CALIFA (Calar Alto Legacy Integral Field spectroscopy Area) survey DR3califadr3.objectivo://org.gavo.dc/califa/q3/objectsThe GAVO DC teamSánchez, F.The CALIFA collaboration2022-01-18T13:04:37Z3GAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837disk-galaxiesinterstellar-mediumspectroscopy Object data for DR3 sample.
The photometric and derived quantities are from growth curve analysis
of the SDSS images for galaxies from the mother sample
(califaid<1000), from SDSS DR7/12 photometry otherwise.https://dc.zah.uni-heidelberg.de/tableinfo/califadr3.objectsCalar Alto ObservatoryPMAS/PPAK at 3.5m Telescope6/43,50,56,131,545,552,554,556,568,573,620-621,626-627,721,733,738,907-909,948-949,975,995,1701,2206,2228-2229,2248,2251,2254,2272-2274,2276,2290,2641,4053,4167,4178,4279,4342,4445,4454,4472,4477,4507,4511,4526,4647,4654-4655,4667,4688,4696,4704,4712,4719,4731,4753-4754,4772,4799,4801,4806-4807,4813,4829,4840,4843-4844,4850,4912,4950,4957,4993,5023-5024,5028,5030,5075,5115,5148,5241,5247,5298,5332,5399,5482,5505,5530,5533,5579,5586,5591,5593,5596,5648,5695,5701,5704,5757,5862,5889,5942,5951,5975,5980,6000,6011,6045-6046,6074,6087,6093,6096,6116,6162,6212,6214,6216,6240-6241,6261,6270,6342,6362,6366,6411,6448,6465,6501,6532,6541,6547,6554,6607,6630,6977,7198,7204,7214,7308-7309,7312,7340,7386,7442,7501,7559-7560,7572,7584,7589,7591,7696,7783,7822,7824,7834,8045,8164,8195,8297,8327,8331,8341,8366,8376,8458,8477,8479-8480,8492,8498,8522,8536,8552,8557,8562-8563,8570,8589,8605,8621,8646,8656,8673,8705,8719,8728,8743,8752,8754,8825,8883,8898,8900,8919,8921-8922,8973,8984,8992,9098,9101,9124,9126,9133,9141,9187,9190,9216,9220,9381,9468,9470-9471,9622,9628,9630,9695,9718,9798,9812,9859,9873-9875,9882-9883,9885,9891,9946,9974,9991,10025,10111,10113,10144,10182-10183,10189,10200,10203,10213,10220-10221,10280,10286,10379-10381,10398,10400-10401,10414,10422,10434,10448,10485,10501,10511-10512,10515,10518-10520,10523-10524,10530,10540,10560,10566,10570,10577,10583,10586,10588,10594-10595,10609,10612,10621,10627-10629,10637,10661-10662,10669,10674,10705,10711,10719,10721,10727,10736,10739-10740,10752,10773,10778,10846,10921,10987,11010,11026,11044,11070,11111-11112,11164,11173,11196,11272,11290,11314,11325-11326,11341-11342,11369,11372,11374,11377,11383,11387,11392,11396,11418,11433,11435,11443,11451,11525,11544,11761,11777,11789,11793,11800-11801,11804,11832,11905,11944,12306,12378,12399,12532,12709,13316,13380-13381,13426,13529,15002,15004,16007,16696,16702,16787-16788,16793,17233-17234,17237-17238,17350,17392,17398,17486,17492,17499,17502,17509,17511,17516,17520,17571,17578,17661-17663,17667,17672,17745,17747-17748,17751,17758,17761,17767,17773,17819,17912,17998,18008,18069,18071,18081,18173,18241-18242,18252,18295,18300-18302,18381,18383,18523,18775,18779,18781,18790,18800,18838,18854,18931-18932,18934-18935,18941,19027,19073,19108,19186,19227,19260,19267,19325,19387,19417,19432,19458,19487,19489,19508,19515,19536-19538,19593,19618,19633,19642,19678,19696,19749,19848,19939-19940,19954,19981,19983-19984,19991,19996-19997,20009,20020,20023,20031-20033,20040,20193,20254,20279,20417-20418,20429,21857,22353,22356,22361,22364,22651-22652,22654-22655,22737,22740-22742,22826,23051,23072,23076,23182,23204,23206,23208,23273,23337,23353,23356,23401,23405,24055,26102,26108,26125,26318,26451,26495,26551,27133,27259,27368,27559,27567,27608,27719,27748,27830,27862,27912,27914-27915,28112,28213,28263-28264,28294,28310,28322,28365,28430,28458,28491,28497,28513,28522,28579,28606,28617,28639,29973,31478,31546,31628,31642-31643,31688-31689,31736-31737,32462,32471,32478,32482,32555,32559,32682,36604,36733,36765,36793,36797,36805,36847,36857,36861,48880,49084,49121,49130,4915055357.9 57378.22.64824e-19 5.44232e-19Opticalcalifadr3CALIFA (Calar Alto Legacy Integral Field spectroscopy Area) survey DR3
The Calar Alto Legacy Integral Field Area (CALIFA) survey provides
spatially resolved spectroscopic information for 667 galaxies, mainly
within the local universe (0.005 < z < 0.03).
CALIFA data was obtained using the PPAK integral field unit (IFU), with a
hexagonal field-of-view of 1.3 square arcmin, with a 100% covering factor
by adopting a three-pointing dithering scheme. has been taken in two
setups: V500 (6 Å bin size, 646 galaxies) and V1200 (2.3 Å bin size, 484
galaxies). A final product ("COMBO") combining both data sets, covering
3700-7500 Å at 6 Å bin size, is made availble for 484 galaxies.
