{"id":"W4415155295","doi":"10.1051/0004-6361/202450190","title":"The X-ray statistical properties of dust-obscured galaxies detected by eROSITA","year":2025,"lang":"en","type":"article","venue":"Astronomy and Astrophysics","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Planetary Science Division; High Energy Physics; Division of Astronomical Sciences; Russian Academy of Sciences; Eberhard Karls Universität Tübingen; Science and Technology Facilities Council; Leibniz-Gemeinschaft; Science Mission Directorate; Smithsonian Astrophysical Observatory; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Leibniz-Institut für Astrophysik Potsdam; Eötvös Loránd Tudományegyetem; Cabinet Office, Government of Japan; University of Illinois at Urbana-Champaign; Fermilab; Max-Planck-Institut für Astronomie; Rheinische Friedrich-Wilhelms-Universität Bonn; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; Academia Sinica; Office of Science; Integrated Electronics Engineering Center, Binghamton University; Japan Society for the Promotion of Science; Queen's University; University of Edinburgh; Ministry of Education, Culture, Sports, Science and Technology; National Central University; Space Telescope Science Institute; University of Sussex; University of Nottingham; National Aeronautics and Space Administration; University College London; Queen's University Belfast; University of Cambridge; University of Chicago; National Energy Research Scientific Computing Center; University of California, Los Angeles; University of Portsmouth; Princeton University; Johns Hopkins University; Toray Science Foundation; High Energy Accelerator Research Organization; Ohio State University; Japan Science and Technology Agency; Universität Hamburg; California Institute of Technology; Smithsonian Institution; U.S. Department of Energy; National Science Foundation; University of Michigan; Financiadora de Estudos e Projetos; University of Pennsylvania; Durham University","keywords":"Supermassive black hole; Galaxy; Active galactic nucleus; Quasar; Statistical analysis; Galactic nuclei; Virgo Cluster","routes":{"ca_aff":false,"ca_fund":true,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":true},"retraction":null,"screen":{"n_in":0,"stratum":"fund_new","weight":1678.9,"opus":{"tier":"OUT","genre":"empirical","about_ca":false,"confidence":"high","reason":"Astronomy study of the X-ray properties of dust-obscured galaxies in eROSITA data."},"gpt":{"tier":"OUT","genre":"empirical","about_ca":false,"confidence":"high","reason":"It studies the X-ray properties of dust-obscured galaxies, not research itself."},"grok":{"tier":"OUT","genre":"empirical","about_ca":false,"confidence":"high","reason":"Astronomy study of X-ray properties of dust-obscured galaxies; 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