يعرض 1 - 20 نتائج من 2,095 نتيجة بحث عن '"Rich, Michael"', وقت الاستعلام: 0.48s تنقيح النتائج
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    المصدر: Circulation. 147(3)

    وصف الملف: application/pdf

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    Periodical

    المؤلفون: Rich, Michael

    المصدر: New Zealand population review, May 2000; v.26 n.1:p.93-98

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    المصدر: ISSN: 0010-440X ; Comprehensive psychiatry, vol. 133 (2024) 152500.

    Relation: info:eu-repo/semantics/altIdentifier/pmid/38761770; info:eu-repo/grantAgreement/EC/H2020/810580/EU/The self-teaching brain/BrainPlay; https://archive-ouverte.unige.ch/unige:177185; unige:177185

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    المساهمون: Department of Physics

    مصطلحات موضوعية: Astronomy, Space science

    وصف الملف: application/pdf

    Relation: We thank the anonymous referee for their comments that improved the initial version of this study. F.G. thanks the Department of Astronomy of the University of Texas at Austin for the hospitality during the writing of this Letter. F.G. and C.M.C. thank Zhaoxuan Liu and Seiji Fujimoto for the careful reading of a first draft of this Letter. F.G. and M.T. acknowledge the support from grant PRIN MIUR 2017-20173ML3WW_001. \u201COpening the ALMA window on the cosmic evolution of gas, stars, and supermassive black holes.\u201D Support for this work was provided by NASA through grant JWST-GO-01727 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. C.M.C., H.A., M.F., J.M., and A.S.L. acknowledge support from the National Science Foundation through grants AST-2307006, AST-2009577, and the UT Austin College of Natural Sciences for support. C.M.C. also acknowledges support from the Research Corporation for Science Advancement from a 2019 Cottrell Scholar Award sponsored by IF/THEN, an initiative of the Lyda Hill Philanthropies. J.R. was supported by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). D.L. acknowledges the support from the Strategic Priority Research Program of the Chinese Academy of Sciences, grant No. XDB0800401. This work used the CANDIDE computer system at the IAP supported by grants from the PNCG, CNES, and the DIM-ACAV and maintained by S. Rouberol. The JWST data presented in this Letter were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute. The specific observations analyzed can be accessed via doi:10.17909/ahg3-e826.; http://hdl.handle.net/10138/586709; 85204238142; 001312307400001

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