeroen Dobbelaere, Georgios Katsaros and Paul Schanda. We are grateful to ISTA's Graduate School for enabling this interdisciplinary course and to all participating students. We thank the following persons for discussions and/or comments about the manuscript: Helene Van Melckebeke, Mei Hong, Jeff Hoch, Gottfried Otting and Matthias Ernst. For the preparation of the manuscript, AI tools have been used, namely for finding relevant literature (ChatGPT) and for correcting the text (Writefull, within Overleaf LaTeX).","issue":"2","type":"journal_article","OA_type":"gold","status":"public","file_date_updated":"2025-11-24T08:25:19Z","doi":"10.5194/mr-6-243-2025","day":"10","date_updated":"2026-06-10T08:45:11Z","title":"Quantifying the carbon footprint of conference travel: The case of NMR meetings","APC_amount":"1260 EUR","oa_version":"Published Version","language":[{"iso":"eng"}],"intvolume":" 6","abstract":[{"lang":"eng","text":"Conference travel contributes to the climate footprint of academic research. Here, we provide a quantitative estimate of the carbon emissions associated with conference attendance by analyzing travel data from participants of 10 international conferences in the field of magnetic resonance, namely EUROMAR, ENC and ICMRBS. We find that attending a EUROMAR conference produces, on average, more than 1 t CO2 eq.. For the analyzed conferences outside Europe, the corresponding value is about 2–3 times higher, on average, with intercontinental trips amounting to up to 5 t. We compare these conference-related emissions to other activities associated with research and show that conference travel is a substantial portion of the total climate footprint of a researcher in magnetic resonance. We explore several strategies to reduce these emissions, including the impact of selecting conference venues more strategically and the possibility of decentralized conferences. Through a detailed comparison of train versus air travel – accounting for both direct and infrastructure-related emissions – we demonstrate that train travel offers considerable carbon savings. These data may provide a basis for strategic choices of future conferences in the field and for individuals deciding on their conference attendance."}],"DOAJ_listed":"1","file":[{"file_size":3081399,"relation":"main_file","file_name":"2025_MagneticResonance_Kapoor.pdf","date_updated":"2025-11-24T08:25:19Z","access_level":"open_access","date_created":"2025-11-24T08:25:19Z","file_id":"20672","success":1,"checksum":"c63dd47b0e77f9451821436bb77d27c9","creator":"dernst","content_type":"application/pdf"}],"year":"2025","page":"243-256","quality_controlled":"1"},{"abstract":[{"lang":"eng","text":"Glacier melt sustains water discharge from mountain basins during droughts, but ongoing glacier retreat threatens this fundamental capacity. Here, we assess the response of glaciers in the Southern Andes to one of the most severe, persistent, and extensive droughts on record in South America (2010-present), and to projected end-of-century megadroughts. Using glacio-hydrological numerical simulations, we show that despite a mean annual precipitation deficit of 36%, glacier runoff in 2010-2019 remained almost unaltered compared to the preceding decade (2000-2009), sustained by a 10% loss of total ice volume. However, simulations of future glacier evolution indicate that annual and summer glacier runoff could decline by up to 20 ± 11% and 48 ± 6%, respectively, during end-of-century megadroughts compared to pre-2010 levels. Our results project a weakening of the glacier’s buffering role against precipitation deficits during extreme droughts, increasing water scarcity for ecosystems and livelihoods in the mountain regions of South America."}],"article_number":"860","DOAJ_listed":"1","file":[{"file_size":2468843,"relation":"main_file","date_updated":"2025-12-01T09:10:13Z","file_name":"2025_CommEarthEnvir_Ayala.pdf","access_level":"open_access","file_id":"20720","creator":"dernst","success":1,"content_type":"application/pdf","checksum":"1b23ad585d6f305447b54c606be0c46d","date_created":"2025-12-01T09:10:13Z"}],"intvolume":" 6","language":[{"iso":"eng"}],"oa_version":"Published Version","APC_amount":"3654 EUR","day":"01","date_updated":"2026-05-20T08:02:48Z","title":"Less water from glaciers during future megadroughts in the Southern Andes","quality_controlled":"1","isi":1,"year":"2025","external_id":{"isi":["001617609200003"]},"acknowledgement":"This research was funded in whole or in part by the Austrian Science Fund (FWF), DOI: 10.55776/16891. The project MegaWat has received funding from the Austrian Science Fund (FWF), Swiss National Science Foundation (SNSF), the Centre for the Development of Industrial Technology (CDTI), Dutch Research Council (NWO), National Research Council (CNR) and the European Union’s Horizon Europe Programme under the 2022 Joint Transnational Call of the European Partnership Water4all (Grant Agreement n°101060874). Á.A. acknowledges Fondecyt Postdoc No. 3190732, the WSL programme ‘Extremes’ through the EMERGE project and together with S.M. ANID-CENTROS REGIONALES R20F0008. E.M.C. thanks ANID National Master scholarship year 2020 N°22200599 and the Swiss National Science Foundation Grant 200021_214907. P.A.M. acknowledges support from the Fondecyt project No. 11200142, and ANID/PIA project No AFB230001.","date_created":"2025-11-30T23:02:06Z","tmp":{"short":"CC BY (4.0)","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"author":[{"last_name":"Ayala","first_name":"Álvaro","full_name":"Ayala, Álvaro"},{"first_name":"Eduardo","last_name":"Muñoz-Castro","full_name":"Muñoz-Castro, Eduardo"},{"first_name":"Daniel","last_name":"Farinotti","full_name":"Farinotti, Daniel"},{"full_name":"Farías-Barahona, David","first_name":"David","last_name":"Farías-Barahona"},{"first_name":"Pablo A.","last_name":"Mendoza","full_name":"Mendoza, Pablo A."