sasmirala coneivo://org.gavo.dc/sasmirala/q/coneThe GAVO DC teamAsmus, D.Hoenig, S.F.Gandhi, P.Smette, A.Duschl, W.J.2021-07-20T07:04:36ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837active-galactic-nucleiseyfert-galaxiesinfrared-photometry The Subarcsecond mid-infrared (MIR) atlas of local active galactic nuclei (AGN) is a collection of all available N- and Q-band images obtained at ground-based 8-meter class telescopes with public archives (Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR). It includes in total 895 images, of which 60% are perviously unpublished. These correspond to 253 local AGN with a median redshift of 0.016. The atlas contains the uniformly processed and calibrated images and nuclear photometry obtained through Gauss and PSF fitting for all objects and filters. This also includes measurements of the nuclear extensions. In addition, the classifications of extended emission (if present) and derived nuclear monochromatic 12 and 18 micron continuum fluxes are available. Finally, flux ratios with the circumnuclear MIR emission (measured by Spitzer) and total MIR emission of the galaxy (measured by IRAS) are presented.2014MNRAS.439.1648Ahttps://dc.g-vo.org/sasmirala/q/cone/infoIsServedByGAVO Data Center TAP service If you use this atlas please cite the Asmus et al. work given under the "source" metadata item.http://dc.g-vo.org/sasmiralahttps://dc.g-vo.org/sasmiralahttp://dc.g-vo.org/sasmirala/q/cone/scs.xml?https://dc.g-vo.org/sasmirala/q/cone/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealnameCommon object namemeta.id;meta.maincharclsOptical classification (References for the collected optical AGN classifications are given in App. B of 2014MNRAS.439.1648A)src.classchardDistanceMpcrealn_extNuclear morphology at subarcsecond resolutionmeta.code;src.morphcharflu12Nuclear subarcsecond-scale monochromatic flux density at restframe 12 µmmJyphot.flux.density;em.IRrealflu18Nuclear subarcsecond-scale monochromatic flux density at restframe 18 µmmJyphot.flux.density;em.IRrealresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true338.9425-26.0505560.01http://dc.g-vo.org/sasmirala/q/cone/capabilitieshttps://dc.g-vo.org/sasmirala/q/cone/capabilitieshttp://dc.g-vo.org/sasmirala/q/cone/availabilityhttps://dc.g-vo.org/sasmirala/q/cone/availabilityhttp://dc.g-vo.org/sasmirala/q/cone/tableMetadatahttps://dc.g-vo.org/sasmirala/q/cone/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapESO VLT, Gemini North & South, Subaru, Spitzer, IRASVISIR, T-ReCS, Michelle, COMICS, IRAC, IRS, MIPS, IRAS6/18,650,1701,4116,4381,4439,4447,4993,5091,5116,5202,5975-5976,6098,7552,7606,7659,7869,7959,8195,8264,8299,8492,8675,8922,9770,10265,10355,10364,10454,10465,10475,10817,10839,10856,10912,10924-10925,10927,10977,11027,11029,11457,11512,12241,12306,12335,12380,13564,13707,14744,14858,16301,16434,16655,16690,16712,17075,17183,17264,17369,17525,17727,17748,17754,17795,17814,17819,17850,18017,18242,18365,18432,18484,18524,18683,18714,18838,18895,18897,18935,19283,19373,19376,19433,19611,19619,19730,19746,19932,20000,20489,21016,21036,21450,22654,22721,22890,22912,22976,23167,23269,23323,23469,24842,25035,25083,25182,25518,25610,25790,25890,25907,26028,26091,26148,26264,26292,26303,26313,26338,26365,26393,26547,26937,27030,27191,27255,27382,27426,27512,27515,27699,27714,27719,27721,27765,27767,27773,27909,27914,27945,28075,28167,28173,28184,28221,28249,28259,28495,28535,29795,30140,31080,31158,31352,33034,33716,33930,