[{"volume":119,"_id":"361","type":"journal_article","fulldoi":"https://doi.org/10.1021/acs.jpcc.5b06199","title":"Cu2ZnSnS4–PtM (M = Co, Ni) nanoheterostructures for photocatalytic hydrogen evolution","author":[{"full_name":"Yu, Xuelian","first_name":"Xuelian","last_name":"Yu"},{"full_name":"An, Xiaoqiang","first_name":"Xiaoqiang","last_name":"An"},{"full_name":"Genç, Aziz","first_name":"Aziz","last_name":"Genç"},{"id":"43C61214-F248-11E8-B48F-1D18A9856A87","last_name":"Ibáñez","orcid":"0000-0001-5013-2843","full_name":"Ibáñez, Maria","first_name":"Maria"},{"first_name":"Jordi","full_name":"Arbiol, Jordi","last_name":"Arbiol"},{"first_name":"Yihe","full_name":"Zhang, Yihe","last_name":"Zhang"},{"full_name":"Cabot, Andreu","first_name":"Andreu","last_name":"Cabot"}],"date_updated":"2021-01-12T07:44:38Z","oa_version":"None","year":"2015","publication_status":"published","extern":"1","article_processing_charge":"No","acknowledgement":"This work was supported by the National Natural Science Foundation of China (Grant 21401212), Fundamental Research Funds for the Central Universities (2652015086), the Framework 7 program under project SCALENANO (FP7-NMP-ENERGY-2011-284486), and the MICINN project ENE2013-46624-C4-3-R. Authors acknowledge the funding from Generalitat de Catalunya 2014 SGR 1638.","day":"26","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","citation":{"apa":"Yu, X., An, X., Genç, A., Ibáñez, M., Arbiol, J., Zhang, Y., &#38; Cabot, A. (2015). Cu2ZnSnS4–PtM (M = Co, Ni) nanoheterostructures for photocatalytic hydrogen evolution. <i>Journal of Physical Chemistry C</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/acs.jpcc.5b06199\">https://doi.org/10.1021/acs.jpcc.5b06199</a>","ieee":"X. Yu <i>et al.</i>, “Cu2ZnSnS4–PtM (M = Co, Ni) nanoheterostructures for photocatalytic hydrogen evolution,” <i>Journal of Physical Chemistry C</i>, vol. 119, no. 38. American Chemical Society, pp. 21882–21888, 2015.","short":"X. Yu, X. An, A. Genç, M. Ibáñez, J. Arbiol, Y. Zhang, A. Cabot, Journal of Physical Chemistry C 119 (2015) 21882–21888.","mla":"Yu, Xuelian, et al. “Cu2ZnSnS4–PtM (M = Co, Ni) Nanoheterostructures for Photocatalytic Hydrogen Evolution.” <i>Journal of Physical Chemistry C</i>, vol. 119, no. 38, American Chemical Society, 2015, pp. 21882–88, doi:<a href=\"https://doi.org/10.1021/acs.jpcc.5b06199\">10.1021/acs.jpcc.5b06199</a>.","chicago":"Yu, Xuelian, Xiaoqiang An, Aziz Genç, Maria Ibáñez, Jordi Arbiol, Yihe Zhang, and Andreu Cabot. “Cu2ZnSnS4–PtM (M = Co, Ni) Nanoheterostructures for Photocatalytic Hydrogen Evolution.” <i>Journal of Physical Chemistry C</i>. American Chemical Society, 2015. <a href=\"https://doi.org/10.1021/acs.jpcc.5b06199\">https://doi.org/10.1021/acs.jpcc.5b06199</a>.","ama":"Yu X, An X, Genç A, et al. Cu2ZnSnS4–PtM (M = Co, Ni) nanoheterostructures for photocatalytic hydrogen evolution. <i>Journal of Physical Chemistry C</i>. 2015;119(38):21882-21888. doi:<a href=\"https://doi.org/10.1021/acs.jpcc.5b06199\">10.1021/acs.jpcc.5b06199</a>","ista":"Yu X, An X, Genç A, Ibáñez M, Arbiol J, Zhang Y, Cabot A. 2015. Cu2ZnSnS4–PtM (M = Co, Ni) nanoheterostructures for photocatalytic hydrogen evolution. Journal of Physical Chemistry C. 119(38), 21882–21888."},"status":"public","publication":"Journal of Physical Chemistry C","publist_id":"7468","date_created":"2018-12-11T11:46:01Z","date_published":"2015-08-26T00:00:00Z","month":"08","issue":"38","abstract":[{"lang":"eng","text":"We report the synthesis and photocatalytic and magnetic characterization of colloidal nanoheterostructures formed by combining a Pt-based magnetic metal alloy (PtCo, PtNi) with Cu2ZnSnS4 (CZTS). While CZTS is one of the main candidate materials for solar energy conversion, the introduction of a Pt-based alloy on its surface strongly influences its chemical and electronic properties, ultimately determining its functionality. In this regard, up to a 15-fold increase of the photocatalytic hydrogen evolution activity was obtained with CZTS–PtCo when compared with CZTS. Furthermore, two times higher hydrogen evolution rates were obtained for CZTS–PtCo when compared with CZTS–Pt, in spite of the lower precious metal loading of the former. Besides, the magnetic properties of the PtCo nanoparticles attached to the CZTS nanocrystals were retained in the heterostructures, which could facilitate catalyst purification and recovery for its posterior recycling and/or reutilization."}],"page":"21882 - 21888","publisher":"American Chemical Society","language":[{"iso":"eng"}],"doi":"10.1021/acs.jpcc.5b06199","intvolume":"       119"},{"month":"04","issue":"13","publist_id":"7469","date_created":"2018-12-11T11:46:02Z","publication_identifier":{"issn":["0743-7463"],"eissn":["1520-5827"]},"status":"public","article_type":"original","language":[{"iso":"eng"}],"doi":"10.1021/la504906q","external_id":{"pmid":["25751745"]},"page":"3952 - 3957","oa_version":"None","publication_status":"published","pmid":1,"OA_type":"closed access","fulldoi":"https://doi.org/10.1021/la504906q","title":"Size and aspect ratio control of Pd inf 2 inf Sn nanorods and their water denitration properties","_id":"362","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","citation":{"ista":"Lu Z, Ibáñez M, Antolín A, Genç A, Shavel A, Contreras S, Medina F, Arbiol J, Cabot A. 2015. Size and aspect ratio control of Pd inf 2 inf Sn nanorods and their water denitration properties. Langmuir. 31(13), 3952–3957.","chicago":"Lu, Zhishan, Maria Ibáñez, Ana Antolín, Aziz Genç, Alexey Shavel, Sandra Contreras, Francesc Medina, Jordi Arbiol, and Andreu Cabot. “Size and Aspect Ratio Control of Pd Inf 2 Inf Sn Nanorods and Their Water Denitration Properties.” <i>Langmuir</i>. American Chemical Society, 2015. <a href=\"https://doi.org/10.1021/la504906q\">https://doi.org/10.1021/la504906q</a>.","ama":"Lu Z, Ibáñez M, Antolín A, et al. Size and aspect ratio control of Pd inf 2 inf Sn nanorods and their water denitration properties. <i>Langmuir</i>. 2015;31(13):3952-3957. doi:<a href=\"https://doi.org/10.1021/la504906q\">10.1021/la504906q</a>","mla":"Lu, Zhishan, et al. “Size and Aspect Ratio Control of Pd Inf 2 Inf Sn Nanorods and Their Water Denitration Properties.” <i>Langmuir</i>, vol. 31, no. 13, American Chemical Society, 2015, pp. 3952–57, doi:<a href=\"https://doi.org/10.1021/la504906q\">10.1021/la504906q</a>.","short":"Z. Lu, M. Ibáñez, A. Antolín, A. Genç, A. Shavel, S. Contreras, F. Medina, J. Arbiol, A. Cabot, Langmuir 31 (2015) 3952–3957.","ieee":"Z. Lu <i>et al.</i>, “Size and aspect ratio control of Pd inf 2 inf Sn nanorods and their water denitration properties,” <i>Langmuir</i>, vol. 31, no. 13. American Chemical Society, pp. 3952–3957, 2015.","apa":"Lu, Z., Ibáñez, M., Antolín, A., Genç, A., Shavel, A., Contreras, S., … Cabot, A. (2015). Size and aspect ratio control of Pd inf 2 inf Sn nanorods and their water denitration properties. <i>Langmuir</i>. American Chemical Society. <a href=\"https://doi.org/10.1021/la504906q\">https://doi.org/10.1021/la504906q</a>"},"day":"07","quality_controlled":"1","date_published":"2015-04-07T00:00:00Z","publication":"Langmuir","publisher":"American Chemical Society","intvolume":"        31","abstract":[{"text":"Monodisperse Pd2Sn nanorods with tuned size and aspect ratio were prepared by co-reduction of metal salts in the presence of trioctylphosphine, amine, and chloride ions. Asymmetric Pd2Sn nanostructures were achieved by the selective desorption of a surfactant mediated by chlorine ions. A preliminary evaluation of the geometry influence on catalytic properties evidenced Pd2Sn nanorods to have improved catalytic performance. In view of these results, Pd2Sn nanorods were also evaluated for water denitration. ","lang":"eng"}],"year":"2015","author":[{"last_name":"Lu","full_name":"Lu, Zhishan","first_name":"Zhishan"},{"full_name":"Ibáñez, Maria","first_name":"Maria","id":"43C61214-F248-11E8-B48F-1D18A9856A87","last_name":"Ibáñez","orcid":"0000-0001-5013-2843"},{"last_name":"Antolín","first_name":"Ana","full_name":"Antolín, Ana"},{"last_name":"Genç","first_name":"Aziz","full_name":"Genç, Aziz"},{"last_name":"Shavel","first_name":"Alexey","full_name":"Shavel, Alexey"},{"last_name":"Contreras","first_name":"Sandra","full_name":"Contreras, Sandra"},{"full_name":"Medina, Francesc","first_name":"Francesc","last_name":"Medina"},{"last_name":"Arbiol","full_name":"Arbiol, Jordi","first_name":"Jordi"},{"last_name":"Cabot","first_name":"Andreu","full_name":"Cabot, Andreu"}],"date_updated":"2026-05-19T08:52:57Z","volume":31,"type":"journal_article","scopus_import":"1","article_processing_charge":"No","extern":"1"},{"abstract":[{"text":"We use ultrafast optical spectroscopy to observe binding of charged single-particle excitations (SE) in the magnetically frustrated Mott insulator Na2IrO3. Above the antiferromagnetic ordering temperature (TN) the system response is due to both Hubbard excitons (HE) and their constituent unpaired SE. The SE response becomes strongly suppressed immediately below TN. We argue that this increase in binding energy is due to a unique interplay between the frustrated Kitaev and the weak Heisenberg-type ordering term in the Hamiltonian, mediating an effective interaction between the spin-singlet SE. This interaction grows with distance causing the SE to become trapped in the HE, similar to quark confinement inside hadrons. This binding of charged particles, induced by magnetic ordering, is a result of a confinement-deconfinement transition of spin excitations. This observation provides evidence for spin liquid type behavior which is expected in Na2IrO3.","lang":"eng"}],"intvolume":"       114","publisher":"American Physical Society","date_published":"2015-07-07T00:00:00Z","publication":"Physical Review Letters","quality_controlled":"1","extern":"1","article_processing_charge":"No","type":"journal_article","volume":114,"main_file_link":[{"open_access":"1","url":"https://dspace.mit.edu/handle/1721.1/92979"}],"year":"2015","author":[{"last_name":"Alpichshev","orcid":"0000-0002-7183-5203","id":"45E67A2A-F248-11E8-B48F-1D18A9856A87","full_name":"Alpichshev, Zhanybek","first_name":"Zhanybek"},{"last_name":"Mahmood","first_name":"Fahad","full_name":"Mahmood, Fahad"},{"last_name":"Cao","full_name":"Cao, Gang","first_name":"Gang"},{"first_name":"Nuh","full_name":"Gedik, Nuh","last_name":"Gedik"}],"date_updated":"2021-01-12T07:52:54Z","oa":1,"doi":"10.1103/PhysRevLett.114.017203","article_type":"original","language":[{"iso":"eng"}],"publist_id":"7441","date_created":"2018-12-11T11:46:11Z","status":"public","issue":"1","month":"07","day":"07","citation":{"ista":"Alpichshev Z, Mahmood F, Cao G, Gedik N. 2015. Confinement deconfinement transition as an indication of spin liquid type behavior in Na2IrO3. Physical Review Letters. 114(1).","ama":"Alpichshev Z, Mahmood F, Cao G, Gedik N. Confinement deconfinement transition as an indication of spin liquid type behavior in Na2IrO3. <i>Physical Review Letters</i>. 