},{"first_name":"Shelley","last_name":"Macdonell","full_name":"Macdonell, Shelley"},{"full_name":"Mcphee, James","first_name":"James","last_name":"Mcphee"},{"last_name":"Vargas","first_name":"Ximena","full_name":"Vargas, Ximena"},{"full_name":"Pellicciotti, Francesca","id":"b28f055a-81ea-11ed-b70c-a9fe7f7b0e70","first_name":"Francesca","orcid":"0000-0002-5554-8087","last_name":"Pellicciotti"}],"ddc":["550"],"OA_type":"gold","file_date_updated":"2025-12-01T09:10:13Z","doi":"10.1038/s43247-025-02845-6","status":"public","type":"journal_article","citation":{"ama":"Ayala Á, Muñoz-Castro E, Farinotti D, et al. Less water from glaciers during future megadroughts in the Southern Andes. Communications Earth and Environment. 2025;6. doi:10.1038/s43247-025-02845-6","chicago":"Ayala, Álvaro, Eduardo Muñoz-Castro, Daniel Farinotti, David Farías-Barahona, Pablo A. Mendoza, Shelley Macdonell, James Mcphee, Ximena Vargas, and Francesca Pellicciotti. “Less Water from Glaciers during Future Megadroughts in the Southern Andes.” Communications Earth and Environment. Springer Nature, 2025. https://doi.org/10.1038/s43247-025-02845-6.","ieee":"Á. Ayala et al., “Less water from glaciers during future megadroughts in the Southern Andes,” Communications Earth and Environment, vol. 6. Springer Nature, 2025.","mla":"Ayala, Álvaro, et al. “Less Water from Glaciers during Future Megadroughts in the Southern Andes.” Communications Earth and Environment, vol. 6, 860, Springer Nature, 2025, doi:10.1038/s43247-025-02845-6.","apa":"Ayala, Á., Muñoz-Castro, E., Farinotti, D., Farías-Barahona, D., Mendoza, P. A., Macdonell, S., … Pellicciotti, F. (2025). Less water from glaciers during future megadroughts in the Southern Andes. Communications Earth and Environment. Springer Nature. https://doi.org/10.1038/s43247-025-02845-6","ista":"Ayala Á, Muñoz-Castro E, Farinotti D, Farías-Barahona D, Mendoza PA, Macdonell S, Mcphee J, Vargas X, Pellicciotti F. 2025. Less water from glaciers during future megadroughts in the Southern Andes. Communications Earth and Environment. 6, 860.","short":"Á. Ayala, E. Muñoz-Castro, D. Farinotti, D. Farías-Barahona, P.A. Mendoza, S. Macdonell, J. Mcphee, X. Vargas, F. Pellicciotti, Communications Earth and Environment 6 (2025)."},"volume":6,"department":[{"_id":"FrPe"}],"article_processing_charge":"Yes","article_type":"original","related_material":{"link":[{"description":"News on ISTA website","url":"https://ista.ac.at/en/news/the-future-fate-of-water-in-the-andes/","relation":"press_release"}]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"12","date_published":"2025-12-01T00:00:00Z","publication_status":"published","publication_identifier":{"eissn":["2662-4435"]},"_id":"20703","publication":"Communications Earth and Environment","PlanS_conform":"1","publisher":"Springer Nature","scopus_import":"1","fulldoi":"https://doi.org/10.1038/s43247-025-02845-6","has_accepted_license":"1","oa":1,"OA_place":"publisher","project":[{"name":"Megadroughts in the Water towers of Europe - from process understanding to strategies for","grant_number":"I06891","_id":"8e4c5b0b-16d5-11f0-9cad-9fa5f341393c"},{"_id":"3AC91DDA-15DF-11EA-824D-93A3E7B544D1","name":"FWF Open Access Fund","call_identifier":"FWF"}]},{"fulldoi":"https://doi.org/10.1140/epjqt/s40507-025-00344-3","supplementarymaterial":"no","publisher":"Springer Nature","scopus_import":"1","publication":"EPJ Quantum Technology","publication_identifier":{"eissn":["2196-0763"]},"_id":"19636","arxiv":1,"OA_place":"publisher","oa":1,"has_accepted_license":"1","das_tickbox":"1","article_processing_charge":"Yes","department":[{"_id":"OnHo"}],"volume":12,"citation":{"ama":"Abdalla A, Abe M, Abend S, et al. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. 2025;12. doi:10.1140/epjqt/s40507-025-00344-3","chicago":"Abdalla, Adam, Mahiro Abe, Sven Abend, Mouine Abidi, Monika Aidelsburger, Ashkan Alibabaei, Baptiste Allard, et al. “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop.” EPJ Quantum Technology. Springer Nature, 2025. https://doi.org/10.1140/epjqt/s40507-025-00344-3.","short":"A. Abdalla, M. Abe, S. Abend, M. Abidi, M. Aidelsburger, A. Alibabaei, B. Allard, J. Antoniadis, G. Arduini, N. Augst, P. Balamatsias, A. Balaž, H. Banks, R.L. Barcklay, M. Barone, M. Barsanti, M.G. Bason, A. Bassi, J.B. Bayle, C.F.A. Baynham, Q. Beaufils, S. Beldjoudi, A. Belić, S. Bennetts, J. Bernabeu, A. Bertoldi, C. Bigard, N.P. Bigelow, R. Bingham, D. Blas, A. Bobrick, S. Boehringer, A. Bogojević, K. Bongs, D. Bortoletto, P. Bouyer, C. Brand, O. Buchmueller, G. Buica, S. Calatroni, L. Calmels, P. Canizares, B. Canuel, A. Caramete, L.I. Caramete, M. Carlesso, J. Carlton, S.P. Carman, A. Carroll, M. Casariego, M. Chairetis, V. Charmandaris, U. Chauhan, J. Chen, M.L.M.L.M. Chiofalo, D. Ciampini, A. Cimbri, P. Cladé, J. Coleman, F.L. Constantin, C.R. Contaldi, R. Corgier, B. Dash, G.J. Davies, C. De Rham, A. De Roeck, D. Derr, S. Dey, F. Di Pumpo, G.S. Djordjevic, B. Döbrich, P. Dornan, M. Doser, G. Drougakis, J. Dunningham, A. Duspayev, S. Easo, J. Eby, M. Efremov, G. Elertas, J. Ellis, N. Entin, S. Fairhurst, M. Fanì, F. Fassi, P. Fayet, D. Felea, J. Feng, R. Flack, C. Foot, T. Freegarde, E. Fuchs, N. Gaaloul, D. Gao, S. Gardner, B.M. Garraway, C.L. Garrido