J/ApJS/269/24ivo://CDS.VizieR/J/ApJS/269/24doi:10.26093/cds/vizier.22690024CDSKawamuro T.Ricci C.Mushotzky R.F.Imanishi M.Bauer F.E.Ricci F.,Koss M.J.Privon G.C.Trakhtenbrot B.Izumi T.Ichikawa K.,Rojas A.F.Smith K.L.Shimizu T.Oh K.den Brok J.S.Baba S.,Balokovic M.Chang C.-S.Kakkad D.Pfeifle R.W.Temple M.J.Ueda Y.,Harrison F.Powell M.C.Stern D.Urry M.Sanders D.B.2024-11-06T20:30:19Z2024-02-29T12:29:56ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleimillimeter-astronomysubmillimeter-astronomygamma-ray-astronomyx-ray-sourcesredshiftedWe present a catalog of the millimeter-wave (mm-wave) continuum properties of 98 nearby (z<0.05) active galactic nuclei (AGNs) selected from the 70 month Swift/BAT hard-X-ray catalog that have precisely determined X-ray spectral properties and subarcsecond-resolution Atacama Large Millimeter/submillimeter Array Band 6 (211-275GHz) observations as of 2021 April. Due to the hard-X-ray (>10keV) selection, the sample is nearly unbiased for obscured systems at least up to Compton-thick-level obscuration, and provides the largest number of AGNs with high-physical-resolution mm-wave data (<~100-200pc). Our catalog reports emission peak coordinates, spectral indices, and peak fluxes and luminosities at 1.3mm (230GHz). Additionally, high-resolution mm-wave images are provided. Using the images and creating radial surface brightness profiles of mm-wave emission, we identify emission extending from the central sources and isolated blob-like emission. Flags indicating the presence of these emission features are tabulated. Among 90 AGNs with significant detections of nuclear emission, 37 AGNs (~41%) appear to have both or one of extended or blob-like components. We, in particular, investigate AGNs that show well-resolved mm-wave components and find that these seem to have a variety of origins (i.e., a jet, radio lobes, a secondary AGN, stellar clusters, a narrow-line region, galaxy disk, active star formation regions, or AGN-driven outflows), and some components have currently unclear origins.2023ApJS..269...24Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/269/24CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994)J/ApJS/103/81 : 1.425GHz atlas of IRAS bright galaxies. II. (Condon+, 1996)J/A+A/495/691 : Multifreq. catalog of blazars, Roma-BZCAT (Massaro+, 2009)J/ApJ/728/58 : Swift-BAT survey of AGNs (Burlon+, 2011)J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 6yrs (Baumgartner+, 2013)J/ApJ/815/L13 : Compton-thick AGNs from 70-month Swift/BAT (Ricci+, 2015)J/ApJ/822/109 : MIR view of polar dust emission in local AGNs (Asmus+, 2016)J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)J/ApJ/835/223 : A catalog of nearby galaxies with Chandra obs. (She+, 2017)J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019)J/MNRAS/495/3943 : Hard-X-ray-selected AGNs I (Chiaraluce+, 2020)J/A+A/633/A79 : NGC 6240 MUSE observations (Kollatschny+, 2020)J/ApJ/910/104 : subarcsec MIR view of local AGN. IV. ISAAC (Isbell+, 2021)J/ApJS/261/2 : BASS. XXII. Swift/BAT AGN Sp. Survey DR2 cat. (Koss+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/269/24https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/269/24http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/269/24https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/269/24https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/269/24http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/269/24GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/269/24/agns (Basic properties of our targets (Table 1) and complete list of mm-wave properties (Table 3))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/269/24/agns?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/269/24/agns?