J/ApJ/794/152ivo://CDS.VizieR/J/ApJ/794/152doi:10.26093/cds/vizier.17940152CDSMelendez M.Mushotzky R.F.Shimizu T.T.Barger A.J.Cowie L.L.2017-05-23T10:10:13Z2016-11-25T07:48:02ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleigalaxiesinfrared-sourcesmillimeter-astronomyphotometrysubmillimeter-astronomyFar-Infrared (FIR) photometry from the Photodetector Array Camera and Spectrometer on the Herschel Space Observatory is presented for 313 nearby, hard X-ray selected galaxies from the 58 month Swift Burst Alert Telescope (BAT) Active Galactic Nuclei catalog. The present data do not distinguish between the FIR luminosity distributions at 70 and 160{mu}m for Seyfert 1 and Seyfert 2 galaxies. This result suggests that if the FIR emission is from the nuclear obscuring material surrounding the accretion disk, then it emits isotropically, independent of orientation. Alternatively, a significant fraction of the 70 and 160{mu}m luminosity could be from star formation, independent of active galactic nucleus (AGN) type. Using a non-parametric test for partial correlation with censored data, we find a statistically significant correlation between the AGN intrinsic power (in the 14-195keV band) and the FIR emission at 70 and 160{mu}m for Seyfert 1 galaxies. We find no correlation between the 14-195keV and FIR luminosities in Seyfert 2 galaxies. The observed correlations suggest two possible scenarios: (1) if we assume that the FIR luminosity is a good tracer of star formation, then there is a connection between star formation and the AGN at sub-kiloparsec scales, or (2) dust heated by the AGN has a statistically significant contribution to the FIR emission. Using a Spearman rank-order analysis, the 14-195keV luminosities for the Seyfert 1 and 2 galaxies are weakly statistically correlated with the F_70_/F_160_ratios.2014ApJ...794..152Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/794/152CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/456/3335 : SPIRE observations of Herschel-BAT sample (Shimizu+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/794/152https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/794/152http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/794/152https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/794/152https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/794/152http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/794/152GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/794/152/table1 (Galaxy and far-infrared flux densities)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/794/152/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/794/152/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/794/152/table1?GETtext/xml+votable180.050000true1.5812520.2027780.0055555555555555566/134 745 941 1121 1263 1405 1566 1677 1841 2216 2221 2251 2390 2551 2564 2764 3223 3309 3762 4439 4488 4535 4540 4558 4834 5149 5514 5762 5976 5989 6212 6241 6376 6665 6752 6977 7157 7277 7361 7386 7422 7424 7560 7628 7642 7728 7869 7921 7952 8029 8085 8216 8299 8870 8921 8922 9005 9707 9894 10141 10228 10454 10475 10662 10788 10847 10912 10925 10927 10977 10984 11006 11071 11191 11388 11392 11416 11490 11683 11705 11712 11898 12154 13021 13541 13720 13832 14051 14653 14810 14960 15015 15481 15825 16042 16100 16690 16892 16962 17408 17525 17548 17727 17795 17814 18307 18402 18524 18794 18897 18918 19283 19296 19318 19400 19797 19883 19996 20000 20014 20201 20379 20489 20556 20750 21036 21088 21186 21237 21245 21450 21785 21996 22355 22365 22626 22632 22637 22708 22890 22912 22975 23010 23081 23224 23237 23278 23323 23332 24120 24123 24381 24748 24842 24976 25035 25054 25182 25273 25572 25585 25610 25619 25735 25742 25773 25790 25907 26041 26071 26300 26375 26393 26515 26547 26861 27143 27477 27486 27501 27699 27721 27722 27767 27815 28075 28275 28350 28517 28563 28593 28609 28639 28654 28719 28848 29466 29574 29795 29906 30026 31158 31509 32986 33034 33716 33953 34104 34294 34318 34499 34531 34881 35049 35071 35085 35246 35284 35407 35447 35623 35717 35899 36073 36158 36216 36323 36618 36668 36765 36785 36786 36861 36896 37287 37850 37913 38129 38268 38479 38653 38696 38704 38817 38868 38948 39138 39182 39295 39349 39613 39717 40013 40221 40250 40258 40410 40818 41423 41435 41679 41876 41929 41982 42012 42016 42027 42120 42852 43057 43064 43262 43520 43546 43634 43677 43806 43825 43860 43877 43983 44017 44448 44507 44551 44660 44698 44722 44892 45222 45735 45779 45883 46399 46544 46615 46831 46987 47064 47120 47154 47169 47222 47245 47597 48321 48798 49001 490429.699422546568423e-22 3.243176138527326e-21https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/794/152?format=asciiInfraredRadiodefaultJ/ApJ/794/152/table1Galaxy and far-infrared flux densitiesSimbadNameSimbad column added by the CDSmeta.idcharNameNamemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPapIIDisplay data of Paper II (Shimizu et al., SPIRE observations, 2016, Cat. J/MNRAS/456/3335meta.ref.urlcharf_Name[b] Flag on Name (1)meta.codecharRAJ2000Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainDistLuminosity distance (2)Mpcpos.distancefloatMTypeGalaxy type (3)src.morph.typecharl_F70Limit flag on F70meta.code.errorcharF70Herschel/PACS 70 micron band flux densityJyphot.flux.density;em.IR.30-60umfloate_F70? rms uncertainty in F70Jystat.errorfloatnullablel_F160Limit flag on F160meta.code.errorcharF160Herschel/PACS 160 micron band flux densityJyphot.flux.density;em.mm.1500-3000GHzfloate_F160? Uncertainty in F160Jystat.errorfloatnullableBATSwift/BAT 14-195keV flux (10^-12^ erg/s/cm^2^)1e-15W.m**-2phot.flux;em.X-rayfloatA70Herschel/PACS 70 micron aperture size (4)phys.angSize;em.IR.60-100um;instr.fovcharA160Herschel/PACS 160 micron aperture size (4)phys.angSize;em.mm.1500-3000GHz;instr.fovcharIDProgram ID (5)meta.id;obsint