J/ApJS/230/1ivo://CDS.VizieR/J/ApJS/230/1doi:10.26093/cds/vizier.22300001CDSLu N.Zhao Y.Diaz-Santos T.Xu C.K.Gao Y.Armus L.Isaak K.G.,Mazzarella J.M.van der Werf P.P.Appleton P.N.Charmandaris V.,Evans A.S.Howell J.Iwasawa K.Leech J.Lord S.Petric A.O.,Privon G.C.Sanders D.B.Schulz B.Surace J.A.2017-09-27T15:17:12Z2017-08-02T07:04:20ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesinfrared-astronomyspectroscopyradial-velocityradio-spectroscopyWe describe a Herschel Space Observatory 194-671{mu}m spectroscopic survey of a sample of 121 local luminous infrared galaxies and report the fluxes of the CO J to J-1 rotational transitions for 4<=J<=13, the [NII] 205{mu}m line, the [CI] lines at 609 and 370{mu}m, as well as additional and usually fainter lines. The CO spectral line energy distributions (SLEDs) presented here are consistent with our earlier work, which was based on a smaller sample, that calls for two distinct molecular gas components in general: (i) a cold component, which emits CO lines primarily at J<~4 and likely represents the same gas phase traced by CO (1-0), and (ii) a warm component, which dominates over the mid-J regime (4<J<~10) and is intimately related to current star formation. We present evidence that the CO line emission associated with an active galactic nucleus is significant only at J>10. The flux ratios of the two [CI] lines imply modest excitation temperatures of 15-30K; the [CI] 370{mu}m line scales more linearly in flux with CO (4-3) than with CO (7-6). These findings suggest that the [CI] emission is predominantly associated with the gas component defined in (i) above. Our analysis of the stacked spectra in different far-infrared (FIR) color bins reveals an evolution of the SLED of the rotational transitions of H_2_O vapor as a function of the FIR color in a direction consistent with infrared photon pumping.2017ApJS..230....1Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/230/1CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVI/139 : Herschel Observation Log (Herschel Science Centre, 2013)J/ApJS/229/25 : GOALS sample PACS and SPIRE fluxes (Chu+, 2017)J/ApJ/829/93 : CO, [CI] & [NII] lines from Herschel (Kamenetzky+, 2016)J/A+A/591/A136 : Galaxies and QSOs FIR size & surface brightness (Lutz+, 2016)J/ApJ/819/69 : [NII]205um emission in local LIRGs (Zhao+, 2016)J/ApJ/790/124 : Dust and gas physics of the GOALS sample (Stierwalt+, 2014)J/A+A/568/A90 : Herschel/SPIRE spectra in Arp 299 (Rosenberg+, 2014)J/ApJ/777/156 : Spitzer/IRS spectra of GOALS LIRGs (Inami+, 2013)J/A+A/558/A87 : NGC6240 high resolution mapping of CO(1-0) (Feruglio+, 2013)J/ApJ/774/68 : [CII]157.7um feature in LIRGs (Diaz-Santos+, 2013)J/ApJS/206/1 : Mid-IR properties of GOALS nearby LIRGs (Stierwalt+, 2013)J/A+A/549/A51 : Extended CO structures in NGC6240 (Feruglio+, 2013)J/ApJ/741/32 : Spatial extent of LIRGs in the MIR. II. (Diaz-Santos+, 2011)J/ApJ/715/572 : GOALS UV and FIR properties (Howell+, 2010)J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/230/1https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/230/1http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/230/1https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/230/1https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/230/1http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/230/1GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/230/1/lirgs (SPIRE/FTS observations and fluxes of the CO, [CI] and [NII] lines (tables 1 and 4))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/230/1/lirgs?