2015;114(1). doi:<a href=\"https://doi.org/10.1103/PhysRevLett.114.017203\">10.1103/PhysRevLett.114.017203</a>","chicago":"Alpichshev, Zhanybek, Fahad Mahmood, Gang Cao, and Nuh Gedik. “Confinement Deconfinement Transition as an Indication of Spin Liquid Type Behavior in Na2IrO3.” <i>Physical Review Letters</i>. American Physical Society, 2015. <a href=\"https://doi.org/10.1103/PhysRevLett.114.017203\">https://doi.org/10.1103/PhysRevLett.114.017203</a>.","ieee":"Z. Alpichshev, F. Mahmood, G. Cao, and N. Gedik, “Confinement deconfinement transition as an indication of spin liquid type behavior in Na2IrO3,” <i>Physical Review Letters</i>, vol. 114, no. 1. American Physical Society, 2015.","apa":"Alpichshev, Z., Mahmood, F., Cao, G., &#38; Gedik, N. (2015). Confinement deconfinement transition as an indication of spin liquid type behavior in Na2IrO3. <i>Physical Review Letters</i>. American Physical Society. <a href=\"https://doi.org/10.1103/PhysRevLett.114.017203\">https://doi.org/10.1103/PhysRevLett.114.017203</a>","short":"Z. Alpichshev, F. Mahmood, G. Cao, N. Gedik, Physical Review Letters 114 (2015).","mla":"Alpichshev, Zhanybek, et al. “Confinement Deconfinement Transition as an Indication of Spin Liquid Type Behavior in Na2IrO3.” <i>Physical Review Letters</i>, vol. 114, no. 1, American Physical Society, 2015, doi:<a href=\"https://doi.org/10.1103/PhysRevLett.114.017203\">10.1103/PhysRevLett.114.017203</a>."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","fulldoi":"https://doi.org/10.1103/PhysRevLett.114.017203","title":"Confinement deconfinement transition as an indication of spin liquid type behavior in Na2IrO3","_id":"388","publication_status":"published","oa_version":"Published Version"},{"volume":6,"scopus_import":"1","type":"journal_article","year":"2015","date_updated":"2026-05-19T09:52:55Z","author":[{"last_name":"Cohen","full_name":"Cohen, Michael","first_name":"Michael"},{"id":"3959A2A0-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0003-4509-4998","last_name":"Kicheva","first_name":"Anna","full_name":"Kicheva, Anna"},{"last_name":"Ribeiro","full_name":"Ribeiro, Ana","first_name":"Ana"},{"full_name":"Blassberg, Robert","first_name":"Robert","last_name":"Blassberg"},{"last_name":"Page","full_name":"Page, Karen","first_name":"Karen"},{"last_name":"Barnes","full_name":"Barnes, Chris","first_name":"Chris"},{"first_name":"James","full_name":"Briscoe, James","last_name":"Briscoe"}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1038/ncomms7709"}],"article_processing_charge":"No","extern":"1","acknowledgement":"C.P.B. gratefully acknowledges funding from the Wellcome Trust through a Research Career Development Fellowship (097319/Z/11/Z). This work was supported by the Medical Research Council (U117560541) and Wellcome Trust (WT098326MA, WT098325MA).","date_published":"2015-04-02T00:00:00Z","OA_place":"publisher","publication":"Nature Communications","quality_controlled":"1","DOAJ_listed":"1","abstract":[{"lang":"eng","text":"In the vertebrate neural tube, the morphogen Sonic Hedgehog (Shh) establishes a characteristic pattern of gene expression. Here we quantify the Shh gradient in the developing mouse neural tube and show that while the amplitude of the gradient increases over time, the activity of the pathway transcriptional effectors, Gli proteins, initially increases but later decreases. Computational analysis of the pathway suggests three mechanisms that could contribute to this adaptation: transcriptional upregulation of the inhibitory receptor Ptch1, transcriptional downregulation of Gli and the differential stability of active and inactive Gli isoforms. Consistent with this, Gli2 protein expression is downregulated during neural tube patterning and adaptation continues when the pathway is stimulated downstream of Ptch1. Moreover, the Shh-induced upregulation of Gli2 transcription prevents Gli activity levels from adapting in a different cell type, NIH3T3 fibroblasts, despite the upregulation of Ptch1. Multiple mechanisms therefore contribute to the intracellular dynamics of Shh signalling, resulting in different signalling dynamics in different cell types."}],"publisher":"Springer Nature","intvolume":"         6","fulldoi":"https://doi.org/10.1038/ncomms7709","title":"Ptch1 and Gli regulate Shh signalling dynamics via multiple mechanisms","article_number":"6709","_id":"1728","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"oa_version":"Published Version","publication_status":"published","OA_type":"gold","pmid":1,"day":"02","user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","citation":{"short":"M. Cohen, A. Kicheva, A. Ribeiro, R. Blassberg, K. Page, C. Barnes, J. Briscoe, Nature Communications 6 (2015).","mla":"Cohen, Michael, et al. “Ptch1 and Gli Regulate Shh Signalling Dynamics via Multiple Mechanisms.” <i>Nature Communications</i>, vol. 6, 6709, Springer Nature, 2015, doi:<a href=\"https://doi.org/10.1038/ncomms7709\">10.1038/ncomms7709</a>.","apa":"Cohen, M., Kicheva, A., Ribeiro, A., Blassberg, R., Page, K., Barnes, C., &#38; Briscoe, J. (2015). Ptch1 and Gli regulate Shh signalling dynamics via multiple mechanisms. <i>Nature Communications</i>. Springer Nature. <a href=\"https://doi.org/10.1038/ncomms7709\">https://doi.org/10.1038/ncomms7709</a>","ieee":"M. Cohen <i>et al.</i>, “Ptch1 and Gli regulate Shh signalling dynamics via multiple mechanisms,” <i>Nature Communications</i>, vol. 6. Springer Nature, 2015.","ama":"Cohen M, Kicheva A, Ribeiro A, et al. Ptch1 and Gli regulate Shh signalling dynamics via multiple mechanisms. <i>Nature Communications</i>. 2015;6. doi:<a href=\"https://doi.org/10.1038/ncomms7709\">10.1038/ncomms7709</a>","chicago":"Cohen, Michael, Anna Kicheva, Ana Ribeiro, Robert Blassberg, Karen Page, Chris Barnes, and James Briscoe. “Ptch1 and Gli Regulate Shh Signalling Dynamics via Multiple Mechanisms.” <i>Nature Communications</i>. Springer Nature, 2015. <a href=\"https://doi.org/10.1038/ncomms7709\">https://doi.org/10.1038/ncomms7709</a>.","ista":"Cohen M, Kicheva A, Ribeiro A, Blassberg R, Page K, Barnes C, Briscoe J. 2015. Ptch1 and Gli regulate Shh signalling dynamics via multiple mechanisms. Nature Communications. 6, 6709."},"date_created":"2018-12-11T11:53:42Z","publication_identifier":{"eissn":["2041-1723"]},"publist_id":"5399","status":"public","month":"04","external_id":{"pmid":["25833741"]},"oa":1,"article_type":"original","doi":"10.1038/ncomms7709","language":[{"iso":"eng"}]},{"related_material":{"record":[{"relation":"later_version","id":"1338","status":"public"},{"id":"1130","status":"public","relation":"dissertation_contains"}]},"department":[{"_id":"ToHe"}],"volume":9207,"scopus_import":"1","type":"conference","date_updated":"2026-04-09T10:54:00Z","author":[{"first_name":"Pavol","full_name":"Cerny, Pavol","id":"4DCBEFFE-F248-11E8-B48F-1D18A9856A87","last_name":"Cerny"},{"last_name":"Clarke","full_name":"Clarke, Edmund","first_name":"Edmund"},{"orcid":"0000−0002−2985−7724","last_name":"Henzinger","id":"40876CD8-F248-11E8-B48F-1D18A9856A87","full_name":"Henzinger, Thomas A","first_name":"Thomas A"},{"last_name":"Radhakrishna","id":"3B51CAC4-F248-11E8-B48F-1D18A9856A87","first_name":"Arjun","full_name":"Radhakrishna, Arjun"},{"last_name":"Ryzhyk","full_name":"Ryzhyk, Leonid","first_name":"Leonid"},{"first_name":"Roopsha","full_name":"Samanta, Roopsha","id":"3D2AAC08-F248-11E8-B48F-1D18A9856A87","last_name":"Samanta"},{"orcid":"0000-0003-4409-8487","last_name":"Tarrach","id":"3D6E8F2C-F248-11E8-B48F-1D18A9856A87","first_name":"Thorsten","full_name":"Tarrach, Thorsten"}],"year":"2015","isi":1,"article_processing_charge":"No","pubrep_id":"336","date_published":"2015-07-01T00:00:00Z","OA_place":"repository","series_title":"Lecture Notes in Computer Science","has_accepted_license":"1","quality_controlled":"1","ddc":["000"],"abstract":[{"text":"We present a computer-aided programming approach to concurrency. The approach allows programmers to program assuming a friendly, non-preemptive scheduler, and our synthesis procedure inserts synchronization to ensure that the final program works even with a preemptive scheduler. The correctness specification is implicit, inferred from the non-preemptive behavior. Let us consider sequences of calls that the program makes to an external interface. The specification requires that any such sequence produced under a preemptive scheduler should be included in the set of such sequences produced under a non-preemptive scheduler. The solution is based on a finitary abstraction, an algorithm for bounded language inclusion modulo an independence relation, and rules for inserting synchronization. We apply the approach to device-driver programming, where the driver threads call the software interface of the device and the API provided by the operating system. Our experiments demonstrate that our synthesis method is precise and efficient, and, since it does not require explicit specifications, is more practical than the conventional approach based on user-provided assertions.","lang":"eng"}],"publisher":"Springer","intvolume":"      9207","conference":{"name":"CAV: Computer Aided Verification","end_date":"2015-07-24","start_date":"2015-07-18","location":"San Francisco, CA, United States"},"_id":"1729","title":"From non-preemptive to preemptive scheduling using synchronization synthesis","fulldoi":"https://doi.org/10.1007/978-3-319-21668-3_11","oa_version":"Submitted Version","OA_type":"green","publication_status":"published","day":"01","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","file_date_updated":"2025-06-26T07:12:35Z","ec_funded":1,"citation":{"ista":"Cerny P, Clarke E, Henzinger TA, Radhakrishna A, Ryzhyk L, Samanta R, Tarrach T. 2015. From non-preemptive to preemptive scheduling using synchronization synthesis. 9207, 180–197.","chicago":"Cerny, Pavol, Edmund Clarke, Thomas A Henzinger, Arjun Radhakrishna, Leonid Ryzhyk, Roopsha Samanta, and Thorsten Tarrach. “From Non-Preemptive to Preemptive Scheduling Using Synchronization Synthesis.” Lecture Notes in Computer Science. Springer, 2015. <a href=\"https://doi.org/10.1007/978-3-319-21668-3_11\">https://doi.org/10.1007/978-3-319-21668-3_11</a>.","ama":"Cerny P, Clarke E, Henzinger TA, et al. From non-preemptive to preemptive scheduling using synchronization synthesis. 2015;9207:180-197. doi:<a href=\"https://doi.org/10.1007/978-3-319-21668-3_11\">10.1007/978-3-319-21668-3_11</a>","ieee":"P. Cerny <i>et al.</i>, “From non-preemptive to preemptive scheduling using synchronization synthesis,” vol. 9207. Springer, pp. 180–197, 2015.","apa":"Cerny, P., Clarke, E., Henzinger, T. A., Radhakrishna, A., Ryzhyk, L., Samanta, R., &#38; Tarrach, T. (2015). From non-preemptive to preemptive scheduling using synchronization synthesis. Presented at the CAV: Computer Aided Verification, San Francisco, CA, United States: Springer. <a href=\"https://doi.org/10.1007/978-3-319-21668-3_11\">https://doi.org/10.1007/978-3-319-21668-3_11</a>","mla":"Cerny, Pavol, et al. <i>From Non-Preemptive to Preemptive Scheduling Using Synchronization Synthesis</i>. Vol. 9207, Springer, 2015, pp. 180–97, doi:<a href=\"https://doi.org/10.1007/978-3-319-21668-3_11\">10.1007/978-3-319-21668-3_11</a>.","short":"P. Cerny, E. Clarke, T.A. Henzinger, A. Radhakrishna, L. Ryzhyk, R. Samanta, T. Tarrach, 9207 (2015) 180–197."