Alzar, A. Gauguet, E. Giese, P. Gill, G.F. Giudice, E.P. Glasbrenner, J. Glick, P.W. Graham, E. Granados, P.F. Griffin, J. Gué, S. Guellati-Khelifa, S. Gupta, V. Gupta, L. Hackermueller, M. Haehnelt, T. Hakulinen, K. Hammerer, E.T. Hanımeli, T. Harte, S. Hartmann, L. Hawkins, A. Hees, A. Herbst, T.M. Hird, R. Hobson, J. Hogan, B. Holst, M. Holynski, O. Hosten, C.C. Hsu, W.C.W. Huang, K.M. Hughes, K. Hussain, G. Hütsi, A. Iovino, M.C. Isfan, G. Janson, P. Jeglič, P. Jetzer, Y. Jiang, G. Juzeliūnas, W. Kaenders, M. Kalliokoski, A. Kehagias, E. Kilian, C. Klempt, P. Knight, S. Koley, B. Konrad, T. Kovachy, M. Krutzik, M. Kumar, P. Kumar, H. Labiad, S.Y. Lan, A. Landragin, G. Landsberg, M. Langlois, B. Lanigan, B. Leone, C. Le Poncin-Lafitte, S. Lellouch, M. Lewicki, Y.H. Lien, L. Lombriser, E.L. Asamar, J.L. Lopez-Gonzalez, C. Lu, G.G. Luciano, N. Lundblad, C. De J. López Monjaraz, A. Lowe, M. Mackoit-Sinkevičienė, M. Maggiore, A. Majumdar, K. Makris, A. Maleknejad, A.L. Marchant, A. Mariotti, C. Markou, B. Matthews, A. Mazumdar, C. Mccabe, M. Meister, G. Mentasti, J. Menu, G. Messineo, B. Meyer-Hoppe, S. Micalizio, F. Migliaccio, P. Millington, M. Milosevic, A. Mishra, J. Mitchell, G.W. Morley, N. Mouelle, J. Müller, D. Newbold, W.T. Ni, C. Niehof, J. Noller, S. Odžak, D.K.L. Oi, A. Oikonomou, Y. Omar, C. Overstreet, V. Puthiya Veettil, J. Pahl, S. Paling, Z. Pan, G. Pappas, V. Pareek, E. Pasatembou, M. Paternostro, V.K. Pathak, E. Pelucchi, F. Pereira Dos Santos, A. Peters, A. Pichery, I. Pikovski, A. Pilaftsis, F.C. Pislan, R. Plunkett, R. Poggiani, M. Prevedelli, J. Rafelski, J. Raidal, M. Raidal, E.M. Rasel, S. Renaux-Petel, A. Richaud, P. Rivero-Antunez, T. Rodzinka, A. Roura, J. Rudolph, D. Sabulsky, M.S. Safronova, M. Sakellariadou, L. Salvi, M. Sameed, S. Sarkar, P. Schach, S.A. Schäffer, J. Schelfhout, M. Schilling, V. Schkolnik, W.P. Schleich, D. Schlippert, U. Schneider, F. Schreck, A. Schwartzman, N. Schwersenz, O. Sergijenko, H.R. Sfar, L. Shao, I. Shipsey, J. Shu, Y. Singh, C.F. Sopuerta, M. Sorba, F. Sorrentino, A.D.A.M. Spallicci, P. Stefanescu, N. Stergioulas, D. Stoerk, H. Thaivalappil Sunilkumar, J. Ströhle, Z. Tam, D. Tandon, Y. Tang, D. Tell, J. Tempere, D.J. Temples, R.P. Thampy, I.C. Tietje, G.M. Tino, J.N. Tinsley, O. Tintareanu Mircea, K. Tkalčec, A.J. Tolley, V. Tornatore, A. Torres-Orjuela, P. Treutlein, A. Trombettoni, C. Ufrecht, J. Urrutia, T. Valenzuela, L.R. Valerio, M. Van Der Grinten, V. Vaskonen, V. Vázquez-Aceves, H. Veermäe, F. Vetrano, N.V. Vitanov, W. Von Klitzing, S. Wald, T. Walker, R. Walser, J. Wang, Y. Wang, C.A. Weidner, A. Wenzlawski, M. Werner, L. Wörner, M.E. Yahia, E. Yazgan, E. Zambrini Cruzeiro, M. Zarei, M. Zhan, S. Zhang, L. Zhou, E. Zupanič, EPJ Quantum Technology 12 (2025).","apa":"Abdalla, A., Abe, M., Abend, S., Abidi, M., Aidelsburger, M., Alibabaei, A., … Zupanič, E. (2025). Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. Springer Nature. https://doi.org/10.1140/epjqt/s40507-025-00344-3","ista":"Abdalla A et al. 2025. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop. EPJ Quantum Technology. 12, 42.","mla":"Abdalla, Adam, et al. “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop.” EPJ Quantum Technology, vol. 12, 42, Springer Nature, 2025, doi:10.1140/epjqt/s40507-025-00344-3.","ieee":"A. Abdalla et al., “Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop,” EPJ Quantum Technology, vol. 12. Springer Nature, 2025."},"date_published":"2025-04-03T00:00:00Z","publication_status":"published","month":"04","user_id":"68b8ca59-c5b3-11ee-8790-cd641c68093d","article_type":"review","ddc":["530"],"author":[{"full_name":"Abdalla, Adam","first_name":"Adam","last_name":"Abdalla"},{"full_name":"Abe, Mahiro","first_name":"Mahiro","last_name":"Abe"},{"full_name":"Abend, Sven","last_name":"Abend","first_name":"Sven"},{"full_name":"Abidi, Mouine","last_name":"Abidi","first_name":"Mouine"},{"first_name":"Monika","last_name":"Aidelsburger","full_name":"Aidelsburger, Monika"},{"full_name":"Alibabaei, Ashkan","last_name":"Alibabaei","first_name":"Ashkan"},{"full_name":"Allard, Baptiste","last_name":"Allard","first_name":"Baptiste"},{"full_name":"Antoniadis, John","last_name":"Antoniadis","first_name":"John"},{"full_name":"Arduini, Gianluigi","last_name":"Arduini","first_name":"Gianluigi"},{"full_name":"Augst, Nadja","first_name":"Nadja","last_name":"Augst"},{"first_name":"Philippos","last_name":"Balamatsias","full_name":"Balamatsias, Philippos"},{"last_name":"Balaž","first_name":"Antun","full_name":"Balaž, Antun"},{"full_name":"Banks, Hannah","first_name":"Hannah","last_name":"Banks"},{"full_name":"Barcklay, Rachel L.","last_name":"Barcklay","first_name":"Rachel L."},{"first_name":"Michele","last_name":"Barone","full_name":"Barone, Michele"},{"full_name":"Barsanti, Michele","first_name":"Michele","last_name":"Barsanti"},{"full_name":"Bason, Mark G.","first_name":"Mark G.","last_name":"Bason"},{"full_name":"Bassi, Angelo","last_name":"Bassi","first_name":"Angelo"},{"full_name":"Bayle, Jean Baptiste","last_name":"Bayle","first_name":"Jean Baptiste"},{"last_name":"Baynham","first_name":"Charles F.A.","full_name":"Baynham, Charles F.A."