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/230/1/lirgs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/230/1/lirgs?GETtext/xml+votable180.050000true2.472525.9238890.0055555555555555566/226 231 538 650 700 1276 1521 1701 1702 1918 2363 2518 2680 3446 3824 4993 5130 6098 6348 6781 7552 8106 8111 8266 8482 8562 8673 8997 9133 9895 10210 10453 10465 11101 11180 11206 12537 13021 13523 15323 16045 16690 16755 16758 17183 17252 17736 17754 18406 18714 18897 18932 19283 19619 20060 20061 20208 20254 21016 22468 22721 23339 23921 24144 24163 24232 24584 24855 24957 24958 25610 26198 26264 26811 28393 29439 29680 30027 30810 30822 31081 31158 31430 31503 32740 34397 34627 34695 35067 35576 35608 37559 37821 38129 38139 38285 39472 39960 41276 41402 41430 41982 42010 43078 43107 43147 43298 43925 43994 44626 46077 46079 46130 46399 46811 46882 47029 47162 47235 47543 47854https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/230/1?format=asciiInfraredOpticalRadiodefaultJ/ApJS/230/1/table5Additional detected linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharLineLine descriptionmeta.id;spect.lineFlux[-11.5/14.3] Line flux (1)1e-17W.m**-2phot.flux;spect.linefloatf_FluxFlag on Flux (2)meta.codechare_Flux[0.04/1.2] Uncertainty in Flux1e-17W.m**-2stat.error;phot.fluxfloatnu[515.9/1491.9] Observed line frequencyGHzem.freq;spect.linefloate_nu[0.02/0.8] Uncertainty in nuGHzstat.errorfloatnudiff[-2.2/2.1] Observed minus expected frequencies (3)GHzstat.fit.residualfloatfnu[-9.7/12.1] Peak line flux density (4)Jyphot.fluxfloatS/N[2.9/34.5] Signal-to-Noise for peak line flux densitystat.snrfloatQ[1/4] Quality flag (G1)meta.code.qualintJ/ApJS/230/1/lirgsSPIRE/FTS observations and fluxes of the CO, [CI] and [NII] lines (tables 1 and 4)SimbadNameSimbad column added by the CDSmeta.idcharn_IDNote on object (2)meta.notecharCFCO10-9? CO (10-9) central frequency (7)GHzem.freqfloatnullableCFCO9-8? CO (9-8) central frequency (7)GHzem.freqfloatnullablee_CFCO10-9? Uncertainty in CF-CO10-9GHzstat.errorfloatnullablee_CFCO9-8? Uncertainty in CF-CO9-8GHzstat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifier (1)meta.id;meta.maincharprimaryNlNumber of additional detected lines for this galaxymeta.numberintnullableONameOther identifiermeta.idcharRAJ2000Hour of Right Ascension (J2000) (3)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000) (3)pos.eq.dec;meta.mainOffset[0/5.7] Systematic pointing offsetarcsecpos.angDistancefloate_CFCI370? Uncertainty in CF-CI370GHzstat.errorfloatnullablelogLIR[10.8/12.6]? Log adopted IR luminositylog(solLum)phys.luminosity;em.IRfloatnullablef_logLIR[*] *: Target in a multiple system of 2 or more galaxiesmeta.codecharCFIR[0.3/1.4]? FIR color; 60/100 micron band ratiophot.flux;arith.ratiofloatnullableDL[15/271]? Luminosity distanceMpcpos.distance;pos.heliocentricfloatnullableHVel[100/17880] Heliocentric velocitykm/sspect.dopplerVeloc;pos.heliocentricintObsIdHerschel observation identifiermeta.id;obs.param;obscharExp[1584/16996] Exposure timestime.duration;obs.exposureintFTSFourier transform spectrometer (FTS) of SPIRE program identifiermeta.id;obscharf_IDFlag on ID (4)meta.codecharFCO4-3[-4.4/25.6] CO (4-3) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO4-3? Uncertainty in F-CO4-3 (6)1e-17W.m**-2stat.errorfloatnullableFCO5-4[-2.4/23.2] CO (5-4) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO5-4? Uncertainty in F-CO5-4 (6)1e-17W.m**-2stat.errorfloatnullableFCO6-5[-1.1/22.1] CO (6-5) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO6-5? Uncertainty in F-CO6-5 (6)1e-17W.m**-2stat.errorfloatnullableFCO7-6[-0.9/20.2] CO (7-6) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO7-6? Uncertainty in F-CO7-6 (6)1e-17W.m**-2stat.errorfloatnullableFCO8-7[-1.8/20.2] CO (8-7) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO8-7? Uncertainty in