J/MNRAS/480/1022ivo://CDS.VizieR/J/MNRAS/480/1022doi:10.26093/cds/vizier.74801022CDSYang G.Brandt W.N.Darvish B.Chen C.-T.J.Vito F.Alexander D.M.,Bauer F.E.Trump J.R.2024-08-18T20:20:56Z2022-05-17T13:50:52ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fractive-galactic-nucleiblack-holesgalaxiesx-ray-sourcesIt is well known that environment affects galaxy evolution, which is broadly related to supermassive black hole (SMBH) growth. We investigate whether SMBH evolution also depends on host-galaxy local (sub-Mpc) and global (~1-10Mpc) environment. We construct the surface-density field (local environment) and cosmic web (global environment) in the Cosmic Evolution Survey (COSMOS) field at z=0.3-3.0. The environments in COSMOS range from the field to clusters (M_halo_~<1014M_{sun}_), covering the environments where ~99 per cent of galaxies in the Universe reside. We measure sample-averaged SMBH accretion rate ({mean}BHAR) from X-ray observations, and study its dependence on overdensity and cosmic-web environment at different redshifts while controlling for galaxy stellar mass (M_*_). Our results show that {mean}BHAR does not significantly depend on overdensity or cosmic-web environment once M_*_ is controlled, indicating that environment-related physical mechanisms (e.g. tidal interaction and ram-pressure stripping) might not significantly affect SMBH growth. We find that {mean}BBHAR is strongly related to host-galaxy M_*_, regardless of environment.2018MNRAS.480.1022Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/480/1022CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/480/1022https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/480/1022http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/480/1022https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/480/1022https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/480/1022http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/480/1022GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/480/1022/table2 (Source catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/480/1022/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/480/1022/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/480/1022/table2?GETtext/xml+votable180.050000true149.411496112.7123150.0055555555555555565/6814 6/27245 27247 273447.952274030004205e-20 1.0188844282367877e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/480/1022?format=asciiX-raydefaultJ/MNRAS/480/1022/table2Source catalogueWeb[0/2] Cosmic-web environment (0:cluster; 1:filament; 2:field) (4)meta.codeintlogLx? X-ray luminosity (rest-frame 2-10keV) (5)log(1e-07W)phys.luminosity;em.X-raydoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right Ascension (J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000)degpos.eq.dec;meta.mainindexedKsmagKs AB magnitude from the COSMOS2015 catalogue (Laigle et al. 2016ApJS..224...24L, Cat. J/ApJS/224/24)magphot.mag;em.IR.KfloatzRedshift (1)src.redshiftdoublee_zRedshift 1{sigma} lower limit (2)stat.error;src.redshiftdoubleE_zRedshift 1{sigma} upper limit (2)stat.error;stat.maxdoublelogMstarStellar masslog(solMass)phys.massdoubleTypegal[0/1] Galaxy type (0:quiescent; 1:star-forming)meta.codeintlog(1+d)Overdensity (3)arith.zpdouble