},"status":"public","date_created":"2018-12-11T11:53:42Z","publist_id":"5398","file":[{"access_level":"open_access","file_name":"IST-2015-336-v1+1_long_version.pdf","date_created":"2018-12-12T10:08:53Z","content_type":"application/pdf","relation":"main_file","date_updated":"2025-06-26T07:12:35Z","checksum":"6ff58ac220e2f20cb001ba35d4924495","file_id":"4715","creator":"system","file_size":481922}],"month":"07","alternative_title":["LNCS"],"project":[{"call_identifier":"FP7","_id":"25EE3708-B435-11E9-9278-68D0E5697425","grant_number":"267989","name":"Quantitative Reactive Modeling"},{"grant_number":"Z211","call_identifier":"FWF","_id":"25F42A32-B435-11E9-9278-68D0E5697425","name":"Formal methods for the design and analysis of complex systems"},{"call_identifier":"FWF","_id":"25832EC2-B435-11E9-9278-68D0E5697425","grant_number":"S 11407_N23","name":"Rigorous Systems Engineering"}],"oa":1,"external_id":{"isi":["000491470400011"]},"page":"180 - 197","doi":"10.1007/978-3-319-21668-3_11","language":[{"iso":"eng"}]},{"day":"02","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"apa":"Colin De Verdière, É., Hubard, A., &#38; de Mesmay, A. N. (2015). Discrete systolic inequalities and decompositions of triangulated surfaces. <i>Discrete &#38; Computational Geometry</i>. Springer. <a href=\"https://doi.org/10.1007/s00454-015-9679-9\">https://doi.org/10.1007/s00454-015-9679-9</a>","ieee":"É. Colin De Verdière, A. Hubard, and A. N. de Mesmay, “Discrete systolic inequalities and decompositions of triangulated surfaces,” <i>Discrete &#38; Computational Geometry</i>, vol. 53, no. 3. Springer, pp. 587–620, 2015.","mla":"Colin De Verdière, Éric, et al. “Discrete Systolic Inequalities and Decompositions of Triangulated Surfaces.” <i>Discrete &#38; Computational Geometry</i>, vol. 53, no. 3, Springer, 2015, pp. 587–620, doi:<a href=\"https://doi.org/10.1007/s00454-015-9679-9\">10.1007/s00454-015-9679-9</a>.","short":"É. Colin De Verdière, A. Hubard, A.N. de Mesmay, Discrete &#38; Computational Geometry 53 (2015) 587–620.","chicago":"Colin De Verdière, Éric, Alfredo Hubard, and Arnaud N de Mesmay. “Discrete Systolic Inequalities and Decompositions of Triangulated Surfaces.” <i>Discrete &#38; Computational Geometry</i>. Springer, 2015. <a href=\"https://doi.org/10.1007/s00454-015-9679-9\">https://doi.org/10.1007/s00454-015-9679-9</a>.","ama":"Colin De Verdière É, Hubard A, de Mesmay AN. Discrete systolic inequalities and decompositions of triangulated surfaces. <i>Discrete &#38; Computational Geometry</i>. 2015;53(3):587-620. doi:<a href=\"https://doi.org/10.1007/s00454-015-9679-9\">10.1007/s00454-015-9679-9</a>","ista":"Colin De Verdière É, Hubard A, de Mesmay AN. 2015. Discrete systolic inequalities and decompositions of triangulated surfaces. Discrete &#38; Computational Geometry. 53(3), 587–620."},"_id":"1730","title":"Discrete systolic inequalities and decompositions of triangulated surfaces","fulldoi":"https://doi.org/10.1007/s00454-015-9679-9","oa_version":"Preprint","publication_status":"published","oa":1,"page":"587 - 620","external_id":{"arxiv":["1408.4036"],"isi":["000353895200006"]},"doi":"10.1007/s00454-015-9679-9","language":[{"iso":"eng"}],"status":"public","publist_id":"5397","date_created":"2018-12-11T11:53:42Z","month":"04","issue":"3","arxiv":1,"article_processing_charge":"No","volume":53,"department":[{"_id":"UlWa"}],"type":"journal_article","scopus_import":"1","date_updated":"2025-09-23T08:27:38Z","author":[{"last_name":"Colin De Verdière","full_name":"Colin De Verdière, Éric","first_name":"Éric"},{"last_name":"Hubard","first_name":"Alfredo","full_name":"Hubard, Alfredo"},{"last_name":"De Mesmay","id":"3DB2F25C-F248-11E8-B48F-1D18A9856A87","first_name":"Arnaud N","full_name":"De Mesmay, Arnaud N"}],"year":"2015","isi":1,"main_file_link":[{"open_access":"1","url":"http://arxiv.org/abs/1408.4036"}],"abstract":[{"text":"How much cutting is needed to simplify the topology of a surface? We provide bounds for several instances of this question, for the minimum length of topologically non-trivial closed curves, pants decompositions, and cut graphs with a given combinatorial map in triangulated combinatorial surfaces (or their dual cross-metric counterpart). Our work builds upon Riemannian systolic inequalities, which bound the minimum length of non-trivial closed curves in terms of the genus and the area of the surface. We first describe a systematic way to translate Riemannian systolic inequalities to a discrete setting, and vice-versa. This implies a conjecture by Przytycka and Przytycki (Graph structure theory. Contemporary Mathematics, vol. 147, 1993), a number of new systolic inequalities in the discrete setting, and the fact that a theorem of Hutchinson on the edge-width of triangulated surfaces and Gromov’s systolic inequality for surfaces are essentially equivalent. We also discuss how these proofs generalize to higher dimensions. Then we focus on topological decompositions of surfaces. Relying on ideas of Buser, we prove the existence of pants decompositions of length O(g^(3/2)n^(1/2)) for any triangulated combinatorial surface of genus g with n triangles, and describe an O(gn)-time algorithm to compute such a decomposition. Finally, we consider the problem of embedding a cut graph (or more generally a cellular graph) with a given combinatorial map on a given surface. Using random triangulations, we prove (essentially) that, for any choice of a combinatorial map, there are some surfaces on which any cellular embedding with that combinatorial map has length superlinear in the number of triangles of the triangulated combinatorial surface. There is also a similar result for graphs embedded on polyhedral triangulations.","lang":"eng"}],"publisher":"Springer","intvolume":"        53","publication":"Discrete & Computational Geometry","date_published":"2015-04-02T00:00:00Z","quality_controlled":"1"},{"publication":"Information and Computation","date_published":"2015-12-01T00:00:00Z","corr_author":"1","quality_controlled":"1","abstract":[{"lang":"eng","text":"We consider two-player zero-sum games on graphs. These games can be classified on the basis of the information of the players and on the mode of interaction between them. On the basis of information the classification is as follows: (a) partial-observation (both players have partial view of the game); (b) one-sided complete-observation (one player has complete observation); and (c) complete-observation (both players have complete view of the game). On the basis of mode of interaction we have the following classification: (a) concurrent (both players interact simultaneously); and (b) turn-based (both players interact in turn). The two sources of randomness in these games are randomness in transition function and randomness in strategies. In general, randomized strategies are more powerful than deterministic strategies, and randomness in transitions gives more general classes of games. In this work we present a complete characterization for the classes of games where randomness is not helpful in: (a) the transition function probabilistic transition can be simulated by deterministic transition); and (b) strategies (pure strategies are as powerful as randomized strategies). As consequence of our characterization we obtain new undecidability results for these games. "}],"publisher":"Elsevier","intvolume":"       245","related_material":{"record":[{"id":"3856","status":"public","relation":"earlier_version"}]},"department":[{"_id":"KrCh"},{"_id":"ToHe"}],"volume":245,"type":"journal_article","scopus_import":"1","date_updated":"2025-09-23T10:32:00Z","author":[{"first_name":"Krishnendu","full_name":"Chatterjee, Krishnendu","last_name":"Chatterjee","orcid":"0000-0002-4561-241X","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Doyen, Laurent","first_name":"Laurent","last_name":"Doyen"},{"last_name":"Gimbert","first_name":"Hugo","full_name":"Gimbert, Hugo"},{"full_name":"Henzinger, Thomas A","first_name":"Thomas A","last_name":"Henzinger","orcid":"0000−0002−2985−7724","id":"40876CD8-F248-11E8-B48F-1D18A9856A87"}],"year":"2015","isi":1,"main_file_link":[{"open_access":"1","url":"http://arxiv.org/abs/1006.0673"}],"arxiv":1,"article_processing_charge":"No","status":"public","publist_id":"5395","date_created":"2018-12-11T11:53:42Z","month":"12","issue":"12","project":[{"grant_number":"P 23499-N23","call_identifier":"FWF","_id":"2584A770-B435-11E9-9278-68D0E5697425","name":"Modern Graph Algorithmic Techniques in Formal Verification"},{"_id":"25863FF4-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","grant_number":"S11407","name":"Game Theory"},{"call_identifier":"FP7","_id":"2581B60A-B435-11E9-9278-68D0E5697425","grant_number":"279307","name":"Quantitative Graph Games: Theory and Applications"},{"_id":"2587B514-B435-11E9-9278-68D0E5697425","name":"Microsoft Research Faculty Fellowship"},{"name":"Quantitative Reactive Modeling","grant_number":"267989","call_identifier":"FP7","_id":"25EE3708-B435-11E9-9278-68D0E5697425"},{"grant_number":"215543","call_identifier":"FP7","_id":"25EFB36C-B435-11E9-9278-68D0E5697425","name":"COMponent-Based Embedded Systems design Techniques"},{"grant_number":"214373","call_identifier":"FP7","_id":"25F1337C-B435-11E9-9278-68D0E5697425","name":"Design for Embedded Systems"},{"grant_number":"S 11407_N23","_id":"25832EC2-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","name":"Rigorous Systems Engineering"}],"oa":1,"page":"3 - 16","external_id":{"isi":["000368899100002"],"arxiv":["1006.0673"]},"doi":"10.1016/j.ic.2015.06.003","language":[{"iso":"eng"}],"_id":"1731","title":"Randomness for free","fulldoi":"https://doi.org/10.1016/j.ic.2015.06.003","oa_version":"Preprint","publication_status":"published","day":"01","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"ista":"Chatterjee K, Doyen L, Gimbert H, Henzinger TA. 2015. Randomness for free. Information and Computation. 245(12), 3–16.","ama":"Chatterjee K, Doyen L, Gimbert H, Henzinger TA. Randomness for free. <i>Information and Computation</i>. 2015;245(12):3-16. doi:<a href=\"https://doi.org/10.1016/j.ic.2015.06.003\">10.1016/j.ic.2015.06.003</a>","chicago":"Chatterjee, Krishnendu, Laurent Doyen, Hugo Gimbert, and Thomas A Henzinger. “Randomness for Free.” <i>Information and Computation</i>. Elsevier, 2015. <a href=\"https://doi.org/10.1016/j.ic.2015.06.003\">https://doi.org/10.1016/j.ic.2015.06.003</a>.","ieee":"K. Chatterjee, L. Doyen, H. Gimbert, and T. A. Henzinger, “Randomness for free,” <i>Information and Computation</i>, vol. 245, no. 12. Elsevier, pp. 3–16, 2015.","apa":"Chatterjee, K., Doyen, L., Gimbert, H., &#38; Henzinger, T. A. (2015). Randomness for free. <i>Information and Computation</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.ic.2015.06.003\">https://doi.org/10.1016/j.ic.2015.06.003</a>","mla":"Chatterjee, Krishnendu, et al. “Randomness for Free.” <i>Information and Computation</i>, vol. 245, no. 12, Elsevier, 2015, pp. 3–16, doi:<a href=\"https://doi.org/10.1016/j.ic.2015.06.003\">10.1016/j.ic.2015.06.003</a>.","short":"K. Chatterjee, L. Doyen, H. Gimbert, T.A. Henzinger, Information and Computation 245 (2015) 3–16."