J/ApJ/755/171ivo://CDS.VizieR/J/ApJ/755/171doi:10.26093/cds/vizier.17550171CDSSargsyan L.Lebouteiller V.Weedman D.Spoon H.Bernard-Salas J.,Engels D.Stacey G.Houck J.Barry D.Miles J.Samsonyan A.2017-12-21T15:26:30Z2014-04-17T15:30:33ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiredshiftedline-intensitiesinfrared-astronomyspectroscopyResults are presented for [CII] 158{mu}m line fluxes observed with the Herschel PACS instrument in 112 sources with both starburst and active galactic nucleus (AGN) classifications, of which 102 sources have confident detections. Results are compared with mid-infrared spectra from the Spitzer Infrared Spectrometer and with L_ir_ from IRAS fluxes; AGN/starburst classifications are determined from equivalent width of the 6.2{mu}m polycyclic aromatic hydrocarbon (PAH) feature. It is found that the [CII] line flux correlates closely with the flux of the 11.3{mu}m PAH feature independent of AGN/starburst classification, log[f([CII]158{mu}m)/f(11.3{mu}mPAH)]=-0.22+/-0.25. It is concluded that the [CII] line flux measures the photodissociation region associated with starbursts in the same fashion as the PAH feature. A calibration of star formation rate (SFR) for the starburst component in any source having [CII] is derived comparing [CII] luminosity L([CII]) to L_ir_ with the result that logSFR=logL([CII)])-7.08+/-0.3, for SFR in M_{sun}_/yr and L([CII]) in L_{sun}_. The decreasing ratio of L([CII]) to L_ir_ in more luminous sources (the "[CII] deficit") is shown to be a consequence of the dominant contribution to L_ir_arising from a luminous AGN component because the sources with the largest L_ir_ and smallest L([CII])/L_ir_ are AGNs.2012ApJ...755..171Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/755/171CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVI/139 : Herschel Observation Log (Herschel Science Centre, 2013)J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013)J/AJ/143/125 : SED of 113 dust-obscured galaxies at z~2 (Melbourne+, 2012)J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012)J/ApJ/730/19 : IR spectra and SEDs for starbursts and AGNs (Sargsyan+, 2011)J/MNRAS/409/2 : Herschel sources SED model parameters (Rowan-Robinson+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/755/171https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/755/171http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/755/171https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/755/171https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/755/171http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/755/171GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/755/171/table1 ([CII] line fluxes and luminosities)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/755/171/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/755/171/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/755/171/table1?GETtext/xml+votable180.050000true0.790083321.96016670.0055555555555555566/231 295 629 953 1008 1677 2433 2518 3934 4215 5379 6458 6781 7132 7386 7713 7777 8410 8637 8922 9194 9231 9617 9998 10039 10081 10265 10321 10364 10444 10487 10653 10716 11623 11668 11836 13523 15351 16115 16641 16758 17252 17506 17525 17727 18260 18432 18753 18783 18794 18919 19296 20118 20230 20489 20896 21416 22890 23233 23323 24855 25610 25790 25965 26310 26540 28074 28609 28999 30822 30879 31503 32408 32548 32931 33204 33313 33978 34010 34627 34695 34737 34913 35067 35284 35608 36733 37027 37113 37564 38246 38786 38868 38919 40818 41276 42010 43634 43677 43806 44660 44812 45222 45779 46077 46296 46615 47120 47162 47169 47543 48865https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/755/171?format=asciiOpticalInfrareddefaultJ/ApJ/755/171/table1[CII] line fluxes and luminositiesl_L158/LirLimit flag on L158/Lirmeta.code.errorcharl_F/7Limit flag on F/7meta.code.errorcharl_L158Limit flag on L158meta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/112] Running sequence numbermeta.id;meta.mainintNameTarget namemeta.idcharf_Name[j] Observation on 2 cycles (1)meta.codecharRAJ2000Hour of right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of declination (J2000)pos.eq.dec;meta.mainz[0.003/0.4] Redshiftsrc.redshiftfloatl_EWLimit flag on EWmeta.code.error;spect.line.eqWidthcharEW[0.001/0.6] Rest-frame equivalent width of 6.2um PAH emission feature (2)umspect.line.eqWidth;em.IR.4-8umfloatf_EW[kl] Flag on spectrum (1)meta.codecharl_F158Limit flag on F158meta.code.errorcharF158Total flux of [CII] 158um emission line (3)W.m**-2phot.flux;em.mm.1500-3000GHz;spect.linedoublef_F158[i] Asymmetric CII line (1)meta.codecharS/N[0.1/249] Signal-to-noise ratio (4)stat.snrfloatf_S/N[h] displaced spaxel (1)meta.codecharl_F/11Limit flag on F/11meta.code.errorcharF/11Ratio of flux in [CII] 158um to flux of PAH 11.3um emission feature (5)phot.flux;arith.ratiofloatf_F/11[l] PAH measure from Wu et al. (1)meta.codecharF/7[-4.1/-1.6] Ratio FCII/{nu}f_{nu}_(7.8um) (5)phot.flux;arith.ratiofloatL158[6.12/9.26] [CII] 158um emission line luminosity (6)log(solLum)phys.luminosity;em.IRfloatL158/Lir[-4.3/-2.5] Ratio of [CII] IR luminosity (7)phys.luminosity;arith.ratiofloatObsIdHerschel observation numbermeta.numberS11Display the data from Sargsyan et al. (2011, Cat. J/ApJ/730/19)meta.ref.urlcharSimbadNameSimbad column added by the CDSmeta.idcharNEDSimbad column added by the CDSmeta.ref.urlchar