<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2016-04-04T08:34:00Z" status="active" updated="2026-01-08T10:08:40Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://dc.g-vo.org/ColStats-1 http://vo.ari.uni-heidelberg.de/docs/schemata/Colstats.xsd http://www.ivoa.net/xml/RegistryInterface/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/RegistryInterface.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogResource"><title>CALIFA (Calar Alto Legacy Integral Field spectroscopy Area) survey DR3</title><shortName>califadr3.object</shortName><identifier>ivo://org.gavo.dc/califa/q3/objects</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>Sánchez, F.</name></creator><creator><name>The CALIFA collaboration</name></creator><date role="Updated">2026-01-14T08:18:41Z</date><version>3</version><contact><name>GAVO Data Centre Team</name><address>Mönchhofstrasse 12-14, D-69120 Heidelberg</address><email>gavo@ari.uni-heidelberg.de</email><telephone>+49 6221 54 1837</telephone></contact></curation><content><subject>disk-galaxies</subject><subject>interstellar-medium</subject><subject>spectroscopy</subject><description> 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&lt;1000), from SDSS DR7/12 photometry otherwise.</description><source format="bibcode">2016A&amp;A...594A..36S</source><referenceURL>https://dc.g-vo.org/tableinfo/califadr3.objects</referenceURL></content><facility>Calar Alto Observatory</facility><instrument>PMAS/PPAK at 3.5m Telescope</instrument><coverage><spatial>6/43,50,56,131,545,552,554,556,568,573,620-621,626-627,721,733,738,907-909,948-949,975,995,1701,2206,2228-2229,2248,2251,2254,2272-2274,2276,2290,2641,4053,4167,4178,4279,4342,4445,4454,4472,4477,4507,4511,4526,4647,4654-4655,4667,4688,4696,4704,4712,4719,4731,4753-4754,4772,4799,4801,4806-4807,4813,4829,4840,4843-4844,4850,4912,4950,4957,4993,5023-5024,5028,5030,5075,5115,5148,5241,5247,5298,5332,5399,5482,5505,5530,5533,5579,5586,5591,5593,5596,5648,5695,5701,5704,5757,5862,5889,5942,5951,5975,5980,6000,6011,6045-6046,6074,6087,6093,6096,6116,6162,6212,6214,6216,6240-6241,6261,6270,6342,6362,6366,6411,6448,6465,6501,6532,6541,6547,6554,6607,6630,6977,7198,7204,7214,7308-7309,7312,7340,7386,7442,7501,7559-7560,7572,7584,7589,7591,7696,7783,7822,7824,7834,8045,8164,8195,8297,8327,8331,8341,8366,8376,8458,8477,8479-8480,8492,8498,8522,8536,8552,8557,8562-8563,8570,8589,8605,8621,8646,8656,8673,8705,8719,8728,8743,8752,8754,8825,8883,8898,8900,8919,8921-8922,8973,8984,8992,9098,9101,9124,9126,9133,9141,9187,9190,9216,9220,9381,9468,9470-9471,9622,9628,9630,9695,9718,9798,9812,9859,9873-9875,9882-9883,9885,9891,9946,9974,9991,10025,10111,10113,10144,10182-10183,10189,10200,10203,10213,10220-10221,10280,10286,10379-10381,10398,10400-10401,10414,10422,10434,10448,10485,10501,10511-10512,10515,10518-10520,10523-10524,10530,10540,10560,10566,10570,10577,10583,10586,10588,10594-10595,10609,10612,10621,10627-10629,10637,10661-10662,10669,10674,10705,10711,10719,10721,10727,10736,10739-10740,10752,10773,10778,10846,10921,10987,11010,11026,11044,11070,11111-11112,11164,11173,11196,11272,11290,11314,11325-11326,11341-11342,11369,11372,11374,11377,11383,11387,11392,11396,11418,11433,11435,11443,11451,11525,11544,11761,11777,11789,11793,11800-11801,11804,11832,11905,11944,12306,12378,12399,12532,12709,13316,13380-13381,13426,13529,15002,15004,16007,16696,16702,16787-16788,16793,17233-17234,17237-17238,17350,17392,17398,17486,17492,17499,17502,17509,17511,17516,17520,17571,17578,17661-17663,17667,17672,17745,17747-17748,17751,17758,17761,17767,17773,17819,17912,17998,18008,18069,18071,18081,18173,18241-18242,18252,18295,18300-18302,18381,18383,18523,18775,18779,18781,18790,18800,18838,18854,18931-18932,18934-18935,18941,19027,19073,19108,19186,19227,19260,19267,19325,19387,19417,19432,19458,19487,19489,19508,19515,19536-19538,19593,19618,19633,19642,19678,19696,19749,19848,19939-19940,19954,19981,19983-19984,19991,19996-19997,20009,20020,20023,20031-20033,20040,20193,20254,20279,20417-20418,20429,21857,22353,22356,22361,22364,22651-22652,22654-22655,22737,22740-22742,22826,23051,23072,23076,23182,23204,23206,23208,23273,23337,23353,23356,23401,23405,24055,26102,26108,26125,26318,26451,26495,26551,27133,27259,27368,27559,27567,27608,27719,27748,27830,27862,27912,27914-27915,28112,28213,28263-28264,28294,28310,28322,28365,28430,28458,28491,28497,28513,28522,28579,28606,28617,28639,29973,31478,31546,31628,31642-31643,31688-31689,31736-31737,32462,32471,32478,32482,32555,32559,32682,36604,36733,36765,36793,36797,36805,36847,36857,36861,48880,49084,49121,49130,49150</spatial><temporal>55357.9 57378.2</temporal><spectral>2.64824e-19 5.44232e-19</spectral><waveband>Optical</waveband></coverage><tableset><schema><name>califadr3</name><title>CALIFA (Calar Alto Legacy Integral Field spectroscopy Area) survey DR3</title><description>
The Calar Alto Legacy Integral Field Area (CALIFA) survey provides
spatially resolved spectroscopic information for 667 galaxies, mainly
within the local universe (0.005 &lt; z &lt; 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.  This is the VO/TAP publication with a simple web
interface on top.  See http://califa.caha.es/ for the upstream
