[{"file_date_updated":"2021-12-13T09:24:42Z","has_accepted_license":"1","status":"public","isi":1,"day":"07","publication_identifier":{"issn":["2050-7534"],"eissn":["2050-7526"]},"article_processing_charge":"No","department":[{"_id":"MaIb"}],"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","publication_status":"published","external_id":{"isi":["000688135700001"]},"intvolume":"         9","doi":"10.1039/d1tc02753k","acknowledgement":"J. D. gratefully acknowledges the China Scholarship Council (CSC No. 201606340158) for supporting his PhD studies. S. S. thanks J. Antoja-Lleonart for insightful discussions on simulating the X-ray diffraction patterns. Part of the work was sponsored by NWO Exact and Natural Sciences for the use of supercomputer facilities (Contract no. 17197 7095). Regarding S. S., R. A., R. W. A. H., J. C. H., and M. A. L., this is a publication by the FOM Focus Group “Next Generation Organic Photovoltaics”, participating in the Dutch Institute for Fundamental Energy Research (DIFFER). The ESRF is acknowledged for providing the beamtime. J. D. and G. P. are grateful to the BM26B staff for their great support during the beamtime. M. A. L., D. M. B. are grateful for the financial support of the European Research Council via a Starting Grant (HySPOD, No. 306983).","ddc":["540"],"volume":9,"scopus_import":"1","publication":"Journal of Materials Chemistry C","year":"2021","article_type":"original","date_published":"2021-12-07T00:00:00Z","issue":"45","file":[{"file_size":4979390,"creator":"cchlebak","date_created":"2021-12-13T09:24:42Z","file_name":"2021_JMaterChemC_Dong.pdf","date_updated":"2021-12-13T09:24:42Z","relation":"main_file","file_id":"10538","access_level":"open_access","success":1,"checksum":"6b73c214ce54a6894a5854b4364413d7","content_type":"application/pdf"}],"date_created":"2021-12-12T23:01:27Z","title":"Fullerene derivatives with oligoethylene-glycol side chains: An investigation on the origin of their outstanding transport properties","author":[{"first_name":"Jingjin","full_name":"Dong, Jingjin","last_name":"Dong"},{"last_name":"Sami","first_name":"Selim","full_name":"Sami, Selim"},{"orcid":"0000-0001-7597-043X","last_name":"Balazs","id":"302BADF6-85FC-11EA-9E3B-B9493DDC885E","full_name":"Balazs, Daniel","first_name":"Daniel"},{"last_name":"Alessandri","full_name":"Alessandri, Riccardo","first_name":"Riccardo"},{"last_name":"Jahani","full_name":"Jahani, Fatimeh","first_name":"Fatimeh"},{"last_name":"Qiu","first_name":"Li","full_name":"Qiu, Li"},{"last_name":"Marrink","first_name":"Siewert J.","full_name":"Marrink, Siewert J."},{"full_name":"Havenith, Remco W.A.","first_name":"Remco W.A.","last_name":"Havenith"},{"first_name":"Jan C.","full_name":"Hummelen, Jan C.","last_name":"Hummelen"},{"full_name":"Loi, Maria A.","first_name":"Maria A.","last_name":"Loi"},{"full_name":"Portale, Giuseppe","first_name":"Giuseppe","last_name":"Portale"}],"oa_version":"Published Version","publisher":"Royal Society of Chemistry","quality_controlled":"1","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"language":[{"iso":"eng"}],"date_updated":"2023-08-17T06:18:44Z","abstract":[{"lang":"eng","text":"For many years, fullerene derivatives have been the main n-type material of organic electronics and optoelectronics. Recently, fullerene derivatives functionalized with ethylene glycol (EG) side chains have been showing important properties such as enhanced dielectric constants, facile doping and enhanced self-assembly capabilities. Here, we have prepared field-effect transistors using a series of these fullerene derivatives equipped with EG side chains of different lengths. Transport data show the beneficial effect of increasing the EG side chain. In order to understand the material properties, full structural determination of these fullerene derivatives has been achieved by coupling the X-ray data with molecular dynamics (MD) simulations. The increase in transport properties is paired with the formation of extended layered structures, efficient molecular packing and an increase in the crystallite alignment. The layer-like structure is composed of conducting layers, containing of closely packed C60 balls approaching the inter-distance of 1 nm, that are separated by well-defined EG layers, where the EG chains are rather splayed with the chain direction almost perpendicular to the layer normal. Such a layered structure appears highly ordered and highly aligned with the C60 planes oriented parallel to the substrate in the thin film configuration. The order inside the thin film increases with the EG chain length, allowing the systems to achieve mobilities as high as 0.053 cm2 V−1 s−1. Our work elucidates the structure of these interesting semiconducting organic molecules and shows that the synergistic use of X-ray structural analysis and MD simulations is a powerful tool to identify the structure of thin organic films for optoelectronic applications."}],"_id":"10534","citation":{"ama":"Dong J, Sami S, Balazs D, et al. Fullerene derivatives with oligoethylene-glycol side chains: An investigation on the origin of their outstanding transport properties. <i>Journal of Materials Chemistry C</i>. 2021;9(45):16217-16225. doi:<a href=\"https://doi.org/10.1039/d1tc02753k\">10.1039/d1tc02753k</a>","ista":"Dong J, Sami S, Balazs D, Alessandri R, Jahani F, Qiu L, Marrink SJ, Havenith RWA, Hummelen JC, Loi MA, Portale G. 2021. Fullerene derivatives with oligoethylene-glycol side chains: An investigation on the origin of their outstanding transport properties. Journal of Materials Chemistry C. 9(45), 16217–16225.","chicago":"Dong, Jingjin, Selim Sami, Daniel Balazs, Riccardo Alessandri, Fatimeh Jahani, Li Qiu, Siewert J. Marrink, et al. “Fullerene Derivatives with Oligoethylene-Glycol Side Chains: An Investigation on the Origin of Their Outstanding Transport Properties.” <i>Journal of Materials Chemistry C</i>. Royal Society of Chemistry, 2021. <a href=\"https://doi.org/10.1039/d1tc02753k\">https://doi.org/10.1039/d1tc02753k</a>.","short":"J. Dong, S. Sami, D. Balazs, R. Alessandri, F. Jahani, L. Qiu, S.J. Marrink, R.W.A. Havenith, J.C. Hummelen, M.A. Loi, G. Portale, Journal of Materials Chemistry C 9 (2021) 16217–16225.","apa":"Dong, J., Sami, S., Balazs, D., Alessandri, R., Jahani, F., Qiu, L., … Portale, G. (2021). Fullerene derivatives with oligoethylene-glycol side chains: An investigation on the origin of their outstanding transport properties. <i>Journal of Materials Chemistry C</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d1tc02753k\">https://doi.org/10.1039/d1tc02753k</a>","mla":"Dong, Jingjin, et al. “Fullerene Derivatives with Oligoethylene-Glycol Side Chains: An Investigation on the Origin of Their Outstanding Transport Properties.” <i>Journal of Materials Chemistry C</i>, vol. 9, no. 45, Royal Society of Chemistry, 2021, pp. 16217–25, doi:<a href=\"https://doi.org/10.1039/d1tc02753k\">10.1039/d1tc02753k</a>.","ieee":"J. Dong <i>et al.</i>, “Fullerene derivatives with oligoethylene-glycol side chains: An investigation on the origin of their outstanding transport properties,” <i>Journal of Materials Chemistry C</i>, vol. 9, no. 45. Royal Society of Chemistry, pp. 16217–16225, 2021."},"type":"journal_article","month":"12","page":"16217-16225","oa":1},{"issue":"12","file":[{"file_size":2299486,"creator":"dernst","date_created":"2022-05-16T08:53:11Z","file_name":"2021_PLOsComBio_Bodova.pdf","date_updated":"2022-05-16T08:53:11Z","relation":"main_file","checksum":"dcd185d4f7e0acee25edf1d6537f447e","content_type":"application/pdf","access_level":"open_access","success":1,"file_id":"11383"}],"date_created":"2021-12-12T23:01:27Z","title":"Dynamic maximum entropy provides accurate approximation of structured population dynamics","author":[{"full_name":"Bod'ová, Katarína","first_name":"Katarína","orcid":"0000-0002-7214-0171","id":"2BA24EA0-F248-11E8-B48F-1D18A9856A87","last_name":"Bod'ová"},{"full_name":"Szep, Eniko","first_name":"Eniko","last_name":"Szep","id":"485BB5A4-F248-11E8-B48F-1D18A9856A87"},{"id":"4880FE40-F248-11E8-B48F-1D18A9856A87","last_name":"Barton","orcid":"0000-0002-8548-5240","first_name":"Nicholas H","full_name":"Barton, Nicholas H"}],"article_number":"e1009661","article_type":"original","date_published":"2021-12-01T00:00:00Z","volume":17,"scopus_import":"1","pmid":1,"year":"2021","publication":"PLoS Computational Biology","intvolume":"        17","doi":"10.1371/journal.pcbi.1009661","acknowledgement":"Computational resources for the study were provided by the Institute of Science and Technology, Austria.\r\nKB received funding from the Scientific Grant Agency of the Slovak Republic under the Grants Nos. 1/0755/19 and 1/0521/20.","ddc":["570"],"article_processing_charge":"No","department":[{"_id":"NiBa"},{"_id":"GaTk"}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","external_id":{"arxiv":["2102.03669"],"pmid":["34851948"]},"status":"public","has_accepted_license":"1","publication_identifier":{"eissn":["1553-7358"],"issn":["1553-734X"]},"day":"01","file_date_updated":"2022-05-16T08:53:11Z","month":"12","type":"journal_article","citation":{"apa":"Bodova, K., Szep, E., &#38; Barton, N. H. (2021). Dynamic maximum entropy provides accurate approximation of structured population dynamics. <i>PLoS Computational Biology</i>. Public Library of Science. <a href=\"https://doi.org/10.1371/journal.pcbi.1009661\">https://doi.org/10.1371/journal.pcbi.1009661</a>","short":"K. Bodova, E. Szep, N.H. Barton, PLoS Computational Biology 17 (2021).","ama":"Bodova K, Szep E, Barton NH. Dynamic maximum entropy provides accurate approximation of structured population dynamics. <i>PLoS Computational Biology</i>. 2021;17(12). doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1009661\">10.1371/journal.pcbi.1009661</a>","ista":"Bodova K, Szep E, Barton NH. 2021. Dynamic maximum entropy provides accurate approximation of structured population dynamics. PLoS Computational Biology. 17(12), e1009661.","chicago":"Bodova, Katarina, Eniko Szep, and Nicholas H Barton. “Dynamic Maximum Entropy Provides Accurate Approximation of Structured Population Dynamics.” <i>PLoS Computational Biology</i>. Public Library of Science, 2021. <a href=\"https://doi.org/10.1371/journal.pcbi.1009661\">https://doi.org/10.1371/journal.pcbi.1009661</a>.","ieee":"K. Bodova, E. Szep, and N. H. Barton, “Dynamic maximum entropy provides accurate approximation of structured population dynamics,” <i>PLoS Computational Biology</i>, vol. 17, no. 12. Public Library of Science, 2021.","mla":"Bodova, Katarina, et al. “Dynamic Maximum Entropy Provides Accurate Approximation of Structured Population Dynamics.” <i>PLoS Computational Biology</i>, vol. 17, no. 12, e1009661, Public Library of Science, 2021, doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1009661\">10.1371/journal.pcbi.1009661</a>."