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/269/24/agns?GETtext/xml+votable180.050000true10.72002889-23.541048890.0055555555555555566/1121 4215 4439 8922 13021 16690 16892 17492 17525 17754 18484 18524 18897 19283 19373 20489 20556 20660 21016 21450 21785 21996 22890 22912 23010 23081 24120 24123 25054 25273 25403 25585 25790 25907 26071 26148 26375 27143 27721 27767 28075 28517 28535 28848 29906 31158 33958 34294 34531 35284 35447 35608 35623 35899 36618 36765 36786 36861 36896 38268 38653 38704 38868 39295 40221 40250 40258 40410 40818 41136 41423 41586 41982 42016 42120 43233 43339 43634 43677 43806 43825 43877 44017 44507 44551 44660 44722 44892 45779 45883 46399 46811 46987 47047 47154 47245 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/269/24?format=asciiGamma-rayX-rayMillimeterdefaultJ/ApJS/269/24/agnsBasic properties of our targets (Table 1) and complete list of mm-wave properties (Table 3)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/98] Identification numbermeta.idintprimaryIndexBAT index in previous papersmeta.idcharSWIFTBAT name (JHHMM.m+DDMMAN) from Ricci+ 2017, J/ApJS/233/17meta.id;meta.maincharRefReference for the position (1)meta.ref;pos.framecharSpInd[-2.5/5]? Spectral index (10)spect.indexfloatnullablee_SpInd[0.2/3]? Uncertainty in spectral indexstat.errorfloatnullableMFlagMorphology flag (11)meta.code;src.morphcharNansig[1/26]? Number of annuli with significant non-nuclear emissionmeta.numberfloatnullableSimbadNameSimbad column added by the CDSmeta.idcharnullableNEDNED column added by the CDSmeta.numbercharLEDAmeta.ref.urlcharCNameCounterpart name from Ricci+ 2017, J/ApJS/233/17meta.id.crosscharRAJ2000Right ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainz[0.001/0.05] Redshift (2)src.redshiftdoubleDist[3.5/216] Distance (2) (3)Mpcpos.distancefloate_Dist[0.1/14] Uncertainty in Dist (2) (3)Mpcstat.errorfloatf_Dist[a] Flag on Dist (4)meta.codecharType[1.0/2.0] Seyfert type (2)src.classfloatNobsNumber of ALMA observations for this target (link to Table 2)meta.numberintnullablef_Seqa: The data of IC 4709 is based on a clean process with robust=2meta.codecharNspw[0/8] Number of spectral windows (5)meta.numberintNwUsed[1/8] Number of spectral windows used for continuum detectionsmeta.numberintFreq[220.8/266.3] Central frequency (6)GHzem.freqfloatFreqtot[220.8/266.4] Central frequency for entire data setGHzem.freqfloatBand[1/7.2] Aggregate bandwidth (7)GHzinstr.bandwidthfloatBandtot[1.9/8] Aggregate bandwidth for entire data setGHzinstr.bandwidthfloatFluxDen[0.05/38] Flux density per beam of peak emission (8)mJyphot.flux.densityfloatSigma[0.008/0.2] Noise level; mJy/beam (8)mJystat.stdevfloatSignif[2/1147] Detection significance of peak emissionstat.likelihood;obsfloatUppLimUpper 5sigma limit flag for logF and logLmeta.codecharlogFlux[-15.7/-13] Log of mm-wave flux; erg/cm^2^/slog(mW.m**-2)phot.flux.density;em.mm.200-400GHzfloatlogLum[36.2/41.1] Log of mm-wave luminosity; erg/slog(1e-07W)phys.luminosity;em.mm.200-400GHzfloatErr[0.04/0.1]? Errors in logF and logL (9)stat.errorfloatnullableJ/ApJS/269/24/table2Basic information of ALMA dataSeq[1/98] Identification numbermeta.idintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintProjectALMA project codemeta.id;obscharOUSIDMember observation unit set (OUS) identifierobs.param;obscharMosaicMosaic observation or not ("mosaic"=12 occurrences)meta.notecharMRS[0.3/13.6]? Maximum recoverable scale (1)arcsecphys.angSize;srcfloatnullableFOV[21.9/227.1]? Field of view from ALMA archivearcsecphys.angSize;instr.fovfloatnullableExp[65/19813]? Exposure from ALMA archivestime.expointnullableDateObservation date (UT) from ALMA archivetime.epoch;obsnullableBmaj[0.02/1.7]? Angular beam size along major axis (2)arcsecphys.angSize;instr.beamfloatnullableBmin[0.018/1]? Angular beam size along minor axis (2)arcsecphys.angSize;instr.beamfloatnullableBmajpc[0.5/670]? Physical beam size along major axis (2)pcphys.size;instr.beamfloatnullableBminpc[0.4/530]? Physical beam size along minor axis (2)pcphys.size;instr.beamfloatnullable