},{"full_name":"Beaufils, Quentin","last_name":"Beaufils","first_name":"Quentin"},{"last_name":"Beldjoudi","first_name":"Sélyan","full_name":"Beldjoudi, Sélyan"},{"full_name":"Belić, Aleksandar","first_name":"Aleksandar","last_name":"Belić"},{"first_name":"Shayne","last_name":"Bennetts","full_name":"Bennetts, Shayne"},{"last_name":"Bernabeu","first_name":"Jose","full_name":"Bernabeu, Jose"},{"last_name":"Bertoldi","first_name":"Andrea","full_name":"Bertoldi, Andrea"},{"first_name":"Clara","last_name":"Bigard","full_name":"Bigard, Clara"},{"full_name":"Bigelow, N. P.","first_name":"N. P.","last_name":"Bigelow"},{"full_name":"Bingham, Robert","first_name":"Robert","last_name":"Bingham"},{"full_name":"Blas, Diego","last_name":"Blas","first_name":"Diego"},{"full_name":"Bobrick, Alexey","first_name":"Alexey","last_name":"Bobrick"},{"last_name":"Boehringer","first_name":"Samuel","full_name":"Boehringer, Samuel"},{"last_name":"Bogojević","first_name":"Aleksandar","full_name":"Bogojević, Aleksandar"},{"full_name":"Bongs, Kai","first_name":"Kai","last_name":"Bongs"},{"full_name":"Bortoletto, Daniela","last_name":"Bortoletto","first_name":"Daniela"},{"full_name":"Bouyer, Philippe","last_name":"Bouyer","first_name":"Philippe"},{"last_name":"Brand","first_name":"Christian","full_name":"Brand, Christian"},{"first_name":"Oliver","last_name":"Buchmueller","full_name":"Buchmueller, Oliver"},{"last_name":"Buica","first_name":"Gabriela","full_name":"Buica, Gabriela"},{"last_name":"Calatroni","first_name":"Sergio","full_name":"Calatroni, Sergio"},{"last_name":"Calmels","first_name":"Léo","full_name":"Calmels, Léo"},{"full_name":"Canizares, Priscilla","last_name":"Canizares","first_name":"Priscilla"},{"first_name":"Benjamin","last_name":"Canuel","full_name":"Canuel, Benjamin"},{"last_name":"Caramete","first_name":"Ana","full_name":"Caramete, Ana"},{"full_name":"Caramete, Laurentiu Ioan","first_name":"Laurentiu Ioan","last_name":"Caramete"},{"last_name":"Carlesso","first_name":"Matteo","full_name":"Carlesso, Matteo"},{"full_name":"Carlton, John","first_name":"John","last_name":"Carlton"},{"full_name":"Carman, Samuel P.","last_name":"Carman","first_name":"Samuel P."},{"full_name":"Carroll, Andrew","first_name":"Andrew","last_name":"Carroll"},{"full_name":"Casariego, Mateo","first_name":"Mateo","last_name":"Casariego"},{"full_name":"Chairetis, Minoas","last_name":"Chairetis","first_name":"Minoas"},{"full_name":"Charmandaris, Vassilis","first_name":"Vassilis","last_name":"Charmandaris"},{"last_name":"Chauhan","first_name":"Upasna","full_name":"Chauhan, Upasna"},{"first_name":"Jiajun","last_name":"Chen","full_name":"Chen, Jiajun"},{"full_name":"Chiofalo, Maria Luisa Maria Luisa Marilù","first_name":"Maria Luisa Maria Luisa Marilù","last_name":"Chiofalo"},{"full_name":"Ciampini, Donatella","last_name":"Ciampini","first_name":"Donatella"},{"full_name":"Cimbri, Alessia","last_name":"Cimbri","first_name":"Alessia"},{"full_name":"Cladé, Pierre","first_name":"Pierre","last_name":"Cladé"},{"first_name":"Jonathon","last_name":"Coleman","full_name":"Coleman, Jonathon"},{"full_name":"Constantin, Florin Lucian","last_name":"Constantin","first_name":"Florin Lucian"},{"last_name":"Contaldi","first_name":"Carlo R.","full_name":"Contaldi, Carlo R."},{"first_name":"Robin","last_name":"Corgier","full_name":"Corgier, Robin"},{"full_name":"Dash, Bineet","last_name":"Dash","first_name":"Bineet"},{"first_name":"G. J.","last_name":"Davies","full_name":"Davies, G. J."},{"last_name":"De Rham","first_name":"Claudia","full_name":"De Rham, Claudia"},{"first_name":"Albert","last_name":"De Roeck","full_name":"De Roeck, Albert"},{"last_name":"Derr","first_name":"Daniel","full_name":"Derr, Daniel"},{"full_name":"Dey, Soumyodeep","last_name":"Dey","first_name":"Soumyodeep"},{"full_name":"Di Pumpo, Fabio","last_name":"Di Pumpo","first_name":"Fabio"},{"full_name":"Djordjevic, Goran S.","last_name":"Djordjevic","first_name":"Goran S."},{"full_name":"Döbrich, Babette","last_name":"Döbrich","first_name":"Babette"},{"first_name":"Peter","last_name":"Dornan","full_name":"Dornan, Peter"},{"full_name":"Doser, Michael","first_name":"Michael","last_name":"Doser"},{"last_name":"Drougakis","first_name":"Giannis","full_name":"Drougakis, Giannis"},{"first_name":"Jacob","last_name":"Dunningham","full_name":"Dunningham, Jacob"},{"last_name":"Duspayev","first_name":"Alisher","full_name":"Duspayev, Alisher"},{"last_name":"Easo","first_name":"Sajan","full_name":"Easo, Sajan"},{"full_name":"Eby, Joshua","first_name":"Joshua","last_name":"Eby"},{"full_name":"Efremov, Maxim","last_name":"Efremov","first_name":"Maxim"},{"last_name":"Elertas","first_name":"Gedminas","full_name":"Elertas, Gedminas"},{"full_name":"Ellis, John","first_name":"John","last_name":"Ellis"},{"full_name":"Entin, Nicholas","last_name":"Entin","first_name":"Nicholas"},{"full_name":"Fairhurst, Stephen","last_name":"Fairhurst","first_name":"Stephen"},{"full_name":"Fanì, Mattia","first_name":"Mattia","last_name":"Fanì"},{"first_name":"Farida","last_name":"Fassi","full_name":"Fassi, Farida"},{"last_name":"Fayet","first_name":"Pierre","full_name":"Fayet, Pierre"},{"last_name":"Felea","first_name":"Daniel","full_name":"Felea, Daniel"},{"last_name":"Feng","first_name":"Jie","full_name":"Feng, Jie"},{"full_name":"Flack, Robert","first_name":"Robert","last_name":"Flack"},{"full_name":"Foot, Chris","first_name":"Chris","last_name":"Foot"},{"last_name":"Freegarde","first_name":"Tim","full_name":"Freegarde, Tim"},{"first_name":"Elina","last_name":"Fuchs","full_name":"Fuchs, Elina"},{"first_name":"Naceur","last_name":"Gaaloul","full_name":"Gaaloul, Naceur"},{"first_name":"Dongfeng","last_name":"Gao","full_name":"Gao, Dongfeng"},{"last_name":"Gardner","first_name":"Susan","full_name":"Gardner, Susan"},{"full_name":"Garraway, Barry M.","first_name":"Barry M.","last_name":"Garraway"},{"full_name":"Garrido Alzar, Carlos L.","first_name":"Carlos L.","last_name":"Garrido Alzar"},{"full_name":"Gauguet, Alexandre","first_name":"Alexandre","last_name":"Gauguet"},{"full_name":"Giese, Enno","last_name":"Giese","first_name":"Enno"},{"last_name":"Gill","first_name":"Patrick","full_name":"Gill, Patrick"},{"full_name":"Giudice, Gian F.","first_name":"Gian F.","last_name":"Giudice"},{"full_name":"Glasbrenner, Eric P.","first_name":"Eric P.","last_name":"Glasbrenner"},{"last_name":"Glick","first_name":"Jonah","full_name":"Glick, Jonah"},{"first_name":"Peter W.","last_name":"Graham","full_name":"Graham, Peter W."