Multiwavelength catalog in the SEP field. II.

Multiwavelength catalog in the SEP field. II.J/ApJ/857/64ivo://CDS.VizieR/J/ApJ/857/64doi:10.26093/cds/vizier.18570064CDSBaronchelli I.Rodighiero G.Teplitz H.I.Scarlata C.M.,Franceschini A.Berta S.Barrufet L.Vaccari M.Bonato M.Ciesla L.,Zanella A.Carraro R.Mancini C.Puglisi A.Malkan M.Mei S.,Marchetti L.Colbert J.Sedgwick C.Serjeant S.Pearson C.,Radovich M.Grado A.Limatola L.Covone G.2018-10-05T13:37:43Z2018-10-05T12:34:14ZCDS support team

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

cds-question@unistra.frsurveysgalaxiesphotometryinfrared-photometrymillimeter-astronomysubmillimeter-astronomyultraviolet-photometryvisible-astronomysloan-photometryWide-band photometryFor a sample of star-forming galaxies in the redshift interval 0.15<z<0.3, we study how both the relative strength of the active galactic nucleus (AGN) infrared emission, compared to that due to the star formation (SF), and the numerical fraction of AGNs change as a function of the total stellar mass of the hosting galaxy group (M_group_^*^) between 10^10.25^ and 10^11.9^M_{sun}_. Using a multicomponent spectral energy distribution SED fitting analysis, we separate the contribution of stars, AGN torus, and star formation to the total emission at different wavelengths. This technique is applied to a new multiwavelength data set in the SIMES field (23 not-redundant photometric bands), spanning the wavelength range from the UV (GALEX) to the far-IR (Herschel) and including crucial AKARI and WISE mid-IR observations (4.5{mu}m<{lambda}<24{mu}m), where the black hole thermal emission is stronger. This new photometric catalog, which includes our best photo-z estimates, is released through the NASA/IPAC Infrared Science Archive (IRSA). Groups are identified through a friends-of-friends algorithm (~62% purity, ~51% completeness). We identified a total of 45 galaxies requiring an AGN emission component, 35 of which are in groups and 10 in the field. We find the black hole accretion rate (BHAR){prop.to}(M_group_^*^)^1.21+/-0.27^ and (BHAR/SFR) {\prop} (M_group_^*^)^1.04+/- 0.24^, while, in the same range of M_group_^*^, we do not observe any sensible change in the numerical fraction of AGNs. Our results indicate that the nuclear activity (i.e., the BHAR and the BHAR/SFR ratio) is enhanced when galaxies are located in more massive and richer groups.2018ApJ...857...64Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/857/64CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/223/1 : Multiwavelength catalog in the SEP field (Baronchelli+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/857/64https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/857/64http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/857/64https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/857/64https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/857/64http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/857/64GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/857/64/catalog (SEP multiwavelength photometric catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/857/64/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/857/64/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/857/64/catalog?GETtext/xml+votable180.050000true70.7803779831341-54.8582837548326050.0055555555555555565/8486 8487 8496 6/33935 33939 33941 33942 33943 33957 33968 33992-3.4771685954054845e-18 