},"oa":1,"abstract":[{"text":"Realistic models of biological processes typically involve interacting components on multiple scales, driven by changing environment and inherent stochasticity. Such models are often analytically and numerically intractable. We revisit a dynamic maximum entropy method that combines a static maximum entropy with a quasi-stationary approximation. This allows us to reduce stochastic non-equilibrium dynamics expressed by the Fokker-Planck equation to a simpler low-dimensional deterministic dynamics, without the need to track microscopic details. Although the method has been previously applied to a few (rather complicated) applications in population genetics, our main goal here is to explain and to better understand how the method works. We demonstrate the usefulness of the method for two widely studied stochastic problems, highlighting its accuracy in capturing important macroscopic quantities even in rapidly changing non-stationary conditions. For the Ornstein-Uhlenbeck process, the method recovers the exact dynamics whilst for a stochastic island model with migration from other habitats, the approximation retains high macroscopic accuracy under a wide range of scenarios in a dynamic environment.","lang":"eng"}],"_id":"10535","arxiv":1,"acknowledged_ssus":[{"_id":"ScienComp"}],"tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"language":[{"iso":"eng"}],"date_updated":"2024-10-09T21:01:16Z","oa_version":"Published Version","corr_author":"1","publisher":"Public Library of Science","quality_controlled":"1"},{"author":[{"full_name":"Stefanescu, Cristina","first_name":"Cristina","last_name":"Stefanescu"},{"first_name":"Merel","full_name":"Van Gogh, Merel","last_name":"Van Gogh"},{"full_name":"Roblek, Marko","first_name":"Marko","orcid":"0000-0001-9588-1389","id":"3047D808-F248-11E8-B48F-1D18A9856A87","last_name":"Roblek"},{"last_name":"Heikenwalder","first_name":"Mathias","full_name":"Heikenwalder, Mathias"},{"last_name":"Borsig","full_name":"Borsig, Lubor","first_name":"Lubor"}],"title":"TGFβ signaling in myeloid cells promotes lung and liver metastasis through different mechanisms","date_created":"2021-12-12T23:01:27Z","article_number":"765151","file":[{"file_name":"2021_Frontiers_Stefanescu.pdf","relation":"main_file","date_updated":"2021-12-13T13:32:37Z","file_id":"10539","access_level":"open_access","success":1,"checksum":"56cbac80e6891ce750511a30161b7792","content_type":"application/pdf","file_size":9245199,"creator":"alisjak","date_created":"2021-12-13T13:32:37Z"}],"date_published":"2021-11-18T00:00:00Z","article_type":"original","year":"2021","publication":"Frontiers in Oncology","pmid":1,"scopus_import":"1","volume":11,"ddc":["610"],"doi":"10.3389/fonc.2021.765151","acknowledgement":"The authors acknowledge the assistance of the Laboratory Animal Services Center (LASC) – UZH, Center for Microscopy and Image Analysis, and the Flow Cytometry Center of the University of Zurich.","intvolume":"        11","external_id":{"isi":["000726603400001"],"pmid":["34868988"]},"publication_status":"published","department":[{"_id":"DaSi"}],"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","article_processing_charge":"No","day":"18","publication_identifier":{"eissn":["2234-943X"]},"status":"public","has_accepted_license":"1","isi":1,"file_date_updated":"2021-12-13T13:32:37Z","oa":1,"type":"journal_article","citation":{"ieee":"C. Stefanescu, M. Van Gogh, M. Roblek, M. Heikenwalder, and L. Borsig, “TGFβ signaling in myeloid cells promotes lung and liver metastasis through different mechanisms,” <i>Frontiers in Oncology</i>, vol. 11. Frontiers, 2021.","mla":"Stefanescu, Cristina, et al. “TGFβ Signaling in Myeloid Cells Promotes Lung and Liver Metastasis through Different Mechanisms.” <i>Frontiers in Oncology</i>, vol. 11, 765151, Frontiers, 2021, doi:<a href=\"https://doi.org/10.3389/fonc.2021.765151\">10.3389/fonc.2021.765151</a>.","apa":"Stefanescu, C., Van Gogh, M., Roblek, M., Heikenwalder, M., &#38; Borsig, L. (2021). TGFβ signaling in myeloid cells promotes lung and liver metastasis through different mechanisms. <i>Frontiers in Oncology</i>. Frontiers. <a href=\"https://doi.org/10.3389/fonc.2021.765151\">https://doi.org/10.3389/fonc.2021.765151</a>","short":"C. Stefanescu, M. Van Gogh, M. Roblek, M. Heikenwalder, L. Borsig, Frontiers in Oncology 11 (2021).","ista":"Stefanescu C, Van Gogh M, Roblek M, Heikenwalder M, Borsig L. 2021. TGFβ signaling in myeloid cells promotes lung and liver metastasis through different mechanisms. Frontiers in Oncology. 11, 765151.","chicago":"Stefanescu, Cristina, Merel Van Gogh, Marko Roblek, Mathias Heikenwalder, and Lubor Borsig. “TGFβ Signaling in Myeloid Cells Promotes Lung and Liver Metastasis through Different Mechanisms.” <i>Frontiers in Oncology</i>. Frontiers, 2021. <a href=\"https://doi.org/10.3389/fonc.2021.765151\">https://doi.org/10.3389/fonc.2021.765151</a>.","ama":"Stefanescu C, Van Gogh M, Roblek M, Heikenwalder M, Borsig L. TGFβ signaling in myeloid cells promotes lung and liver metastasis through different mechanisms. <i>Frontiers in Oncology</i>. 2021;11. doi:<a href=\"https://doi.org/10.3389/fonc.2021.765151\">10.3389/fonc.2021.765151</a>"},"month":"11","_id":"10536","abstract":[{"lang":"eng","text":"TGFβ overexpression is commonly detected in cancer patients and correlates with poor prognosis and metastasis. Cancer progression is often associated with an enhanced recruitment of myeloid-derived cells to the tumor microenvironment. Here we show that functional TGFβ-signaling in myeloid cells is required for metastasis to the lungs and the liver. Myeloid-specific deletion of Tgfbr2 resulted in reduced spontaneous lung metastasis, which was associated with a reduction of proinflammatory cytokines in the metastatic microenvironment. Notably, CD8+ T cell depletion in myeloid-specific Tgfbr2-deficient mice rescued lung metastasis. Myeloid-specific Tgfbr2-deficiency resulted in reduced liver metastasis with an almost complete absence of myeloid cells within metastatic foci. On contrary, an accumulation of Tgfβ-responsive myeloid cells was associated with an increased recruitment of monocytes and granulocytes and higher proinflammatory cytokine levels in control mice. Monocytic cells isolated from metastatic livers of Tgfbr2-deficient mice showed increased polarization towards the M1 phenotype, Tnfα and Il-1β expression, reduced levels of M2 markers and reduced production of chemokines responsible for myeloid-cell recruitment. No significant differences in Tgfβ levels were observed at metastatic sites of any model. These data demonstrate that Tgfβ signaling in monocytic myeloid cells suppresses CD8+ T cell activity during lung metastasis, while these cells actively contribute to tumor growth during liver metastasis. Thus, myeloid cells modulate metastasis through different mechanisms in a tissue-specific manner."}],"date_updated":"2023-08-17T06:20:32Z","language":[{"iso":"eng"}],"tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"quality_controlled":"1","publisher":"Frontiers","oa_version":"Published Version"},{"acknowledgement":"Open access funding provided by Institute of Science and Technology (IST Austria). SN acknowledges partial support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – project number 405009441.","doi":"10.1007/s00205-021-01686-9","ddc":["530"],"intvolume":"       242","scopus_import":"1","year":"2021","publication":"Archive for Rational Mechanics and Analysis","volume":242,"date_published":"2021-06-30T00:00:00Z","article_type":"original","title":"Optimal homogenization rates in stochastic homogenization of nonlinear uniformly elliptic equations and systems","date_created":"2021-12-16T12:12:33Z","author":[{"first_name":"Julian L","full_name":"Fischer, Julian L","last_name":"Fischer","id":"2C12A0B0-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-0479-558X"},{"first_name":"Stefan","full_name":"Neukamm, Stefan","last_name":"Neukamm"}],"issue":"1","file":[{"file_size":1640121,"creator":"cchlebak","date_created":"2021-12-16T14:58:08Z","file_name":"2021_ArchRatMechAnalysis_Fischer.pdf","relation":"main_file","date_updated":"2021-12-16T14:58:08Z","content_type":"application/pdf","checksum":"cc830b739aed83ca2e32c4e0ce266a4c","access_level":"open_access","file_id":"10558","success":1}],"file_date_updated":"2021-12-16T14:58:08Z","day":"30","publication_identifier":{"issn":["0003-9527"],"eissn":["1432-0673"]},"isi":1,"status":"public","has_accepted_license":"1","publication_status":"published","external_id":{"arxiv":["1908.02273"],"isi":["000668431200001"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","article_processing_charge":"Yes (via OA deal)","department":[{"_id":"JuFi"}],"arxiv":1,"keyword":["Mechanical Engineering","Mathematics (miscellaneous)","Analysis"],"_id":"10549","abstract":[{"lang":"eng","text":"We derive optimal-order homogenization rates for random nonlinear elliptic PDEs with monotone nonlinearity in the uniformly elliptic case. More precisely, for a random monotone operator on \\mathbb {R}^d with stationary law (that is spatially homogeneous statistics) and fast decay of correlations on scales larger than the microscale \\varepsilon >0, we establish homogenization error estimates of the order \\varepsilon in case d\\geqq 3, and of the order \\varepsilon |\\log \\varepsilon |^{1/2} in case d=2. Previous results in nonlinear stochastic homogenization have been limited to a small algebraic rate of convergence \\varepsilon ^\\delta . We also establish error estimates for the approximation of the homogenized operator by the method of representative volumes of the order (L/\\varepsilon )^{-d/2} for a representative volume of size L. Our results also hold in the case of systems for which a (small-scale) C^{1,\\alpha } regularity theory is available."}],"page":"343-452","oa":1,"citation":{"ieee":"J. L. Fischer and S. Neukamm, “Optimal homogenization rates in stochastic homogenization of nonlinear uniformly elliptic equations and systems,” <i>Archive for Rational Mechanics and Analysis</i>, vol. 242, no. 1. Springer Nature, pp. 343–452, 2021.","mla":"Fischer, Julian L., and Stefan Neukamm. “Optimal Homogenization Rates in Stochastic Homogenization of Nonlinear Uniformly Elliptic Equations and Systems.” <i>Archive for Rational Mechanics and Analysis</i>, vol. 242, no. 1, Springer Nature, 2021, pp. 343–452, doi:<a href=\"https://doi.org/10.1007/s00205-021-01686-9\">10.1007/s00205-021-01686-9</a>.","ama":"Fischer JL, Neukamm S. Optimal homogenization rates in stochastic homogenization of nonlinear uniformly elliptic equations and systems. <i>Archive for Rational Mechanics and Analysis</i>. 2021;242(1):343-452. doi:<a href=\"https://doi.org/10.1007/s00205-021-01686-9\">10.1007/s00205-021-01686-9</a>","ista":"Fischer JL, Neukamm S. 2021. Optimal homogenization rates in stochastic homogenization of nonlinear uniformly elliptic equations and systems. Archive for Rational Mechanics and Analysis. 242(1), 343–452.","chicago":"Fischer, Julian L, and Stefan Neukamm. “Optimal Homogenization Rates in Stochastic Homogenization of Nonlinear Uniformly Elliptic Equations and Systems.” <i>Archive for Rational Mechanics and Analysis</i>. Springer Nature, 2021. <a href=\"https://doi.org/10.1007/s00205-021-01686-9\">https://doi.org/10.1007/s00205-021-01686-9</a>.","short":"J.L. Fischer, S. Neukamm, Archive for Rational Mechanics and Analysis 242 (2021) 343–452.","apa":"Fischer, J. L., &#38; Neukamm, S. (2021). Optimal homogenization rates in stochastic homogenization of nonlinear uniformly elliptic equations and systems. <i>Archive for Rational Mechanics and Analysis</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00205-021-01686-9\">https://doi.org/10.1007/s00205-021-01686-9</a>"},"month":"06","type":"journal_article","publisher":"Springer Nature","quality_controlled":"1","oa_version":"Published Version","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"date_updated":"2023-08-17T06:23:21Z","language":[{"iso":"eng"}]},{"month":"07","citation":{"ieee":"S. Dengler, P. K. Mandal, L. Allmendinger, C. Douat, and I. Huc, “Conformational interplay in hybrid peptide–helical aromatic foldamer macrocycles,” <i>Chemical Science</i>, vol. 12, no. 33. Royal Society of Chemistry, pp. 11004–11012, 2021.","mla":"Dengler, Sebastian, et al. “Conformational Interplay in Hybrid Peptide–Helical Aromatic Foldamer Macrocycles.” <i>Chemical Science</i>, vol. 12, no. 33, Royal Society of Chemistry, 2021, pp. 11004–12, doi:<a href=\"https://doi.org/10.1039/d1sc03640h\">10.1039/d1sc03640h</a>.","chicago":"Dengler, Sebastian, Pradeep K Mandal, Lars Allmendinger, Céline Douat, and Ivan Huc. “Conformational Interplay in Hybrid Peptide–Helical Aromatic Foldamer Macrocycles.” <i>Chemical Science</i>. Royal Society of Chemistry, 2021. <a href=\"https://doi.org/10.1039/d1sc03640h\">https://doi.org/10.1039/d1sc03640h</a>.","ista":"Dengler S, Mandal PK, Allmendinger L, Douat C, Huc I. 2021. Conformational interplay in hybrid peptide–helical aromatic foldamer macrocycles. Chemical Science. 12(33), 11004–11012.","ama":"Dengler S, Mandal PK, Allmendinger L, Douat C, Huc I. Conformational interplay in hybrid peptide–helical aromatic foldamer macrocycles. <i>Chemical Science</i>. 2021;12(33):11004-11012. doi:<a href=\"https://doi.org/10.1039/d1sc03640h\">10.1039/d1sc03640h</a>","apa":"Dengler, S., Mandal, P. K., Allmendinger, L., Douat, C., &#38; Huc, I. (2021). Conformational interplay in hybrid peptide–helical aromatic foldamer macrocycles. <i>Chemical Science</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d1sc03640h\">https://doi.org/10.1039/d1sc03640h</a>","short":"S. Dengler, P.K. Mandal, L. Allmendinger, C. Douat, I. Huc, Chemical Science 12 (2021) 11004–11012."