},{"first_name":"Eduardo","last_name":"Granados","full_name":"Granados, Eduardo"},{"full_name":"Griffin, Paul F.","first_name":"Paul F.","last_name":"Griffin"},{"full_name":"Gué, Jordan","first_name":"Jordan","last_name":"Gué"},{"last_name":"Guellati-Khelifa","first_name":"Saïda","full_name":"Guellati-Khelifa, Saïda"},{"full_name":"Gupta, Subhadeep","first_name":"Subhadeep","last_name":"Gupta"},{"full_name":"Gupta, Vishu","first_name":"Vishu","last_name":"Gupta"},{"first_name":"Lucia","last_name":"Hackermueller","full_name":"Hackermueller, Lucia"},{"first_name":"Martin","last_name":"Haehnelt","full_name":"Haehnelt, Martin"},{"first_name":"Timo","last_name":"Hakulinen","full_name":"Hakulinen, Timo"},{"last_name":"Hammerer","first_name":"Klemens","full_name":"Hammerer, Klemens"},{"first_name":"Ekim T.","last_name":"Hanımeli","full_name":"Hanımeli, Ekim T."},{"full_name":"Harte, Tiffany","last_name":"Harte","first_name":"Tiffany"},{"first_name":"Sabrina","last_name":"Hartmann","full_name":"Hartmann, Sabrina"},{"full_name":"Hawkins, Leonie","last_name":"Hawkins","first_name":"Leonie"},{"first_name":"Aurelien","last_name":"Hees","full_name":"Hees, Aurelien"},{"full_name":"Herbst, Alexander","first_name":"Alexander","last_name":"Herbst"},{"last_name":"Hird","first_name":"Thomas M.","full_name":"Hird, Thomas M."},{"full_name":"Hobson, Richard","last_name":"Hobson","first_name":"Richard"},{"full_name":"Hogan, Jason","last_name":"Hogan","first_name":"Jason"},{"last_name":"Holst","first_name":"Bodil","full_name":"Holst, Bodil"},{"last_name":"Holynski","first_name":"Michael","full_name":"Holynski, Michael"},{"first_name":"Onur","id":"4C02D85E-F248-11E8-B48F-1D18A9856A87","last_name":"Hosten","orcid":"0000-0002-2031-204X","full_name":"Hosten, Onur"},{"full_name":"Hsu, Chung Chuan","last_name":"Hsu","first_name":"Chung Chuan"},{"first_name":"Wayne Cheng Wei","last_name":"Huang","full_name":"Huang, Wayne Cheng Wei"},{"full_name":"Hughes, Kenneth M.","first_name":"Kenneth M.","last_name":"Hughes"},{"first_name":"Kamran","last_name":"Hussain","full_name":"Hussain, Kamran"},{"last_name":"Hütsi","first_name":"Gert","full_name":"Hütsi, Gert"},{"first_name":"Antonio","last_name":"Iovino","full_name":"Iovino, Antonio"},{"full_name":"Isfan, Maria Catalina","first_name":"Maria Catalina","last_name":"Isfan"},{"full_name":"Janson, Gregor","last_name":"Janson","first_name":"Gregor"},{"full_name":"Jeglič, Peter","first_name":"Peter","last_name":"Jeglič"},{"full_name":"Jetzer, Philippe","last_name":"Jetzer","first_name":"Philippe"},{"full_name":"Jiang, Yijun","first_name":"Yijun","last_name":"Jiang"},{"last_name":"Juzeliūnas","first_name":"Gediminas","full_name":"Juzeliūnas, Gediminas"},{"full_name":"Kaenders, Wilhelm","first_name":"Wilhelm","last_name":"Kaenders"},{"last_name":"Kalliokoski","first_name":"Matti","full_name":"Kalliokoski, Matti"},{"last_name":"Kehagias","first_name":"Alex","full_name":"Kehagias, Alex"},{"full_name":"Kilian, Eva","last_name":"Kilian","first_name":"Eva"},{"first_name":"Carsten","last_name":"Klempt","full_name":"Klempt, Carsten"},{"first_name":"Peter","last_name":"Knight","full_name":"Knight, Peter"},{"full_name":"Koley, Soumen","first_name":"Soumen","last_name":"Koley"},{"first_name":"Bernd","last_name":"Konrad","full_name":"Konrad, Bernd"},{"full_name":"Kovachy, Tim","first_name":"Tim","last_name":"Kovachy"},{"full_name":"Krutzik, Markus","last_name":"Krutzik","first_name":"Markus"},{"first_name":"Mukesh","last_name":"Kumar","full_name":"Kumar, Mukesh"},{"full_name":"Kumar, Pradeep","first_name":"Pradeep","last_name":"Kumar"},{"full_name":"Labiad, Hamza","last_name":"Labiad","first_name":"Hamza"},{"full_name":"Lan, Shau Yu","last_name":"Lan","first_name":"Shau Yu"},{"full_name":"Landragin, Arnaud","last_name":"Landragin","first_name":"Arnaud"},{"first_name":"Greg","last_name":"Landsberg","full_name":"Landsberg, Greg"},{"full_name":"Langlois, Mehdi","last_name":"Langlois","first_name":"Mehdi"},{"full_name":"Lanigan, Bryony","first_name":"Bryony","last_name":"Lanigan"},{"last_name":"Leone","first_name":"Bruno","full_name":"Leone, Bruno"},{"first_name":"Christophe","last_name":"Le Poncin-Lafitte","full_name":"Le Poncin-Lafitte, Christophe"},{"first_name":"Samuel","last_name":"Lellouch","full_name":"Lellouch, Samuel"},{"full_name":"Lewicki, Marek","last_name":"Lewicki","first_name":"Marek"},{"full_name":"Lien, Yu Hung","first_name":"Yu Hung","last_name":"Lien"},{"full_name":"Lombriser, Lucas","first_name":"Lucas","last_name":"Lombriser"},{"full_name":"Asamar, Elias Lopez","first_name":"Elias Lopez","last_name":"Asamar"},{"first_name":"J. Luis","last_name":"Lopez-Gonzalez","full_name":"Lopez-Gonzalez, J. Luis"},{"full_name":"Lu, Chen","first_name":"Chen","last_name":"Lu"},{"full_name":"Luciano, Giuseppe Gaetano","first_name":"Giuseppe Gaetano","last_name":"Luciano"},{"first_name":"Nathan","last_name":"Lundblad","full_name":"Lundblad, Nathan"},{"first_name":"Cristian","last_name":"De J. López Monjaraz","full_name":"De J. López Monjaraz, Cristian"},{"full_name":"Lowe, Adam","first_name":"Adam","last_name":"Lowe"},{"full_name":"Mackoit-Sinkevičienė, Mažena","last_name":"Mackoit-Sinkevičienė","first_name":"Mažena"},{"last_name":"Maggiore","first_name":"Michele","full_name":"Maggiore, Michele"},{"first_name":"Anirban","last_name":"Majumdar","full_name":"Majumdar, Anirban"},{"full_name":"Makris, Konstantinos","first_name":"Konstantinos","last_name":"Makris"},{"full_name":"Maleknejad, Azadeh","first_name":"Azadeh","last_name":"Maleknejad"},{"full_name":"Marchant, Anna