F-CO8-7 (6)1e-17W.m**-2stat.errorfloatnullableFCO9-8[-2/17.2] CO (9-8) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO9-8? Uncertainty in F-CO9-8 (6)1e-17W.m**-2stat.errorfloatnullableFCO10-9[-1.9/153.2] CO (10-9) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO10-9[0.06/6.756e+06]? Uncertainty in F-CO10-9 (6)1e-17W.m**-2stat.errordoublenullableFCO11-10[-2.1/12.7] CO (11-10) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO11-10? Uncertainty in F-CO11-10 (6)1e-17W.m**-2stat.errorfloatnullableFCO12-11[-1.6/11] CO (12-11) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO12-11? Uncertainty in F-CO12-11 (6)1e-17W.m**-2stat.errorfloatnullableFCO13-12[-4.1/9.4] CO (13-12) line flux (5)1e-17W.m**-2phot.flux;em.line.COfloate_FCO13-12? Uncertainty in F-CO13-12 (6)1e-17W.m**-2stat.errorfloatnullableFCI609[-3.5/16.4] The [CI] 609um line flux (5)1e-17W.m**-2phot.flux;em.mm.400-750GHz;spect.linefloate_FCI609? Uncertainty in F-CI609 (6)1e-17W.m**-2stat.errorfloatnullableFCI370[-0.7/29.6] The [CI] 370um line flux (5)1e-17W.m**-2phot.flux;em.mm.750-1500GHz;spect.linefloate_FCI370? Uncertainty in F-CI370 (6)1e-17W.m**-2stat.errorfloatnullableFNII[-1.2/102.5] The [NII] 205um line flux1e-17W.m**-2phot.flux;em.mm.750-1500GHz;spect.linefloate_FNII? Uncertainty in F-NII (6)1e-17W.m**-2stat.errorfloatnullableCFCO4-3? CO (4-3) central frequency (7)GHzem.freqfloatnullablee_CFCO4-3? Uncertainty in CF-CO4-3GHzstat.errorfloatnullableCFCO5-4? CO (5-4) central frequency (7)GHzem.freqfloatnullablee_CFCO5-4? Uncertainty in CF-CO5-4GHzstat.errorfloatnullableCFCO6-5? CO (6-5) central frequency (7)GHzem.freqfloatnullablee_CFCO6-5? Uncertainty in CF-CO6-5GHzstat.errorfloatnullableCFCO7-6? CO (7-6) central frequency (7)GHzem.freqfloatnullablee_CFCO7-6? Uncertainty in CF-CO7-6GHzstat.errorfloatnullableCFCO8-7? CO (8-7) central frequency (7)GHzem.freqfloatnullablee_CFCO8-7? Uncertainty in CF-CO8-7GHzstat.errorfloatnullableCFCO11-10? CO (11-10) central frequency (7)GHzem.freqfloatnullablee_CFCO11-10? Uncertainty in CF-CO11-10GHzstat.errorfloatnullableCFCO12-11? CO (12-11) central frequency (7)GHzem.freqfloatnullablee_CFCO12-11? Uncertainty in CF-CO12-11GHzstat.errorfloatnullableCFCO13-12? CO (13-12) central frequency (7)GHzem.freqfloatnullablee_CFCO13-12? Uncertainty in CF-CO13-12GHzstat.errorfloatnullableCFCI609? The [CI] 609 micron line central frequency (7)GHzem.freqfloatnullablee_CFCI609? Uncertainty in CF-CI609GHzstat.errorfloatnullableCFCI370? The [CI] 370 micron line central frequency (7)GHzem.freqfloatnullableCFNII? The [NII] 205 micron line central frequency (7)GHzem.freqfloatnullablee_CFNII? Uncertainty in CF-NIIGHzstat.errorfloatnullableDCO4-3? CO (4-3) line difference (8)GHzstat.fit.residualfloatnullableDCO5-4? CO (5-4) line difference (8)GHzstat.fit.residualfloatnullableDCO6-5? CO (6-5) line difference (8)GHzstat.fit.residualfloatnullableDCO7-6? CO (7-6) line difference (8)GHzstat.fit.residualfloatnullableDCO8-7? CO (8-7) line difference (8)GHzstat.fit.residualfloatnullableDCO9-8? CO (9-8) line difference (8)GHzstat.fit.residualfloatnullableDCO10-9? CO (10-9) line difference (8)GHzstat.fit.residualfloatnullableDCO11-10? CO (11-10) line difference (8)GHzstat.fit.residualfloatnullableDCO12-11? CO (12-11) line difference (8)GHzstat.fit.residualfloatnullableDCO13-12? CO (13-12) line difference (8)GHzstat.fit.residualfloatnullableDCI609? The [CI] 609um line difference (8)GHzstat.fit.residualfloatnullableDCI370? The [CI] 370um line difference (8)GHzstat.fit.residualfloatnullableDNII? The [NII] 205um line difference (8)GHzstat.fit.residualfloatnullablePCO4-3? Peak CO (4-3) line flux densityJyphot.fluxfloatnullablePCO5-4? Peak CO (5-4) line flux