},"type":"journal_article","page":"11004-11012","oa":1,"abstract":[{"text":"Macrocyclic peptides are an important class of bioactive substances. When inserting an aromatic foldamer segment in a macrocyclic peptide, the strong folding propensity of the former may influence the conformation and alter the properties of the latter. Such an insertion is relevant because some foldamer–peptide hybrids have recently been shown to be tolerated by the ribosome, prior to forming macrocycles, and can thus be produced using an in vitro translation system. We have investigated the interplay of peptide and foldamer conformations in such hybrid macrocycles. We show that foldamer helical folding always prevails and stands as a viable means to stretch, i.e. unfold, peptides in a solvent dependent manner. Conversely, the peptide systematically has a reciprocal influence and gives rise to strong foldamer helix handedness bias as well as foldamer helix stabilisation. The hybrid macrocycles also show resistance towards proteolytic degradation.","lang":"eng"}],"_id":"21081","OA_place":"publisher","tmp":{"short":"CC BY-NC (3.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc/3.0/legalcode","name":"Creative Commons Attribution-NonCommercial 3.0 Unported (CC BY-NC 3.0)","image":"/images/cc_by_nc.png"},"language":[{"iso":"eng"}],"date_updated":"2026-02-20T06:57:41Z","oa_version":"Published Version","publisher":"Royal Society of Chemistry","quality_controlled":"1","issue":"33","title":"Conformational interplay in hybrid peptide–helical aromatic foldamer macrocycles","date_created":"2026-01-29T15:15:12Z","author":[{"last_name":"Dengler","first_name":"Sebastian","full_name":"Dengler, Sebastian"},{"full_name":"Mandal, Pradeep K","first_name":"Pradeep K","orcid":"0000-0001-5996-956X","id":"6a3def15-d4b4-11ef-9fa9-a24c1f545ec3","last_name":"Mandal"},{"first_name":"Lars","full_name":"Allmendinger, Lars","last_name":"Allmendinger"},{"last_name":"Douat","first_name":"Céline","full_name":"Douat, Céline"},{"full_name":"Huc, Ivan","first_name":"Ivan","last_name":"Huc"}],"article_type":"original","date_published":"2021-07-27T00:00:00Z","volume":12,"publication":"Chemical Science","year":"2021","intvolume":"        12","doi":"10.1039/d1sc03640h","ddc":["540"],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"Yes","publication_status":"published","extern":"1","main_file_link":[{"url":"https://doi.org/10.1039/D1SC03640H","open_access":"1"}],"status":"public","has_accepted_license":"1","day":"27","publication_identifier":{"eissn":["2041-6539"],"issn":["2041-6520"]},"OA_type":"gold"},{"date_updated":"2026-02-20T07:01:01Z","language":[{"iso":"eng"}],"oa_version":"None","publisher":"Royal Society of Chemistry","quality_controlled":"1","citation":{"ieee":"D. Bindl, E. Heinemann, P. K. Mandal, and I. Huc, “Quantitative helix handedness bias through a single H vs. CH3 stereochemical differentiation,” <i>Chemical Communications</i>, vol. 57, no. 46. Royal Society of Chemistry, pp. 5662–5665, 2021.","mla":"Bindl, Daniel, et al. “Quantitative Helix Handedness Bias through a Single H vs. CH3 Stereochemical Differentiation.” <i>Chemical Communications</i>, vol. 57, no. 46, Royal Society of Chemistry, 2021, pp. 5662–65, doi:<a href=\"https://doi.org/10.1039/d1cc01452h\">10.1039/d1cc01452h</a>.","short":"D. Bindl, E. Heinemann, P.K. Mandal, I. Huc, Chemical Communications 57 (2021) 5662–5665.","apa":"Bindl, D., Heinemann, E., Mandal, P. K., &#38; Huc, I. (2021). Quantitative helix handedness bias through a single H vs. CH3 stereochemical differentiation. <i>Chemical Communications</i>. Royal Society of Chemistry. <a href=\"https://doi.org/10.1039/d1cc01452h\">https://doi.org/10.1039/d1cc01452h</a>","ama":"Bindl D, Heinemann E, Mandal PK, Huc I. Quantitative helix handedness bias through a single H vs. CH3 stereochemical differentiation. <i>Chemical Communications</i>. 2021;57(46):5662-5665. doi:<a href=\"https://doi.org/10.1039/d1cc01452h\">10.1039/d1cc01452h</a>","chicago":"Bindl, Daniel, Elisabeth Heinemann, Pradeep K Mandal, and Ivan Huc. “Quantitative Helix Handedness Bias through a Single H vs. CH3 Stereochemical Differentiation.” <i>Chemical Communications</i>. Royal Society of Chemistry, 2021. <a href=\"https://doi.org/10.1039/d1cc01452h\">https://doi.org/10.1039/d1cc01452h</a>.","ista":"Bindl D, Heinemann E, Mandal PK, Huc I. 2021. Quantitative helix handedness bias through a single H vs. CH3 stereochemical differentiation. Chemical Communications. 57(46), 5662–5665."},"month":"04","type":"journal_article","page":"5662-5665","abstract":[{"lang":"eng","text":"A novel chiral aromatic δ-amino acid building block was shown to fully induce handedness in quinoline oligoamide foldamers with the possibility of further increasing the bias by combining multiples of these units in the same sequence. Through its incorporation within the helix, both N- and C-termini are still accessible for further functionalisation."}],"_id":"21082","OA_type":"closed access","article_processing_charge":"No","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","extern":"1","publication_status":"published","external_id":{"pmid":["33972976 "]},"has_accepted_license":"1","status":"public","day":"29","publication_identifier":{"issn":["1359-7345"],"eissn":["1364-548X"]},"volume":57,"pmid":1,"year":"2021","publication":"Chemical Communications","intvolume":"        57","doi":"10.1039/d1cc01452h","issue":"46","date_created":"2026-01-29T15:18:02Z","author":[{"full_name":"Bindl, Daniel","first_name":"Daniel","last_name":"Bindl"},{"full_name":"Heinemann, Elisabeth","first_name":"Elisabeth","last_name":"Heinemann"},{"full_name":"Mandal, Pradeep K","first_name":"Pradeep K","orcid":"0000-0001-5996-956X","id":"6a3def15-d4b4-11ef-9fa9-a24c1f545ec3","last_name":"Mandal"},{"last_name":"Huc","full_name":"Huc, Ivan","first_name":"Ivan"}],"title":"Quantitative helix handedness bias through a single H vs. CH3 stereochemical differentiation","article_type":"original","date_published":"2021-04-29T00:00:00Z"},{"article_type":"original","date_published":"2021-05-14T00:00:00Z","issue":"5","title":"What we can and what we cannot see with extracellular multielectrodes","date_created":"2024-06-11T14:43:37Z","author":[{"orcid":"0000-0003-4252-1608","last_name":"Chintaluri","id":"BA06AFEE-A4BA-11EA-AE5C-14673DDC885E","full_name":"Chintaluri, Chaitanya","first_name":"Chaitanya"},{"full_name":"Bejtka, Marta","first_name":"Marta","last_name":"Bejtka"},{"last_name":"Średniawa","full_name":"Średniawa, Władysław","first_name":"Władysław"},{"last_name":"Czerwiński","full_name":"Czerwiński, Michał","first_name":"Michał"},{"full_name":"Dzik, Jakub M.","first_name":"Jakub M.","last_name":"Dzik"},{"last_name":"Jędrzejewska-Szmek","first_name":"Joanna","full_name":"Jędrzejewska-Szmek, Joanna"},{"first_name":"Kacper","full_name":"Kondrakiewicz, Kacper","last_name":"Kondrakiewicz"},{"last_name":"Kublik","full_name":"Kublik, Ewa","first_name":"Ewa"},{"last_name":"Wójcik","first_name":"Daniel K.","full_name":"Wójcik, Daniel K."}],"article_number":"e1008615","intvolume":"        17","doi":"10.1371/journal.pcbi.1008615","volume":17,"publication":"PLOS Computational Biology","year":"2021","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1371/journal.pcbi.1008615"}],"status":"public","has_accepted_license":"1","publication_identifier":{"issn":["1553-7358"]},"day":"14","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","extern":"1","publication_status":"published","abstract":[{"text":"<jats:p>Extracellular recording is an accessible technique used in animals and humans to study the brain physiology and pathology. As the number of recording channels and their density grows it is natural to ask how much improvement the additional channels bring in and how we can optimally use the new capabilities for monitoring the brain. Here we show that for any given distribution of electrodes we can establish exactly what information about current sources in the brain can be recovered and what information is strictly unobservable. We demonstrate this in the general setting of previously proposed kernel Current Source Density method and illustrate it with simplified examples as well as using evoked potentials from the barrel cortex obtained with a Neuropixels probe and with compatible model data. We show that with conceptual separation of the estimation space from experimental setup one can recover sources not accessible to standard methods.</jats:p>","lang":"eng"}],"_id":"17132","citation":{"ieee":"C. Chintaluri <i>et al.</i>, “What we can and what we cannot see with extracellular multielectrodes,” <i>PLOS Computational Biology</i>, vol. 17, no. 5. Public Library of Science, 2021.","mla":"Chintaluri, Chaitanya, et al. “What We Can and What We Cannot See with Extracellular Multielectrodes.” <i>PLOS Computational Biology</i>, vol. 17, no. 5, e1008615, Public Library of Science, 2021, doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1008615\">10.1371/journal.pcbi.1008615</a>.","apa":"Chintaluri, C., Bejtka, M., Średniawa, W., Czerwiński, M., Dzik, J. M., Jędrzejewska-Szmek, J., … Wójcik, D. K. (2021). What we can and what we cannot see with extracellular multielectrodes. <i>PLOS Computational Biology</i>. Public Library of Science. <a href=\"https://doi.org/10.1371/journal.pcbi.1008615\">https://doi.org/10.1371/journal.pcbi.1008615</a>","short":"C. Chintaluri, M. Bejtka, W. Średniawa, M. Czerwiński, J.M. Dzik, J. Jędrzejewska-Szmek, K. Kondrakiewicz, E. Kublik, D.K. Wójcik, PLOS Computational Biology 17 (2021).","ista":"Chintaluri C, Bejtka M, Średniawa W, Czerwiński M, Dzik JM, Jędrzejewska-Szmek J, Kondrakiewicz K, Kublik E, Wójcik DK. 2021. What we can and what we cannot see with extracellular multielectrodes. PLOS Computational Biology. 17(5), e1008615.","chicago":"Chintaluri, Chaitanya, Marta Bejtka, Władysław Średniawa, Michał Czerwiński, Jakub M. Dzik, Joanna Jędrzejewska-Szmek, Kacper Kondrakiewicz, Ewa Kublik, and Daniel K. Wójcik. “What We Can and What We Cannot See with Extracellular Multielectrodes.” <i>PLOS Computational Biology</i>. Public Library of Science, 2021. <a href=\"https://doi.org/10.1371/journal.pcbi.1008615\">https://doi.org/10.1371/journal.pcbi.1008615</a>.","ama":"Chintaluri C, Bejtka M, Średniawa W, et al. What we can and what we cannot see with extracellular multielectrodes. <i>PLOS Computational Biology</i>. 2021;17(5). doi:<a href=\"https://doi.org/10.1371/journal.pcbi.1008615\">10.1371/journal.pcbi.1008615</a>"},"type":"journal_article","month":"05","oa":1,"oa_version":"Published Version","quality_controlled":"1","publisher":"Public Library of Science","date_updated":"2024-06-17T10:48:15Z","language":[{"iso":"eng"}]},{"date_created":"2024-08-05T06:30:27Z","title":"3D weaving with curved ribbons","page":"1-15","author":[{"first_name":"Yingying","full_name":"Ren, Yingying","last_name":"Ren","id":"93d68d10-3540-11ef-a265-f748a50dba3d"},{"last_name":"Panetta","full_name":"Panetta, Julian","first_name":"Julian"},{"last_name":"Chen","full_name":"Chen, Tian","first_name":"Tian"},{"full_name":"Isvoranu, Florin","first_name":"Florin","last_name":"Isvoranu"},{"last_name":"Poincloux","first_name":"Samuel","full_name":"Poincloux, Samuel"},{"first_name":"Christopher","full_name":"Brandt, Christopher","last_name":"Brandt"},{"first_name":"Alison","full_name":"Martin, Alison","last_name":"Martin"},{"last_name":"Pauly","first_name":"Mark","full_name":"Pauly, Mark"}],"citation":{"mla":"Ren, Yingying, et al. “3D Weaving with Curved Ribbons.” <i>ACM Transactions on Graphics</i>, vol. 40, no. 4, Association for Computing Machinery, 2021, pp. 1–15, doi:<a href=\"https://doi.org/10.1145/3450626.3459788\">10.1145/3450626.3459788</a>.","ieee":"Y. Ren <i>et al.</i>, “3D weaving with curved ribbons,” <i>ACM Transactions on Graphics</i>, vol. 40, no. 4. Association for Computing Machinery, pp. 1–15, 2021.","apa":"Ren, Y., Panetta, J., Chen, T., Isvoranu, F., Poincloux, S., Brandt, C., … Pauly, M. (2021). 