},"ec_funded":1},{"abstract":[{"text":"We consider partially observable Markov decision processes (POMDPs), that are a standard framework for robotics applications to model uncertainties present in the real world, with temporal logic specifications. All temporal logic specifications in linear-time temporal logic (LTL) can be expressed as parity objectives. We study the qualitative analysis problem for POMDPs with parity objectives that asks whether there is a controller (policy) to ensure that the objective holds with probability 1 (almost-surely). While the qualitative analysis of POMDPs with parity objectives is undecidable, recent results show that when restricted to finite-memory policies the problem is EXPTIME-complete. While the problem is intractable in theory, we present a practical approach to solve the qualitative analysis problem. We designed several heuristics to deal with the exponential complexity, and have used our implementation on a number of well-known POMDP examples for robotics applications. Our results provide the first practical approach to solve the qualitative analysis of robot motion planning with LTL properties in the presence of uncertainty.","lang":"eng"}],"conference":{"name":"ICRA: International Conference on Robotics and Automation","end_date":"2015-05-30","start_date":"2015-05-26","location":"Seattle, WA, United States"},"publisher":"IEEE","date_published":"2015-01-01T00:00:00Z","quality_controlled":"1","arxiv":1,"type":"conference","scopus_import":1,"department":[{"_id":"KrCh"}],"related_material":{"record":[{"relation":"earlier_version","status":"public","id":"5424"},{"relation":"earlier_version","id":"5426","status":"public"}]},"main_file_link":[{"url":"http://arxiv.org/abs/1409.3360","open_access":"1"}],"year":"2015","date_updated":"2023-02-23T12:25:52Z","author":[{"full_name":"Chatterjee, Krishnendu","first_name":"Krishnendu","last_name":"Chatterjee","orcid":"0000-0002-4561-241X","id":"2E5DCA20-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Chmelik","id":"3624234E-F248-11E8-B48F-1D18A9856A87","first_name":"Martin","full_name":"Chmelik, Martin"},{"full_name":"Gupta, Raghav","first_name":"Raghav","last_name":"Gupta"},{"first_name":"Ayush","full_name":"Kanodia, Ayush","last_name":"Kanodia"}],"external_id":{"arxiv":["1409.3360"]},"page":"325 - 330","oa":1,"project":[{"_id":"2584A770-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","grant_number":"P 23499-N23","name":"Modern Graph Algorithmic Techniques in Formal Verification"},{"name":"Game Theory","_id":"25863FF4-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","grant_number":"S11407"},{"name":"Quantitative Graph Games: Theory and Applications","grant_number":"279307","call_identifier":"FP7","_id":"2581B60A-B435-11E9-9278-68D0E5697425"}],"language":[{"iso":"eng"}],"doi":"10.1109/ICRA.2015.7139019","publist_id":"5394","date_created":"2018-12-11T11:53:43Z","status":"public","month":"01","day":"01","ec_funded":1,"citation":{"ista":"Chatterjee K, Chmelik M, Gupta R, Kanodia A. 2015. Qualitative analysis of POMDPs with temporal logic specifications for robotics applications. ICRA: International Conference on Robotics and Automation, 325–330.","ama":"Chatterjee K, Chmelik M, Gupta R, Kanodia A. Qualitative analysis of POMDPs with temporal logic specifications for robotics applications. In: IEEE; 2015:325-330. doi:<a href=\"https://doi.org/10.1109/ICRA.2015.7139019\">10.1109/ICRA.2015.7139019</a>","chicago":"Chatterjee, Krishnendu, Martin Chmelik, Raghav Gupta, and Ayush Kanodia. “Qualitative Analysis of POMDPs with Temporal Logic Specifications for Robotics Applications,” 325–30. IEEE, 2015. <a href=\"https://doi.org/10.1109/ICRA.2015.7139019\">https://doi.org/10.1109/ICRA.2015.7139019</a>.","ieee":"K. Chatterjee, M. Chmelik, R. Gupta, and A. Kanodia, “Qualitative analysis of POMDPs with temporal logic specifications for robotics applications,” presented at the ICRA: International Conference on Robotics and Automation, Seattle, WA, United States, 2015, pp. 325–330.","apa":"Chatterjee, K., Chmelik, M., Gupta, R., &#38; Kanodia, A. (2015). Qualitative analysis of POMDPs with temporal logic specifications for robotics applications (pp. 325–330). Presented at the ICRA: International Conference on Robotics and Automation, Seattle, WA, United States: IEEE. <a href=\"https://doi.org/10.1109/ICRA.2015.7139019\">https://doi.org/10.1109/ICRA.2015.7139019</a>","short":"K. Chatterjee, M. Chmelik, R. Gupta, A. Kanodia, in:, IEEE, 2015, pp. 325–330.","mla":"Chatterjee, Krishnendu, et al. <i>Qualitative Analysis of POMDPs with Temporal Logic Specifications for Robotics Applications</i>. IEEE, 2015, pp. 325–30, doi:<a href=\"https://doi.org/10.1109/ICRA.2015.7139019\">10.1109/ICRA.2015.7139019</a>."},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","fulldoi":"https://doi.org/10.1109/ICRA.2015.7139019","title":"Qualitative analysis of POMDPs with temporal logic specifications for robotics applications","_id":"1732","publication_status":"published","oa_version":"Preprint"},{"day":"01","citation":{"mla":"Klehm, Oliver, et al. “Recent Advances in Facial Appearance Capture.” <i>Computer Graphics Forum</i>, vol. 34, no. 2, Wiley-Blackwell, 2015, pp. 709–33, doi:<a href=\"https://doi.org/10.1111/cgf.12594\">10.1111/cgf.12594</a>.","short":"O. Klehm, F. Rousselle, M. Papas, D. Bradley, C. Hery, B. Bickel, W. Jarosz, T. Beeler, Computer Graphics Forum 34 (2015) 709–733.","apa":"Klehm, O., Rousselle, F., Papas, M., Bradley, D., Hery, C., Bickel, B., … Beeler, T. (2015). Recent advances in facial appearance capture. <i>Computer Graphics Forum</i>. Wiley-Blackwell. <a href=\"https://doi.org/10.1111/cgf.12594\">https://doi.org/10.1111/cgf.12594</a>","ieee":"O. Klehm <i>et al.</i>, “Recent advances in facial appearance capture,” <i>Computer Graphics Forum</i>, vol. 34, no. 2. Wiley-Blackwell, pp. 709–733, 2015.","chicago":"Klehm, Oliver, Fabrice Rousselle, Marios Papas, Derek Bradley, Christophe Hery, Bernd Bickel, Wojciech Jarosz, and Thabo Beeler. “Recent Advances in Facial Appearance Capture.” <i>Computer Graphics Forum</i>. Wiley-Blackwell, 2015. <a href=\"https://doi.org/10.1111/cgf.12594\">https://doi.org/10.1111/cgf.12594</a>.","ama":"Klehm O, Rousselle F, Papas M, et al. Recent advances in facial appearance capture. <i>Computer Graphics Forum</i>. 2015;34(2):709-733. doi:<a href=\"https://doi.org/10.1111/cgf.12594\">10.1111/cgf.12594</a>","ista":"Klehm O, Rousselle F, Papas M, Bradley D, Hery C, Bickel B, Jarosz W, Beeler T. 2015. Recent advances in facial appearance capture. Computer Graphics Forum. 34(2), 709–733."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","fulldoi":"https://doi.org/10.1111/cgf.12594","title":"Recent advances in facial appearance capture","_id":"1734","publication_status":"published","oa_version":"None","external_id":{"isi":["000358326600063"]},"page":"709 - 733","language":[{"iso":"eng"}],"doi":"10.1111/cgf.12594","publist_id":"5391","date_created":"2018-12-11T11:53:43Z","status":"public","issue":"2","month":"05","article_processing_charge":"No","scopus_import":"1","type":"journal_article","department":[{"_id":"BeBi"}],"volume":34,"main_file_link":[{"url":"https://graphics.ethz.ch/~mpapas/publications/fac_star.pdf"}],"isi":1,"year":"2015","author":[{"last_name":"Klehm","first_name":"Oliver","full_name":"Klehm, Oliver"},{"full_name":"Rousselle, Fabrice","first_name":"Fabrice","last_name":"Rousselle"},{"first_name":"Marios","full_name":"Papas, Marios","last_name":"Papas"},{"last_name":"Bradley","full_name":"Bradley, Derek","first_name":"Derek"},{"full_name":"Hery, Christophe","first_name":"Christophe","last_name":"Hery"},{"last_name":"Bickel","orcid":"0000-0001-6511-9385","id":"49876194-F248-11E8-B48F-1D18A9856A87","first_name":"Bernd","full_name":"Bickel, Bernd"},{"first_name":"Wojciech","full_name":"Jarosz, Wojciech","last_name":"Jarosz"},{"last_name":"Beeler","full_name":"Beeler, Thabo","first_name":"Thabo"}],"date_updated":"2025-09-23T10:32:38Z","abstract":[{"text":"Facial appearance capture is now firmly established within academic research and used extensively across various application domains, perhaps most prominently in the entertainment industry through the design of virtual characters in video games and films. While significant progress has occurred over the last two decades, no single survey currently exists that discusses the similarities, differences, and practical considerations of the available appearance capture techniques as applied to human faces. A central difficulty of facial appearance capture is the way light interacts with skin-which has a complex multi-layered structure-and the interactions that occur below the skin surface can, by definition, only be observed indirectly. In this report, we distinguish between two broad strategies for dealing with this complexity. &quot;Image-based methods&quot; try to exhaustively capture the exact face appearance under different lighting and viewing conditions, and then render the face through weighted image combinations. &quot;Parametric methods&quot; instead fit the captured reflectance data to some parametric appearance model used during rendering, allowing for a more lightweight and flexible representation but at the cost of potentially increased rendering complexity or inexact reproduction. The goal of this report is to provide an overview that can guide practitioners and researchers in assessing the tradeoffs between current approaches and identifying directions for future advances in facial appearance capture.","lang":"eng"}],"intvolume":"        34","publisher":"Wiley-Blackwell","date_published":"2015-05-01T00:00:00Z","publication":"Computer Graphics Forum","quality_controlled":"1"},{"article_processing_charge":"No","acknowledgement":"The first author was supported by a JSPS Postdoctoral Fellowship for Research Abroad","scopus_import":"1","type":"journal_article","volume":34,"department":[{"_id":"ChWo"}],"isi":1,"author":[{"last_name":"Ando","first_name":"Ryoichi","full_name":"Ando, Ryoichi"},{"full_name":"Thürey, Nils","first_name":"Nils","last_name":"Thürey"},{"last_name":"Wojtan","orcid":"0000-0001-6646-5546","id":"3C61F1D2-F248-11E8-B48F-1D18A9856A87","first_name":"Christopher J","full_name":"Wojtan, Christopher J"}],"date_updated":"2025-09-22T14:29:19Z","year":"2015","abstract":[{"text":"This work presents a method for efficiently simplifying the pressure projection step in a liquid simulation. We first devise a straightforward dimension reduction technique that dramatically reduces the cost of solving the pressure projection. Next, we introduce a novel change of basis that satisfies free-surface boundary conditions exactly, regardless of the accuracy of the pressure solve. When combined, these ideas greatly reduce the computational complexity of the pressure solve without compromising free surface boundary conditions at the highest level of detail. Our techniques are easy to parallelize, and they effectively eliminate the computational bottleneck for large liquid simulations.","lang":"eng"}],"intvolume":"        34","publisher":"Wiley","pubrep_id":"607","publication":"Computer Graphics Forum","date_published":"2015-05-01T00:00:00Z","quality_controlled":"1","ddc":["000"],"has_accepted_license":"1","day":"01","file_date_updated":"2020-07-14T12:45:15Z","citation":{"chicago":"Ando, Ryoichi, Nils Thürey, and Chris Wojtan. “A Dimension-Reduced Pressure Solver for Liquid Simulations.” <i>Computer Graphics Forum</i>. Wiley, 2015. <a href=\"https://doi.org/10.1111/cgf.12576\">https://doi.org/10.1111/cgf.12576</a>.","ama":"Ando R, Thürey N, Wojtan C. A dimension-reduced pressure solver for liquid simulations. <i>Computer Graphics Forum</i>. 2015;34(2):473-480. doi:<a href=\"https://doi.org/10.1111/cgf.12576\">10.1111/cgf.12576</a>","ista":"Ando R, Thürey N, Wojtan C. 2015. A dimension-reduced pressure solver for liquid simulations. Computer Graphics Forum. 34(2), 473–480.","apa":"Ando, R., Thürey, N., &#38; Wojtan, C. (2015). A dimension-reduced pressure solver for liquid simulations. <i>Computer Graphics Forum</i>. Wiley. <a href=\"https://doi.org/10.1111/cgf.12576\">https://doi.org/10.1111/cgf.12576</a>","ieee":"R. Ando, N. Thürey, and C. Wojtan, “A dimension-reduced pressure solver for liquid simulations,” <i>Computer Graphics Forum</i>, vol. 34, no. 2. Wiley, pp. 473–480, 2015.","mla":"Ando, Ryoichi, et al. “A Dimension-Reduced Pressure Solver for Liquid Simulations.” <i>Computer Graphics Forum</i>, vol. 34, no. 2, Wiley, 2015, pp. 473–80, doi:<a href=\"https://doi.org/10.1111/cgf.12576\">10.1111/cgf.12576</a>.","short":"R. Ando, N. Thürey, C. Wojtan, Computer Graphics Forum 34 (2015) 473–480."