L.","first_name":"Anna L.","last_name":"Marchant"},{"full_name":"Mariotti, Agnese","first_name":"Agnese","last_name":"Mariotti"},{"full_name":"Markou, Christos","last_name":"Markou","first_name":"Christos"},{"full_name":"Matthews, Barnaby","last_name":"Matthews","first_name":"Barnaby"},{"full_name":"Mazumdar, Anupam","last_name":"Mazumdar","first_name":"Anupam"},{"full_name":"Mccabe, Christopher","last_name":"Mccabe","first_name":"Christopher"},{"first_name":"Matthias","last_name":"Meister","full_name":"Meister, Matthias"},{"full_name":"Mentasti, Giorgio","last_name":"Mentasti","first_name":"Giorgio"},{"first_name":"Jonathan","last_name":"Menu","full_name":"Menu, Jonathan"},{"full_name":"Messineo, Giuseppe","last_name":"Messineo","first_name":"Giuseppe"},{"full_name":"Meyer-Hoppe, Bernd","first_name":"Bernd","last_name":"Meyer-Hoppe"},{"full_name":"Micalizio, Salvatore","first_name":"Salvatore","last_name":"Micalizio"},{"full_name":"Migliaccio, Federica","last_name":"Migliaccio","first_name":"Federica"},{"last_name":"Millington","first_name":"Peter","full_name":"Millington, Peter"},{"full_name":"Milosevic, Milan","last_name":"Milosevic","first_name":"Milan"},{"full_name":"Mishra, Abhay","first_name":"Abhay","last_name":"Mishra"},{"last_name":"Mitchell","first_name":"Jeremiah","full_name":"Mitchell, Jeremiah"},{"full_name":"Morley, Gavin W.","first_name":"Gavin W.","last_name":"Morley"},{"first_name":"Noam","last_name":"Mouelle","full_name":"Mouelle, Noam"},{"full_name":"Müller, Jürgen","last_name":"Müller","first_name":"Jürgen"},{"last_name":"Newbold","first_name":"David","full_name":"Newbold, David"},{"first_name":"Wei Tou","last_name":"Ni","full_name":"Ni, Wei Tou"},{"full_name":"Niehof, Christian","first_name":"Christian","last_name":"Niehof"},{"last_name":"Noller","first_name":"Johannes","full_name":"Noller, Johannes"},{"full_name":"Odžak, Senad","last_name":"Odžak","first_name":"Senad"},{"last_name":"Oi","first_name":"Daniel K.L.","full_name":"Oi, Daniel K.L."},{"last_name":"Oikonomou","first_name":"Andreas","full_name":"Oikonomou, Andreas"},{"last_name":"Omar","first_name":"Yasser","full_name":"Omar, Yasser"},{"last_name":"Overstreet","first_name":"Chris","full_name":"Overstreet, Chris"},{"first_name":"Vishnupriya","last_name":"Puthiya Veettil","full_name":"Puthiya Veettil, Vishnupriya"},{"first_name":"Julia","last_name":"Pahl","full_name":"Pahl, Julia"},{"full_name":"Paling, Sean","first_name":"Sean","last_name":"Paling"},{"last_name":"Pan","first_name":"Zhongyin","full_name":"Pan, Zhongyin"},{"full_name":"Pappas, George","first_name":"George","last_name":"Pappas"},{"last_name":"Pareek","first_name":"Vinay","full_name":"Pareek, Vinay"},{"full_name":"Pasatembou, Elizabeth","last_name":"Pasatembou","first_name":"Elizabeth"},{"last_name":"Paternostro","first_name":"Mauro","full_name":"Paternostro, Mauro"},{"last_name":"Pathak","first_name":"Vishal K.","full_name":"Pathak, Vishal K."},{"first_name":"Emanuele","last_name":"Pelucchi","full_name":"Pelucchi, Emanuele"},{"first_name":"Franck","last_name":"Pereira Dos Santos","full_name":"Pereira Dos Santos, Franck"},{"full_name":"Peters, Achim","last_name":"Peters","first_name":"Achim"},{"full_name":"Pichery, Annie","last_name":"Pichery","first_name":"Annie"},{"full_name":"Pikovski, Igor","last_name":"Pikovski","first_name":"Igor"},{"last_name":"Pilaftsis","first_name":"Apostolos","full_name":"Pilaftsis, Apostolos"},{"full_name":"Pislan, Florentina Crenguta","first_name":"Florentina Crenguta","last_name":"Pislan"},{"first_name":"Robert","last_name":"Plunkett","full_name":"Plunkett, Robert"},{"first_name":"Rosa","last_name":"Poggiani","full_name":"Poggiani, Rosa"},{"last_name":"Prevedelli","first_name":"Marco","full_name":"Prevedelli, Marco"},{"full_name":"Rafelski, Johann","last_name":"Rafelski","first_name":"Johann"},{"full_name":"Raidal, Juhan","first_name":"Juhan","last_name":"Raidal"},{"full_name":"Raidal, Martti","last_name":"Raidal","first_name":"Martti"},{"full_name":"Rasel, Ernst Maria","last_name":"Rasel","first_name":"Ernst Maria"},{"full_name":"Renaux-Petel, Sébastien","first_name":"Sébastien","last_name":"Renaux-Petel"},{"first_name":"Andrea","last_name":"Richaud","full_name":"Richaud, Andrea"},{"last_name":"Rivero-Antunez","first_name":"Pedro","full_name":"Rivero-Antunez, Pedro"},{"full_name":"Rodzinka, Tangui","first_name":"Tangui","last_name":"Rodzinka"},{"first_name":"Albert","last_name":"Roura","full_name":"Roura, Albert"},{"last_name":"Rudolph","first_name":"Jan","full_name":"Rudolph, Jan"},{"last_name":"Sabulsky","first_name":"Dylan","full_name":"Sabulsky, Dylan"},{"last_name":"Safronova","first_name":"Marianna S.","full_name":"Safronova, Marianna S."},{"first_name":"Mairi","last_name":"Sakellariadou","full_name":"Sakellariadou, Mairi"},{"last_name":"Salvi","first_name":"Leonardo","full_name":"Salvi, Leonardo"},{"first_name":"Muhammed","last_name":"Sameed","full_name":"Sameed, Muhammed"},{"last_name":"Sarkar","first_name":"Sumit","full_name":"Sarkar, Sumit"},{"first_name":"Patrik","last_name":"Schach","full_name":"Schach, Patrik"},{"full_name":"Schäffer, Stefan Alaric","last_name":"Schäffer","first_name":"Stefan Alaric"},{"full_name":"Schelfhout, Jesse","first_name":"Jesse","last_name":"Schelfhout"},{"full_name":"Schilling, Manuel","first_name":"Manuel","last_name":"Schilling"},{"full_name":"Schkolnik, Vladimir","first_name":"Vladimir","last_name":"Schkolnik"},{"full_name":"Schleich, Wolfgang P.","last_name":"Schleich","first_name":"Wolfgang P."