يعرض 21 - 30 نتائج من 577 نتيجة بحث عن '"HALO-MASS"', وقت الاستعلام: 0.89s تنقيح النتائج
  1. 21
    دورية أكاديمية

    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), Institut Lagrange de Paris

    المصدر: ISSN: 1550-7998.

    العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/1910.07553; hal-02382042; https://hal.science/hal-02382042Test; https://hal.science/hal-02382042/documentTest; https://hal.science/hal-02382042/file/zhang2020.pdfTest; ARXIV: 1910.07553; INSPIRE: 1759557

  2. 22
    رسالة جامعية
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  5. 25
    دورية أكاديمية

    المساهمون: Niels Bohr Institute Copenhagen (NBI), Faculty of Science Copenhagen, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Kavli Institute for Cosmological Physics Chicago (KICP), University of Chicago, Enrico Fermi Institute, Instituto de Física Teórica UAM/CSIC (IFT), Consejo Superior de Investigaciones Cientificas España = Spanish National Research Council Spain (CSIC)-Universidad Autónoma de Madrid (UAM), Cosmologie et Gravitation, Laboratoire de physique de l'ENS - ENS Paris (LPENS), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Département de Physique de l'ENS-PSL, École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Département de Physique de l'ENS-PSL, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), European Project: 847523,INTERACTIONS

    المصدر: ISSN: 0031-9007.

    العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2207.06317; info:eu-repo/grantAgreement//847523/EU/NBIA INTERACTIONS POSTDOCTORAL PROGRAMME/INTERACTIONS; hal-03726399; https://hal.science/hal-03726399Test; ARXIV: 2207.06317; INSPIRE: 2111438

  6. 26
    دورية أكاديمية

    المساهمون: Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)

    المصدر: ISSN: 0035-8711.

    العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/1907.03161; hal-02266601; https://hal.science/hal-02266601Test; https://hal.science/hal-02266601/documentTest; https://hal.science/hal-02266601/file/stz1882.pdfTest; ARXIV: 1907.03161; INSPIRE: 1742842

  7. 27
    دورية أكاديمية

    المساهمون: Department of Physics, Helsinki Institute of Physics, Particle Physics and Astrophysics

    وصف الملف: application/pdf

    العلاقة: This work has been supported by grants from the Finnish Academy of Science to the University of Helsinki and the Euclid project, decision numbers 266918 and 1295113. GG wishes to thank Mr. Donald Smart for very useful comments. ST acknowledges support from the ERC Consolidator Grant funding scheme (project Context, grant no. 648179). The Cosmic Dawn Center is funded by the Danish National Research Foundation. We used data of the Millennium simulation from the web application providing online access, constructed as activities of the German Astrophysics Virtual Observatory.; Gozaliasl , G , Finoguenov , A , Tanaka , M , Dolag , K , Montanari , F , Kirkpatrick , C C , Vardoulaki , E , Khosroshahi , H G , Salvato , M , Laigle , C , McCracken , H J , Ilbert , O , Cappelluti , N , Daddi , E , Hasinger , G , Capak , P , Scoville , N Z , Toft , S , Civano , F , Griffiths , R E , Balogh , M , Li , Y , Ahoranta , J , Mei , S , Iovino , A , Henriques , B M B & Erfanianfar , G 2019 , ' Chandra centres for COSMOS X-ray galaxy groups : differences in stellar properties between central dominant and offset brightest group galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 483 , no. 3 , pp. 3545-3565 . https://doi.org/10.1093/mnras/sty3203Test; ORCID: /0000-0003-0741-1382/work/56406150; 1755e25f-a0c7-4b4b-9ae6-12a8115e80d4; http://hdl.handle.net/10138/300793Test; 000462280000044

  8. 28
    دورية أكاديمية

    المساهمون: Department of Physics, Helsinki Institute of Physics

    وصف الملف: application/pdf

    العلاقة: EDF was supported by the Oxford physics summer student program when completing this work. CL is supported by a Beecroft Fellowship. AS and JD acknowledge funding support from Adrian Beecroft and the STFC. CL would like to thank Oliver Hahn for very relevant suggestions, Yiqing Liu and Hyunmi Song for useful discussions and advices, and the Korean Astronomy and Space science Institute for hospitality when most of this work was finalized. CP thanks Sandrine Codis for advices and the Royal Observatory in Edinburgh for hospitality when this work was initiated. This work relied on the HPC resources of CINES (Jade) under the allocation 2013047012 and c2014047012 made by GENCI and on the HORIZON and CANDIDE clusters hosted by Institut d'Astrophysique de Paris. We warmly thank S. Rouberol for running the cluster on which the simulation was post-processed. This research is also partly supported by the Centre National d'Etudes Spatiales (CNES) and by the National Science Foundation under Grant No. NSF PHY-1748958. This work is based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO programme ID 179.A-2005 and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. We thank D. Munro for freely distributing his YORICK programming language and opengl interface (available at http://yorick.sourceforge.netTest/).; Ford , E D , Laigle , C , Gozaliasl , G , Pichon , C , Devriendt , J , Slyz , A , Arnouts , S , Dubois , Y , Finoguenov , A , Griffiths , R , Kraljic , K , Pan , H , Peirani , S & Sarron , F 2019 , ' Group connectivity in COSMOS : a tracer of mass assembly history ' , Monthly Notices of the Royal Astronomical Society , vol. 489 , no. 4 , pp. 5695-5708 . https://doi.org/10.1093/mnras/stz2490Test; 67ee0261-2a4d-4090-8e99-e82c19611b48; http://hdl.handle.net/10138/308470Test; 000489302400090

  9. 29
    دورية أكاديمية
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    المساهمون: HEP, INSPIRE, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

    المصدر: Monthly Notices of the Royal Astronomical Society
    Monthly Notices of the Royal Astronomical Society, 2023, Vol.520(1), pp.702-721 [Peer Reviewed Journal]
    Monthly Notices of the Royal Astronomical Society, 2023, 520 (1), pp.702-721. ⟨10.1093/mnras/stad140⟩

    وصف الملف: application/pdf