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","_id":"1735","fulldoi":"https://doi.org/10.1111/cgf.12576","title":"A dimension-reduced pressure solver for liquid simulations","publication_status":"published","oa_version":"Submitted Version","oa":1,"external_id":{"isi":["000358326600045"]},"page":"473 - 480","language":[{"iso":"eng"}],"doi":"10.1111/cgf.12576","file":[{"relation":"main_file","date_updated":"2020-07-14T12:45:15Z","content_type":"application/pdf","date_created":"2018-12-12T10:16:30Z","file_name":"IST-2016-607-v1+1_coarsegrid.pdf","access_level":"open_access","file_size":6312352,"creator":"system","file_id":"5218","checksum":"590752bf977855b337a80f78a9bc2404"}],"status":"public","publist_id":"5389","date_created":"2018-12-11T11:53:44Z","issue":"2","month":"05"},{"status":"public","date_created":"2024-09-05T13:31:30Z","publication_identifier":{"issn":["0035-8711","1365-2966"]},"month":"07","issue":"3","oa":1,"page":"2540-2545","doi":"10.1093/mnras/stv1457","article_type":"original","language":[{"iso":"eng"}],"_id":"17615","fulldoi":"https://doi.org/10.1093/mnras/stv1457","title":"A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102?","oa_version":"Published Version","publication_status":"published","day":"24","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"chicago":"D’Orazio, D. J., Zoltán Haiman, P. Duffell, B. D. Farris, and A. I. MacFadyen. “A Reduced Orbital Period for the Supermassive Black Hole Binary Candidate in the Quasar PG 1302-102?” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv1457\">https://doi.org/10.1093/mnras/stv1457</a>.","ama":"D’Orazio DJ, Haiman Z, Duffell P, Farris BD, MacFadyen AI. A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102? <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;452(3):2540-2545. doi:<a href=\"https://doi.org/10.1093/mnras/stv1457\">10.1093/mnras/stv1457</a>","ista":"D’Orazio DJ, Haiman Z, Duffell P, Farris BD, MacFadyen AI. 2015. A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102? Monthly Notices of the Royal Astronomical Society. 452(3), 2540–2545.","apa":"D’Orazio, D. J., Haiman, Z., Duffell, P., Farris, B. D., &#38; MacFadyen, A. I. (2015). A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102? <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv1457\">https://doi.org/10.1093/mnras/stv1457</a>","ieee":"D. J. D’Orazio, Z. Haiman, P. Duffell, B. D. Farris, and A. I. MacFadyen, “A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102?,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 452, no. 3. Oxford University Press, pp. 2540–2545, 2015.","short":"D.J. D’Orazio, Z. Haiman, P. Duffell, B.D. Farris, A.I. MacFadyen, Monthly Notices of the Royal Astronomical Society 452 (2015) 2540–2545.","mla":"D’Orazio, D. J., et al. “A Reduced Orbital Period for the Supermassive Black Hole Binary Candidate in the Quasar PG 1302-102?” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 452, no. 3, Oxford University Press, 2015, pp. 2540–45, doi:<a href=\"https://doi.org/10.1093/mnras/stv1457\">10.1093/mnras/stv1457</a>."},"publication":"Monthly Notices of the Royal Astronomical Society","date_published":"2015-07-24T00:00:00Z","quality_controlled":"1","abstract":[{"lang":"eng","text":"Graham et al. have detected a 5.2 yr periodic optical variability of the quasar PG 1302-102 at redshift z = 0.3, which they interpret as the redshifted orbital period (1 + z)tbin of a putative supermassive black hole binary (SMBHB). Here, we consider the implications of a 3–8 times shorter orbital period, suggested by hydrodynamical simulations of circumbinary discs (CBDs) with nearly equal-mass SMBHBs (q ≡ M2/M1 ≳ 0.3). With the corresponding 2–4 times tighter binary separation, PG 1302 would be undergoing gravitational wave dominated inspiral, and serve as a proof that the BHs can be fuelled and produce bright emission even in this late stage of the merger. The expected fraction of binaries with the shorter tbin, among bright quasars, would be reduced by one to two orders of magnitude, compared to the 5.2 yr period, in better agreement with the rarity of candidates reported by Graham et al. Finally, shorter periods would imply higher binary speeds, possibly imprinting periodicity on the light curves from relativistic beaming, as well as measurable relativistic effects on the Fe K α line. The CBD model predicts additional periodic variability on time-scales of tbin and ≈0.5tbin, as well as periodic variation of broad line widths and offsets relative to the narrow lines, which are consistent with the observations. Future observations will be able to test these predictions and hence the binary+CBD hypothesis for PG 1302."}],"publisher":"Oxford University Press","intvolume":"       452","volume":452,"type":"journal_article","scopus_import":"1","author":[{"last_name":"D'Orazio","first_name":"D. J.","full_name":"D'Orazio, D. J."},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"P.","full_name":"Duffell, P.","last_name":"Duffell"},{"first_name":"B. D.","full_name":"Farris, B. D.","last_name":"Farris"},{"first_name":"A. I.","full_name":"MacFadyen, A. I.","last_name":"MacFadyen"}],"date_updated":"2024-09-24T07:58:52Z","year":"2015","main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stv1457"}],"article_processing_charge":"No","extern":"1"},{"quality_controlled":"1","date_published":"2015-09-11T00:00:00Z","publication":"Monthly Notices of the Royal Astronomical Society: Letters","intvolume":"       454","publisher":"Oxford University Press","abstract":[{"lang":"eng","text":"Graham et al. discovered a supermassive black hole binary (SMBHB) candidate and identified the detected 5.2 yr period of the optical variability as the orbital period of the binary. Hydrodynamical simulations predict multiple periodic components for the variability of SMBHBs, thus raising the possibility that the true period of the binary is different from 5.2 yr. We analyse the periodogram of PG1302 and find no compelling evidence for additional peaks. We also point out that, despite the 5.2 yr peak being significant if a single source is considered, further analysis is required to account for the fact that PG1302 was selected among a large sample of 247 000 quasars. We derive upper limits on any additional periodic modulations in the available data, by modelling the light curve as the sum of stochastic noise and the known 5.2 yr periodic component, and injecting additional sinusoidal signals. We find that, with the current data, we would be able to detect with high significance (false alarm probability <1 per cent) secondary periodic terms, with periods in the range predicted by the simulations, if the amplitude of the variability was at least ∼0.06 mag (compared to 0.14 mag for the main sinusoid). A three-year follow-up monitoring campaign with weekly observations can increase the sensitivity for detecting secondary peaks by ≈50 per cent, and would allow a more robust test of predictions from hydrodynamical simulations."}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnrasl/slv111"}],"year":"2015","author":[{"last_name":"Charisi","first_name":"M.","full_name":"Charisi, M."},{"last_name":"Bartos","first_name":"I.","full_name":"Bartos, I."},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"first_name":"A. M.","full_name":"Price-Whelan, A. M.","last_name":"Price-Whelan"},{"last_name":"Márka","full_name":"Márka, S.","first_name":"S."}],"date_updated":"2024-09-24T08:34:12Z","scopus_import":"1","type":"journal_article","volume":454,"article_processing_charge":"No","extern":"1","issue":"1","month":"09","publication_identifier":{"issn":["1745-3933","1745-3925"]},"date_created":"2024-09-05T13:51:39Z","status":"public","article_type":"original","doi":"10.1093/mnrasl/slv111","language":[{"iso":"eng"}],"page":"L21-L25","oa":1,"publication_status":"published","oa_version":"Published Version","fulldoi":"https://doi.org/10.1093/mnrasl/slv111","title":"Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102?","_id":"17622","citation":{"mla":"Charisi, M., et al. “Multiple Periods in the Variability of the Supermassive Black Hole Binary Candidate Quasar PG1302-102?” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 454, no. 1, Oxford University Press, 2015, pp. L21–25, doi:<a href=\"https://doi.org/10.1093/mnrasl/slv111\">10.1093/mnrasl/slv111</a>.","short":"M. Charisi, I. Bartos, Z. Haiman, A.M. Price-Whelan, S. Márka, Monthly Notices of the Royal Astronomical Society: Letters 454 (2015) L21–L25.","apa":"Charisi, M., Bartos, I., Haiman, Z., Price-Whelan, A. M., &#38; Márka, S. (2015). Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102? <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnrasl/slv111\">https://doi.org/10.1093/mnrasl/slv111</a>","ieee":"M. Charisi, I. Bartos, Z. Haiman, A. M. Price-Whelan, and S. Márka, “Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102?,” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>, vol. 454, no. 1. Oxford University Press, pp. L21–L25, 2015.","chicago":"Charisi, M., I. Bartos, Zoltán Haiman, A. M. Price-Whelan, and S. Márka. “Multiple Periods in the Variability of the Supermassive Black Hole Binary Candidate Quasar PG1302-102?” <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnrasl/slv111\">https://doi.org/10.1093/mnrasl/slv111</a>.","ama":"Charisi M, Bartos I, Haiman Z, Price-Whelan AM, Márka S. Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102? <i>Monthly Notices of the Royal Astronomical Society: Letters</i>. 2015;454(1):L21-L25. doi:<a href=\"https://doi.org/10.1093/mnrasl/slv111\">10.1093/mnrasl/slv111</a>","ista":"Charisi M, Bartos I, Haiman Z, Price-Whelan AM, Márka S. 2015. Multiple periods in the variability of the supermassive black hole binary candidate quasar PG1302-102? Monthly Notices of the Royal Astronomical Society: Letters. 454(1), L21–L25."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"11"},{"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stv1234"}],"author":[{"full_name":"Prieto, Joaquin","first_name":"Joaquin","last_name":"Prieto"},{"first_name":"Raul","full_name":"Jimenez, Raul","last_name":"Jimenez"},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"González","first_name":"Roberto E.","full_name":"González, Roberto E."}],"date_updated":"2024-09-24T11:52:00Z","year":"2015","scopus_import":"1","type":"journal_article","volume":452,"article_processing_charge":"No","extern":"1","quality_controlled":"1","publication":"Monthly Notices of the Royal Astronomical Society","date_published":"2015-07-08T00:00:00Z","intvolume":"       452","publisher":"Oxford University Press","abstract":[{"text":"In order to elucidate the origin of spin in both dark matter and baryons in galaxies, we have performed hydrodynamical simulations from cosmological initial conditions. We study atomic cooling haloes in the redshift range 100>z>9 with masses of order 109M⊙ at redshift z=10. We assume that the gas has primordial composition and that H2-cooling and prior star-formation in the haloes have been suppressed. We present a comprehensive analysis of the gas and dark matter properties of four halos with very low (λ≈0.01), low (λ≈0.04), high (λ≈0.06) and very high (λ≈0.1) spin parameter. Our main conclusion is that the spin orientation and magnitude is initially well described by tidal torque linear theory, but later on is determined by the merging and accretion history of each halo. We provide evidence that the topology of the merging region, i.e. the number of colliding filaments, gives an accurate prediction for the spin of dark matter and gas: halos at the center of knots will have low spin while those in the center of filaments will have high spin. The spin of a halo is given by λ≈0.05×(7.6/numberoffilaments)^5.1","lang":"eng"}],"publication_status":"published","oa_version":"Published Version","_id":"17641","fulldoi":"https://doi.org/10.1093/mnras/stv1234","title":"The origin of spin in galaxies: Clues from simulations of atomic cooling haloes","citation":{"mla":"Prieto, Joaquin, et al. “The Origin of Spin in Galaxies: Clues from Simulations of Atomic Cooling Haloes.