},{"full_name":"Schlippert, Dennis","last_name":"Schlippert","first_name":"Dennis"},{"full_name":"Schneider, Ulrich","first_name":"Ulrich","last_name":"Schneider"},{"full_name":"Schreck, Florian","first_name":"Florian","last_name":"Schreck"},{"last_name":"Schwartzman","first_name":"Ariel","full_name":"Schwartzman, Ariel"},{"last_name":"Schwersenz","first_name":"Nico","full_name":"Schwersenz, Nico"},{"first_name":"Olga","last_name":"Sergijenko","full_name":"Sergijenko, Olga"},{"first_name":"Haifa Rejeb","last_name":"Sfar","full_name":"Sfar, Haifa Rejeb"},{"full_name":"Shao, Lijing","first_name":"Lijing","last_name":"Shao"},{"full_name":"Shipsey, Ian","first_name":"Ian","last_name":"Shipsey"},{"full_name":"Shu, Jing","last_name":"Shu","first_name":"Jing"},{"full_name":"Singh, Yeshpal","first_name":"Yeshpal","last_name":"Singh"},{"last_name":"Sopuerta","first_name":"Carlos F.","full_name":"Sopuerta, Carlos F."},{"last_name":"Sorba","first_name":"Marianna","full_name":"Sorba, Marianna"},{"full_name":"Sorrentino, Fiodor","first_name":"Fiodor","last_name":"Sorrentino"},{"last_name":"Spallicci","first_name":"Alessandro D.A.M.","full_name":"Spallicci, Alessandro D.A.M."},{"full_name":"Stefanescu, Petruta","last_name":"Stefanescu","first_name":"Petruta"},{"full_name":"Stergioulas, Nikolaos","last_name":"Stergioulas","first_name":"Nikolaos"},{"full_name":"Stoerk, Daniel","last_name":"Stoerk","first_name":"Daniel"},{"last_name":"Thaivalappil Sunilkumar","first_name":"Hrudya","full_name":"Thaivalappil Sunilkumar, Hrudya"},{"full_name":"Ströhle, Jannik","last_name":"Ströhle","first_name":"Jannik"},{"first_name":"Zoie","last_name":"Tam","full_name":"Tam, Zoie"},{"full_name":"Tandon, Dhruv","first_name":"Dhruv","last_name":"Tandon"},{"first_name":"Yijun","last_name":"Tang","full_name":"Tang, Yijun"},{"first_name":"Dorothee","last_name":"Tell","full_name":"Tell, Dorothee"},{"full_name":"Tempere, Jacques","last_name":"Tempere","first_name":"Jacques"},{"full_name":"Temples, Dylan J.","last_name":"Temples","first_name":"Dylan J."},{"full_name":"Thampy, Rohit P.","last_name":"Thampy","first_name":"Rohit P."},{"full_name":"Tietje, Ingmari C.","first_name":"Ingmari C.","last_name":"Tietje"},{"full_name":"Tino, Guglielmo M.","first_name":"Guglielmo M.","last_name":"Tino"},{"last_name":"Tinsley","first_name":"Jonathan N.","full_name":"Tinsley, Jonathan N."},{"last_name":"Tintareanu Mircea","first_name":"Ovidiu","full_name":"Tintareanu Mircea, Ovidiu"},{"first_name":"Kimberly","last_name":"Tkalčec","full_name":"Tkalčec, Kimberly"},{"full_name":"Tolley, Andrew J.","first_name":"Andrew J.","last_name":"Tolley"},{"first_name":"Vincenza","last_name":"Tornatore","full_name":"Tornatore, Vincenza"},{"first_name":"Alejandro","last_name":"Torres-Orjuela","full_name":"Torres-Orjuela, Alejandro"},{"full_name":"Treutlein, Philipp","first_name":"Philipp","last_name":"Treutlein"},{"last_name":"Trombettoni","first_name":"Andrea","full_name":"Trombettoni, Andrea"},{"full_name":"Ufrecht, Christian","last_name":"Ufrecht","first_name":"Christian"},{"last_name":"Urrutia","first_name":"Juan","full_name":"Urrutia, Juan"},{"full_name":"Valenzuela, Tristan","first_name":"Tristan","last_name":"Valenzuela"},{"full_name":"Valerio, Linda R.","first_name":"Linda R.","last_name":"Valerio"},{"full_name":"Van Der Grinten, Maurits","last_name":"Van Der Grinten","first_name":"Maurits"},{"last_name":"Vaskonen","first_name":"Ville","full_name":"Vaskonen, Ville"},{"full_name":"Vázquez-Aceves, Verónica","first_name":"Verónica","last_name":"Vázquez-Aceves"},{"full_name":"Veermäe, Hardi","first_name":"Hardi","last_name":"Veermäe"},{"last_name":"Vetrano","first_name":"Flavio","full_name":"Vetrano, Flavio"},{"first_name":"Nikolay V.","last_name":"Vitanov","full_name":"Vitanov, Nikolay V."},{"full_name":"Von Klitzing, Wolf","last_name":"Von Klitzing","first_name":"Wolf"},{"full_name":"Wald, Sebastian","first_name":"Sebastian","id":"133F200A-B015-11E9-AD41-0EDAE5697425","orcid":"0000-0002-5869-1604","last_name":"Wald"},{"full_name":"Walker, Thomas","last_name":"Walker","first_name":"Thomas"},{"full_name":"Walser, Reinhold","last_name":"Walser","first_name":"Reinhold"},{"last_name":"Wang","first_name":"Jin","full_name":"Wang, Jin"},{"last_name":"Wang","first_name":"Yan","full_name":"Wang, Yan"},{"first_name":"C. A.","last_name":"Weidner","full_name":"Weidner, C. A."},{"full_name":"Wenzlawski, André","last_name":"Wenzlawski","first_name":"André"},{"first_name":"Michael","last_name":"Werner","full_name":"Werner, Michael"},{"last_name":"Wörner","first_name":"Lisa","full_name":"Wörner, Lisa"},{"full_name":"Yahia, Mohamed E.","first_name":"Mohamed E.","last_name":"Yahia"},{"first_name":"Efe","last_name":"Yazgan","full_name":"Yazgan, Efe"},{"full_name":"Zambrini Cruzeiro, Emmanuel","last_name":"Zambrini Cruzeiro","first_name":"Emmanuel"},{"first_name":"M.","last_name":"Zarei","full_name":"Zarei, M."},{"first_name":"Mingsheng","last_name":"Zhan","full_name":"Zhan, Mingsheng"},{"full_name":"Zhang, Shengnan","last_name":"Zhang","first_name":"Shengnan"},{"full_name":"Zhou, Lin","last_name":"Zhou","first_name":"Lin"},{"last_name":"Zupanič","first_name":"Erik","full_name":"Zupanič, Erik"}],"tmp":{"short":"CC BY-NC-ND (4.0)","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode"},"dataavailabilitystatement":"No datasets were generated or analysed during the current study.","date_created":"2025-05-04T22:02:30Z","acknowledgement":"We acknowledge the support of the CERN Physics Beyond Collider activity, the CERN Quantum Technology Initiative, the Long Range Broad Agency Announcement (BAA) for the Navy and Marine Corps Science and Technology programme, Hannover Leibniz University, and the Physics Department at Imperial College London, whose contributions were instrumental in supporting the workshop that laid the foundation for this paper.