3D weaving with curved ribbons. <i>ACM Transactions on Graphics</i>. Association for Computing Machinery. <a href=\"https://doi.org/10.1145/3450626.3459788\">https://doi.org/10.1145/3450626.3459788</a>","short":"Y. Ren, J. Panetta, T. Chen, F. Isvoranu, S. Poincloux, C. Brandt, A. Martin, M. Pauly, ACM Transactions on Graphics 40 (2021) 1–15.","ista":"Ren Y, Panetta J, Chen T, Isvoranu F, Poincloux S, Brandt C, Martin A, Pauly M. 2021. 3D weaving with curved ribbons. ACM Transactions on Graphics. 40(4), 1–15.","chicago":"Ren, Yingying, Julian Panetta, Tian Chen, Florin Isvoranu, Samuel Poincloux, Christopher Brandt, Alison Martin, and Mark Pauly. “3D Weaving with Curved Ribbons.” <i>ACM Transactions on Graphics</i>. Association for Computing Machinery, 2021. <a href=\"https://doi.org/10.1145/3450626.3459788\">https://doi.org/10.1145/3450626.3459788</a>.","ama":"Ren Y, Panetta J, Chen T, et al. 3D weaving with curved ribbons. <i>ACM Transactions on Graphics</i>. 2021;40(4):1-15. doi:<a href=\"https://doi.org/10.1145/3450626.3459788\">10.1145/3450626.3459788</a>"},"type":"journal_article","month":"08","issue":"4","date_published":"2021-08-01T00:00:00Z","_id":"17384","abstract":[{"lang":"eng","text":"Basket weaving is a traditional craft for creating curved surfaces as an interwoven array of thin, flexible, and initially straight ribbons. The three-dimensional shape of a woven structure emerges through a complex interplay of the elastic bending behavior of the ribbons and the contact forces at their crossings. Curvature can be injected by carefully placing topological singularities in the otherwise regular weaving pattern. However, shape control through topology is highly non-trivial and inherently discrete, which severely limits the range of attainable woven geometries. Here, we demonstrate how to construct arbitrary smooth free-form surface geometries by weaving carefully optimized curved ribbons. We present an optimization-based approach to solving the inverse design problem for such woven structures. Our algorithm computes the ribbons' planar geometry such that their interwoven assembly closely approximates a given target design surface in equilibrium. We systematically validate our approach through a series of physical prototypes to show a broad range of new woven geometries that is not achievable by existing methods. We anticipate our computational approach to significantly enhance the capabilities for the design of new woven structures. Facilitated by modern digital fabrication technology, we see potential applications in material science, bio- and mechanical engineering, art, design, and architecture."}],"article_type":"original","year":"2021","publication":"ACM Transactions on Graphics","scopus_import":"1","volume":40,"doi":"10.1145/3450626.3459788","intvolume":"        40","extern":"1","publication_status":"published","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","publication_identifier":{"issn":["0730-0301"],"eissn":["1557-7368"]},"day":"01","status":"public","date_updated":"2024-08-12T09:38:19Z","language":[{"iso":"eng"}],"quality_controlled":"1","publisher":"Association for Computing Machinery","oa_version":"None"},{"_id":"17422","abstract":[{"text":"Inspired by motion patterns of some commercially available mobile robots, we investigate the power of robots that move forward in straight lines until colliding with an environment boundary, at which point they can rotate in place and move forward again; we visualize this as the robot “bouncing” off boundaries. We define bounce rules governing how the robot should reorient after reaching a boundary, such as reorienting relative to its heading prior to collision, or relative to the normal of the boundary. We then generate plans as sequences of rules, using the bounce visibility graph generated from a polygonal environment definition, while assuming we have unavoidable non-determinism in our actuation. Our planner can be queried to determine the feasibility of tasks such as reaching goal sets and patrolling (repeatedly visiting a sequence of goals). If the task is found feasible, the planner provides a sequence of non-deterministic interaction rules, which also provide information on how precisely the robot must execute the plan to succeed. We also show how to compute stable cyclic trajectories and use these to limit uncertainty in the robot’s position. </jats:p>","lang":"eng"}],"oa":1,"page":"1196-1211","month":"09","citation":{"mla":"Nilles, Alexandra Q., et al. “A Visibility-Based Approach to Computing Non-Deterministic Bouncing Strategies.” <i>The International Journal of Robotics Research</i>, vol. 40, no. 10–11, SAGE Publications, 2021, pp. 1196–211, doi:<a href=\"https://doi.org/10.1177/0278364921992788\">10.1177/0278364921992788</a>.","ieee":"A. Q. Nilles, Y. Ren, I. Becerra, and S. M. LaValle, “A visibility-based approach to computing non-deterministic bouncing strategies,” <i>The International Journal of Robotics Research</i>, vol. 40, no. 10–11. SAGE Publications, pp. 1196–1211, 2021.","ama":"Nilles AQ, Ren Y, Becerra I, LaValle SM. A visibility-based approach to computing non-deterministic bouncing strategies. <i>The International Journal of Robotics Research</i>. 2021;40(10-11):1196-1211. doi:<a href=\"https://doi.org/10.1177/0278364921992788\">10.1177/0278364921992788</a>","ista":"Nilles AQ, Ren Y, Becerra I, LaValle SM. 2021. A visibility-based approach to computing non-deterministic bouncing strategies. The International Journal of Robotics Research. 40(10–11), 1196–1211.","chicago":"Nilles, Alexandra Q, Yingying Ren, Israel Becerra, and Steven M LaValle. “A Visibility-Based Approach to Computing Non-Deterministic Bouncing Strategies.” <i>The International Journal of Robotics Research</i>. SAGE Publications, 2021. <a href=\"https://doi.org/10.1177/0278364921992788\">https://doi.org/10.1177/0278364921992788</a>.","short":"A.Q. Nilles, Y. Ren, I. Becerra, S.M. LaValle, The International Journal of Robotics Research 40 (2021) 1196–1211.","apa":"Nilles, A. Q., Ren, Y., Becerra, I., &#38; LaValle, S. M. (2021). A visibility-based approach to computing non-deterministic bouncing strategies. <i>The International Journal of Robotics Research</i>. SAGE Publications. <a href=\"https://doi.org/10.1177/0278364921992788\">https://doi.org/10.1177/0278364921992788</a>"},"type":"journal_article","quality_controlled":"1","publisher":"SAGE Publications","oa_version":"Published Version","date_updated":"2024-08-12T10:15:14Z","language":[{"iso":"eng"}],"doi":"10.1177/0278364921992788","intvolume":"        40","year":"2021","publication":"The International Journal of Robotics Research","scopus_import":"1","volume":40,"date_published":"2021-09-01T00:00:00Z","article_type":"original","author":[{"last_name":"Nilles","full_name":"Nilles, Alexandra Q","first_name":"Alexandra Q"},{"last_name":"Ren","id":"93d68d10-3540-11ef-a265-f748a50dba3d","full_name":"Ren, Yingying","first_name":"Yingying"},{"first_name":"Israel","full_name":"Becerra, Israel","last_name":"Becerra"},{"last_name":"LaValle","first_name":"Steven M","full_name":"LaValle, Steven M"}],"title":"A visibility-based approach to computing non-deterministic bouncing strategies","date_created":"2024-08-12T10:01:27Z","issue":"10-11","publication_identifier":{"issn":["0278-3649"],"eissn":["1741-3176"]},"day":"01","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1177/0278364921992788"}],"status":"public","extern":"1","publication_status":"published","article_processing_charge":"No","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87"},{"extern":"1","publication_status":"published","article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"18","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1145/3453483.3454036"}],"status":"public","date_updated":"2024-09-10T11:54:22Z","language":[{"iso":"eng"}],"quality_controlled":"1","publisher":"Association for Computing Machinery","oa_version":"Published Version","oa":1,"date_created":"2024-09-05T08:34:50Z","page":"158-174","conference":{"location":"virtual","end_date":"2021-06-25","name":"PLDI: Conference on Programming Language Design and Implementation","start_date":"2021-06-20"},"title":"RefinedC: Automating the foundational verification of C code with refined ownership types","author":[{"full_name":"Sammler, Michael Joachim","first_name":"Michael Joachim","last_name":"Sammler","id":"510d3901-2a03-11ee-914d-d9ae9011f0a7"},{"first_name":"Rodolphe","full_name":"Lepigre, Rodolphe","last_name":"Lepigre"},{"last_name":"Krebbers","full_name":"Krebbers, Robbert","first_name":"Robbert"},{"last_name":"Memarian","full_name":"Memarian, Kayvan","first_name":"Kayvan"},{"first_name":"Derek","full_name":"Dreyer, Derek","last_name":"Dreyer"},{"first_name":"Deepak","full_name":"Garg, Deepak","last_name":"Garg"}],"citation":{"ieee":"M. J. Sammler, R. Lepigre, R. Krebbers, K. Memarian, D. Dreyer, and D. Garg, “RefinedC: Automating the foundational verification of C code with refined ownership types,” in <i>Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation</i>, virtual, 2021, pp. 158–174.","mla":"Sammler, Michael Joachim, et al. “RefinedC: Automating the Foundational Verification of C Code with Refined Ownership Types.” <i>Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation</i>, Association for Computing Machinery, 2021, pp. 158–74, doi:<a href=\"https://doi.org/10.1145/3453483.3454036\">10.1145/3453483.3454036</a>.","apa":"Sammler, M. J., Lepigre, R., Krebbers, R., Memarian, K., Dreyer, D., &#38; Garg, D. (2021). RefinedC: Automating the foundational verification of C code with refined ownership types. In <i>Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation</i> (pp. 158–174). virtual: Association for Computing Machinery. <a href=\"https://doi.org/10.1145/3453483.3454036\">https://doi.org/10.1145/3453483.3454036</a>","short":"M.J. Sammler, R. Lepigre, R. Krebbers, K. Memarian, D. Dreyer, D. Garg, in:, Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation, Association for Computing Machinery, 2021, pp. 158–174.","ista":"Sammler MJ, Lepigre R, Krebbers R, Memarian K, Dreyer D, Garg D. 2021. RefinedC: Automating the foundational verification of C code with refined ownership types. Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation. PLDI: Conference on Programming Language Design and Implementation, 158–174.","chicago":"Sammler, Michael Joachim, Rodolphe Lepigre, Robbert Krebbers, Kayvan Memarian, Derek Dreyer, and Deepak Garg. “RefinedC: Automating the Foundational Verification of C Code with Refined Ownership Types.” In <i>Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation</i>, 158–74. Association for Computing Machinery, 2021. <a href=\"https://doi.org/10.1145/3453483.3454036\">https://doi.org/10.1145/3453483.3454036</a>.","ama":"Sammler MJ, Lepigre R, Krebbers R, Memarian K, Dreyer D, Garg D. RefinedC: Automating the foundational verification of C code with refined ownership types. In: <i>Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation</i>. Association for Computing Machinery; 2021:158-174. doi:<a href=\"https://doi.org/10.1145/3453483.3454036\">10.1145/3453483.3454036</a>"},"type":"conference","month":"06","date_published":"2021-06-18T00:00:00Z","_id":"17505","abstract":[{"lang":"eng","text":"Given the central role that C continues to play in systems software, and the difficulty of writing safe and correct C code, it remains a grand challenge to develop effective formal methods for verifying C programs. In this paper, we propose a new approach to this problem: a type system we call RefinedC, which combines ownership types (for modular reasoning about shared state and concurrency) with refinement types (for encoding precise invariants on C data types and Hoare-style specifications for C functions).\r\nRefinedC is both automated (requiring minimal user intervention) and foundational (producing a proof of program correctness in Coq), while at the same time handling a range of low-level programming idioms such as pointer arithmetic. In particular, following the approach of RustBelt, the soundness of the RefinedC type system is justified semantically by interpretation into the Coq-based Iris framework for higher-order concurrent separation logic. However, the typing rules of RefinedC are also designed to be encodable in a new “separation logic programming” language we call Lithium. By restricting to a carefully chosen (yet expressive) fragment of separation logic, Lithium supports predictable, automatic, goal-directed proof search without backtracking. We demonstrate the effectiveness of RefinedC on a range of representative examples of C code."