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 452, no. 1, Oxford University Press, 2015, pp. 784–802, doi:<a href=\"https://doi.org/10.1093/mnras/stv1234\">10.1093/mnras/stv1234</a>.","short":"J. Prieto, R. Jimenez, Z. Haiman, R.E. González, Monthly Notices of the Royal Astronomical Society 452 (2015) 784–802.","apa":"Prieto, J., Jimenez, R., Haiman, Z., &#38; González, R. E. (2015). The origin of spin in galaxies: Clues from simulations of atomic cooling haloes. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv1234\">https://doi.org/10.1093/mnras/stv1234</a>","ieee":"J. Prieto, R. Jimenez, Z. Haiman, and R. E. González, “The origin of spin in galaxies: Clues from simulations of atomic cooling haloes,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 452, no. 1. Oxford University Press, pp. 784–802, 2015.","ama":"Prieto J, Jimenez R, Haiman Z, González RE. The origin of spin in galaxies: Clues from simulations of atomic cooling haloes. <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;452(1):784-802. doi:<a href=\"https://doi.org/10.1093/mnras/stv1234\">10.1093/mnras/stv1234</a>","chicago":"Prieto, Joaquin, Raul Jimenez, Zoltán Haiman, and Roberto E. González. “The Origin of Spin in Galaxies: Clues from Simulations of Atomic Cooling Haloes.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv1234\">https://doi.org/10.1093/mnras/stv1234</a>.","ista":"Prieto J, Jimenez R, Haiman Z, González RE. 2015. The origin of spin in galaxies: Clues from simulations of atomic cooling haloes. Monthly Notices of the Royal Astronomical Society. 452(1), 784–802."},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","day":"08","issue":"1","month":"07","status":"public","publication_identifier":{"issn":["0035-8711","1365-2966"]},"date_created":"2024-09-06T07:18:53Z","doi":"10.1093/mnras/stv1234","article_type":"original","language":[{"iso":"eng"}],"oa":1,"page":"784-802"},{"publication_identifier":{"issn":["0028-0836","1476-4687"]},"date_created":"2024-09-06T07:30:45Z","status":"public","month":"09","issue":"7569","page":"351-353","external_id":{"arxiv":["1509.04301"]},"oa":1,"article_type":"original","doi":"10.1038/nature15262","language":[{"iso":"eng"}],"title":"Relativistic boost as the cause of periodicity in a massive black-hole binary candidate","fulldoi":"https://doi.org/10.1038/nature15262","_id":"17652","oa_version":"Preprint","publication_status":"published","day":"16","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"ista":"D’Orazio DJ, Haiman Z, Schiminovich D. 2015. Relativistic boost as the cause of periodicity in a massive black-hole binary candidate. Nature. 525(7569), 351–353.","ama":"D’Orazio DJ, Haiman Z, Schiminovich D. Relativistic boost as the cause of periodicity in a massive black-hole binary candidate. <i>Nature</i>. 2015;525(7569):351-353. doi:<a href=\"https://doi.org/10.1038/nature15262\">10.1038/nature15262</a>","chicago":"D’Orazio, Daniel J., Zoltán Haiman, and David Schiminovich. “Relativistic Boost as the Cause of Periodicity in a Massive Black-Hole Binary Candidate.” <i>Nature</i>. Springer Science and Business Media LLC, 2015. <a href=\"https://doi.org/10.1038/nature15262\">https://doi.org/10.1038/nature15262</a>.","ieee":"D. J. D’Orazio, Z. Haiman, and D. Schiminovich, “Relativistic boost as the cause of periodicity in a massive black-hole binary candidate,” <i>Nature</i>, vol. 525, no. 7569. Springer Science and Business Media LLC, pp. 351–353, 2015.","apa":"D’Orazio, D. J., Haiman, Z., &#38; Schiminovich, D. (2015). Relativistic boost as the cause of periodicity in a massive black-hole binary candidate. <i>Nature</i>. Springer Science and Business Media LLC. <a href=\"https://doi.org/10.1038/nature15262\">https://doi.org/10.1038/nature15262</a>","short":"D.J. D’Orazio, Z. Haiman, D. Schiminovich, Nature 525 (2015) 351–353.","mla":"D’Orazio, Daniel J., et al. “Relativistic Boost as the Cause of Periodicity in a Massive Black-Hole Binary Candidate.” <i>Nature</i>, vol. 525, no. 7569, Springer Science and Business Media LLC, 2015, pp. 351–53, doi:<a href=\"https://doi.org/10.1038/nature15262\">10.1038/nature15262</a>."},"date_published":"2015-09-16T00:00:00Z","publication":"Nature","quality_controlled":"1","abstract":[{"text":"Because most large galaxies contain a central black hole, and galaxies often merge, black-hole binaries are expected to be common in galactic nuclei. Although they cannot be imaged, periodicities in the light curves of quasars have been interpreted as evidence for binaries, most recently in PG~1302-102, with a short rest-frame optical period of 4 years. If the orbital period matches this value, then for the range of estimated black hole masses the components would be separated by 0.007-0.017 pc, implying relativistic orbital speeds. There has been much debate over whether black hole orbits could be smaller than 1 pc. Here we show that the amplitude and the sinusoid-like shape of the variability of PG~1302-102 can be fit by relativistic Doppler boosting of emission from a compact, steadily accreting, unequal-mass binary. We predict that brightness variations in the ultraviolet light curve track those in the optical, but with a 2-3 times larger amplitude. This prediction is relatively insensitive to the details of the emission process, and is consistent with archival UV data. Follow-up UV and optical observations in the next few years can test this prediction and confirm the existence of a binary black hole in the relativistic regime.","lang":"eng"}],"publisher":"Springer Science and Business Media LLC","intvolume":"       525","volume":525,"type":"journal_article","scopus_import":"1","year":"2015","author":[{"last_name":"D'Orazio","first_name":"Daniel J.","full_name":"D'Orazio, Daniel J."},{"last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"David","full_name":"Schiminovich, David","last_name":"Schiminovich"}],"date_updated":"2024-09-24T13:22:24Z","main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1509.04301"}],"extern":"1","article_processing_charge":"No","arxiv":1},{"quality_controlled":"1","publication":"Monthly Notices of the Royal Astronomical Society","date_published":"2015-09-16T00:00:00Z","publisher":"Oxford University Press","intvolume":"       453","abstract":[{"lang":"eng","text":"Recently, Planck measured a value of the cosmic microwave background (CMB) optical depth due to electron scattering of τ=0.066±0.016. Here we show that this low value leaves essentially no room for an early partial reionisation of the intergalactic medium (IGM) by high-redshift Population III (Pop III) stars, expected to have formed in low-mass minihaloes. We perform semi-analytic calculations of reionisation which include the contribution from Pop II stars in atomic cooling haloes, calibrated with high-redshift galaxy observations, and Pop III stars in minihaloes with feedback due to Lyman-Werner (LW) radiation and metal enrichment. We find that without LW feedback or prompt metal enrichment (and assuming a minihalo escape fraction of 0.5) the Pop III star formation efficiency cannot exceed ∼a few×10−4, without violating the constraints set by Planck data. This excludes massive Pop III star formation in typical 106M⊙ minihaloes. Including LW feedback and metal enrichment alleviates this tension, allowing large Pop III stars to form early on before they are quenched by feedback. We find that the total density of Pop III stars formed across cosmic time is ≲104−5 M⊙ Mpc−3 and does not depend strongly on the feedback prescription adopted. Additionally, we perform a simple estimate of the possible impact on reionisation of X-rays produced by accretion onto black hole remnants of Pop III stars. We find that unless the accretion duty cycle is very low (≲0.01), this could lead to an optical depth inconsistent with Planck."}],"author":[{"last_name":"Visbal","first_name":"Eli","full_name":"Visbal, Eli"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"first_name":"Greg L.","full_name":"Bryan, Greg L.","last_name":"Bryan"}],"date_updated":"2024-09-25T07:32:20Z","year":"2015","main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1505.06359"}],"volume":453,"type":"journal_article","scopus_import":"1","arxiv":1,"extern":"1","article_processing_charge":"No","month":"09","issue":"4","status":"public","publication_identifier":{"issn":["0035-8711","1365-2966"]},"date_created":"2024-09-06T07:40:38Z","language":[{"iso":"eng"}],"doi":"10.1093/mnras/stv1941","article_type":"original","oa":1,"page":"4457-4467","external_id":{"arxiv":["1505.06359"]},"oa_version":"Preprint","publication_status":"published","_id":"17663","title":"Limits on population III star formation in minihaloes implied by Planck","fulldoi":"https://doi.org/10.1093/mnras/stv1941","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"ama":"Visbal E, Haiman Z, Bryan GL. Limits on population III star formation in minihaloes implied by Planck. <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;453(4):4457-4467. doi:<a href=\"https://doi.org/10.1093/mnras/stv1941\">10.1093/mnras/stv1941</a>","chicago":"Visbal, Eli, Zoltán Haiman, and Greg L. Bryan. “Limits on Population III Star Formation in Minihaloes Implied by Planck.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv1941\">https://doi.org/10.1093/mnras/stv1941</a>.","ista":"Visbal E, Haiman Z, Bryan GL. 2015. Limits on population III star formation in minihaloes implied by Planck. Monthly Notices of the Royal Astronomical Society. 453(4), 4457–4467.","apa":"Visbal, E., Haiman, Z., &#38; Bryan, G. L. (2015). Limits on population III star formation in minihaloes implied by Planck. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv1941\">https://doi.org/10.1093/mnras/stv1941</a>","ieee":"E. Visbal, Z. Haiman, and G. L. Bryan, “Limits on population III star formation in minihaloes implied by Planck,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 453, no. 4. Oxford University Press, pp. 4457–4467, 2015.","short":"E. Visbal, Z. Haiman, G.L. Bryan, Monthly Notices of the Royal Astronomical Society 453 (2015) 4457–4467.","mla":"Visbal, Eli, et al. “Limits on Population III Star Formation in Minihaloes Implied by Planck.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 453, no. 4, Oxford University Press, 2015, pp. 4457–67, doi:<a href=\"https://doi.org/10.1093/mnras/stv1941\">10.1093/mnras/stv1941</a>."