smakced H imagesivo://org.gavo.dc/smakced/q/imThe GAVO DC teamJanz, J.Laurikainen, E.Lisker, T.Salo, H.Peletier, R. F.Niemi, S.-M.Toloba, E.Hensler, G.Falcón-Barroso, J.Boselli, A.den Brok, M.Hansson, K. S. A.Meyer, H. T.Ryś, A.Paudel, S.2026-09-07T15:53:43ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837dwarf-galaxiesearly-type-galaxiesvirgo-clustersurface-photometryinfrared-photometry The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED_) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with `resulting decompositions`_ and other properties of the galaxies in the sample. .. _SMAKCED: http://smakced.net .. _resulting decompositions: http://smakced.net/data.html2014ApJ...786..105Jhttp://dc.g-vo.org/smakced/q/im/inforelated-toSMAKCED Census of Structure in Early-type Dwarf GalaxiesIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/smakced/q/im/siap2.xml?https://dc.g-vo.org/smakced/q/im/siap2.xml?GETapplication/x-votable+xmlPOSA spatial constraint using SIAPv2 CIRCLE, RANGE, or POLYGON shapes and respective values in decimal degrees.charBANDWavelength interval that should intersect with the dataset coveragerealTIMETime interval that should intersect with the dataset coveragerealPOLPolarisation states as per Obscore (i.e., from the set I Q U V RR LL RL LR XX YY XY YX POLI POLAcharFOVLower and upper bound for the field of view of the observationdegrealSPATRESLower and upper bound for the spatial resolution of the image(s)degrealSPECRPLower and upper bound for the spectral resolving power λ/Δλ in spectrally resolved observationsrealEXPTIMELower and upper bound for the integration times of the observationsrealTIMERESLower and upper bound for the (absolute) resolution on the time axissrealIDA dataset identifier to match. Note that contrary to the SIAP v2 REC, we do not compare the IVOIDs case-insensitively. This should not be an issue if you got the IVOID from this service. For IVOIDs obtained in other ways, you may need to use ILIKE or a similar facility through ObsTAP.charCOLLECTIONA name of a data collection within the service (use ObsTAP to find out the possible values).charFACILITYA name of a facility (usually a telescope) used to make the observation.charINSTRUMENTA name of an instrument used to acquire the data.charDPTYPESelect either image or cube.charCALIBCalibration level of the data (0=raw data .. 3=processed science-ready data)integerTARGETA name of an observation target.charFORMATMedia type (like application/fits) or similar of the data product searchedcharobjectVCC identifier (like 'VCC0009')meta.idVCC0009VCC0021VCC0033VCC0140VCC0165VCC0170VCC0173VCC0178VCC0200VCC0209VCC0216VCC0218VCC0227VCC0230VCC0308VCC0319VCC0389VCC0407VCC0437VCC0490VCC0510VCC0523VCC0543VCC0571VCC0575VCC0608VCC0634VCC0698VCC0745VCC0750VCC0751VCC0758VCC0762VCC0781VCC0786VCC0794VCC0816VCC0856VCC0870VCC0916VCC0917VCC0929VCC0940VCC0949VCC0951VCC0990VCC1010VCC1036VCC1049VCC1073VCC1075VCC1087VCC1104VCC1122VCC1148VCC1167VCC1178VCC1183VCC1185VCC1196VCC1254VCC1261VCC1283VCC1297VCC1304VCC1308VCC1348VCC1355VCC1386VCC1392VCC1407VCC1422VCC1431VCC1440VCC1453VCC1475VCC1479VCC1488VCC1491VCC1501VCC1512VCC1514VCC1521VCC1528VCC1545VCC1549VCC1567VCC1614VCC1627VCC1684VCC1695VCC1743VCC1779VCC1827VCC1828VCC1833VCC1836VCC1857VCC1861VCC1871VCC1876VCC1890VCC1895VCC1896VCC1897VCC1902VCC1910VCC1912VCC1945VCC1947VCC1949VCC2008VCC2012VCC2019VCC2042VCC2048VCC2050VCC2080VCC2083charRESPONSEFORMATFile format requested for output.meta.code.mimetext/tab-separated-valuestsvtext/plaintxttext/csvcsv_baretext/csv;header=presentcsvapplication/jsonjsonapplication/geo+jsongeojsonapplication/x-votable+xmlvotableapplication/x-votable+xml;serialization=binary2votable/b2votableb2application/x-votable+xml;serialization=tabledatatext/xmlvotable/tdvotabletdapplication/x-votable+xml;serialization=tabledata;version=1.1text/xmlvotabletd1.1application/x-votable+xml;version=1.1text/xmlvotable1.1application/x-votable+xml;serialization=tabledata;version=1.2text/xmlvotabletd1.2application/x-votable+xml;serialization=tabledata;version=1.6vodmlapplication/x-votable+xml;version=1.6vodmlbtext/htmlhtmlapplication/fitsfitscharMAXRECMaximum 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.123integerPointed1000000187.03559424307312.09418828094710.010.01http://dc.g-vo.org/smakced/q/web/formhttps://dc.g-vo.org/smakced/q/web/formhttp://dc.g-vo.org/smakced/q/im/capabilitieshttps://dc.g-vo.org/smakced/q/im/capabilitieshttp://dc.g-vo.org/smakced/q/im/availabilityhttps://dc.g-vo.org/smakced/q/im/availabilityhttp://dc.g-vo.org/smakced/q/im/tableMetadatahttps://dc.g-vo.org/smakced/q/im/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tap4/1733,1746 5/6929,6931,6937,6941-6943,6965,6976,6978-6979,7008-7009,7011 