4.139003408266671e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/857/64?format=asciiMillimeterUVInfraredOpticaldefaultJ/ApJ/857/64/catalogSEP multiwavelength photometric catalogFW1? WISE W1 flux (FLUX_W1)mJyphot.mag;em.IR.3-4umdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDID number (ID)meta.id;meta.mainintRAJ2000Right Ascension (J2000) of IRAC 3.6 micron source (ra)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) of IRAC 3.6 micron source (dec)degpos.eq.dec;meta.mainindexedzph? Photometric redshift (PHOTO_Z)src.redshiftdoublenullablee_zph? Photometric redshift uncertainty (PHOTO_Z_ERR)stat.errordoublenullableF3.6? IRAC 3.6 micron total flux (FLUX_I1)mJyphot.mag;em.IR.3-4umdoublenullablee_F3.6? IRAC 3.6 micron total flux uncertainty (FLUXERR_I1)mJystat.errordoublenullableS/N? IRAC 3.6 micron signal to noise ratio (N_SIGMA)stat.snrdoublenullableF4.5? IRAC 4.5 micron total flux (FLUX_I2)mJyphot.mag;em.IR.4-8umdoublenullablee_F4.5? IRAC 4.5 micron total flux uncertainty (FLUXERR_I2)mJystat.errordoublenullableS/GSExtractor CLASS_STAR parameter at IRAC 3.6 micron (CLASS_STAR_I1)src.class.starGalaxydoubleamaj? Semi-major axis (A_I1)arcsecphys.angSize;srcdoublenullablebmin? Semi-minor axis (B_I1)arcsecphys.angSize.sminAxisdoublenullableRA24degC? Corrected RA of 24 micron sources (RA_24)degpos.eq.ranullableDE24degC? Corrected Dec of 24 micron sources (DEC_24)degpos.eq.decnullableRA24deg? Original RA of 24 micron sources (O_RA_24)degpos.eq.ranullableDE24deg? Original Dec of 24 micron sources (O_DEC_24)degpos.eq.decnullableF24? MIPS 24 micron flux (FLUX_24)mJyphot.flux.density;em.IR.15-30umdoublenullablee_F24? MIPS 24 micron flux uncertainty (FLUXERR_24)mJystat.errordoublenullableF70? MIPS 70 micron flux (FLUX_70)mJyphot.flux.density;em.IR.30-60umfloatnullablee_F70? MIPS 70 micron flux uncertainty (FLUXERR_70)mJystat.errordoublenullableRASdegC? Corrected RA of SPIRE sources (RA_SPIRE)degpos.eq.ranullableDESdegC? Corrected Dec of SPIRE sources (DEC_SPIRE)degpos.eq.decnullableRASdeg? Original RA of SPIRE sources (O_RA_SPIRE)degpos.eq.ranullableDESdeg? Original Dec of SPIRE sources (O_DEC_SPIRE)degpos.eq.decnullableF250? SPIRE 250 micron flux (FLUX_250)mJyphot.flux.density;em.mm.750-1500GHzdoublenullablee_F250? SPIRE 250 micron flux uncertainty (FLUXERR_250)mJystat.errordoublenullableF350? SPIRE 350 micron flux (FLUX_350)mJyphot.flux.density;em.mm.750-1500GHzdoublenullablee_F350? SPIRE 350 micron flux uncertainty (FLUXERR_350)mJystat.errordoublenullableF500? SPIRE 500 micron flux (FLUX_500)mJyphot.flux.density;em.mm.400-750GHzdoublenullablee_F500? SPIRE 500 micron flux uncertainty (FLUXERR_500)mJystat.errordoublenullableRAGdegC? Corrected RA of GALEX sources (RA_GALEX)degpos.eq.ranullableDEGdegC? Corrected Dec of GALEX sources (DEC_GALEX)degpos.eq.decnullableRAGdeg? Original RA of GALEX sources (O_RA_GALEX)degpos.eq.ranullableDEGdeg? Original Dec of GALEX sources (O_DEC_GALEX)degpos.eq.decnullableFFUV? GALEX FUV flux (FLUX_FUV_GALEX)mJyphot.flux.density;em.UV.100-200nmdoublenullablee_FFUV? GALEX FUV flux uncertainty (FLUXERR_FUV_GALEX)mJystat.errordoublenullableFNUV? GALEX NUV flux (FLUX_NUV_GALEX)mJyphot.flux.density;em.UV.200-300nmdoublenullablee_FNUV? GALEX NUV flux uncertainty (FLUXERR_NUV_GALEX)mJystat.errordoublenullableRAOdeg? average RA for optical sources (RA_OPT)degpos.eq.ranullableDEOdeg? average Dec for optical sources (DEC_OPT)degpos.eq.decnullableFuctio? CTIO u-band flux (FLUX_U)mJyphot.mag;em.opt.Udoublenullablee_Fuctio? CTIO