CALIFA is a legacy survey, intended for the community. This is the (final)
Data Release 3.
califadr3.objects Object data for DR3 sample.
The photometric and derived quantities are from growth curve analysis
of the SDSS images for galaxies from the mother sample
(califaid<1000), from SDSS DR7/12 photometry otherwise.667target_nameObject a targeted observation targetedmeta.id;srcobscore:Target.NamecharnullablecalifaidCALIFA internal object keymeta.id;meta.mainshortraj2000Right ascension of the galaxy center, J2000 (from NED)degpos.eq.ra;meta.maindoublenullabledej2000Right ascension of the galaxy center, J2000 (from NED)degpos.eq.dec;meta.maindoublenullableredshiftRedshift, from growth curve analysis photometry for mother sample galaxies, from SDSS DR7/12 petrosian photometry otherwise.src.redshiftfloatnullablesdss_zRedshift taken from SDSS DR7src.redshiftfloatnullablemaj_axisApparent isophotal major axis from SDSSarcsecphys.angSize;srcfloatnullablemstarStellar masslog(solMass)phys.massfloatnullablemstar_min3 sigma lower limit of Stellar masslog(solMass)phys.mass;stat.minfloatnullablemstar_max3 sigma upper limit of Stellar masslog(solMass)phys.mass;stat.maxfloatnullablechi2χ² of best fitstat.fit.chi2floatnullablevmax_nocorrSurvey volume for this galaxy from apparent isophotal diameter and measured redshift (cf. 2014A&A...569A...1W)Mpc**3stat.weightfloatnullablevmax_denscorrV_max additionally corrected for cosmic variance (cf. 2014A&A...569A...1W)Mpc**3stat.weightfloatnullablemaguMagnitude in the u band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.Ufloatnullableerr_maguError in m_ustat.error;phot.mag;em.opt.Ufloatnullableu_extExtinction in the u bandphys.absorption;em.opt.Ufloatnullableabs_u_min3 sigma lower limit of the absolute magnitude in uphot.mag;em.opt.U;stat.minfloatnullableabs_u_max3 sigma upper limit of the absolute magnitude in uphot.mag;em.opt.U;stat.maxfloatnullablemaggMagnitude in the g band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.Vfloatnullableerr_maggError in m_gstat.error;phot.mag;em.opt.Vfloatnullableg_extExtinction in the g bandphys.absorption;em.opt.Vfloatnullableabs_g_min3 sigma lower limit of the absolute magnitude in gphot.mag;em.opt.V;stat.minfloatnullableabs_g_max3 sigma upper limit of the absolute magnitude in gphot.mag;em.opt.V;stat.maxfloatnullablemagrMagnitude in the r band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.Rfloatnullableerr_magrError in m_rstat.error;phot.mag;em.opt.Rfloatnullabler_extExtinction in the r bandphys.absorption;em.opt.Rfloatnullableabs_r_min3 sigma lower limit of the absolute magnitude in rphot.mag;em.opt.R;stat.minfloatnullableabs_r_max3 sigma upper limit of the absolute magnitude in rphot.mag;em.opt.R;stat.maxfloatnullablemagiMagnitude in the i band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.Ifloatnullableerr_magiError in m_istat.error;phot.mag;em.opt.Ifloatnullablei_extExtinction in the i bandphys.absorption;em.opt.Ifloatnullableabs_i_min3 sigma lower limit of the absolute magnitude in iphot.mag;em.opt.I;stat.minfloatnullableabs_i_max3 sigma upper limit of the absolute magnitude in iphot.mag;em.opt.I;stat.maxfloatnullablemagzMagnitude in the z band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.Ifloatnullableerr_magzError in m_zstat.error;phot.mag;em.opt.Ifloatnullablez_extExtinction in the z bandphys.absorption;em.opt.Ifloatnullableabs_z_min3 sigma lower limit of the absolute magnitude in zphot.mag;em.opt.I;stat.minfloatnullableabs_z_max3 sigma upper limit of the absolute magnitude in zphot.mag;em.opt.I;stat.maxfloatnullablehubtypMorphological type from CALIFA's own visual classification (see 2014A&A...569A...1W for details). (M) indicates definite merging going on, (m) indicates likely merging, (i) indicates signs of interaction.src.morph.typecharminhubtypEarliest morphological type in CALIFA's estimationsrc.morph.typecharmaxhubtypLatest morphological type in CALIFA's estimationsrc.morph.typecharbarBar strength, A -- strong bar, AB -- intermediate, B -- weak bar; with minimum and maximum estimates.meta.code;src.morphcharnullableflag_release_combCube in setup COMB available?meta.code;meta.datasetshortflag_release_v1200Cube in setup V1200 available?meta.code;meta.datasetshortflag_release_v500Cube in setup V500 available?meta.code;meta.datasetshortaxis_ratiob/a axis ratio of a moment-based anaylsis of the SDSS DR7 images (cf. 2014A&A...569A...1W).phys.angSize;arith.ratiofloatnullableposition_anglePosition angle wrt north.degpos.posAngfloatnullableel_hlrPetrosian half-light radius in r bandarcsecphys.angSize;srcfloatnullablemodmag_rModel magnitude in r bandmagphot.mag;meta.modelledfloatnullable