J/ApJ/905/57ivo://CDS.VizieR/J/ApJ/905/57doi:10.26093/cds/vizier.19050057CDSRunco J.N.Malkan M.A.Fernandez-Ontiveros J.A.Spinoglio L.,Pereira-Santaella M.2022-08-26T06:34:44Z2022-06-22T13:00:51ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiseyfert-galaxiesinfrared-astronomyspectroscopyline-intensitiesWe investigated the 65, 71, 79, 84, 119, and 163{mu}m OH doublets of 178 local (0<z<0.35) galaxies. They were observed using the Herschel/Photoconductor Array Camera and Spectrometer, including Seyfert galaxies, low-ionization nuclear emission-line regions, and star-forming galaxies. We observe these doublets exclusively in absorption (OH71), primarily in absorption (OH65, OH84), mostly in emission (OH79), only in emission (OH163), and an approximately even mix of the both (OH119). In 19 galaxies we find P Cygni or reverse P Cygni line profiles in the OH doublets. We use several galaxy observables to probe spectral classification, brightness of a central active galactic nucleus (AGN)/starburst component, and radiation field strength. We find that OH79, OH119, and OH163 are more likely to display strong emission for bright, unobscured AGNs. For less luminous, obscured AGNs and nonactive galaxies, we find populations of strong absorption (OH119), weaker emission (OH163), and a mix of weak emission and weak absorption (OH79). For OH65, OH71, and OH84, we do not find significant correlations with the observables listed above. For OH79 and OH119, we find relationships with both the 9.7{mu}m silicate feature and Balmer decrement dust extinction tracers in which more dust leads to weaker emission/stronger absorption. The origin of emission for the observed OH doublets, whether from collisional excitation or from radiative pumping by infrared photons, is discussed.2020ApJ...905...57Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/905/57CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)J/ApJ/453/616 : JHKL photometry of 12 micron galaxy sample (Spinoglio+ 1995)J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)J/A+A/417/515 : I Zw 1 unusual emission line spectrum (Veron-Cetty+, 2004)J/A+A/432/369 : Leiden Atomic & Molecular Database (LAMDA) (Schoeier+, 2005)J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)J/ApJS/190/233 : Spectroscopy & abund. of SINGS galaxies (Moustakas+, 2010)J/ApJ/709/1257 : Spitzer-IRS sp. of Seyfert galaxies. II. (Tommasin+, 2010)J/MNRAS/414/702 : Optical classification of southern ULIRGs (Lee+, 2011)J/A+A/578/A74 : Nuclear obscuration in LINERs (Gonzalez-Martin+, 2015)J/ApJ/803/109 : Spitzer/IRS sp. decompositon of AGN (Hernan-Caballero+, 2015)J/ApJS/226/19 : FIR sp. of AGNs from Herschel (Fernandez-Ontiveros+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/905/57https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/905/57http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/905/57https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/905/57https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/905/57http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/905/57GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/905/57/sample (data (Table 2), IRAS data (Table 3), 9.7um Silicate and Balmer data (Table 4), derived OH integrated flux values (Table 5) and equivalent widths (Table 6))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/905/57/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/905/57/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/905/57/sample?GETtext/xml+votable180.050000true0.79001583321.9602240.0055555555555555566/650 953 1008 1701-1702 1918 2564 3446 4215 4439 5284 5311 5492 5715 5751 5863 5975 6458 7132 7241 7424 7552 7606 7642 7713 7777 7869 8106 8264 8673 8845 8922 9084 9194 9231 9468 9894-9895 10265 10364 10404 10454 10475 10761 10856 10912 10925 10927 11029 11101 11206 11410 11512 11668 12380 13021 13632 14744 15351 16091 16655 16712 16740 17506 17525 17727 17754 17819 18398 18432 18683 18714 18794 18897 18932 19070 19283 19296 19619 19730 20000 20208 20230 21016 21450 23178 23233 23323 24123 25083 25561 25610 25790 25907 25965 26148 26264 26271 26292 26491 26540 26902 26937 27514 27767 27914 27937 28074 28123 28496 28535 28609 29795 30027 31081 31158 31258 31430 32930 33325 33409 33958 34273 34531 34534 34627 34695 34737 34913 35284 36733 36831 36896 38139 38268 38390 