u-band flux uncertainty (FLUXERR_U)mJystat.errordoublenullableFBctio? CTIO B-band flux (FLUX_B)mJyphot.flux.density;em.opt.Bdoublenullablee_FBctio? CTIO B-band flux uncertainty (FLUXERR_B)mJystat.errordoublenullableFVctio? CTIO V-band flux (FLUX_V)mJyphot.flux.density;em.opt.Vdoublenullablee_FVctio? CTIO V-band flux uncertainty (FLUXERR_V)mJystat.errordoublenullableFIctio? CTIO I-band flux (FLUX_I)mJyphot.flux.density;em.opt.Idoublenullablee_FIctio? CTIO I-band flux uncertainty (FLUXERR_I)mJystat.errordoublenullableFRcwfi? WFI Rc-band flux (FLUX_R_WFI)mJyphot.mag;em.opt.Rdoublenullablee_FRcwfi? WFI Rc-band flux uncertainty (FLUXERR_R_WFI)mJystat.errordoublenullableFgvst? VST g-band flux (FLUX_G_VST)mJyphot.mag;em.opt.Bdoublenullablee_Fgvst? VST g-band flux uncertainty (FLUXERR_G_VST)mJystat.errordoublenullableFivst? VST i-band flux (FLUX_I_VST)mJyphot.mag;em.opt.Idoublenullablee_Fivst? VST i-band flux uncertainty (FLUXERR_I_VST)mJystat.errordoublenullableFzvst? VST z-band flux (FLUX_Z_VST)mJyphot.mag;em.opt.Idoublenullablee_Fzvst? VST z-band flux uncertainty (FLUXERR_Z_VST)mJystat.errordoublenullableRAVdegC? Corrected RA of VISTA sources (RA_VISTA)degpos.eq.ranullableDEVdegC? Corrected Dec of VISTA sources (DEC_VISTA)degpos.eq.decnullableRAVdeg? Original RA of VISTA sources (O_RA_VISTA)degpos.eq.ranullableDEVdeg? Original Dec of VISTA sources (O_DEC_VISTA)degpos.eq.decnullableFJvista? VISTA J-band flux (FLUX_J_VISTA)mJyphot.flux.density;em.IR.Jdoublenullablee_FJvista? VISTA J-band flux uncertainty (FLUXERR_J_VISTA)mJystat.errordoublenullableFHvista? VISTA H-band flux (FLUX_H_VISTA)mJyphot.flux.density;em.IR.Hdoublenullablee_FHvista? VISTA H-band flux uncertainty (FLUXERR_H_VISTA)mJystat.errordoublenullableFKsvista? VISTA Ks-band flux (FLUX_KS_VISTA)mJyphot.mag;em.IR.Kdoublenullablee_FKsvista? VISTA Ks-band flux uncertainty (FLUXERR_KS_VISTA)mJystat.errordoublenullableRAWdegC? Corrected RA of WISE sources (RA_W)degpos.eq.ranullableDEWdegC? Corrected Dec of WISE sources (DEC_W)degpos.eq.decnullableRAWdeg? Original RA of WISE sources (O_RA_W)degpos.eq.ranullableDEWdeg? Original Dec of WISE sources (O_DEC_W)degpos.eq.decnullablee_FW1? WISE W1 flux uncertainty (FLUXERR_W1)mJystat.errordoublenullableFW2? WISE W2 flux (FLUX_W2)mJyphot.mag;em.IR.4-8umdoublenullablee_FW2? WISE W2 flux uncertainty (FLUXERR_W2)mJystat.errordoublenullableFW3? WISE W3 flux (FLUX_W3)mJyphot.flux.density;em.IR.8-15umdoublenullablee_FW3? WISE W3 flux uncertainty (FLUXERR_W3)mJystat.errordoublenullableFW4? WISE W4 flux (FLUX_W4)mJyphot.flux.density;em.IR.15-30umdoublenullablee_FW4? WISE W4 flux uncertainty (FLUXERR_W4)mJystat.errordoublenullableRAN3degC? Corrected RA of AKARI N3 sources (RA_N3)degpos.eq.ranullableDEN3degC? Corrected Dec of AKARI N3 sources (DEC_N3)degpos.eq.decnullableRAN3deg? Original RA of AKARI N3 sources (O_RA_N3)degpos.eq.ranullableDEN3deg? Original Dec of AKARI N3 sources (O_DEC_N3)degpos.eq.decnullableFN3? AKARI N3 flux (FLUX_N3)mJyphot.flux.density;em.IR.3-4umdoublenullablee_FN3? AKARI N3 flux uncertainty (FLUXERR_N3)mJystat.errordoublenullableRAN4degC? Corrected RA of AKARI N4 sources (RA_N4)degpos.eq.ranullableDEN4degC? Corrected Dec of AKARI N4 sources (DEC_N4)degpos.eq.decnullableRAN4deg? Original RA of AKARI N4 sources (O_RA_N4)degpos.eq.ranullableDEN4deg? Original Dec of AKARI N4 sources (O_DEC_N4)degpos.eq.decnullableFN4? AKARI N4 flux (FLUX_N4)mJyphot.flux.density;em.IR.3-4umdoublenullablee_FN4? AKARI