densityJyphot.fluxfloatnullablePCO6-5? Peak CO (6-5) line flux densityJyphot.fluxfloatnullablePCO7-6? Peak CO (7-6) line flux densityJyphot.fluxfloatnullablePCO8-7? Peak CO (8-7) line flux densityJyphot.fluxfloatnullablePCO9-8? Peak CO (9-8) line flux densityJyphot.fluxfloatnullablePCO10-9? Peak CO (10-9) line flux densityJyphot.fluxfloatnullablePCO11-10? Peak CO (11-10) line flux densityJyphot.fluxfloatnullablePCO12-11? Peak CO (12-11) line flux densityJyphot.fluxfloatnullablePCO13-12? Peak CO (13-12) line flux densityJyphot.fluxfloatnullablePCI609? Peak [CI] 609um line flux densityJyphot.fluxfloatnullablePCI370? Peak [CI] 370um line flux densityJyphot.fluxfloatnullablePNII? Peak [NII] 205um line flux densityJyphot.fluxfloatnullableS/NCO4-3? Signal-to-Noise for CO (4-3) line (9)stat.snrfloatnullableS/NCO5-4? Signal-to-Noise for CO (5-4) line (9)stat.snrfloatnullableS/NCO6-5? Signal-to-Noise for CO (6-5) line (9)stat.snrfloatnullableS/NCO7-6? Signal-to-Noise for CO (7-6) line (9)stat.snrfloatnullableS/NCO8-7? Signal-to-Noise for CO (8-7) line (9)stat.snrfloatnullableS/NCO9-8? Signal-to-Noise for CO (9-8) line (9)stat.snrfloatnullableS/NCO10-9? Signal-to-Noise for CO (10-9) line (9)stat.snrfloatnullableS/NCO11-10? Signal-to-Noise for CO (11-10) line (9)stat.snrfloatnullableS/NCO12-11? Signal-to-Noise for CO (12-11) line (9)stat.snrfloatnullableS/NCO13-12? Signal-to-Noise for CO (13-12) line (9)stat.snrfloatnullableS/NCI609? Signal-to-Noise for [CI] 609um line (9)stat.snrfloatnullableS/NCI370? Signal-to-Noise for [CI] 370um line (9)stat.snrfloatnullableS/NNII? Signal-to-Noise for [NII] 205um line (9)stat.snrfloatnullableq_CO4-3? Quality flag for CO (4-3) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO5-4? Quality flag for CO (5-4) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO6-5? Quality flag for CO (6-5) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO7-6? Quality flag for CO (7-6) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO8-7? Quality flag for CO (8-7) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO9-8? Quality flag for CO (9-8) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO10-9? Quality flag for CO (10-9) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO11-10? Quality flag for CO (11-10) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO12-11? Quality flag for CO (12-11) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CO13-12? Quality flag for CO (13-12) line (1=robust detection) (G1)meta.code.qualfloatnullableq_CI609? Quality flag for [CI] 609um line (1=robust detection) (G1)meta.code.qualfloatnullableq_CI370? Quality flag for [CI] 370um line (1=robust detection) (G1)meta.code.qualfloatnullableq_NII? Quality flag for [NII] 205um line (1=robust detection) (G1)meta.code.qualfloatnullableWCO9-8? CO (9-8) line FWHM (10)km/sspect.line.widthfloatnullableWCO10-9? CO (10-9) line FWHM (10)km/sspect.line.widthfloatnullableWCO11-10? CO (11-10) line FWHM (10)km/sspect.line.widthfloatnullableWCO12-11? CO (12-11) line FWHM (10)km/sspect.line.widthfloatnullableWCO13-12? CO (13-12) line FWHM (10)km/sspect.line.widthfloatnullableWNII? The [NII] 205um line FWHM (10)km/sspect.line.widthfloatnullableF70-35? The 70 micron fractional flux with 35" beam (11)phot.flux.density;em.IR.30-60umfloatnullableF70-30? The 70 micron fractional flux with 30" beam (12)phot.flux.density;em.IR.30-60umfloatnullableF70-17? The 70 micron fractional flux with 17" beam (13)phot.flux.density;em.IR.30-60umfloatnullableC17Display SPIRE data from Chu+, 2017, J/ApJS/229/25, within 30"meta.ref.urlintnullableDS13Display data from Diaz-Santos+, 2013, J/ApJ/774/68, within 30"meta.ref.urlintnullableNEDNED column added by the CDSmeta.ref.urlchar