},"day":"16"},{"oa":1,"page":"484-492","article_type":"original","doi":"10.1093/mnras/stv2371","language":[{"iso":"eng"}],"status":"public","date_created":"2024-09-06T08:20:30Z","publication_identifier":{"issn":["0035-8711","1365-2966"]},"issue":"1","month":"11","day":"02","citation":{"ieee":"P. Raffai, Z. Haiman, and Z. Frei, “A statistical method to search for recoiling supermassive black holes in active galactic nuclei,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 455, no. 1. Oxford University Press, pp. 484–492, 2015.","apa":"Raffai, P., Haiman, Z., &#38; Frei, Z. (2015). A statistical method to search for recoiling supermassive black holes in active galactic nuclei. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv2371\">https://doi.org/10.1093/mnras/stv2371</a>","short":"P. Raffai, Z. Haiman, Z. Frei, Monthly Notices of the Royal Astronomical Society 455 (2015) 484–492.","mla":"Raffai, P., et al. “A Statistical Method to Search for Recoiling Supermassive Black Holes in Active Galactic Nuclei.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 455, no. 1, Oxford University Press, 2015, pp. 484–92, doi:<a href=\"https://doi.org/10.1093/mnras/stv2371\">10.1093/mnras/stv2371</a>.","ista":"Raffai P, Haiman Z, Frei Z. 2015. A statistical method to search for recoiling supermassive black holes in active galactic nuclei. Monthly Notices of the Royal Astronomical Society. 455(1), 484–492.","chicago":"Raffai, P., Zoltán Haiman, and Z. Frei. “A Statistical Method to Search for Recoiling Supermassive Black Holes in Active Galactic Nuclei.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv2371\">https://doi.org/10.1093/mnras/stv2371</a>.","ama":"Raffai P, Haiman Z, Frei Z. A statistical method to search for recoiling supermassive black holes in active galactic nuclei. <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;455(1):484-492. doi:<a href=\"https://doi.org/10.1093/mnras/stv2371\">10.1093/mnras/stv2371</a>"},"user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","_id":"17685","title":"A statistical method to search for recoiling supermassive black holes in active galactic nuclei","fulldoi":"https://doi.org/10.1093/mnras/stv2371","publication_status":"published","oa_version":"Published Version","abstract":[{"lang":"eng","text":"We propose an observational test for gravitationally recoiling supermassive black holes (BHs) in active galactic nuclei, based on a correlation between the velocities of BHs relative to their host galaxies, |\\Delta v|, and their obscuring dust column densities, \\Sigma_{dust} (both measured along the line of sight). We use toy models for the distribution of recoil velocities, BH trajectories, and the geometry of obscuring dust tori in galactic centres, to simulate 2.5x10^5 random observations of recoiling quasars. BHs with recoil velocities comparable to the escape velocity from the galactic centre remain bound to the nucleus, and do not fully settle back to the centre of the torus due to dynamical friction in a typical quasar lifetime. We find that |\\Delta v| and \\Sigma_ {dust} for these BHs are positively correlated. For obscured (\\Sigma_{dust}>0) and for partially obscured (0<\\Sigma_{dust}<~2.3 g/m^2) quasars with |\\Delta v|>=45 km/s, the sample correlation coefficient between log10(|\\Delta v|) and \\Sigma_{dust} is r_{45} = 0.28+/-0.02 and r_{45} = 0.13+/-0.02, respectively. Allowing for random +/-100 km/s errors in |\\Delta v| unrelated to the recoil dilutes the correlation for the partially obscured quasars to r_{45} = 0.026+/-0.004 measured between |\\Delta v| and \\Sigma_{dust}. A random sample of >~3,500 obscured quasars with |\\Delta v|>=45 km/s would allow rejection of the no-correlation hypothesis with 3 sigma significance 95% of the time. Finally, we find that the fraction of obscured quasars, F_{obs}(|\\Delta v|), decreases with |\\Delta v| from F_{obs}(<10 km/s)>~0.8 to F_{obs}(>10^3 km/s)<~0.4. This predicted trend can be compared to the observed fraction of type II quasars, and can further test combinations of recoil, trajectory, and dust torus models."}],"intvolume":"       455","publisher":"Oxford University Press","publication":"Monthly Notices of the Royal Astronomical Society","date_published":"2015-11-02T00:00:00Z","quality_controlled":"1","article_processing_charge":"No","extern":"1","type":"journal_article","scopus_import":"1","volume":455,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stv2371"}],"date_updated":"2024-09-25T09:18:47Z","author":[{"last_name":"Raffai","first_name":"P.","full_name":"Raffai, P."},{"full_name":"Haiman, Zoltán","first_name":"Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"first_name":"Z.","full_name":"Frei, Z.","last_name":"Frei"}],"year":"2015"},{"extern":"1","article_processing_charge":"No","volume":450,"scopus_import":"1","type":"journal_article","year":"2015","date_updated":"2024-09-25T10:05:24Z","author":[{"first_name":"Eli","full_name":"Visbal, Eli","last_name":"Visbal"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman"},{"last_name":"Bryan","full_name":"Bryan, Greg L.","first_name":"Greg L."}],"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1093/mnras/stv785"}],"abstract":[{"lang":"eng","text":"Constraining the properties of Population III (Pop III) stars will be very challenging because they reside in small galaxies at high redshift which will be difficult to directly detect. In this paper, we suggest that intensity mapping may be a promising method to study Pop III stars. Intensity mapping is a technique proposed to measure large-scale fluctuations of galaxy line emission in three dimensions without resolving individual sources. This technique is well suited for observing many faint galaxies because it can measure their cumulative emission even if they cannot be directly detected. We focus on intensity mapping of He ii recombination lines. These lines are much stronger in Pop III stars than Pop II stars because the harder spectra of Pop III stars are expected to produce many He ii ionizing photons. Measuring the He ii 1640 Å intensity mapping signal, along with the signals from other lines such as Lyα, Hα, and metal lines, could give constraints on the initial mass function (IMF) and star formation rate density of Pop III stars as a function of redshift. To demonstrate the feasibility of these observations, we estimate the strength of the Pop III He ii 1640 Å intensity mapping signal from z = 10–20. We show that at z ≈ 10, the signal could be measured accurately by two different hypothetical future instruments, one which cross-correlates He ii 1640 Å with CO(1–0) line emission from galaxies and the other with 21 cm emission from the intergalactic medium."}],"publisher":"Oxford University Press","intvolume":"       450","date_published":"2015-05-06T00:00:00Z","publication":"Monthly Notices of the Royal Astronomical Society","quality_controlled":"1","day":"06","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"ama":"Visbal E, Haiman Z, Bryan GL. Looking for Population III stars with He ii line intensity mapping. <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;450(3):2506-2513. doi:<a href=\"https://doi.org/10.1093/mnras/stv785\">10.1093/mnras/stv785</a>","chicago":"Visbal, Eli, Zoltán Haiman, and Greg L. Bryan. “Looking for Population III Stars with He Ii Line Intensity Mapping.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv785\">https://doi.org/10.1093/mnras/stv785</a>.","ista":"Visbal E, Haiman Z, Bryan GL. 2015. Looking for Population III stars with He ii line intensity mapping. Monthly Notices of the Royal Astronomical Society. 450(3), 2506–2513.","apa":"Visbal, E., Haiman, Z., &#38; Bryan, G. L. (2015). Looking for Population III stars with He ii line intensity mapping. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv785\">https://doi.org/10.1093/mnras/stv785</a>","ieee":"E. Visbal, Z. Haiman, and G. L. Bryan, “Looking for Population III stars with He ii line intensity mapping,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 450, no. 3. Oxford University Press, pp. 2506–2513, 2015.","short":"E. Visbal, Z. Haiman, G.L. Bryan, Monthly Notices of the Royal Astronomical Society 450 (2015) 2506–2513.","mla":"Visbal, Eli, et al. “Looking for Population III Stars with He Ii Line Intensity Mapping.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 450, no. 3, Oxford University Press, 2015, pp. 2506–13, doi:<a href=\"https://doi.org/10.1093/mnras/stv785\">10.1093/mnras/stv785</a>."},"fulldoi":"https://doi.org/10.1093/mnras/stv785","title":"Looking for Population III stars with He ii line intensity mapping","_id":"17694","oa_version":"Published Version","publication_status":"published","page":"2506-2513","oa":1,"language":[{"iso":"eng"}],"article_type":"original","doi":"10.1093/mnras/stv785","publication_identifier":{"issn":["0035-8711","1365-2966"]},"date_created":"2024-09-06T08:40:33Z","status":"public","month":"05","issue":"3"},{"day":"15","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"mla":"Petri, Andrea, et al. “Emulating the CFHTLenS Weak Lensing Data: Cosmological Constraints from Moments and Minkowski Functionals.” <i>Physical Review D</i>, vol. 91, no. 10, 103511, American Physical Society, 2015, doi:<a href=\"https://doi.org/10.1103/physrevd.91.103511\">10.1103/physrevd.91.103511</a>.","short":"A. Petri, J. Liu, Z. Haiman, M. May, L. Hui, J.M. Kratochvil, Physical Review D 91 (2015).","apa":"Petri, A., Liu, J., Haiman, Z., May, M., Hui, L., &#38; Kratochvil, J. M. (2015). Emulating the CFHTLenS weak lensing data: Cosmological constraints from moments and Minkowski functionals. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevd.91.103511\">https://doi.org/10.1103/physrevd.91.103511</a>","ieee":"A. Petri, J. Liu, Z. Haiman, M. May, L. Hui, and J. M. Kratochvil, “Emulating the CFHTLenS weak lensing data: Cosmological constraints from moments and Minkowski functionals,” <i>Physical Review D</i>, vol. 91, no. 10. American Physical Society, 2015.","ama":"Petri A, Liu J, Haiman Z, May M, Hui L, Kratochvil JM. Emulating the CFHTLenS weak lensing data: Cosmological constraints from moments and Minkowski functionals. <i>Physical Review D</i>. 2015;91(10). doi:<a href=\"https://doi.org/10.1103/physrevd.91.103511\">10.1103/physrevd.91.103511</a>","chicago":"Petri, Andrea, Jia Liu, Zoltán Haiman, Morgan May, Lam Hui, and Jan M. Kratochvil. “Emulating the CFHTLenS Weak Lensing Data: Cosmological Constraints from Moments and Minkowski Functionals.” <i>Physical Review D</i>. American Physical Society, 2015. <a href=\"https://doi.org/10.1103/physrevd.91.103511\">https://doi.org/10.1103/physrevd.91.103511</a>.","ista":"Petri A, Liu J, Haiman Z, May M, Hui L, Kratochvil JM. 2015. Emulating the CFHTLenS weak lensing data: Cosmological constraints from moments and Minkowski functionals. Physical Review D. 91(10), 103511."