33954,33958,34099,34104,34273,34294,34318,34343,34412,34493,34531,34534,34695,34737,34881,34913,35246,35447,35608,35623,35691,35993,36005,36158,36668,36765,36785-36786,36861,36896,37650,38268,38479,38653,38704,38853,38868,38887,38948,39182,39487,39836,40221,40410,40777,40818,41586,41982,42016,42027,43233,43242,43262,43339,43625,43634,43677,43748,43806,43877,43925,44507,44551,44650,44660,45587,45735,45779,45816,45883,46079,46399,46442,46481,46568,46615,46715,46811,46987,47047,47107,47120,47154,47169,47325,47415,4904252975 557271.528e-20 2.838e-20https://dc.g-vo.org/sasmirala/q/cone/coverageInfraredsasmirala The Subarcsecond mid-infrared (MIR) atlas of local active galactic nuclei (AGN) is a collection of all available N- and Q-band images obtained at ground-based 8-meter class telescopes with public archives (Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR). It includes in total 895 images, of which 60% are perviously unpublished. These correspond to 253 local AGN with a median redshift of 0.016. The atlas contains the uniformly processed and calibrated images and nuclear photometry obtained through Gauss and PSF fitting for all objects and filters. This also includes measurements of the nuclear extensions. In addition, the classifications of extended emission (if present) and derived nuclear monochromatic 12 and 18 micron continuum fluxes are available. Finally, flux ratios with the circumnuclear MIR emission (measured by Spitzer) and total MIR emission of the galaxy (measured by IRAS) are presented.output The Subarcsecond mid-infrared (MIR) atlas of local active galactic nuclei (AGN) is a collection of all available N- and Q-band images obtained at ground-based 8-meter class telescopes with public archives (Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR). It includes in total 895 images, of which 60% are perviously unpublished. These correspond to 253 local AGN with a median redshift of 0.016. The atlas contains the uniformly processed and calibrated images and nuclear photometry obtained through Gauss and PSF fitting for all objects and filters. This also includes measurements of the nuclear extensions. In addition, the classifications of extended emission (if present) and derived nuclear monochromatic 12 and 18 micron continuum fluxes are available. Finally, flux ratios with the circumnuclear MIR emission (measured by Spitzer) and total MIR emission of the galaxy (measured by IRAS) are presented._rDistance to cone centerdegpos.angDistancedoublenullablenameCommon object namemeta.id;meta.main1H 0419-5771RXS J112716.6+1909142MASX J03565655-40414532MASX J09180027+04250663C 1053C 1203C 1353C 2273C 2643C 2733C 2853C 293C 2933C 3053C 3173C 3213C 3273C 333C 3533C 3823C 390.33C 4033C 4243C 4453C 4493C 4523C 4593C 783C 933C 984C +73.08Ark 120Cen ACircinusCygnus AESO 103-35ESO 121-28ESO 138-1ESO 141-55ESO 198-24ESO 209-12ESO 253-3ESO 263-13ESO 286-19ESO 297-18ESO 323-32ESO 323-77ESO 33-2ESO 362-18ESO 416-2ESO 420-13ESO 428-14ESO 5-4ESO 500-34ESO 506-27ESO 511-30ESO 548-81ESO 602-25Fairall 49Fairall 51Fairall 9Fornax AH 0557-385H1143-182Hydra AI Zw 1IC 1459IC 3639IC 4329AIC 4518WIC 5063IC 883III Zw 35NIRAS 00188-0856IRAS 01003-2238IRAS 04103-2838IRAS 05189-2524IRAS 08572+3915IRAS 09149-6206IRAS 11095-0238IRAS 13349+2438IRAS 15250+3609LEDA 13946LEDA 170194LEDA 178130LEDA 549777M51aM81M87MCG-1-13-25MCG-1-24-12MCG-1-5-47MCG-2-8-14MCG-2-8-39MCG-3-34-64MCG-5-23-16MCG-6-30-15MR 2251-178Mrk 1014Mrk 1018Mrk 1239Mrk 266NEMrk 266SWMrk 