\r\nThe workshop was partially funded by contributions from the Long Range Broad Agency Announcement (BAA) for the Navy and Marine Corps Science and Technology programme, Hannover Leibniz University, and the Physics Department at Imperial College London.","type":"journal_article","file_date_updated":"2025-05-05T10:52:52Z","doi":"10.1140/epjqt/s40507-025-00344-3","status":"public","OA_type":"gold","researchdata_availability":"no","date_updated":"2026-07-08T09:29:52Z","title":"Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the second workshop","day":"03","oa_version":"Published Version","language":[{"iso":"eng"}],"intvolume":" 12","file":[{"access_level":"open_access","file_name":"2025_EPJQuantumTech_Abdalla.pdf","date_updated":"2025-05-05T10:52:52Z","date_created":"2025-05-05T10:52:52Z","success":1,"creator":"dernst","content_type":"application/pdf","checksum":"00c7a97d87f7a6314df5b0c2213fbb02","file_id":"19653","file_size":14352192,"relation":"main_file"}],"DOAJ_listed":"1","article_number":"42","abstract":[{"lang":"eng","text":"This summary of the second Terrestrial Very-Long-Baseline Atom Interferometry (TVLBAI) Workshop provides a comprehensive overview of our meeting held in London in April 2024 (Second Terrestrial Very-Long-Baseline Atom Interferometry Workshop, Imperial College, April 2024), building on the initial discussions during the inaugural workshop held at CERN in March 2023 (First Terrestrial Very-Long-Baseline Atom Interferometry Workshop, CERN, March 2023). Like the summary of the first workshop (Abend et al. in AVS Quantum Sci. 6:024701, 2024), this document records a critical milestone for the international atom interferometry community. It documents our concerted efforts to evaluate progress, address emerging challenges, and refine strategic directions for future large-scale atom interferometry projects. Our commitment to collaboration is manifested by the integration of diverse expertise and the coordination of international resources, all aimed at advancing the frontiers of atom interferometry physics and technology, as set out in a Memorandum of Understanding signed by over 50 institutions (Memorandum of Understanding for the Terrestrial Very Long Baseline Atom Interferometer Study)."}],"external_id":{"isi":["001489653300001"],"arxiv":["2412.14960"]},"year":"2025","isi":1,"quality_controlled":"1"},{"abstract":[{"lang":"eng","text":"We prove matching upper and lower bounds for the average of the6-torsionof class groups of quadratic fields. Furthermore, we count the number of integer solutions on an affine quartic threefold."}],"article_number":"18","language":[{"iso":"eng"}],"oa_version":"Preprint","day":"07","date_updated":"2026-07-16T09:35:52Z","title":"6-torision and integral points on quartic threefolds","year":"2025","external_id":{"arxiv":["2403.13359"]},"main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.2403.13359"}],"date_created":"2025-04-05T10:49:27Z","corr_author":"1","author":[{"full_name":"Chan, Yik Tung","id":"c4c0afc8-9262-11ed-9231-d8b0bc743af1","first_name":"Yik Tung","last_name":"Chan","orcid":"0000-0001-8467-4106"},{"full_name":"Koymans, Peter","first_name":"Peter","last_name":"Koymans"},{"full_name":"Pagano, Carlo","first_name":"Carlo","last_name":"Pagano"},{"full_name":"Sofos, Efthymios","last_name":"Sofos","first_name":"Efthymios"}],"researchdata_availability":"no","OA_type":"green","status":"public","doi":"10.2422/2036-2145.202412_006","type":"journal_article","citation":{"ieee":"S. Chan, P. Koymans, C. Pagano, and E. Sofos, “6-torision and integral points on quartic threefolds,” Annali della Scuola Normale Superiore di Pisa, Classe di Scienze. Scuola Normale Superiore - Edizioni della Normale, 2025.","apa":"Chan, S., Koymans, P., Pagano, C., & Sofos, E. (2025). 6-torision and integral points on quartic threefolds. Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze. Scuola Normale Superiore - Edizioni della Normale. https://doi.org/10.2422/2036-2145.202412_006","mla":"Chan, Stephanie, et al. “6-Torision and Integral Points on Quartic Threefolds.” Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze, 18, Scuola Normale Superiore - Edizioni della Normale, 2025, doi:10.2422/2036-2145.202412_006.","ista":"Chan S, Koymans P, Pagano C, Sofos E. 2025. 6-torision and integral points on quartic threefolds. Annali della Scuola Normale Superiore di Pisa, Classe di Scienze., 18.","short":"S. Chan, P. Koymans, C. Pagano, E. Sofos, Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze (2025).","ama":"Chan S, Koymans P, Pagano C, Sofos E. 6-torision and integral points on quartic threefolds. Annali della Scuola Normale Superiore di Pisa, Classe di Scienze. 2025. doi:10.2422/2036-2145.202412_006","chicago":"Chan, Stephanie, Peter Koymans, Carlo Pagano, and Efthymios Sofos. “6-Torision and Integral Points on Quartic Threefolds.” Annali Della Scuola Normale Superiore Di Pisa, Classe Di Scienze. Scuola Normale Superiore - Edizioni della Normale, 2025. https://doi.org/10.2422/2036-2145.202412_006."},"department":[{"_id":"TiBr"}],"article_processing_charge":"No","das_tickbox":"0","article_type":"original","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","month":"03","date_published":"2025-03-07T00:00:00Z","publication_status":"epub_ahead","publication_identifier":{"eissn":["2036-2145"],"issn":["0391-173X"]},"_id":"19483","publication":"Annali della Scuola Normale Superiore di Pisa, Classe di Scienze","publisher":"Scuola Normale Superiore - Edizioni della Normale","supplementarymaterial":"no","fulldoi":"https://doi.org/10.2422/2036-2145.202412_006","oa":1,"arxiv":1,"OA_place":"repository"}]