}],"year":"2021","publication":"Proceedings of the 42nd ACM SIGPLAN International Conference on Programming Language Design and Implementation","scopus_import":"1","doi":"10.1145/3453483.3454036"},{"month":"05","type":"journal_article","citation":{"ieee":"L. I. Gurvits <i>et al.</i>, “THEZA: TeraHertz exploration and zooming-in for astrophysics,” <i>Experimental Astronomy</i>, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 559–594, 2021.","mla":"Gurvits, Leonid I., et al. “THEZA: TeraHertz Exploration and Zooming-in for Astrophysics.” <i>Experimental Astronomy</i>, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 559–94, doi:<a href=\"https://doi.org/10.1007/s10686-021-09714-y\">10.1007/s10686-021-09714-y</a>.","ama":"Gurvits LI, Paragi Z, Casasola V, et al. THEZA: TeraHertz exploration and zooming-in for astrophysics. <i>Experimental Astronomy</i>. 2021;51(3):559-594. doi:<a href=\"https://doi.org/10.1007/s10686-021-09714-y\">10.1007/s10686-021-09714-y</a>","ista":"Gurvits LI, Paragi Z, Casasola V, Conway J, Davelaar J, Falcke H, Fender R, Frey S, Fromm CM, Miró CG, Garrett MA, Giroletti M, Goddi C, Gómez J-L, van der Gucht J, Guirado JC, Haiman Z, Helmich F, Humphreys E, Impellizzeri V, Kramer M, Lindqvist M, Linz H, Liuzzo E, Lobanov AP, Mizuno Y, Rezzolla L, Roelofs F, Ros E, Rygl KLJ, Savolainen T, Schuster K, Venturi T, Wiedner MC, Zensus JA. 2021. THEZA: TeraHertz exploration and zooming-in for astrophysics. Experimental Astronomy. 51(3), 559–594.","chicago":"Gurvits, Leonid I., Zsolt Paragi, Viviana Casasola, John Conway, Jordy Davelaar, Heino Falcke, Rob Fender, et al. “THEZA: TeraHertz Exploration and Zooming-in for Astrophysics.” <i>Experimental Astronomy</i>. Springer Science and Business Media LLC, 2021. <a href=\"https://doi.org/10.1007/s10686-021-09714-y\">https://doi.org/10.1007/s10686-021-09714-y</a>.","short":"L.I. Gurvits, Z. Paragi, V. Casasola, J. Conway, J. Davelaar, H. Falcke, R. Fender, S. Frey, C.M. Fromm, C.G. Miró, M.A. Garrett, M. Giroletti, C. Goddi, J.-L. Gómez, J. van der Gucht, J.C. Guirado, Z. Haiman, F. Helmich, E. Humphreys, V. Impellizzeri, M. Kramer, M. Lindqvist, H. Linz, E. Liuzzo, A.P. Lobanov, Y. Mizuno, L. Rezzolla, F. Roelofs, E. Ros, K.L.J. Rygl, T. Savolainen, K. Schuster, T. Venturi, M.C. Wiedner, J.A. Zensus, Experimental Astronomy 51 (2021) 559–594.","apa":"Gurvits, L. I., Paragi, Z., Casasola, V., Conway, J., Davelaar, J., Falcke, H., … Zensus, J. A. (2021). THEZA: TeraHertz exploration and zooming-in for astrophysics. <i>Experimental Astronomy</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1007/s10686-021-09714-y\">https://doi.org/10.1007/s10686-021-09714-y</a>"},"oa":1,"page":"559-594","abstract":[{"text":"This paper presents the ESA Voyage 2050 White Paper for a concept of TeraHertz Exploration and Zooming-in for Astrophysics (THEZA). It addresses the science case and some implementation issues of a space-borne radio interferometric system for ultra-sharp imaging of celestial radio sources at the level of angular resolution down to (sub-) microarcseconds. THEZA focuses at millimetre and sub-millimetre wavelengths (frequencies above \r\n300 GHz), but allows for science operations at longer wavelengths too. The THEZA concept science rationale is focused on the physics of spacetime in the vicinity of supermassive black holes as the leading science driver. The main aim of the concept is to facilitate a major leap by providing researchers with orders of magnitude improvements in the resolution and dynamic range in direct imaging studies of the most exotic objects in the Universe, black holes. The concept will open up a sizeable range of hitherto unreachable parameters of observational astrophysics. It unifies two major lines of development of space-borne radio astronomy of the past decades: Space VLBI (Very Long Baseline Interferometry) and mm- and sub-mm astrophysical studies with “single dish” instruments. It also builds upon the recent success of the Earth-based Event Horizon Telescope (EHT) – the first-ever direct image of a shadow of the super-massive black hole in the centre of the galaxy M87. As an amalgam of these three major areas of modern observational astrophysics, THEZA aims at facilitating a breakthrough in high-resolution high image quality studies in the millimetre and sub-millimetre domain of the electromagnetic spectrum.","lang":"eng"}],"_id":"17508","language":[{"iso":"eng"}],"date_updated":"2024-09-10T12:15:42Z","oa_version":"Published Version","quality_controlled":"1","publisher":"Springer Science and Business Media LLC","issue":"3","title":"THEZA: TeraHertz exploration and zooming-in for astrophysics","author":[{"last_name":"Gurvits","full_name":"Gurvits, Leonid I.","first_name":"Leonid I."},{"last_name":"Paragi","first_name":"Zsolt","full_name":"Paragi, Zsolt"},{"last_name":"Casasola","first_name":"Viviana","full_name":"Casasola, Viviana"},{"first_name":"John","full_name":"Conway, John","last_name":"Conway"},{"full_name":"Davelaar, Jordy","first_name":"Jordy","last_name":"Davelaar"},{"full_name":"Falcke, Heino","first_name":"Heino","last_name":"Falcke"},{"last_name":"Fender","first_name":"Rob","full_name":"Fender, Rob"},{"last_name":"Frey","full_name":"Frey, Sándor","first_name":"Sándor"},{"last_name":"Fromm","first_name":"Christian M.","full_name":"Fromm, Christian M."},{"full_name":"Miró, Cristina García","first_name":"Cristina García","last_name":"Miró"},{"last_name":"Garrett","first_name":"Michael A.","full_name":"Garrett, Michael A."},{"first_name":"Marcello","full_name":"Giroletti, Marcello","last_name":"Giroletti"},{"last_name":"Goddi","full_name":"Goddi, Ciriaco","first_name":"Ciriaco"},{"first_name":"José-Luis","full_name":"Gómez, José-Luis","last_name":"Gómez"},{"first_name":"Jeffrey","full_name":"van der Gucht, Jeffrey","last_name":"van der Gucht"},{"full_name":"Guirado, José Carlos","first_name":"José Carlos","last_name":"Guirado"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"Helmich","first_name":"Frank","full_name":"Helmich, Frank"},{"first_name":"Elizabeth","full_name":"Humphreys, Elizabeth","last_name":"Humphreys"},{"last_name":"Impellizzeri","first_name":"Violette","full_name":"Impellizzeri, Violette"},{"first_name":"Michael","full_name":"Kramer, Michael","last_name":"Kramer"},{"last_name":"Lindqvist","full_name":"Lindqvist, Michael","first_name":"Michael"},{"last_name":"Linz","first_name":"Hendrik","full_name":"Linz, Hendrik"},{"full_name":"Liuzzo, Elisabetta","first_name":"Elisabetta","last_name":"Liuzzo"},{"first_name":"Andrei P.","full_name":"Lobanov, Andrei P.","last_name":"Lobanov"},{"last_name":"Mizuno","first_name":"Yosuke","full_name":"Mizuno, Yosuke"},{"first_name":"Luciano","full_name":"Rezzolla, Luciano","last_name":"Rezzolla"},{"last_name":"Roelofs","full_name":"Roelofs, Freek","first_name":"Freek"},{"first_name":"Eduardo","full_name":"Ros, Eduardo","last_name":"Ros"},{"first_name":"Kazi L.J.","full_name":"Rygl, Kazi L.J.","last_name":"Rygl"},{"last_name":"Savolainen","first_name":"Tuomas","full_name":"Savolainen, Tuomas"},{"last_name":"Schuster","first_name":"Karl","full_name":"Schuster, Karl"},{"first_name":"Tiziana","full_name":"Venturi, Tiziana","last_name":"Venturi"},{"last_name":"Wiedner","full_name":"Wiedner, Martina C.","first_name":"Martina C."},{"full_name":"Zensus, J. Anton","first_name":"J. Anton","last_name":"Zensus"}],"date_created":"2024-09-05T08:46:17Z","article_type":"original","date_published":"2021-05-27T00:00:00Z","volume":51,"year":"2021","publication":"Experimental Astronomy","scopus_import":"1","intvolume":"        51","doi":"10.1007/s10686-021-09714-y","article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_status":"published","extern":"1","status":"public","main_file_link":[{"url":"https://doi.org/10.1007/s10686-021-09714-y","open_access":"1"}],"alternative_title":["An ESA Voyage 2050 White Paper"],"day":"27","publication_identifier":{"issn":["0922-6435","1572-9508"]}},{"publication_identifier":{"issn":["0004-637X","1538-4357"]},"day":"24","main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/abd555"}],"status":"public","extern":"1","publication_status":"published","article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","doi":"10.3847/1538-4357/abd555","intvolume":"       908","publication":"The Astrophysical Journal","year":"2021","scopus_import":"1","volume":908,"date_published":"2021-02-24T00:00:00Z","article_type":"original","author":[{"full_name":"Tagawa, Hiromichi","first_name":"Hiromichi","last_name":"Tagawa"},{"full_name":"Kocsis, Bence","first_name":"Bence","last_name":"Kocsis"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"last_name":"Bartos","full_name":"Bartos, Imre","first_name":"Imre"},{"full_name":"Omukai, Kazuyuki","first_name":"Kazuyuki","last_name":"Omukai"},{"first_name":"Johan","full_name":"Samsing, Johan","last_name":"Samsing"}],"title":"Mass-gap mergers in active galactic nuclei","date_created":"2024-09-05T08:47:46Z","article_number":"194","issue":"2","quality_controlled":"1","publisher":"American Astronomical Society","oa_version":"Published Version","date_updated":"2024-09-10T12:36:17Z","language":[{"iso":"eng"}],"_id":"17509","abstract":[{"text":"The recently discovered gravitational wave sources GW190521 and GW190814 have shown evidence of BH mergers with masses and spins outside of the range expected from isolated stellar evolution. These merging objects could have undergone previous mergers. Such hierarchical mergers are predicted to be frequent in active galactic nuclei (AGNs) disks, where binaries form and evolve efficiently by dynamical interactions and gaseous dissipation. Here we compare the properties of these observed events to the theoretical models of mergers in AGN disks, which are obtained by performing one-dimensional N-body simulations combined with semi-analytical prescriptions. The high BH masses in GW190521 are consistent with mergers of high-generation (high-g) BHs where the initial progenitor stars had high metallicity, 2g BHs if the original progenitors were metal-poor, or 1g BHs that had gained mass via super-Eddington accretion. Other measured properties related to spin parameters in GW190521 are also consistent with mergers in AGN disks. Furthermore, mergers in the lower mass gap or those with low mass ratio as found in GW190814 and GW190412 are also reproduced by mergers of 2g–1g or 1g–1g objects with significant accretion in AGN disks. Finally, due to gas accretion, the massive neutron star merger reported in GW190425 can be produced in an AGN disk.","lang":"eng"}],"oa":1,"month":"02","type":"journal_article","citation":{"apa":"Tagawa, H., Kocsis, B., Haiman, Z., Bartos, I., Omukai, K., &#38; Samsing, J. (2021). Mass-gap mergers in active galactic nuclei. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/abd555\">https://doi.org/10.3847/1538-4357/abd555</a>","short":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, J. Samsing, The Astrophysical Journal 908 (2021).","ama":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. Mass-gap mergers in active galactic nuclei. <i>The Astrophysical Journal</i>. 2021;908(2). doi:<a href=\"https://doi.org/10.3847/1538-4357/abd555\">10.3847/1538-4357/abd555</a>","chicago":"Tagawa, Hiromichi, Bence Kocsis, Zoltán Haiman, Imre Bartos, Kazuyuki Omukai, and Johan Samsing. “Mass-Gap Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/abd555\">https://doi.org/10.3847/1538-4357/abd555</a>.","ista":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. 2021. Mass-gap mergers in active galactic nuclei. The Astrophysical Journal. 908(2), 194.","ieee":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, and J. Samsing, “Mass-gap mergers in active galactic nuclei,” <i>The Astrophysical Journal</i>, vol. 908, no. 2. American Astronomical Society, 2021.","mla":"Tagawa, Hiromichi, et al. “Mass-Gap Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal</i>, vol. 908, no. 2, 194, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/abd555\">10.3847/1538-4357/abd555</a>."