يعرض 1 - 10 نتائج من 61 نتيجة بحث عن '"mass calibration"', وقت الاستعلام: 0.90s تنقيح النتائج
  1. 1
    دورية أكاديمية
  2. 2
    دورية أكاديمية
  3. 3
    دورية أكاديمية
  4. 4
    دورية أكاديمية
  5. 5
    دورية أكاديمية

    المساهمون: Helsinki Institute of Physics, Department of Physics

    وصف الملف: application/pdf

    العلاقة: The authors wish to acknowledge CSC -IT Center for Science, Finland, for computational resources. We acknowledge grants of computer capacity from the Finnish Grid and Cloud Infrastructure (persistent identifier urn:nbn:fi:research-infras-2016072533). Based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofisica de Canarias. The authors gratefully acknowledge the Gauss Centre for Supercomputing e.V. (www.gauss-centre.eu) and the Partnership for Advanced Supercomputing in Europe (PRACE, www.prace-ri.eu) for funding the MultiDark simulation project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre (LRZ, www.lrz.de).Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy O ffice of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University ofWashington, University of Wisconsin, Vanderbilt University, and Yale University.; Lindholm , V , Finoguenov , A , Comparat , J , Kirkpatrick , C C , Rykoff , E , Clerc , N , Collins , C , Damsted , S , Chitham , J I & Padilla , N 2021 , ' Clustering of CODEX clusters ' , Astronomy & Astrophysics , vol. 646 , A8 . https://doi.org/10.1051/0004-6361/202038807Test; ORCID: /0000-0003-2317-5471/work/90906824; ORCID: /0000-0003-2097-0330/work/127007313; 85100182847; 3827ce0c-cbc8-483d-b248-42623b0b44b7; http://hdl.handle.net/10138/328220Test; 000615917300002

  6. 6
  7. 7
    دورية أكاديمية

    المساهمون: Department of Physics, Helsinki Institute of Physics

    وصف الملف: application/pdf

    العلاقة: The authors thank the referee for their comments which increased the quality of this paper. The authors thank E. Rykoff for providing the data of Fig. 5. Some of the results in this paper have been derived using the HEALPIX (Gorski et al. 2005) package, the MATPLOTLIB package (Hunter 2007), and ASTROPY,7 (Astropy Collaboration 2013; Price-Whelan et al. 2018). This research has made use of 'Aladin sky atlas' developed at CDS, Strasbourg Observatory, France (Bonnarel et al. 2000; Boch & Fernique 2014). It has made use of TOPCAT (Taylor 2005). Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This work was supported by CNES. AF, CK, and JIC acknowledge travel support from the Finnish Centre for Astronomy with ESO (FINCA). NC acknowledges travel support from the Institut Francais de Finlande, the Embassy of France in Finland, the French Ministry of Higher Education, Research and Innovation, the Finnish Society of Sciences and Letters and the Finnish Academy of Science and Letters. CK and NC acknowledge this research was supported by the DFG cluster of excellence 'Origin and Structure of the Universe' (www.universe-cluster.de).AS is supported by the ERCStG 'ClustersXCosmo' grant agreement 716762, and by the FAREMIUR grant 'ClustersXEuclid' R165SBKTMA. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSSIV acknowledges support and resources from the Center for HighPerformance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut f ur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, NewMexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.; Clerc , N , Kirkpatrick , C C , Finoguenov , A , Capasso , R , Comparat , J , Damsted , S , Furnell , K , Kukkola , A E , Chitham , J I , Merloni , A , Salvato , M , Gueguen , A , Dwelly , T , Collins , C , Saro , A , Erfanianfar , G , Schneider , D P , Brownstein , J , Mamon , G A , Padilla , N , Jullo , E & Bizyaev , D 2020 , ' SPIDERS : overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release ' , Monthly Notices of the Royal Astronomical Society , vol. 497 , no. 3 , pp. 3976-3992 . https://doi.org/10.1093/mnras/staa2066Test; ORCID: /0000-0003-2097-0330/work/127007296; http://hdl.handle.net/10138/320999Test; 64292c76-4f88-4bd6-8fc2-268979f0ee1e; 000577137200104

  8. 8
    دورية أكاديمية

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

    وصف الملف: application/pdf

    العلاقة: We thank the referee for their comments which improved the quality of this paper. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the US Department of Energy O ffice of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org.SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University ofWashington, University ofWisconsin, Vanderbilt University, and Yale University. Based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofisica de Canarias.; Finoguenov , A , Rykoff , E , Clerc , N , Costanzi , M , Hagstotz , S , Chitham , J I , Kiiveri , K , Kirkpatrick , C C , Capasso , R , Comparat , J , Damsted , S , Dupke , R , Erfanianfar , G , Henry , J P , Kaefer , F , Kneib , J -P , Lindholm , V , Rozo , E , van Waerbeke , L & Weller , J 2020 , ' CODEX clusters : Survey, catalog, and cosmology of the X-ray luminosity function ' , Astronomy & Astrophysics , vol. 638 , A114 . https://doi.org/10.1051/0004-6361/201937283Test; ORCID: /0000-0003-2317-5471/work/79180562; ORCID: /0000-0002-3711-3346/work/79180654; ORCID: /0000-0003-2097-0330/work/127007298; b4ba4ee1-b335-4f94-80b0-ca6184517176; http://hdl.handle.net/10138/320861Test; 000545014600003

  9. 9
    دورية أكاديمية

    المساهمون: Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), ANR-11-IDEX-0001,Amidex,INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE(2011), ANR-11-LABX-0060,OCEVU,Origines, Constituants et EVolution de l'Univers(2011)

    المصدر: ISSN: 0004-6361.

    العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/1908.00163; hal-02283538; https://hal.science/hal-02283538Test; https://hal.science/hal-02283538/documentTest; https://hal.science/hal-02283538/file/aa36423-19.pdfTest; ARXIV: 1908.00163; INSPIRE: 1747612

  10. 10