38653 38868 38935 40221 40410 40468 40777 40818 41059 41586 41982 42016 42027 42120 43107 43233 43262 43634 43677 43748 43806 43877 43881 44660 44812 45587 45735 45779 45883 46399 46615 46811 46987 47047 47120 47154 47169 47543 48865 490422.4696718532768785e-21 9.957392048645222e-21https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/905/57?format=asciiInfrareddefaultJ/ApJ/905/57/sampledata (Table 2), IRAS data (Table 3), 9.7um Silicate and Balmer data (Table 4), derived OH integrated flux values (Table 5) and equivalent widths (Table 6)l_F60Limit flag on F60meta.code.errorcharCatIRAS catalog used (4)instr.setup;meta.tablecharl_F25Limit flag on F25meta.code.errorcharSimbadNameSimbad column added by the CDSmeta.idcharnullableNEDNED column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Hour of Right Ascension (J2000) (1)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000) (1)pos.eq.dec;meta.mainz[0.00067/0.33] Spectroscopic redshift from NEDsrc.redshiftfloatF25[0.02/274.3]? IRAS 25 micron band flux densityJyphot.flux.density;em.IR.15-30umfloatnullablee_F25[0.014/11]? Uncertainty in F25Jystat.errorfloatnullableF60[0.07/1170]? IRAS 60 micron band flux densityJyphot.flux.density;em.IR.30-60umdoublenullablee_F60[0.009/59]? Uncertainty in F60Jystat.errorfloatnullableSiStr[-4.1/3.5]? Strength of silicate 9.7um feature (5)spect.line.intensityfloatnullablee_SiStr[0.001/1.1]? Uncertainty in SiStrstat.errorfloatnullableHa[0.09/1385]? H{alpha} line flux; in 10^-14^erg/s/cm^2^ units1e-14mW.m**-2meta.unit;spect.linefloatnullableHb[0.05/503]? H{beta} line flux in 10^-14^erg/s/cm^2^ units1e-14mW.m**-2meta.unit;phot.flux;spect.linefloatnullableOH65[-235/28]? OH65 doublet integrated flux (8)1e-14mW.m**-2phot.fluxfloatnullablee_OH65[2/29]? Uncertainty in OH65 (9)1e-14mW.m**-2stat.errorfloatnullableOH71[-446/-4.6]? OH71 doublet integrated flux (8)1e-14mW.m**-2phot.fluxfloatnullablee_OH71[1.9/7.3]? Uncertainty in OH71 (9)1e-14mW.m**-2stat.errorfloatnullableOH79[-790/96.1]? OH79 doublet integrated flux (8)1e-14mW.m**-2phot.fluxfloatnullablee_OH79[0.5/80]? Uncertainty in OH79 (9)1e-14mW.m**-2stat.errorfloatnullableOH84[-641/33]? OH84 doublet integrated flux (8)1e-14mW.m**-2phot.fluxfloatnullablee_OH84[0.4/103]? Uncertainty in OH84 (9)1e-14mW.m**-2stat.errorfloatnullableOH119[-1909/64]? OH119 doublet integrated flux (8)1e-14mW.m**-2phot.fluxdoublenullablee_OH119[0.14/25]? Uncertainty in OH119 (9)1e-14mW.m**-2stat.errorfloatnullableOH163[-3.8/156]? OH163 doublet integrated flux (8)1e-14mW.m**-2phot.fluxfloatnullablee_OH163[0.27/18.4]? Uncertainty in OH163 (9)1e-14mW.m**-2stat.errorfloatnullableOH65ew[-0.03/0.2]? OH65 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH65ew[0]? Uncertainty in OH65ew (11)umstat.errorfloatnullableOH71ew[-0.02/0.02]? OH71 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH71ew[0.001/0.004]? Uncertainty in OH71ew (11)umstat.errorfloatnullableOH79ew[-0.03/0.64]? OH79 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH79ew[0.001/0.12]? Uncertainty in OH79ew (11)umstat.errorfloatnullablel_OH84ewLimit flag on OH84ewmeta.code.errorcharOH84ew[-0.06/0.05]? OH84 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH84ew[0.001/0.02]? Uncertainty in OH84ew (11)umstat.errorfloatnullablel_OH119ewLimit flag on OH119ewmeta.code.errorcharOH119ew[-0.17/0.4]? OH119 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH119ew[0.001/0.06]? Uncertainty in OH119ew (11)umstat.errorfloatnullablel_OH163ewLimit flag on OH163ewmeta.code.errorcharOH163ew[0.008/0.2]? OH163 doublet equivalent width (10)umspect.line.eqWidthfloatnullablee_OH163ew[0.002/0.04]? Uncertainty in OH163ew (11)umstat.errorfloatnullableIDObject identifiermeta.id;meta.maincharClassOptical spectral classification (2)src.classcharTransOH doublet transition(s) observed (3)umem.wlcharr_SiStrReference code(s) for SiStr (6)meta.ref;pos.framecharRefsReference code(s) for line fluxes (7)meta.ref;pos.framecharl_OH65Limit flag on OH65meta.code.errorcharl_OH71Limit flag on OH71meta.code.errorcharl_OH79Limit flag on OH79meta.code.errorcharl_OH84Limit flag on OH84meta.code.errorcharl_OH119Limit flag on OH119meta.code.errorcharl_OH163Limit flag on OH163meta.code.errorcharl_OH65ewLimit flag on OH65ewmeta.code.errorcharl_OH71ewLimit flag on OH71ewmeta.code.errorcharl_OH79ewLimit flag on OH79ewmeta.code.errorchar