}},{"_id":"17515","abstract":[{"text":"The disks of active galactic nuclei (AGNs) have emerged as a rich environment for the evolution of stars and their compact remnants. The very dense medium favors rapid accretion, while torques and migration traps enhance binary formation and mergers. Both long and short gamma-ray bursts are hence expected. We show that AGN disks constitute an ideal environment for another interesting phenomenon: the accretion-induced collapse (AIC) of neutron stars (NSs) to black holes (BHs). Rapid accretion in the dense disks can cause NSs to grow to the point of exceeding the maximum mass allowed by their equation of state. General relativistic magnetohydrodynamical simulations have shown that electromagnetic signatures are expected if the NS is surrounded by a minidisk prior to collapse, which then rapidly accretes onto the BH, and/or if the NS is highly magnetized, from reconnection of the magnetosphere during collapse. Here we compute the rates of AICs and their locations within the disks for both isolated NSs and for (initially stable) NSs formed from NS-NS mergers. We find that the global AIC rates are ∼0.07–20 Gpc−3 yr−1, and we discuss their observable prospects and signatures as they emerge from the dense disk environments.","lang":"eng"}],"oa":1,"month":"06","type":"journal_article","citation":{"ieee":"R. Perna, H. Tagawa, Z. Haiman, and I. Bartos, “Accretion-induced collapse of neutron stars in the disks of active galactic nuclei,” <i>The Astrophysical Journal</i>, vol. 915, no. 1. American Astronomical Society, 2021.","mla":"Perna, Rosalba, et al. “Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei.” <i>The Astrophysical Journal</i>, vol. 915, no. 1, 10, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/1538-4357/abfdb4\">10.3847/1538-4357/abfdb4</a>.","short":"R. Perna, H. Tagawa, Z. Haiman, I. Bartos, The Astrophysical Journal 915 (2021).","apa":"Perna, R., Tagawa, H., Haiman, Z., &#38; Bartos, I. (2021). Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. <i>The Astrophysical Journal</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/1538-4357/abfdb4\">https://doi.org/10.3847/1538-4357/abfdb4</a>","ama":"Perna R, Tagawa H, Haiman Z, Bartos I. Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. <i>The Astrophysical Journal</i>. 2021;915(1). doi:<a href=\"https://doi.org/10.3847/1538-4357/abfdb4\">10.3847/1538-4357/abfdb4</a>","chicago":"Perna, Rosalba, Hiromichi Tagawa, Zoltán Haiman, and Imre Bartos. “Accretion-Induced Collapse of Neutron Stars in the Disks of Active Galactic Nuclei.” <i>The Astrophysical Journal</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/1538-4357/abfdb4\">https://doi.org/10.3847/1538-4357/abfdb4</a>.","ista":"Perna R, Tagawa H, Haiman Z, Bartos I. 2021. Accretion-induced collapse of neutron stars in the disks of active galactic nuclei. The Astrophysical Journal. 915(1), 10."},"publisher":"American Astronomical Society","quality_controlled":"1","oa_version":"Published Version","date_updated":"2024-09-10T13:47:31Z","language":[{"iso":"eng"}],"doi":"10.3847/1538-4357/abfdb4","intvolume":"       915","scopus_import":"1","publication":"The Astrophysical Journal","year":"2021","volume":915,"date_published":"2021-06-28T00:00:00Z","article_type":"original","date_created":"2024-09-05T08:55:06Z","author":[{"full_name":"Perna, Rosalba","first_name":"Rosalba","last_name":"Perna"},{"first_name":"Hiromichi","full_name":"Tagawa, Hiromichi","last_name":"Tagawa"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"full_name":"Bartos, Imre","first_name":"Imre","last_name":"Bartos"}],"article_number":"10","title":"Accretion-induced collapse of neutron stars in the disks of active galactic nuclei","issue":"1","day":"28","publication_identifier":{"issn":["0004-637X","1538-4357"]},"main_file_link":[{"open_access":"1","url":"https://doi.org/10.3847/1538-4357/abfdb4"}],"status":"public","extern":"1","publication_status":"published","article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345"},{"doi":"10.1093/mnras/stab395","intvolume":"       502","publication":"Monthly Notices of the Royal Astronomical Society","year":"2021","scopus_import":"1","volume":502,"date_published":"2021-02-11T00:00:00Z","article_type":"original","author":[{"last_name":"Osato","first_name":"Ken","full_name":"Osato, Ken"},{"last_name":"Liu","first_name":"Jia","full_name":"Liu, Jia"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán"}],"title":"κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations","date_created":"2024-09-05T08:56:14Z","issue":"4","publication_identifier":{"issn":["0035-8711","1365-2966"]},"day":"11","status":"public","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stab395","open_access":"1"}],"publication_status":"published","extern":"1","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_processing_charge":"No","_id":"17516","abstract":[{"text":"We study the effect of baryonic processes on weak lensing (WL) observables with a suite of mock WL maps, the κTNG, based on the cosmological hydrodynamic simulations IllustrisTNG. We quantify the baryonic effects on the WL angular power spectrum, one-point probability distribution function (PDF), and number counts of peaks and minima. We also show the redshift evolution of the effects, which is a key to distinguish the effect of baryons from fundamental physics such as dark energy, dark matter, and massive neutrinos. We find that baryonic processes reduce the small-scale power, suppress the tails of the PDF, peak and minimum counts, and change the total number of peaks and minima. We compare our results to existing semi-analytical models and hydrodynamic simulations, and discuss the source of discrepancies. The κTNG suite includes 10 000 realizations of $5 \\times 5 \\, \\mathrm{deg}^2$ maps for 40 source redshifts up to zs = 2.6, well covering the range of interest for existing and upcoming WL surveys. We also produce the κTNG-Dark suite of maps, generated based on the corresponding dark matter-only IllustrisTNG simulations. Our mock maps are not only suitable for developing analytical models that incorporate the effect of baryons, but also particularly useful for studies that rely on mass maps, such as non-Gaussian statistics and machine learning with convolutional neural networks. The suite of mock maps is publicly available at Columbia Lensing (http://columbialensing.org).","lang":"eng"}],"oa":1,"page":"5593-5602","type":"journal_article","citation":{"apa":"Osato, K., Liu, J., &#38; Haiman, Z. (2021). κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stab395\">https://doi.org/10.1093/mnras/stab395</a>","short":"K. Osato, J. Liu, Z. Haiman, Monthly Notices of the Royal Astronomical Society 502 (2021) 5593–5602.","ista":"Osato K, Liu J, Haiman Z. 2021. κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. Monthly Notices of the Royal Astronomical Society. 502(4), 5593–5602.","chicago":"Osato, Ken, Jia Liu, and Zoltán Haiman. “ΚTNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2021. <a href=\"https://doi.org/10.1093/mnras/stab395\">https://doi.org/10.1093/mnras/stab395</a>.","ama":"Osato K, Liu J, Haiman Z. κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations. <i>Monthly Notices of the Royal Astronomical Society</i>. 2021;502(4):5593-5602. doi:<a href=\"https://doi.org/10.1093/mnras/stab395\">10.1093/mnras/stab395</a>","ieee":"K. Osato, J. Liu, and Z. Haiman, “κTNG: effect of baryonic processes on weak lensing with IllustrisTNG simulations,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 502, no. 4. Oxford University Press, pp. 5593–5602, 2021.","mla":"Osato, Ken, et al. “ΚTNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 502, no. 4, Oxford University Press, 2021, pp. 5593–602, doi:<a href=\"https://doi.org/10.1093/mnras/stab395\">10.1093/mnras/stab395</a>."},"month":"02","quality_controlled":"1","publisher":"Oxford University Press","oa_version":"Published Version","date_updated":"2024-09-10T13:53:06Z","language":[{"iso":"eng"}]},{"date_updated":"2024-09-11T08:17:16Z","language":[{"iso":"eng"}],"quality_controlled":"1","publisher":"Springer Science and Business Media LLC","oa_version":"Published Version","oa":1,"page":"1441-1470","month":"05","type":"journal_article","citation":{"apa":"Baker, J., Baker, T., Carbone, C., Congedo, G., Contaldi, C., Dvorkin, I., … Zumalacárregui, M. (2021). High angular resolution gravitational wave astronomy. <i>Experimental Astronomy</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1007/s10686-021-09712-0\">https://doi.org/10.1007/s10686-021-09712-0</a>","short":"J. Baker, T. Baker, C. Carbone, G. Congedo, C. Contaldi, I. Dvorkin, J. Gair, Z. Haiman, D.F. Mota, A. Renzini, E.-J. Buis, G. Cusin, J.M. Ezquiaga, G. Mueller, M. Pieroni, J. Quenby, A. Ricciardone, I.D. Saltas, L. Shao, N. Tamanini, G. Tasinato, M. Zumalacárregui, Experimental Astronomy 51 (2021) 1441–1470.","ama":"Baker J, Baker T, Carbone C, et al. High angular resolution gravitational wave astronomy. <i>Experimental Astronomy</i>. 2021;51(3):1441-1470. doi:<a href=\"https://doi.org/10.1007/s10686-021-09712-0\">10.1007/s10686-021-09712-0</a>","ista":"Baker J, Baker T, Carbone C, Congedo G, Contaldi C, Dvorkin I, Gair J, Haiman Z, Mota DF, Renzini A, Buis E-J, Cusin G, Ezquiaga JM, Mueller G, Pieroni M, Quenby J, Ricciardone A, Saltas ID, Shao L, Tamanini N, Tasinato G, Zumalacárregui M. 2021. High angular resolution gravitational wave astronomy. Experimental Astronomy. 51(3), 1441–1470.","chicago":"Baker, John, Tessa Baker, Carmelita Carbone, Giuseppe Congedo, Carlo Contaldi, Irina Dvorkin, Jonathan Gair, et al. “High Angular Resolution Gravitational Wave Astronomy.” <i>Experimental Astronomy</i>. Springer Science and Business Media LLC, 2021. <a href=\"https://doi.org/10.1007/s10686-021-09712-0\">https://doi.org/10.1007/s10686-021-09712-0</a>.","mla":"Baker, John, et al. “High Angular Resolution Gravitational Wave Astronomy.” <i>Experimental Astronomy</i>, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 1441–70, doi:<a href=\"https://doi.org/10.1007/s10686-021-09712-0\">10.1007/s10686-021-09712-0</a>.","ieee":"J. Baker <i>et al.</i>, “High angular resolution gravitational wave astronomy,” <i>Experimental Astronomy</i>, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 1441–1470, 2021."