},"_id":"17702","title":"Emulating the CFHTLenS weak lensing data: Cosmological constraints from moments and Minkowski functionals","fulldoi":"https://doi.org/10.1103/physrevd.91.103511","article_number":"103511","oa_version":"Preprint","publication_status":"published","oa":1,"external_id":{"arxiv":["1503.06214"]},"doi":"10.1103/physrevd.91.103511","language":[{"iso":"eng"}],"article_type":"original","status":"public","date_created":"2024-09-06T08:48:07Z","publication_identifier":{"issn":["1550-7998","1550-2368"]},"month":"05","issue":"10","arxiv":1,"extern":"1","article_processing_charge":"No","volume":91,"scopus_import":"1","type":"journal_article","author":[{"last_name":"Petri","first_name":"Andrea","full_name":"Petri, Andrea"},{"last_name":"Liu","first_name":"Jia","full_name":"Liu, Jia"},{"id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36","last_name":"Haiman","full_name":"Haiman, Zoltán","first_name":"Zoltán"},{"last_name":"May","full_name":"May, Morgan","first_name":"Morgan"},{"full_name":"Hui, Lam","first_name":"Lam","last_name":"Hui"},{"full_name":"Kratochvil, Jan M.","first_name":"Jan M.","last_name":"Kratochvil"}],"date_updated":"2024-09-25T11:29:05Z","year":"2015","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.1503.06214","open_access":"1"}],"abstract":[{"lang":"eng","text":"Weak gravitational lensing is a powerful cosmological probe, with non--Gaussian features potentially containing the majority of the information. We examine constraints on the parameter triplet (Ωm,w,σ8) from non-Gaussian features of the weak lensing convergence field, including a set of moments (up to 4th order) and Minkowski functionals, using publicly available data from the 154deg2 CFHTLenS survey. We utilize a suite of ray--tracing N-body simulations spanning 91 points in (Ωm,w,σ8) parameter space, replicating the galaxy sky positions, redshifts and shape noise in the CFHTLenS catalogs. We then build an emulator that interpolates the simulated descriptors as a function of (Ωm,w,σ8), and use it to compute the likelihood function and parameter constraints. We employ a principal component analysis to reduce dimensionality and to help stabilize the constraints with respect to the number of bins used to construct each statistic. Using the full set of statistics, we find Σ8≡σ8(Ωm/0.27)^0.55=0.75±0.04 (68% C.L.), in agreement with previous values. We find that constraints on the (Ωm,σ8) doublet from the Minkowski functionals suffer a strong bias. However, high-order moments break the (Ωm,σ8) degeneracy and provide a tight constraint on these parameters with no apparent bias. The main contribution comes from quartic moments of derivatives."}],"publisher":"American Physical Society","intvolume":"        91","publication":"Physical Review D","date_published":"2015-05-15T00:00:00Z","quality_controlled":"1"},{"article_processing_charge":"No","extern":"1","arxiv":1,"year":"2015","date_updated":"2024-09-25T12:03:54Z","author":[{"first_name":"Jia","full_name":"Liu, Jia","last_name":"Liu"},{"first_name":"Andrea","full_name":"Petri, Andrea","last_name":"Petri"},{"first_name":"Zoltán","full_name":"Haiman, Zoltán","last_name":"Haiman","id":"7c006e8c-cc0d-11ee-8322-cb904ef76f36"},{"first_name":"Lam","full_name":"Hui, Lam","last_name":"Hui"},{"first_name":"Jan M.","full_name":"Kratochvil, Jan M.","last_name":"Kratochvil"},{"full_name":"May, Morgan","first_name":"Morgan","last_name":"May"}],"main_file_link":[{"open_access":"1","url":" https://doi.org/10.48550/arXiv.1412.0757"}],"volume":91,"type":"journal_article","scopus_import":"1","publisher":"American Physical Society","intvolume":"        91","abstract":[{"lang":"eng","text":"Lensing peaks have been proposed as a useful statistic, containing cosmological information from non-Gaussianities that is inaccessible from traditional two-point statistics such as the power spectrum or two-point correlation functions. Here we examine constraints on cosmological parameters from weak lensing peak counts, using the publicly available data from the 154 deg^2 CFHTLenS survey. We utilize a new suite of ray-tracing N-body simulations on a grid of 91 cosmological models, covering broad ranges of the three parameters Ωm, σ8, and w, and replicating the Galaxy sky positions, redshifts, and shape noise in the CFHTLenS observations. We then build an emulator that interpolates the power spectrum and the peak counts to an accuracy of ≤5%, and compute the likelihood in the three-dimensional parameter space (Ωm, σ8, w) from both observables. We find that constraints from peak counts are comparable to those from the power spectrum, and somewhat tighter when different smoothing scales are combined. Neither observable can constrain w without external data. When the power spectrum and peak counts are combined, the area of the error \"banana'' in the (Ωm, σ8) plane reduces by a factor of ≈2, compared to using the power spectrum alone. For a flat Λ cold dark matter model, combining both statistics, we obtain the constraint σ8(Ωm/0.27)^0.63=0.85+0.03−0.03."}],"quality_controlled":"1","date_published":"2015-03-04T00:00:00Z","publication":"Physical Review D","user_id":"317138e5-6ab7-11ef-aa6d-ffef3953e345","citation":{"ieee":"J. Liu, A. Petri, Z. Haiman, L. Hui, J. M. Kratochvil, and M. May, “Cosmology constraints from the weak lensing peak counts and the power spectrum in CFHTLenS data,” <i>Physical Review D</i>, vol. 91, no. 6. American Physical Society, 2015.","apa":"Liu, J., Petri, A., Haiman, Z., Hui, L., Kratochvil, J. M., &#38; May, M. (2015). Cosmology constraints from the weak lensing peak counts and the power spectrum in CFHTLenS data. <i>Physical Review D</i>. American Physical Society. <a href=\"https://doi.org/10.1103/physrevd.91.063507\">https://doi.org/10.1103/physrevd.91.063507</a>","short":"J. Liu, A. Petri, Z. Haiman, L. Hui, J.M. Kratochvil, M. May, Physical Review D 91 (2015).","mla":"Liu, Jia, et al. “Cosmology Constraints from the Weak Lensing Peak Counts and the Power Spectrum in CFHTLenS Data.” <i>Physical Review D</i>, vol. 91, no. 6, 063507, American Physical Society, 2015, doi:<a href=\"https://doi.org/10.1103/physrevd.91.063507\">10.1103/physrevd.91.063507</a>.","ista":"Liu J, Petri A, Haiman Z, Hui L, Kratochvil JM, May M. 2015. Cosmology constraints from the weak lensing peak counts and the power spectrum in CFHTLenS data. Physical Review D. 91(6), 063507.","chicago":"Liu, Jia, Andrea Petri, Zoltán Haiman, Lam Hui, Jan M. Kratochvil, and Morgan May. “Cosmology Constraints from the Weak Lensing Peak Counts and the Power Spectrum in CFHTLenS Data.” <i>Physical Review D</i>. American Physical Society, 2015. <a href=\"https://doi.org/10.1103/physrevd.91.063507\">https://doi.org/10.1103/physrevd.91.063507</a>.","ama":"Liu J, Petri A, Haiman Z, Hui L, Kratochvil JM, May M. Cosmology constraints from the weak lensing peak counts and the power spectrum in CFHTLenS data. <i>Physical Review D</i>. 2015;91(6). doi:<a href=\"https://doi.org/10.1103/physrevd.91.063507\">10.1103/physrevd.91.063507</a>"},"day":"04","oa_version":"Preprint","publication_status":"published","title":"Cosmology constraints from the weak lensing peak counts and the power spectrum in CFHTLenS data","fulldoi":"https://doi.org/10.1103/physrevd.91.063507","article_number":"063507","_id":"17710","article_type":"original","doi":"10.1103/physrevd.91.063507","language":[{"iso":"eng"}],"external_id":{"arxiv":["1412.0757"]},"oa":1,"month":"03","issue":"6","publication_identifier":{"issn":["1550-7998","1550-2368"]},"date_created":"2024-09-06T08:54:57Z","status":"public"},{"oa":1,"page":"3196 - 3208","external_id":{"pmid":["25836178"]},"article_type":"original","language":[{"iso":"eng"}],"doi":"10.1364/OE.23.003196","status":"public","publication_identifier":{"eissn":["1094-4087"]},"publist_id":"5325","date_created":"2018-12-11T11:54:01Z","issue":"3","month":"02","day":"09","citation":{"ista":"Pitanti A, Fink JM, Safavi Naeini A, Hill J, Lei C, Tredicucci A, Painter O. 2015. Strong opto-electro-mechanical coupling in a silicon photonic crystal cavity. Optics Express. 23(3), 3196–3208.","chicago":"Pitanti, Alessandro, Johannes M Fink, Amir Safavi Naeini, Jeff Hill, Chan Lei, Alessandro Tredicucci, and Oskar Painter. “Strong Opto-Electro-Mechanical Coupling in a Silicon Photonic Crystal Cavity.” <i>Optics Express</i>. Optica Publishing Group, 2015. <a href=\"https://doi.org/10.1364/OE.23.003196\">https://doi.org/10.1364/OE.23.003196</a>.","ama":"Pitanti A, Fink JM, Safavi Naeini A, et al. Strong opto-electro-mechanical coupling in a silicon photonic crystal cavity. <i>Optics Express</i>. 2015;23(3):3196-3208. doi:<a href=\"https://doi.org/10.1364/OE.23.003196\">10.1364/OE.23.003196</a>","ieee":"A. Pitanti <i>et al.</i>, “Strong opto-electro-mechanical coupling in a silicon photonic crystal cavity,” <i>Optics Express</i>, vol. 23, no. 3. Optica Publishing Group, pp. 3196–3208, 2015.","apa":"Pitanti, A., Fink, J. M., Safavi Naeini, A., Hill, J., Lei, C., Tredicucci, A., &#38; Painter, O. (2015). Strong opto-electro-mechanical coupling in a silicon photonic crystal cavity. <i>Optics Express</i>. Optica Publishing Group. <a href=\"https://doi.org/10.1364/OE.23.003196\">https://doi.org/10.1364/OE.23.003196</a>","mla":"Pitanti, Alessandro, et al. “Strong Opto-Electro-Mechanical Coupling in a Silicon Photonic Crystal Cavity.” <i>Optics Express</i>, vol. 23, no. 3, Optica Publishing Group, 2015, pp. 3196–208, doi:<a href=\"https://doi.org/10.1364/OE.23.003196\">10.1364/OE.23.003196</a>.","short":"A. Pitanti, J.M. Fink, A. Safavi Naeini, J. Hill, C. Lei, A. Tredicucci, O. Painter, Optics Express 23 (2015) 3196–3208."},"user_id":"ba8df636-2132-11f1-aed0-ed93e2281fdd","_id":"1788","title":"Strong opto-electro-mechanical coupling in a silicon photonic crystal cavity","fulldoi":"https://doi.org/10.1364/OE.23.003196","pmid":1,"publication_status":"published","OA_type":"gold","tmp":{"name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode"},"oa_version":"Published Version","abstract":[{"lang":"eng","text":"We fabricate and characterize a microscale silicon opto-electromechanical system whose mechanical motion is coupled capacitively to an electrical circuit and optically via radiation pressure to a photonic crystal cavity. To achieve large electromechanical interaction strength, we implement an inverse shadow mask fabrication scheme which obtains capacitor gaps as small as 30 nm while maintaining a silicon surface quality necessary for minimizing optical loss. Using the sensitive optical read-out of the photonic crystal cavity, we characterize the linear and nonlinear capacitive coupling to the fundamental ωm=2π = 63 MHz in-plane flexural motion of the structure, showing that the large electromechanical coupling in such devices may be suitable for realizing efficient microwave-to-optical signal conversion."}],"DOAJ_listed":"1","intvolume":"        23","publisher":"Optica Publishing Group","publication":"Optics Express","OA_place":"publisher","date_published":"2015-02-09T00:00:00Z","quality_controlled":"1","article_processing_charge":"No","acknowledgement":"This work was supported by the DARPA MESO program, the AFOSR Hybrid Nanophotonics MURI, the Institute for Quantum Information and Matter, an NSF Physics Frontiers Center with support of the Gordon and Betty Moore Foundation, and the Kavli Nanoscience Institute at Caltech. AP gratefully acknowledge funding from EU through Marie Curie Actions, project NEMO (GA 298861). AT acknowledges partial financial support from the ERC through the advanced grant SoulMan","extern":"1","scopus_import":"1","type":"journal_article","volume":23,"main_file_link":[{"open_access":"1","url":"https://doi.org/10.1364/OE.23.003196"}],"author":[{"full_name":"Pitanti, Alessandro","first_name":"Alessandro","last_name":"Pitanti"},{"id":"4B591CBA-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8112-028X","last_name":"Fink","first_name":"Johannes M","full_name":"Fink, Johannes M"},{"last_name":"Safavi Naeini","first_name":"Amir","full_name":"Safavi Naeini, Amir"},{"last_name":"Hill","full_name":"Hill, Jeff","first_name":"Jeff"},{"first_name":"Chan","full_name":"Lei, Chan","last_name":"Lei"},{"last_name":"Tredicucci","full_name":"Tredicucci, Alessandro","first_name":"Alessandro"},{"last_name":"Painter","full_name":"Painter, Oskar","first_name":"Oskar"}],"date_updated":"2026-05-19T08:32:24Z","year":"2015"}]