J/A+A/574/A49ivo://CDS.VizieR/J/A+A/574/A49doi:10.26093/cds/vizier.35740049CDSAntonucci M.Talavera A.Vagnetti F.Trevese D.Comastri A.,Paolillo M.Ranalli P.Vignali C.2017-07-11T13:09:14Z2015-01-22T09:00:39ZCDS support team

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

cds-question@unistra.frsurveysgalaxiescatalogsactive-galactic-nucleiultraviolet-photometryultraviolet-astronomyx-ray-sourcesThe XMM-Newton X-ray observatory has performed repeated observations of the CDFS in 33 epochs (2001-2010) through the XMM-CDFS Deep Survey. During the X-ray observations, XMM-OM targeted the central 17x17arcmin^2^ region of the X-ray field of view, providing simultaneous optical/UV coverage of the CDFS. The resulting set of data can be taken into account to build an XMM-OM catalogue of the CDFS, filling the UV spectral coverage between the optical surveys and GALEX observations. We present the UV catalogue of the XMM-CDFS Deep Survey. Its main purpose is to provide complementary UV average photometric measurements of known optical/UV sources in the CDFS, taking advantage of the unique characteristics of the survey. The data reduction is intended also to improve the standard source detection on individual observations, by cataloguing faint sources through the stacking of their exposure images. We reprocessed the XMM-OM data of the survey and we stacked the exposures from consecutive observations using the standard SAS tools to process the data obtained during single observations. Average measurements of detections with SAS good quality flags from individual observations and from stacked images have been joined to compile the catalogue. Sources have been validated through the cross-identification within the EIS and COMBO-17 surveys. Photometric data of 1129 CDFS sources are provided into the catalogue, and optical/UV/X-ray photometric and spectroscopic information from other surveys are also included. The stacking extends the detection limits by ~1 mag in the three UV bands, contributing 30% of the catalogued UV sources. The comparison with the available measurements in similar spectral bands confirms the validity of the XMM-OM calibration. The combined COMBO-17/X-ray classification of the "intermediate" sources (e.g. optically diluted and/or X-ray absorbed AGN) is also discussed.2015A&A...574A..49Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/574/A49CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/xmm : XMM-Newton Observation Log (XMM-Newton SOC, 2012)III/250 : The VIMOS VLT deep survey (VVDS-DEEP) (Le Fevre+ 2005)J/ApJS/155/271 : CDF-South: Optical spectroscopy (Szokoly+, 2004)J/A+A/437/883 : K20 survey: spectroscopic catalogue (Mignoli+, 2005)J/ApJS/191/124 : ECDF-S X-ray sources optical spectroscopy (Silverman+, 2010)J/A+A/512/A12 : VLT/VIMOS spectroscopy in GOODS-South field (Balestra+ 2010)J/A+A/478/83 : GOODS-South Field VLT/FORS2 redshifts. III. (Vanzella+ 2008)J/MNRAS/425/2116 : Arizona CDFS Environment Survey, ACES (Cooper+, 2012)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/574/A49https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/574/A49http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/574/A49https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/574/A49https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/574/A49http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/574/A49GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/574/A49/catalog (Combined table from original tables)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/574/A49/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/574/A49/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/574/A49/catalog?GETtext/xml+votable180.050000true53.126415-27.665283060.0055555555555555566/35935 