المؤلفون: Zhijie (Jay) Xu

مصطلحات موضوعية: cosmology, dark matter, turbulence, astrophysics, energy cascade, mass cascade, correlation functions, supermassive black holes, SMBH-bulge coevolution, Maximum entropy, MOND, scaling laws, halo mass function, halo density profile

العلاقة: https://zenodo.org/record/7508310Test; https://doi.org/10.5281/zenodo.7508310Test; oai:zenodo.org:7508310

الإتاحة: https://doi.org/10.5281/zenodo.7508310Test
https://doi.org/10.5281/zenodo.6569901Test
https://doi.org/10.5281/zenodo.6569898Test
https://doi.org/10.5281/zenodo.6541230Test
https://doi.org/10.5281/zenodo.6586212Test
https://doi.org/10.48550/arXiv.2109.09985Test
https://doi.org/10.48550/arXiv.2109.12244Test
https://doi.org/10.48550/arXiv.2110.03126Test
https://doi.org/10.48550/arXiv.2110.05784Test
https://doi.org/10.48550/arXiv.2110.09676Test

المؤلفون: von Braun-Bates, F.

المساهمون: Ferreira, Pedro, Devriendt, Julien

مصطلحات موضوعية: 523.1, Cosmology, Astrophysics, halo mass function, quasi-static approximation, extended gravity

الوصول الحر: https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.748827Test

المؤلفون: Chitham, J. Ider, Comparat, J., Finoguenov, A., Clerc, N., Kirkpatrick, C. C., Damsted, S., Kukkola, A., Capasso, R., Nandra, K., Merloni, A., Bulbul, E., Rykoff, E. S., Schneider, D. P., Brownstein, J. R.

المساهمون: Department of Physics

مصطلحات موضوعية: cosmological parameters, X-rays: galaxies: clusters, HALO MASS FUNCTION, BARYON ACOUSTIC-OSCILLATIONS, DARK ENERGY, INTRACLUSTER LIGHT, SCALING RELATIONS, REDSHIFT 0.8, SAMPLE, MAXBCG, CALIBRATION, ROSAT, 115 Astronomy, Space science

وصف الملف: application/pdf

العلاقة: This paper represents an effort by both the SDSS-III and SDSS-IV collaborations. Funding for SDSS-III was 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 SloanDigital 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. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site iswww.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 Astrof ' isica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), MaxPlanck-Institut fur Astronomie (MPIA Heidelberg), Max-PlanckInstitut fur Astrophysik (MPA Garching), Max-Planck-Institut f ur Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observat ' ario Nacional/MCTI, The Ohio StateUniversity, Pennsylvania State University, ShanghaiAstronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut ' onoma de M ' exico, University of Arizona, University of Colorado Boulder, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.; Chitham , J I , Comparat , J , Finoguenov , A , Clerc , N , Kirkpatrick , C C , Damsted , S , Kukkola , A , Capasso , R , Nandra , K , Merloni , A , Bulbul , E , Rykoff , E S , Schneider , D P & Brownstein , J R 2020 , ' Cosmological constraints from CODEX galaxy clusters spectroscopically confirmed by SDSS-IV/SPIDERS DR16 ' , Monthly Notices of the Royal Astronomical Society , vol. 499 , no. 4 , pp. 4768-4784 . https://doi.org/10.1093/mnras/staa3044Test; ORCID: /0000-0003-2097-0330/work/127007292; b7c0baad-3f68-48ed-8da4-364354194d4e; http://hdl.handle.net/10138/324594Test; 000599131700013

الإتاحة: http://hdl.handle.net/10138/324594Test

المؤلفون: Hofmann, F., Sanders, J. S., Clerc, N., Nandra, K., Ridl, J., Dennerl, K., Ramos-Ceja, M., Finoguenov, A., Reiprich, T. H.

المساهمون: Department of Physics

مصطلحات موضوعية: galaxies: clusters: general, X-rays: galaxies: clusters, cosmological parameters, HALO MASS FUNCTION, X-RAY, GALAXY CLUSTERS, SPECTRA, CHANDRA, SEARCH, SAMPLE, 115 Astronomy, Space science

وصف الملف: application/pdf

العلاقة: We thank the anonymous referee for very constructive comments that helped to improve the clarity of the paper. We thank J.J. Mohr for helpful discussions. This research has made use of data obtained from the Chandra Data Archive and the Chandra Source Catalog, and software provided by the Chandra X-ray Center (CXC) in the application packages CIAO, ChIPS, and Sherpa. This research has made use of NASA's Astrophysics Data System. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. This research has made use of SAOImage DS9, developed by the Smith-sonian Astrophysical Observatory. This research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. THR acknowledges support by the German Research Association (DFG) through grant RE 1462/6 and the Transregio 33 "The Dark Universe" sub-project B18.; Hofmann , F , Sanders , J S , Clerc , N , Nandra , K , Ridl , J , Dennerl , K , Ramos-Ceja , M , Finoguenov , A & Reiprich , T H 2017 , ' eROSITA cluster cosmology forecasts : Cluster temperature substructure bias ' , Astronomy & Astrophysics , vol. 606 , 118 . https://doi.org/10.1051/0004-6361/201730742Test; 85032293099; bb983112-6581-46b4-b2a8-6e7d1b9f5e9f; http://hdl.handle.net/10138/313153Test; 000413564000007

الإتاحة: http://hdl.handle.net/10138/313153Test

المؤلفون: Vogelsberger M., Marinacci F., Torrey P., Puchwein E.