},"_id":"17525","abstract":[{"text":"Since the very beginning of astronomy the location of objects on the sky has been a fundamental observational quantity that has been taken for granted. While precise two dimensional positional information is easy to obtain for observations in the electromagnetic spectrum, the positional accuracy of current and near future gravitational wave detectors is limited to between tens and hundreds of square degrees, which makes it extremely challenging to identify the host galaxies of gravitational wave events or to detect any electromagnetic counterparts. Gravitational wave observations provide information on source properties that is complementary to the information in any associated electromagnetic emission. Observing systems with multiple messengers thus has scientific potential much greater than the sum of its parts. A gravitational wave detector with higher angular resolution would significantly increase the prospects for finding the hosts of gravitational wave sources and triggering a multi-messenger follow-up campaign. An observatory with arcminute precision or better could be realised within the Voyage 2050 programme by creating a large baseline interferometer array in space and would have transformative scientific potential. Precise positional information of standard sirens would enable precision measurements of cosmological parameters and offer new insights on structure formation; a high angular resolution gravitational wave observatory would allow the detection of a stochastic background and resolution of the anisotropies within it; it would also allow the study of accretion processes around black holes; and it would have tremendous potential for tests of modified gravity and the discovery of physics beyond the Standard Model.","lang":"eng"}],"extern":"1","publication_status":"published","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_processing_charge":"No","day":"04","publication_identifier":{"issn":["0922-6435","1572-9508"]},"main_file_link":[{"url":"https://doi.org/10.1007/s10686-021-09712-0","open_access":"1"}],"status":"public","title":"High angular resolution gravitational wave astronomy","author":[{"full_name":"Baker, John","first_name":"John","last_name":"Baker"},{"first_name":"Tessa","full_name":"Baker, Tessa","last_name":"Baker"},{"first_name":"Carmelita","full_name":"Carbone, Carmelita","last_name":"Carbone"},{"full_name":"Congedo, Giuseppe","first_name":"Giuseppe","last_name":"Congedo"},{"full_name":"Contaldi, Carlo","first_name":"Carlo","last_name":"Contaldi"},{"last_name":"Dvorkin","first_name":"Irina","full_name":"Dvorkin, Irina"},{"full_name":"Gair, Jonathan","first_name":"Jonathan","last_name":"Gair"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","first_name":"Zoltán","full_name":"Haiman, Zoltán"},{"first_name":"David F.","full_name":"Mota, David F.","last_name":"Mota"},{"last_name":"Renzini","full_name":"Renzini, Arianna","first_name":"Arianna"},{"full_name":"Buis, Ernst-Jan","first_name":"Ernst-Jan","last_name":"Buis"},{"full_name":"Cusin, Giulia","first_name":"Giulia","last_name":"Cusin"},{"first_name":"Jose Maria","full_name":"Ezquiaga, Jose Maria","last_name":"Ezquiaga"},{"full_name":"Mueller, Guido","first_name":"Guido","last_name":"Mueller"},{"last_name":"Pieroni","full_name":"Pieroni, Mauro","first_name":"Mauro"},{"full_name":"Quenby, John","first_name":"John","last_name":"Quenby"},{"first_name":"Angelo","full_name":"Ricciardone, Angelo","last_name":"Ricciardone"},{"full_name":"Saltas, Ippocratis D.","first_name":"Ippocratis D.","last_name":"Saltas"},{"first_name":"Lijing","full_name":"Shao, Lijing","last_name":"Shao"},{"first_name":"Nicola","full_name":"Tamanini, Nicola","last_name":"Tamanini"},{"first_name":"Gianmassimo","full_name":"Tasinato, Gianmassimo","last_name":"Tasinato"},{"full_name":"Zumalacárregui, Miguel","first_name":"Miguel","last_name":"Zumalacárregui"}],"date_created":"2024-09-05T09:28:30Z","issue":"3","date_published":"2021-05-04T00:00:00Z","article_type":"original","year":"2021","publication":"Experimental Astronomy","scopus_import":"1","volume":51,"doi":"10.1007/s10686-021-09712-0","intvolume":"        51"},{"abstract":[{"text":"We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.","lang":"eng"}],"_id":"17534","type":"journal_article","citation":{"apa":"Sesana, A., Korsakova, N., Sedda, M. A., Baibhav, V., Barausse, E., Barke, S., … Zumalacarregui, M. (2021). Unveiling the gravitational universe at μ-Hz frequencies. <i>Experimental Astronomy</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1007/s10686-021-09709-9\">https://doi.org/10.1007/s10686-021-09709-9</a>","short":"A. Sesana, N. Korsakova, M.A. Sedda, V. Baibhav, E. Barausse, S. Barke, E. Berti, M. Bonetti, P.R. Capelo, C. Caprini, J. Garcia-Bellido, Z. Haiman, K. Jani, O. Jennrich, P.H. Johansson, F.M. Khan, V. Korol, A. Lamberts, A. Lupi, A. Mangiagli, L. Mayer, G. Nardini, F. Pacucci, A. Petiteau, A. Raccanelli, S. Rajendran, J. Regan, L. Shao, A. Spallicci, N. Tamanini, M. Volonteri, N. Warburton, K. Wong, M. Zumalacarregui, Experimental Astronomy 51 (2021) 1333–1383.","chicago":"Sesana, Alberto, Natalia Korsakova, Manuel Arca Sedda, Vishal Baibhav, Enrico Barausse, Simon Barke, Emanuele Berti, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” <i>Experimental Astronomy</i>. Springer Science and Business Media LLC, 2021. <a href=\"https://doi.org/10.1007/s10686-021-09709-9\">https://doi.org/10.1007/s10686-021-09709-9</a>.","ista":"Sesana A, Korsakova N, Sedda MA, Baibhav V, Barausse E, Barke S, Berti E, Bonetti M, Capelo PR, Caprini C, Garcia-Bellido J, Haiman Z, Jani K, Jennrich O, Johansson PH, Khan FM, Korol V, Lamberts A, Lupi A, Mangiagli A, Mayer L, Nardini G, Pacucci F, Petiteau A, Raccanelli A, Rajendran S, Regan J, Shao L, Spallicci A, Tamanini N, Volonteri M, Warburton N, Wong K, Zumalacarregui M. 2021. Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy. 51(3), 1333–1383.","ama":"Sesana A, Korsakova N, Sedda MA, et al. Unveiling the gravitational universe at μ-Hz frequencies. <i>Experimental Astronomy</i>. 2021;51(3):1333-1383. doi:<a href=\"https://doi.org/10.1007/s10686-021-09709-9\">10.1007/s10686-021-09709-9</a>","ieee":"A. Sesana <i>et al.</i>, “Unveiling the gravitational universe at μ-Hz frequencies,” <i>Experimental Astronomy</i>, vol. 51, no. 3. Springer Science and Business Media LLC, pp. 1333–1383, 2021.","mla":"Sesana, Alberto, et al. “Unveiling the Gravitational Universe at μ-Hz Frequencies.” <i>Experimental Astronomy</i>, vol. 51, no. 3, Springer Science and Business Media LLC, 2021, pp. 1333–83, doi:<a href=\"https://doi.org/10.1007/s10686-021-09709-9\">10.1007/s10686-021-09709-9</a>."},"month":"09","page":"1333-1383","oa":1,"oa_version":"Published Version","publisher":"Springer Science and Business Media LLC","quality_controlled":"1","date_updated":"2024-09-11T14:53:17Z","language":[{"iso":"eng"}],"article_type":"original","date_published":"2021-09-04T00:00:00Z","issue":"3","date_created":"2024-09-05T09:42:29Z","author":[{"full_name":"Sesana, Alberto","first_name":"Alberto","last_name":"Sesana"},{"last_name":"Korsakova","first_name":"Natalia","full_name":"Korsakova, Natalia"},{"full_name":"Sedda, Manuel Arca","first_name":"Manuel Arca","last_name":"Sedda"},{"full_name":"Baibhav, Vishal","first_name":"Vishal","last_name":"Baibhav"},{"last_name":"Barausse","full_name":"Barausse, Enrico","first_name":"Enrico"},{"last_name":"Barke","full_name":"Barke, Simon","first_name":"Simon"},{"full_name":"Berti, Emanuele","first_name":"Emanuele","last_name":"Berti"},{"first_name":"Matteo","full_name":"Bonetti, Matteo","last_name":"Bonetti"},{"full_name":"Capelo, Pedro R.","first_name":"Pedro R.","last_name":"Capelo"},{"full_name":"Caprini, Chiara","first_name":"Chiara","last_name":"Caprini"},{"last_name":"Garcia-Bellido","first_name":"Juan","full_name":"Garcia-Bellido, Juan"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"first_name":"Karan","full_name":"Jani, Karan","last_name":"Jani"},{"full_name":"Jennrich, Oliver","first_name":"Oliver","last_name":"Jennrich"},{"first_name":"Peter H.","full_name":"Johansson, Peter H.","last_name":"Johansson"},{"first_name":"Fazeel Mahmood","full_name":"Khan, Fazeel Mahmood","last_name":"Khan"},{"last_name":"Korol","full_name":"Korol, Valeriya","first_name":"Valeriya"},{"first_name":"Astrid","full_name":"Lamberts, Astrid","last_name":"Lamberts"},{"full_name":"Lupi, Alessandro","first_name":"Alessandro","last_name":"Lupi"},{"last_name":"Mangiagli","full_name":"Mangiagli, Alberto","first_name":"Alberto"},{"last_name":"Mayer","full_name":"Mayer, Lucio","first_name":"Lucio"},{"last_name":"Nardini","first_name":"Germano","full_name":"Nardini, Germano"},{"first_name":"Fabio","full_name":"Pacucci, Fabio","last_name":"Pacucci"},{"full_name":"Petiteau, Antoine","first_name":"Antoine","last_name":"Petiteau"},{"first_name":"Alvise","full_name":"Raccanelli, Alvise","last_name":"Raccanelli"},{"full_name":"Rajendran, Surjeet","first_name":"Surjeet","last_name":"Rajendran"},{"last_name":"Regan","first_name":"John","full_name":"Regan, John"},{"first_name":"Lijing","full_name":"Shao, Lijing","last_name":"Shao"},{"first_name":"Alessandro","full_name":"Spallicci, Alessandro","last_name":"Spallicci"},{"first_name":"Nicola","full_name":"Tamanini, Nicola","last_name":"Tamanini"},{"last_name":"Volonteri","first_name":"Marta","full_name":"Volonteri, Marta"},{"first_name":"Niels","full_name":"Warburton, Niels","last_name":"Warburton"},{"first_name":"Kaze","full_name":"Wong, Kaze","last_name":"Wong"},{"first_name":"Miguel","full_name":"Zumalacarregui, Miguel","last_name":"Zumalacarregui"}],"title":"Unveiling the gravitational universe at μ-Hz frequencies","intvolume":"        51","doi":"10.1007/s10686-021-09709-9","volume":51,"scopus_import":"1","year":"2021","publication":"Experimental Astronomy","main_file_link":[{"url":"https://doi.org/10.1007/s10686-021-09709-9","open_access":"1"}],"status":"public","publication_identifier":{"issn":["0922-6435","1572-9508"]},"day":"04","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_processing_charge":"No","extern":"1","publication_status":"published"},{"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_processing_charge":"No","publication_status":"published","extern":"1","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stab1978","open_access":"1"}],"status":"public","publication_identifier":{"issn":["0035-8711","1365-2966"]},"day":"10","issue":"3","date_created":"2024-09-05T12:17:24Z","author":[{"last_name":"Lu","full_name":"Lu, Tianhuan","first_name":"Tianhuan"},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"title":"The impact of baryons on cosmological inference from weak lensing statistics","article_type":"original","date_published":"2021-07-10T00:00:00Z","volume":506,"scopus_import":"1","year":"2021","publication":"Monthly Notices of the Royal Astronomical Society","intvolume":"       506","doi":"10.1093/mnras/stab1978","language":[{"iso":"eng"}],"date_updated":"2024-09-19T07:43:16Z","oa_version":"Published Version","publisher":"Oxford University Press","quality_controlled":"1","type":"journal_article","month":"07","citation":{"apa":"Lu, T., &#38; Haiman, Z. (2021). The impact of baryons on cosmological inference from weak lensing statistics. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stab1978\">https://doi.org/10.1093/mnras/stab1978</a>","short":"T. Lu, Z. Haiman, Monthly Notices of the Royal Astronomical Society 506 (2021) 3406–3417.","ama":"Lu T, Haiman Z. The impact of baryons on cosmological inference from weak lensing statistics. <i>Monthly Notices of the Royal Astronomical Society</i>. 2021;506(3):3406-3417. doi:<a href=\"https://doi.org/10.1093/mnras/stab1978\">10.1093/mnras/stab1978</a>","chicago":"Lu, Tianhuan, and Zoltán Haiman. “The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2021. <a href=\"https://doi.org/10.1093/mnras/stab1978\">https://doi.org/10.1093/mnras/stab1978</a>.","ista":"Lu T, Haiman Z. 2021. The impact of baryons on cosmological inference from weak lensing statistics. Monthly Notices of the Royal Astronomical Society. 506(3), 3406–3417.","mla":"Lu, Tianhuan, and Zoltán Haiman. “The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 506, no. 3, Oxford University Press, 2021, pp. 3406–17, doi:<a href=\"https://doi.org/10.1093/mnras/stab1978\">10.1093/mnras/stab1978</a>.","ieee":"T. Lu and Z. Haiman, “The impact of baryons on cosmological inference from weak lensing statistics,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 506, no. 3. Oxford University Press, pp. 3406–3417, 2021."