359573.3716657170453808e-19 1.0810035871574334e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/574/A49?format=asciiX-rayUVdefaultJ/A+A/574/A49/catalogCombined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/1129] Sequential number (Cat_srcnum)meta.recordintm_Seq[ab] Multiplicity index on Seq, non-blank for sources in supplementary catalogmeta.code.multipcharRAJ2000Total UV right ascension (Tot_UV_RA) (1)degpos.eq.ra;meta.mainDEJ2000Total UV declination (Tot_UV_Dec) (1)degpos.eq.dec;meta.mainRA2deg? UVW2 right ascension (J2000) (UVW2_RA)degpos.eq.ranullableDE2deg? UVW2 declination (J2000) (UVW2_Dec)degpos.eq.decnullableePos2[0.1/2]? UVW2 position error (UVW2_POSERR)arcsecstat.error;posfloatnullableS.UVW2[3/78]? UVW2 significance (UVW2_SIGNIF)stat.fit.goodnessfloatnullableCRUVW2[0/2.3]? UVW2 count rate (UVW2_CR)ct/sphot.count;em.UVfloatnullablee_CRUVW2[0/0.02]? UVW2 count rate error (UVW2_CR_ERR)ct/sstat.errorfloatnullableFUVW2? UVW2 flux density (UVW2_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux;em.UVdoublenullablee_FUVW2? UVW2 flux density error (UVW2_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_UVW2[os] UVW2 flag for stacking (UVW2_OBS/STACK) (2)meta.codecharUVW2? UVW2 magnitude (UVW2_AB_MAG)magphot.mag;em.UVfloatnullablee_UVW2? UVW2 magnitude error (UVW2_AB_MAG_ERR)magstat.errorfloatnullableo_UVW2[2/23]? UVW2 number of observations (UVW2_GroupSize)meta.numberintnullableRA3deg? UVM2 right ascension (J2000) (UVM2_RA)degpos.eq.ranullableDE3deg? UVM2 declination (J2000) (UVM2_Dec)degpos.eq.decnullableePos3[0.1/2]? UVM2 position error (UVM2_POSERR)arcsecstat.error;posfloatnullableS.UVM2[3/130]? UVM2 significance (UVM2_SIGNIF)stat.fit.goodnessfloatnullableCRUVM2[0/6.5]? UVM2 count rate (UVM2_CR)ct/sphot.count;em.UVfloatnullablee_CRUVM2[0/0.04]? UVM2 count rate error (UVM2_CR_ERR)ct/sstat.errorfloatnullableFUVM2? UVM2 flux density (UVM2_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux;em.UVdoublenullablee_FUVM2? UVM2 flux density error (UVM2_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_UVM2[os] UVM2 flag for stacking (UVM2_OBS/STACK) (2)meta.codecharUVM2? UVM2 magnitude (UVM2_AB_MAG)magphot.mag;em.UVfloatnullablee_UVM2? UVM2 magnitude error (UVM2_AB_MAG_ERR)magstat.errorfloatnullableo_UVM2[2/18]? UVM2 number of observations (UVM2_GroupSize)meta.numberintnullableRA4deg? UVW1 right ascension (J2000) (UVW1_RA)degpos.eq.ranullableDE4deg? UVW1 declination (J2000) (UVW1_Dec)degpos.eq.decnullableePos4[0.1/2]? UVW1 position error (UVW1_POSERR)arcsecstat.error;posfloatnullableS.UVW1[3/270]? UVW1 significance (UVW1_SIGNIF)stat.fit.goodnessfloatnullableCRUVW1[0/21]? UVW1 count rate (UVW1_CR)ct/sphot.count;em.UVfloatnullablee_CRUVW1[0/0.08]? UVW1 count rate error (UVW1_CR_ERR)ct/sstat.errorfloatnullableFUVW1? UVW1 flux density (UVW1_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux;em.UVdoublenullablee_FUVW1? UVW1 flux density error (UVW1_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_UVW1[os] UVW1 flag for stacking (UVW1_OBS/STACK) (2)meta.codecharUVW1? UVW1 magnitude (UVW1_AB_MAG)phot.mag;em.UVfloatnullablee_UVW1? UVW1 magnitude error (UVW1_AB_MAG_ERR)stat.errorfloatnullableo_UVW1[2/30]? UVW1 number of observations (UVW1_GroupSize)meta.numberintnullableRA5deg? U right ascension (J2000) (U_RA)degpos.eq.ranullableDE5deg? U declination (J2000) (U_Dec)degpos.eq.decnullableePos5[0.1/2]? U position error (U_POSERR)arcsecstat.error;pos.cartesian.xfloatnullableS.U[3/270]? U significance (U_SIGNIF)stat.fit.goodnessfloatnullableCRU[0/71]? U count rate (U_CR)ct/sphot.count;em.UVfloatnullablee_CRU[0/0.4]? U