6/26316,26318-26319,26362-26363,26365-26367,26538-26539,26542,27713,27715,27721,27723,27745,27753,27756,27758,27760-27761,27763,27857-27859,27864-27865,27868,27908,27910-27911,27930,27952,27954,27960,28041,28043,2805655211 560011.07375e-19 1.37948e-19http://dc.g-vo.org/smakced/q/im/coverageInfraredsmakced The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED_) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with `resulting decompositions`_ and other properties of the galaxies in the sample. .. _SMAKCED: http://smakced.net .. _resulting decompositions: http://smakced.net/data.htmlsmakced.mainSMAKCED infrared images and derived properties of early-type dwarf galaxies in the Virgo cluster.119dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel0123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.sizelongnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameterfloatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.valuefloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoublenullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extentfloatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.valuefloatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimitfloatnullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimitfloatnullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refvalfloatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.namecharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.namecharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBinsintnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBinsintnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBinsintnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriodfloatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullablebandpass_idFree-form name of the bandpass (filter, detector, whatever else defines the spectral response) this observation was taken in.instr.bandpasscharnullableobjectCommon name of the observed galaxy.meta.id;meta.maincharraj2000ICRS RA of galaxy center from asymmetry centering (unless specified otherwise in remarks).degpos.eq.ra;meta.maindoublenullabledej2000ICRS Declination of galaxy center from asymmetry centering (unless specified otherwise in remarks).degpos.eq.dec;meta.maindoublenullableexptimeTotal integration time for the object (sum of exposure times of all images stacked; note that different telescopes were in use).stime.duration;obs.exposurefloatnullableseeingEstimate for the seeing at observation time.arcsecinstr.obsty.seeingfloatnullablesnrSignal to noise ratio for a pixel at 2 r_e.stat.snrfloatnullablehmagTotal H-band magnitude of the galaxyphot.mag;em.ir.Hfloatnullabler_eEffective radius of the galaxy (semi-major axis of half-light aperture in H).arcsecphys.angSizefloatnullableb_aAxis raio at 2 r_ephys.angSize;arith.ratiofloatnullableconcentrationConcentration index 5 log_80/r_20 as in 2000AJ....119.2645Bphys.size;arith.ratiofloatnullablerho10Local projected number density of cluster galaxies. (see Appendix D in the source)log(deg**-2)src.densityfloatnullableremarksMorphological features from 2006AJ....132.2432L and other remarksmeta.notecharnullablemoreinfoBibcodes of papers containing more information.meta.refcharnullablestructgroupStructural Group (see 2012ApJ...745L..24J) resulting from the decomposition.meta.code.classcharnullablesimp_mIntegrated H-band brightness, simple modelmagphot.mag;em.ir.Hfloatnullablesimp_rcHalf-light radius, simple modelarcsecphys.angSize;srcfloatnullablesimp_nSérsic index, simple modelstat.fit.paramfloatnullablesimp_b_aAxis ratio, simple modelphys.angSize;arith.ratiofloatnullableinner_mIntegrated H-band brightness, inner componentmagphot.mag;em.ir.Hfloatnullableinner_rcHalf-light radius, inner componentarcsecphys.angSize;srcfloatnullableinner_nSérsic index, inner componentstat.fit.paramfloatnullableinner_b_aAxis ratio, inner componentphys.angSize;arith.ratiofloatnullableouter_mIntegrated H-band brightness, global/outer componentmagphot.mag;em.ir.Hfloatnullableouter_rcHalf-light radius, global/outer componentarcsecphys.angSize;srcfloatnullableouter_nSérsic index, global/outer componentstat.fit.paramfloatnullableouter_b_aAxis ratio, global/outer componentphys.angSize;arith.ratiofloatnullablesimpdec_rffResidual flux fraction (2006ApJ...644...30B) for the single decompositionstat.fit.goodnessfloatnullablesimpdec_eviExcess variance index (2011MNRAS.411.2439H) for single decompositionstat.fit.goodnessfloatnullablefinaldec_rffResidual flux fraction (2006ApJ...644...30B) for the final decompositionstat.fit.goodnessfloatnullablefinaldec_eviExcess variance index (2011MNRAS.411.2439H) for final decompositionstat.fit.goodnessfloatnullablecompmorphAdditional information on decomposition.meta.note;src.morphcharnullabledateobsApproximate observation date (essentially, month and year should be about right). NULL for archival materialdtime;obs.exposuredoublenullable