N4 flux uncertainty (FLUXERR_N4)mJystat.errordoublenullableRAS7degC? Corrected RA of AKARI S7 sources (RA_S7)degpos.eq.ranullableDES7degC? Corrected Dec of AKARI S7 sources (DEC_S7)degpos.eq.decnullableRAS7deg? Original RA of AKARI S7 sources (O_RA_S7)degpos.eq.ranullableDES7deg? Original Dec of AKARI S7 sources (O_DEC_S7)degpos.eq.decnullableFS7? AKARI S7 flux (FLUX_S7)mJyphot.flux.density;em.IR.4-8umdoublenullablee_FS7? AKARI S7 flux uncertainty (FLUXERR_S7)mJystat.errordoublenullableRAS11degC? Corrected RA of AKARI S11 sources (RA_S11)degpos.eq.ranullableDES11degC? Corrected Dec of AKARI S11 sources (DEC_S11)degpos.eq.decnullableRAS11deg? Original RA of AKARI S11 sources (O_RA_S11)degpos.eq.ranullableDES11deg? Original Dec of AKARI S11 sources (O_DEC_S11)degpos.eq.decnullableFS11? AKARI S11 flux (FLUX_S11)mJyphot.flux.density;em.IR.8-15umdoublenullablee_FS11? AKARI S11 flux uncertainty (FLUXERR_S11)mJystat.errordoublenullableRAL15degC? Corrected RA of AKARI L15 sources (RA_L15)degpos.eq.ranullableDEL15degC? Corrected Dec of AKARI L15 sources (DEC_L15)degpos.eq.decnullableRAL15deg? Original RA of AKARI L15 sources (O_RA_L15)degpos.eq.ranullableDEL15deg? Original Dec of AKARI L15 sources (O_DEC_L15)degpos.eq.decnullableFL15? AKARI L15 flux (FLUX_L15)mJyphot.flux.density;em.IR.8-15umdoublenullablee_FL15? AKARI L15 flux uncertainty (FLUXERR_L15)mJystat.errordoublenullableRAL24degC? Corrected RA of AKARI L24 sources (RA_L24)degpos.eq.ranullableDEL24degC? Corrected Dec of AKARI L24 sources (DEC_L24)degpos.eq.decnullableRAL24deg? Original RA of AKARI L24 sources (O_RA_L24)degpos.eq.ranullableDEL24deg? Original Dec of AKARI L24 sources (O_DEC_L24)degpos.eq.decnullableFL24? AKARI L24 flux (FLUX_L24)mJyphot.flux.density;em.IR.15-30umdoublenullablee_FL24? AKARI L24 flux uncertainty (FLUXERR_L24)mJystat.errordoublenullableP1? SPIRE-MIPS reliability indicator (P1)stat.fit.goodnessdoublenullableNM-S[0/3]? Number of MIPS counterparts for SPIRE source (N_MIPS_SPIRE)meta.numberintnullableP2? MIPS-IRAC reliability indicator (P2)stat.fit.goodnessdoublenullableNI-M[1/2]? Number of IRAC counterparts for MIPS source (N_IRAC_MIPS)meta.numberintnullableP3? SPIRE-IRAC reliability indicator (P3)stat.fit.goodnessdoublenullableNI-S[1/5]? Number of IRAC counterparts for SPIRE source (N_IRAC_SPIRE)meta.numberintnullableSigmaIRAC 3.6 micron sky sigma (SIGMA)mJystat.stdevdoubleCovAverage coverage (COVERAGE)phys.areadoubleF3.6a1? IRAC 3.6 micron aperture flux - 4.8" (AP1_FLUX_I1)mJyphot.mag;em.IR.3-4umdoublenullablee_F3.6a1? uncertainty in AP1_FLUX_I1 (AP1_FLUXERR_I1)mJystat.errordoublenullableF3.6a2? IRAC 3.6 micron aperture flux - 7.2" (AP2_FLUX_I1)mJyphot.mag;em.IR.3-4umdoublenullablee_F3.6a2? uncertainty in AP2_FLUX_I1 (AP2_FLUXERR_I1)mJystat.errordoublenullableF3.6a3? IRAC 3.6 micron aperture flux - 12" (AP3_FLUX_I1)mJyphot.mag;em.IR.3-4umdoublenullablee_F3.6a3uncertainty in AP3_FLUX_I1 (AP3_FLUXERR_I1)mJystat.errordoubleF4.5a1? IRAC 4.5 micron aperture flux - 4.8" (AP1_FLUX_I2)mJyphot.mag;em.IR.4-8umdoublenullablee_F4.5a1? uncertainty in AP1_FLUX_I2 (AP1_FLUXERR_I2)mJystat.errordoublenullableF4.5a2? IRAC 4.5 micron aperture flux - 7.2" (AP2_FLUX_I2)mJyphot.mag;em.IR.4-8umdoublenullablee_F4.5a2? uncertainty in AP2_FLUX_I2 (AP2_FLUXERR_I2)mJystat.errordoublenullableF4.5a3? IRAC 4.5 micron aperture flux - 12" (AP3_FLUX_I2)mJyphot.mag;em.IR.4-8umdoublenullablee_F4.5a3? uncertainty in AP3_FLUX_I2 (AP3_FLUXERR_I2)mJystat.errordoublenullable