count rate error (U_CR_ERR)ct/sstat.errorfloatnullableFU? U flux density (U_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux.density;em.opt.Udoublenullablee_FU? U flux density error (U_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_Umag[os] U flag for stacking (U_OBS/STACK) (2)meta.codecharUmag? U magnitude (U_AB_MAG)phot.mag;em.opt.Ufloatnullablee_Umag? U magnitude error (U_AB_MAG_ERR)stat.errorfloatnullableo_Umag[2/31]? U number of observations (U_GroupSize)meta.numberintnullableRA6deg? B right ascension (J2000) (B_RA)degpos.eq.ranullableDE6deg? B declination (J2000) (B_Dec)degpos.eq.decnullableePos6[0.1/2]? B position error (B_POSERR)arcsecstat.error;posfloatnullableS.B[3/331]? B significance (B_SIGNIF)stat.fit.goodnessfloatnullableCRB[0/92]? B count rate (B_CR)ct/sphot.countfloatnullablee_CRB[0/0.5]? B count rate error (B_CR_ERR)ct/sstat.errorfloatnullableFB? B flux density (B_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux.density;em.opt.Bdoublenullablee_FB? B flux density error (B_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_Bmag[os] B flag for stacking (B_OBS/STACK) (2)meta.codecharBmag? B magnitude (B_AB_MAG)phot.mag;em.opt.Bfloatnullablee_Bmag? B magnitude error (B_AB_MAG_ERR)stat.errorfloatnullableo_Bmag[2/14]? B number of observations (B_GroupSize)meta.numberintnullableRA7deg? V right ascension (J2000) (V_RA)degpos.eq.ranullableDE7deg? V declination (J2000) (V_Dec)degpos.eq.decnullableePos7[0.1/2]? V position error (V_POSERR)arcsecstat.error;pos.cartesian.yfloatnullableS.V[3/220]? V significance (V_SIGNIF)stat.fit.goodnessfloatnullableCRV[0/19]? V count rate (V_CR)ct/sphot.countfloatnullablee_CRV[0/0.1]? V count rate error (V_CR_ERR)ct/sstat.errorfloatnullableFV? V flux density (V_AB_FLUX) (3)cW.m**-2.nm**-1phot.flux.density;em.opt.Vdoublenullablee_FV? V flux density error (V_AB_FLUX_ERR) (3)cW.m**-2.nm**-1stat.errordoublenullablef_Vmag[os] V flag for stacking (V_OBS/STACK) (2)meta.codecharVmag? V magnitude (V_AB_MAG)phot.mag;em.opt.Vfloatnullablee_Vmag? V magnitude error (V_AB_MAG_ERR)stat.errorfloatnullableo_Vmag[2/7]? V number of observations (V_GroupSize)meta.numberintnullableEISEIS cross-identification (objID_EIS)meta.idcharFiltEIS filter [Up U B V B R I] (EIS_filter)meta.notecharCOMBO? COMBO cross-identification (objID_COMBO)meta.idintnullableCoClCOMBO classification (Class_COMBO) (4)src.classcharCIF? cross-identification flag (CIF) (5)meta.codeintnullableGALEXGALEX cross-identification (objID_GALEX)meta.idcharChandra[1/740]? Chandra cross-identification (objID_Chandra)meta.idintnullableFFCh? Chandra 0.5-8keV flux (Full_FLUX_Chandra) (6)mW.m**-2phot.flux;em.X-raydoublenullableFSCh? Chandra 0.5-2keV flux (Soft_FLUX_Chandra) (6)mW.m**-2phot.flux;em.X-raydoublenullableFHCh? Chandra 2-8keV flux (Hard_FLUX_Chandra) (6)mW.m**-2phot.flux;em.X-raydoublenullableGamma[-0.7/3]? Chandra photon index (PInd_Chandra)spect.indexfloatnullableChCl[AGS] Chandra classification: A=AGN, G=Galaxy, (Class_Chandra)src.classcharXMM[27/504]? XMM-Newton cross-identification (objID_XMM)meta.idintnullableFXMM? XMM-Newton 2-10keV flux (FLUX_XMM)mW.m**-2phot.flux;em.X-raydoublenullablezsp[0/2.6]? Spectroscopic redshift (z_spect)src.redshiftfloatnullabler_zspReference for redshift (z_spect_ref) (7)meta.ref;pos.framecharlogLuv? log specific UV luminosity (logL250nm)log(1e-07W.Hz**-1)phys.luminosity;em.UVfloatnullablelogLx? log specific X-ray luminosity (logL2keV)log(1e-07W.Hz**-1)phys.luminosity;em.X-rayfloatnullableaox? X-ray-to-optical-index {alpha}_ox_ (X-ray-to-optical-index)spect.indexfloatnullableClassAdopted classification (Adopted_Class) (9)src.classcharNotesNotes (Notes)meta.notechar