3Mrk 304Mrk 509Mrk 520Mrk 573Mrk 590Mrk 841Mrk 897Mrk 915Mrk 926Mrk 937NGC 1052NGC 1068NGC 1097NGC 1144NGC 1194NGC 1275NGC 1365NGC 1386NGC 1433NGC 1553NGC 1566NGC 1614NGC 1667NGC 1808NGC 2110NGC 235ANGC 253NGC 2623NGC 2992NGC 3081NGC 3094NGC 3147NGC 3166NGC 3169NGC 3185NGC 3227NGC 3281NGC 3312NGC 3368NGC 3379NGC 3393NGC 34NGC 3486NGC 3521NGC 3607NGC 3623NGC 3627NGC 3628NGC 3660NGC 3690ENGC 3690WNGC 3718NGC 3783NGC 3982NGC 3998NGC 4051NGC 4074NGC 4111NGC 4138NGC 4151NGC 4235NGC 424NGC 4258NGC 4261NGC 4278NGC 4303NGC 4374NGC 4388NGC 4395NGC 4418NGC 4438NGC 4457NGC 4472NGC 4501NGC 4507NGC 454ENGC 4579NGC 4593NGC 4594NGC 4636NGC 4698NGC 4736NGC 4746NGC 4785NGC 4941NGC 4945NGC 4992NGC 5005NGC 5033NGC 5135NGC 5252NGC 5258NGC 526ANGC 5273NGC 5347NGC 5363NGC 5427NGC 5506NGC 5548NGC 5643NGC 5728NGC 5813NGC 5866NGC 5953NGC 5995NGC 612NGC 613NGC 6221NGC 6240NNGC 6240SNGC 6251NGC 6300NGC 676NGC 6810NGC 6814NGC 6860NGC 6890NGC 7130NGC 7172NGC 7212NGC 7213NGC 7314NGC 7469NGC 7479NGC 7496NGC 7552NGC 7582NGC 7590NGC 7592WNGC 7626NGC 7674NGC 7679NGC 7743NGC 788NGC 985PG 0026+129PG 0052+251PG 0844+349PG 2130+099PKS 1417-19PKS 1814-63PKS 1932-46PKS 2158-380PKS 2354-35Pictor ASuperantennae SUGC 12348UGC 5101Z 41-20charnullableraj2000Right Ascension J2000.0degpos.eq.ra;meta.main2.5416714.097184.74349.342359.2531doublenullabledej2000Declination J2000.0degpos.eq.dec;meta.main-86.6319-62.3425-1.3911159.790682.53781doublenullableprodlinkLink to a web page with images, bibliography, and other details on the source.charnullablezRedshiftsrc.redshift-0.00010.0016680.01610.1343840.35711floatnullabledDistanceMpc3.27.8871.7651.2419671floatnullableclsOptical classification (References for the collected optical AGN classifications are given in App. B of 2014MNRAS.439.1648A)src.classcharnullableu_agnClassification as AGN uncertain?meta.codebooleanbatidBAT ID from 9-month catalog (from Winter et al, 2009, 2009ApJ...690.1322W)meta.id15.482.0151.61540.3201581intnullablen_extNuclear morphology at subarcsecond resolutionmeta.code;src.morph-o?circ.ellip.spir.comp.charnullablelim12True if 12 µm flux was not detected. flu12 is a 3-sigma upper level in this case.meta.code;phot.fluxbooleanflu12Nuclear subarcsecond-scale monochromatic flux density at restframe 12 µmmJyphot.flux.density;em.IR1.63.15664.5963.37210205.81floatnullableerr121-σ uncertainty of the 12 µm continuum fluxmJystat.error;phot.flux;em.IR0.51.30918.7222.0273567.20.806324floatnullablelim18True if 18 µm flux was not detected. flu18 is a 3-sigma upper level in this case.meta.code;phot.fluxbooleanflu18Nuclear subarcsecond-scale monochromatic flux density at restframe 18 µmmJyphot.flux.density;em.IR2245.605362.953539.5619950.20.268775floatnullableerr181-σ uncertainty of the 18 µm continuum fluxmJystat.error;phot.flux;em.IR17.2435.7391.61466.50.241107floatnullablephotparLink to detailed information on the photometry sources.meta.ref;photchardunrSize constraint on the nuclear unresolved emission in pc, which is set equal to the minimum PSF FWHM (major axis) measured for the objectpcphys.size;src514124123121351floatnullablermedFlux ratio of nuclear to intermediate scale; the in Spitzer/IRS unresolved flux component is used as measure for the intermediate-scale emission.phot.flux;arith.ratio0.020.060.721.14221.40.84585floatnullablerlarFlux ratio of nuclear to large scale; the IRAS 12 µm flux is used as measure for the large-scale emission.phot.flux;arith.ratio0.00080.003390.30521.377121.82460.833992floatnullable