Sasmirala Basic Object Propertiessasmirala.objectivo://org.gavo.dc/sasmirala/q/objectsThe GAVO DC teamAsmus, D.Hoenig, S.F.Gandhi, P.Smette, A.Duschl, W.J.2021-07-20T07:04:36ZGAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837active-galactic-nucleiseyfert-galaxiesinfrared-photometryBasic object properties and nuclear 12 and 18 micron continuum
fluxes/ratios.http://dc.zah.uni-heidelberg.de/tableinfo/sasmirala.objectsESO 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-20InfraredsasmiralaSasmirala: Subarcsecond mid-infrared atlas of local AGN 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includes in total 895 images, of which 60% are perviously unpublished.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.
sasmirala.objectsSasmirala Basic Object PropertiesBasic object properties and nuclear 12 and 18 micron continuum
fluxes/ratios.253nameCommon object namemeta.id;meta.maincharindexedprimaryraj2000Right Ascension J2000.0degpos.eq.ra;meta.maindoubleindexednullabledej2000Declination J2000.0degpos.eq.dec;meta.maindoubleindexednullableprodlinkLink to a web page with images, bibliography, and other details on the source.charnullablezRedshiftsrc.redshiftfloatnullabledDistanceMpcfloatnullableclsOptical 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.idintnullablen_extNuclear morphology at subarcsecond resolutionmeta.code;src.morphcharnullablelim12True 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.IRfloatnullableerr121-σ uncertainty of the 12 µm continuum fluxmJystat.error;phot.flux;em.IRfloatnullablelim18True 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.IRfloatnullableerr181-σ uncertainty of the 18 µm continuum fluxmJystat.error;phot.flux;em.IRfloatnullablephotparLink 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;srcfloatnullablermedFlux 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.ratiofloatnullablerlarFlux ratio of nuclear to large scale; the IRAS 12 µm flux is used as measure for the large-scale emission.phot.flux;arith.ratiofloatnullablepathcompInterally usedcharnullable