},"page":"3406-3417","oa":1,"abstract":[{"text":"As weak lensing surveys are becoming deeper and cover larger areas, information will be available on small angular scales down to the arcmin level. To extract this extra information, accurate modelling of baryonic effects is necessary. In this work, we adopt a baryonic correction model, which includes gas both bound inside and ejected from dark matter (DM) haloes, a central galaxy, and changes in the DM profile induced by baryons. We use this model to incorporate baryons into a large suite of DM-only N-body simulations, covering a grid of 75 cosmologies in the Ωm–σ8 parameter space. We investigate how baryons affect Gaussian and non-Gaussian weak lensing statistics and the cosmological parameter inferences from these statistics. Our results show that marginalizing over baryonic parameters degrades the constraints in Ωm–σ8 space by a factor of 2–5 compared to those with baryonic parameters fixed. We also find that combining the lensing power spectrum and peak counts can break the degeneracy between cosmological and baryonic parameters and mitigate the impact of the uncertainty in baryonic physics.","lang":"eng"}],"_id":"17574"},{"article_type":"original","date_published":"2021-07-05T00:00:00Z","issue":"2","title":"Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries’","date_created":"2024-09-05T12:19:58Z","author":[{"last_name":"Xin","full_name":"Xin, Chengcheng","first_name":"Chengcheng"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"}],"intvolume":"       506","doi":"10.1093/mnras/stab1856","volume":506,"scopus_import":"1","publication":"Monthly Notices of the Royal Astronomical Society","year":"2021","main_file_link":[{"url":"https://doi.org/10.1093/mnras/stab1856","open_access":"1"}],"status":"public","day":"05","publication_identifier":{"issn":["0035-8711","1365-2966"]},"article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","extern":"1","publication_status":"published","abstract":[{"text":"The Legacy Survey of Space and Time (LSST) by the Vera C. Rubin Observatory is expected to discover tens of millions of quasars. A significant fraction of these could be powered by coalescing massive black hole (MBH) binaries, since many quasars are believed to be triggered by mergers. We show that under plausible assumptions about the luminosity functions, lifetimes, and binary fractions of quasars, we expect the full LSST quasar catalogue to contain between 20 and 100 million compact MBH binaries with masses M = 105–9M⊙, redshifts z = 0–6, and orbital periods P = 1–70 d. Their light-curves are expected to be distinctly periodic, which can be confidently distinguished from stochastic red-noise variability, because LSST will cover dozens, or even hundreds of cycles. A very small subset of 10–150 ultracompact (P ≲ 1 d) binary quasars among these will, over ∼5–15 yr, evolve into the mHz gravitational-wave frequency band and can be detected by LISA. They can therefore be regarded as ‘LISA verification binaries’, analogous to short-period Galactic compact-object binaries. The practical question is how to find these handful of ‘needles in the haystack’ among the large number of quasars: this will likely require a tailored co-adding analysis optimized for this purpose.","lang":"eng"}],"_id":"17577","month":"07","type":"journal_article","citation":{"ieee":"C. Xin and Z. Haiman, “Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries,’” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 506, no. 2. Oxford University Press, pp. 2408–2417, 2021.","mla":"Xin, Chengcheng, and Zoltán Haiman. “Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA ‘Verification Binaries.’” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 506, no. 2, Oxford University Press, 2021, pp. 2408–17, doi:<a href=\"https://doi.org/10.1093/mnras/stab1856\">10.1093/mnras/stab1856</a>.","apa":"Xin, C., &#38; Haiman, Z. (2021). Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries.’ <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stab1856\">https://doi.org/10.1093/mnras/stab1856</a>","short":"C. Xin, Z. Haiman, Monthly Notices of the Royal Astronomical Society 506 (2021) 2408–2417.","ama":"Xin C, Haiman Z. Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries.’ <i>Monthly Notices of the Royal Astronomical Society</i>. 2021;506(2):2408-2417. doi:<a href=\"https://doi.org/10.1093/mnras/stab1856\">10.1093/mnras/stab1856</a>","ista":"Xin C, Haiman Z. 2021. Ultra-short-period massive black hole binary candidates in LSST as LISA ‘verification binaries’. Monthly Notices of the Royal Astronomical Society. 506(2), 2408–2417.","chicago":"Xin, Chengcheng, and Zoltán Haiman. “Ultra-Short-Period Massive Black Hole Binary Candidates in LSST as LISA ‘Verification Binaries.’” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2021. <a href=\"https://doi.org/10.1093/mnras/stab1856\">https://doi.org/10.1093/mnras/stab1856</a>."},"page":"2408-2417","oa":1,"oa_version":"Published Version","publisher":"Oxford University Press","quality_controlled":"1","language":[{"iso":"eng"}],"date_updated":"2024-09-19T08:07:41Z"},{"article_type":"original","date_published":"2021-11-17T00:00:00Z","issue":"10","date_created":"2024-09-05T12:20:50Z","author":[{"full_name":"Sanderbeck, Phoebe Upton","first_name":"Phoebe Upton","last_name":"Sanderbeck"},{"last_name":"Bird","first_name":"Simeon","full_name":"Bird, Simeon"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"}],"title":"Nucleosynthetic signatures of primordial origin around supermassive black holes","article_number":"103022","intvolume":"       104","doi":"10.1103/physrevd.104.103022","volume":104,"scopus_import":"1","year":"2021","publication":"Physical Review D","status":"public","main_file_link":[{"url":"https://doi.org/10.1103/physrevd.104.103022","open_access":"1"}],"publication_identifier":{"issn":["2470-0010","2470-0029"]},"day":"17","article_processing_charge":"No","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","publication_status":"published","extern":"1","abstract":[{"lang":"eng","text":"If primordial black holes (PBHs) seeded the supermassive black holes (SMBHs) at the centers of high-redshift quasars, then the gas surrounding these black holes may reveal nucleosynthetic clues to their primordial origins. We present predictions of altered primordial abundances around PBHs massive enough to seed SMBHs at 𝑧≈6–7.5. We find that if PBHs with initial masses of ∼105  M⊙ are responsible for such SMBHs, they may produce primordial deuterium and Helium fractions enhanced by ≥10%, and lithium abundance depleted by ≥10%, at distances of up to ≈ a comoving kiloparsec away from the black hole after decoupling. We estimate that ∼108  M⊙ of gas is enhanced (or depleted) by at least one percent. Evidence of these modified primordial deuterium, helium, and lithium abundances could still be present if this circum-PBH gas remains unaccreted by the SMBH and in or near the host galaxies of high-redshift quasars. Measuring the abundance anomalies will be challenging, but could offer a novel way to reveal the primordial origin of such SMBH seeds."}],"_id":"17578","type":"journal_article","month":"11","citation":{"mla":"Sanderbeck, Phoebe Upton, et al. “Nucleosynthetic Signatures of Primordial Origin around Supermassive Black Holes.” <i>Physical Review D</i>, vol. 104, no. 10, 103022, American Physical Society, 2021, doi:<a href=\"https://doi.org/10.1103/physrevd.104.103022\">10.1103/physrevd.104.103022</a>.","ieee":"P. U. Sanderbeck, S. Bird, and Z. Haiman, “Nucleosynthetic signatures of primordial origin around supermassive black holes,” <i>Physical Review D</i>, vol. 104, no. 10. American Physical Society, 2021.","apa":"Sanderbeck, P. U., Bird, S., &#38; Haiman, Z. (2021). Nucleosynthetic signatures of primordial origin around supermassive black holes. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevd.104.103022\">https://doi.org/10.1103/physrevd.104.103022</a>","short":"P.U. Sanderbeck, S. Bird, Z. Haiman, Physical Review D 104 (2021).","ama":"Sanderbeck PU, Bird S, Haiman Z. Nucleosynthetic signatures of primordial origin around supermassive black holes. <i>Physical Review D</i>. 2021;104(10). doi:<a href=\"https://doi.org/10.1103/physrevd.104.103022\">10.1103/physrevd.104.103022</a>","chicago":"Sanderbeck, Phoebe Upton, Simeon Bird, and Zoltán Haiman. “Nucleosynthetic Signatures of Primordial Origin around Supermassive Black Holes.” <i>Physical Review D</i>. American Physical Society, 2021. <a href=\"https://doi.org/10.1103/physrevd.104.103022\">https://doi.org/10.1103/physrevd.104.103022</a>.","ista":"Sanderbeck PU, Bird S, Haiman Z. 2021. Nucleosynthetic signatures of primordial origin around supermassive black holes. Physical Review D. 104(10), 103022."},"oa":1,"oa_version":"Published Version","publisher":"American Physical Society","quality_controlled":"1","date_updated":"2024-09-19T08:12:35Z","language":[{"iso":"eng"}]},{"date_updated":"2024-09-19T11:41:11Z","language":[{"iso":"eng"}],"publisher":"American Astronomical Society","quality_controlled":"1","oa_version":"Published Version","oa":1,"type":"journal_article","citation":{"apa":"Tagawa, H., Kocsis, B., Haiman, Z., Bartos, I., Omukai, K., &#38; Samsing, J. (2021). Eccentric black hole mergers in active galactic nuclei. <i>The Astrophysical Journal Letters</i>. American Astronomical Society. <a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">https://doi.org/10.3847/2041-8213/abd4d3</a>","short":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, J. Samsing, The Astrophysical Journal Letters 907 (2021).","ista":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. 2021. Eccentric black hole mergers in active galactic nuclei. The Astrophysical Journal Letters. 907(1), L20.","chicago":"Tagawa, Hiromichi, Bence Kocsis, Zoltán Haiman, Imre Bartos, Kazuyuki Omukai, and Johan Samsing. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal Letters</i>. American Astronomical Society, 2021. <a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">https://doi.org/10.3847/2041-8213/abd4d3</a>.","ama":"Tagawa H, Kocsis B, Haiman Z, Bartos I, Omukai K, Samsing J. Eccentric black hole mergers in active galactic nuclei. <i>The Astrophysical Journal Letters</i>. 2021;907(1). doi:<a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">10.3847/2041-8213/abd4d3</a>","ieee":"H. Tagawa, B. Kocsis, Z. Haiman, I. Bartos, K. Omukai, and J. Samsing, “Eccentric black hole mergers in active galactic nuclei,” <i>The Astrophysical Journal Letters</i>, vol. 907, no. 1. American Astronomical Society, 2021.","mla":"Tagawa, Hiromichi, et al. “Eccentric Black Hole Mergers in Active Galactic Nuclei.” <i>The Astrophysical Journal Letters</i>, vol. 907, no. 1, L20, American Astronomical Society, 2021, doi:<a href=\"https://doi.org/10.3847/2041-8213/abd4d3\">10.3847/2041-8213/abd4d3</a>."},"month":"01","_id":"17583","abstract":[{"text":"The astrophysical origin of gravitational wave transients is a timely open question in the wake of discoveries by the Laser Interferometer Gravitational-Wave Observatory (LIGO)/Virgo. In active galactic nuclei (AGNs), binaries form and evolve efficiently by interaction with a dense population of stars and the gaseous AGN disk. Previous studies have shown that stellar-mass black hole (BH) mergers in such environments can explain the merger rate and the number of suspected hierarchical mergers observed by LIGO/Virgo. The binary eccentricity distribution can provide further information to distinguish between astrophysical models. Here we derive the eccentricity distribution of BH mergers in AGN disks. We find that eccentricity is mainly due to binary–single (BS) interactions, which lead to most BH mergers in AGN disks having a significant eccentricity at 0.01 Hz, detectable by the Laser Interferometer Space Antenna. If BS interactions occur in isotropic-3D directions, then 8%–30% of the mergers in AGN disks will have eccentricities at 10 Hz above e10 Hz ≳ 0.03, detectable by LIGO/Virgo/Kamioka Gravitational Wave Detector, while 5%–17% of mergers have e10 Hz ≥ 0.3. On the other hand, if BS interactions are confined to the AGN–disk plane due to torques from the disk, with 1–20 intermediate binary states during each interaction, or if BHs can migrate to ≲ 10−3 pc from the central supermassive BH, then 10%–70% of the mergers will be highly eccentric (e10 Hz ≥ 0.3), consistent with the possible high eccentricity in GW190521.","lang":"eng"}],"extern":"1","publication_status":"published","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","article_processing_charge":"No","publication_identifier":{"issn":["2041-8205","2041-8213"]},"day":"21","status":"public","main_file_link":[{"url":"https://doi.org/10.3847/2041-8213/abd4d3","open_access":"1"}],"article_number":"L20","date_created":"2024-09-05T12:27:07Z","author":[{"full_name":"Tagawa, Hiromichi","first_name":"Hiromichi","last_name":"Tagawa"},{"full_name":"Kocsis, Bence","first_name":"Bence","last_name":"Kocsis"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"Imre","full_name":"Bartos, Imre","last_name":"Bartos"},{"first_name":"Kazuyuki","full_name":"Omukai, Kazuyuki","last_name":"Omukai"},{"last_name":"Samsing","first_name":"Johan","full_name":"Samsing, Johan"}],"title":"Eccentric black hole mergers in active galactic nuclei","issue":"1","date_published":"2021-01-21T00:00:00Z","article_type":"original","scopus_import":"1","year":"2021","publication":"The Astrophysical Journal Letters","volume":907,"doi":"10.3847/2041-8213/abd4d3","intvolume":"       907"}]