J/MNRAS/456/3335ivo://CDS.VizieR/J/MNRAS/456/3335doi:10.26093/cds/vizier.74563335CDSShimizu T.T.Melendez M.Mushotzky R.F.Koss M.J.Barger A.J.,Cowie L.L.2024-08-15T20:17:33Z2016-11-25T07:49:52ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleigalaxiesinfrared-sourcesmillimeter-astronomyphotometrysubmillimeter-astronomyWe present far-infrared (FIR) and submillimetre photometry from the Herschel Space Observatory's Spectral and Photometric Imaging Receiver (SPIRE) for 313 nearby (z<0.05) active galactic nuclei (AGN). We selected AGN from the 58 month Swift Burst Alert Telescope (BAT) catalogue, the result of an all-sky survey in the 14-195keV energy band, allowing for a reduction in AGN selection effects due to obscuration and host galaxy contamination. We find 46 per cent (143/313) of our sample is detected at all three wavebands and combined with our Photoconductor Array Camera and Spectrometer (PACS) observations represents the most complete FIR spectral energy distributions of local, moderate-luminosity AGN. We find no correlation among the 250, 350, and 500{mu}m luminosities with 14-195keV luminosity, indicating the bulk of the FIR emission is not related to the AGN. However, Seyfert 1s do show a very weak correlation with X-ray luminosity compared to Seyfert 2s and we discuss possible explanations. We compare the SPIRE colours (F_250_/F_350_ and F_350_/F_500_) to a sample of normal star-forming galaxies, finding the two samples are statistically similar, especially after matching in stellar mass. But a colour-colour plot reveals a fraction of the Herschel-BAT AGN are displaced from the normal star-forming galaxies due to excess 500{mu}m emission (E_500_). Our analysis shows E_500_ is strongly correlated with the 14-195keV luminosity and 3.4/4.6{mu}m flux ratio, evidence the excess is related to the AGN. We speculate these sources are experiencing millimetre excess emission originating in the corona of the accretion disc.2016MNRAS.456.3335Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/456/3335CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/794/152 : PACS observations of Herschel-BAT sample (Melendez+, 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/456/3335https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/456/3335http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/456/3335https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/456/3335https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/456/3335http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/456/3335GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/456/3335/table12 (Herschel-BAT with SPIRE flux densities (tables 1 and 2 of the paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/456/3335/table12?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/456/3335/table12?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/456/3335/table12?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 490423.972892068905477e-22 7.945784137810954e-22https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/456/3335?format=asciiInfraredMillimeterdefaultJ/MNRAS/456/3335/table12Herschel-BAT with SPIRE flux densities (tables 1 and 2 of the paper)SimbadNameSimbad column added by the CDSmeta.idcharNameNamemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPapIDisplay data of Paper I (Melendez et al., PACS observations, 2014, Cat. J/ApJ/794/152meta.ref.urlcharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatDistLuminosity distanceMpcpos.distancefloatMTypeAGN classificationsrc.morph.typecharn_MType[a] Note on classification (1)meta.notecharODHerschel Operational Day number for when the observation startedtime.epochintOBSIDHerschel Observation Identification numbermeta.id;obsl_F250Limit flag on F250 (5{sigma} upper limit for undetected sources)meta.code.errorcharF250SPIRE 250um flux densityJyphot.flux.density;em.mm.750-1500GHzfloate_F250? 1{sigma} uncertainty on F250Jystat.errorfloatnullableMet250Method used to extract photometry at 250um (1)meta.notecharFlg250Flag for the photometry at 250um (2)meta.codecharl_F350Limit flag on F350 (5{sigma} upper limit for undetected sources)meta.code.errorcharF350SPIRE 350um flux densityJyphot.flux.density;em.mm.750-1500GHzfloate_F350? 1{sigma} uncertainty on F350Jystat.errorfloatnullableMet350Method used to extract photometry at 350um (1)meta.notecharFlg350Flag for the photometry at 350um (2)meta.codecharl_F500Limit flag on F500 (5{sigma} upper limit for undetected sources)meta.code.errorcharF500SPIRE 500um flux densityJyphot.flux.density;em.mm.400-750GHzfloate_F500? 1{sigma} uncertainty on F500Jystat.errorfloatnullableMet500Method used to extract photometry at 500um (1)meta.notecharFlg500Flag for the photometry at 500um (2)meta.codechar