المساهمون: Vogelsberger M., Marinacci F., Torrey P., Puchwein E.

مصطلحات موضوعية: COLD DARK-MATTER, SMOOTHED PARTICLE HYDRODYNAMICS, ADAPTIVE MESH REFINEMENT, HALO MASS FUNCTION, FEEDBACK-DOMINATED GALAXIES, SUPERMASSIVE BLACK-HOLES, LARGE-SCALE STRUCTURE, CONCENTRATION-REDSHIFT RELATION, SPH CHEMODYNAMICAL SIMULATION, RT RADIATION HYDRODYNAMICS

وصف الملف: STAMPA

العلاقة: info:eu-repo/semantics/altIdentifier/wos/WOS:000542196200010; volume:2; issue:1; firstpage:42; lastpage:66; numberofpages:25; journal:NATURE REVIEWS PHYSICS; http://hdl.handle.net/11585/799379Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85082442717; https://www.nature.com/articles/s42254-019-0127-2Test

الإتاحة: https://doi.org/10.1038/s42254-019-0127-2Test
http://hdl.handle.net/11585/799379Test
https://www.nature.com/articles/s42254-019-0127-2Test

المؤلفون: Xu, Zhijie (Jay)

مصطلحات موضوعية: cosmology, dark matter, turbulence, simulation, astronomy, astrophysics, dark matter halo, correlation, statistical analysis, self-gravitating, collisionless, N body, halo mass function, dark matter flow, mass cascade

العلاقة: https://zenodo.org/record/6639536Test; https://doi.org/10.48550/arXiv.2109.09985Test; oai:zenodo.org:6639536

الإتاحة: https://doi.org/10.48550/arXiv.2109.09985Test
https://doi.org/10.5281/zenodo.6569901Test
https://doi.org/10.5281/zenodo.6569898Test
https://doi.org/10.5281/zenodo.6541230Test
https://doi.org/10.5281/zenodo.6586212Test
https://doi.org/10.48550/arXiv.2109.12244Test
https://doi.org/10.48550/arXiv.2110.03126Test
https://doi.org/10.48550/arXiv.2110.05784Test
https://doi.org/10.48550/arXiv.2110.09676Test
https://doi.org/10.48550/arXiv.2110.13885Test

المؤلفون: Xu, Zhijie (Jay)

مصطلحات موضوعية: cosmology, dark matter, turbulence, simulation, N body, astronomy, astrophysics, dark matter halo, correlation, statistical analysis, self-gravitating, collisionless, Halo mass function, maximum entropy distributions

العلاقة: https://zenodo.org/record/6640325Test; https://doi.org/10.48550/arXiv.2110.09676Test; oai:zenodo.org:6640325

الإتاحة: https://doi.org/10.48550/arXiv.2110.09676Test
https://doi.org/10.5281/zenodo.6569898Test
https://doi.org/10.5281/zenodo.6541230Test
https://doi.org/10.5281/zenodo.6586212Test
https://doi.org/10.5281/zenodo.6569901Test
https://doi.org/10.48550/arXiv.2109.12244Test
https://doi.org/10.48550/arXiv.2110.03126Test
https://doi.org/10.48550/arXiv.2110.05784Test
https://doi.org/10.48550/arXiv.2109.09985Test
https://doi.org/10.48550/arXiv.2110.13885Test

المؤلفون: Taha Dawoodbhoy, Tanja Rindler-Daller, Paul R. Shapiro

المصدر: Monthly Notices of the Royal Astronomical Society. 509:145-173

مصطلحات موضوعية: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cold dark matter, Structure formation, 010308 nuclear & particles physics, Halo mass function, Scalar field dark matter, FOS: Physical sciences, Astronomy and Astrophysics, Context (language use), Astrophysics::Cosmology and Extragalactic Astrophysics, Radius, Lambda, Astrophysics - Astrophysics of Galaxies, 01 natural sciences, High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), 0103 physical sciences, Halo, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Mathematical physics

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e29647aa16d913f53bbf91516a4a9849Test
https://doi.org/10.1093/mnras/stab2884Test

المؤلفون: Jesús Zavala, Francis-Yan Cyr-Racine, Sebastian Bohr, Mark Vogelsberger

المصدر: Monthly Notices of the Royal Astronomical Society. 506:128-138

مصطلحات موضوعية: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cold dark matter, Mass distribution, 010308 nuclear & particles physics, Halo mass function, Dark matter, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Redshift, Space and Planetary Science, 0103 physical sciences, Warm dark matter, Baryon acoustic oscillations, Halo, 010303 astronomy & astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b0b6d61b307608fdcd2b9733eae93b5Test
https://doi.org/10.1093/mnras/stab1758Test

المؤلفون: Timothée Schaeffer, Aurel Schneider

المساهمون: University of Zurich

المصدر: Monthly Notices of the Royal Astronomical Society. 504:3773-3786

مصطلحات موضوعية: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 530 Physics, 010308 nuclear & particles physics, Matter power spectrum, Dark matter, Halo mass function, FOS: Physical sciences, Spectral density, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Redshift, Standard Model, Amplitude, 13. Climate action, Space and Planetary Science, 10231 Institute for Computational Science, 0103 physical sciences, Baryon acoustic oscillations, 010303 astronomy & astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics

وصف الملف: 2101.12229.pdf - application/pdf

الوصول الحر: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d516da3d5a9afe0f2aadbcdad295fdbTest
https://doi.org/10.1093/mnras/stab1116Test