يعرض 1 - 8 نتائج من 8 نتيجة بحث عن '"Fei, Qinyue"', وقت الاستعلام: 0.34s تنقيح النتائج
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    Academic Journal

    المساهمون: Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA), École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Cergy Pontoise (UCP), Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS), Université Paris Cité (UPCité)

    المصدر: Publications of the Astronomical Society of Japan ; https://insu.hal.science/insu-04822418 ; Publications of the Astronomical Society of Japan, 2024, ⟨10.1093/pasj/psae091⟩

    Relation: info:eu-repo/semantics/altIdentifier/arxiv/2410.00104; ARXIV: 2410.00104; BIBCODE: 2024PASJ.tmp.94T

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    المساهمون: Department of Physics

    مصطلحات موضوعية: Astronomy, Space science

    وصف الملف: application/pdf

    Relation: We thank Kei Ito, Makoto Ando, and Suin Matsui for the fruitful discussion. We thank the anonymous referee for helpful feedback. This work is based on observations made with the NASA/ESA/CSA James Webb Space Telescope. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-03127 for JWST. These observations are associated with program IDs 1727 and 1837. Numerical computations were in part carried out on the iDark cluster, Kavli IPMU and the analysis servers at Center for Computational Astrophysics, National Astronomical Observatory of Japan. This work was made possible by utilizing the CANDIDE cluster at the Institut d'Astrophysique de Paris, which was funded through grants from the PNCG, CNES, DIM-ACAV, and the Cosmic Dawn Center and maintained by Stephane Rouberol.; http://hdl.handle.net/10138/588398; 001349412200001; 001374592800001