site.</description><table><name>califadr3.objects</name><description> 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&lt;1000), from SDSS DR7/12 photometry otherwise.</description><nrows>667</nrows><column><name>target_name</name><description>Object a targeted observation targeted</description><ucd>meta.id;src</ucd><utype>obscore:Target.Name</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>califaid</name><description>CALIFA internal object key</description><ucd>meta.id;meta.main</ucd><stats><min>1</min><percentile03>20.98</percentile03><median>728.0</median><percentile97>5009.16</percentile97><max>9009</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>raj2000</name><description>Right ascension of the galaxy center, J2000 (from NED)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><stats><min>0.33241</min><percentile03>8.66344</percentile03><median>179.404</median><percentile97>351.839</percentile97><max>359.903</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>dej2000</name><description>Right ascension of the galaxy center, J2000 (from NED)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><stats><min>-22.5492</min><percentile03>-9.24365</percentile03><median>23.9579</median><percentile97>62.2761</percentile97><max>84.0526</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>redshift</name><description>Redshift, from growth curve analysis photometry for mother sample galaxies, from SDSS DR7/12 petrosian photometry otherwise.</description><ucd>src.redshift</ucd><stats><min>0.0019</min><percentile03>0.0047</percentile03><median>0.0159</median><percentile97>0.0311</percentile97><max>0.0802</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sdss_z</name><description>Redshift taken from SDSS DR7</description><ucd>src.redshift</ucd><stats><min>0</min><percentile03>0</percentile03><median>0.01495</median><percentile97>0.0294035</percentile97><max>0.08041</max><fillFactor>0.998501</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>maj_axis</name><description>Apparent isophotal major axis from SDSS</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><stats><min>-3960.87</min><percentile03>24.1331</percentile03><median>50.98</median><percentile97>71.241</percentile97><max>80.5097</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mstar</name><description>Stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><stats><min>7.0004</min><percentile03>8.77517</percentile03><median>10.606</median><percentile97>11.691</percentile97><max>11.959</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mstar_min</name><description>3 sigma lower limit of Stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass;stat.min</ucd><stats><min>6.8245</min><percentile03>8.6798</percentile03><median>10.491</median><percentile97>11.5521</percentile97><max>11.854</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>mstar_max</name><description>3 sigma upper limit of Stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass;stat.max</ucd><stats><min>7.1976</min><percentile03>8.87713</percentile03><median>10.723</median><percentile97>11.813</percentile97><max>12.169</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>chi2</name><description>χ² of best fit</description><ucd>stat.fit.chi2</ucd><stats><min>0.0022949</min><percentile03>0.0307173</percentile03><median>1.0577</median><percentile97>16.8233</percentile97><max>81.269</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vmax_nocorr</name><description>Survey volume for this galaxy from apparent isophotal diameter and measured redshift (cf. 2014A&amp;A...569A...1W)</description><unit>Mpc**3</unit><ucd>stat.weight</ucd><stats><min>3990</min><percentile03>17823</percentile03><median>360000</median><percentile97>1.4777e+06</percentile97><max>1.51e+06</max><fillFactor>0.812594</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vmax_denscorr</name><description>V_max additionally corrected for cosmic variance (cf. 2014A&amp;A...569A...1W)</description><unit>Mpc**3</unit><ucd>stat.weight</ucd><stats><min>5710</min><percentile03>20746</percentile03><median>238500</median><percentile97>1.62e+06</percentile97><max>1.82e+06</max><fillFactor>0.812594</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magu</name><description>Magnitude in the u band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id&lt;1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.</description><ucd>phot.mag;em.opt.U</ucd><stats><min>12.7975</min><percentile03>13.6734</percentile03><median>15.2394</median><percentile97>17.0723</percentile97><max>23.9369</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>err_magu</name><description>Error in m_u</description><ucd>stat.error;phot.mag;em.opt.U</ucd><stats><min>12.7975</min><percentile03>13.6734</percentile03><median>15.2394</median><percentile97>17.0723</percentile97><max>23.9369</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_ext</name><description>Extinction in the u band</description><ucd>phys.absorption;em.opt.U</ucd><stats><min>0.03765</min><percentile03>0.057944</percentile03><median>0.15629</median><percentile97>0.850041</percentile97><max>1.03809</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_u_min</name><description>3 sigma lower limit of the absolute magnitude in u</description><ucd>phot.mag;em.opt.U;stat.min</ucd><stats><min>-22.345</min><percentile03>-21.0308</percentile03><median>-19.342</median><percentile97>-15.973</percentile97><max>-12.486</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_u_max</name><description>3 sigma upper limit of the absolute magnitude in u</description><ucd>phot.mag;em.opt.U;stat.max</ucd><stats><min>-21.856</min><percentile03>-20.7888</percentile03><median>-19.175</median><percentile97>-15.832</percentile97><max>-12.135</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magg</name><description>Magnitude in the g band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id&lt;1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.</description><ucd>phot.mag;em.opt.V</ucd><stats><min>11.2214</min><percentile03>12.1561</percentile03><median>13.8082</median><percentile97>15.4392</percentile97><max>21.7597</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>err_magg</name><description>Error in m_g</description><ucd>stat.error;phot.mag;em.opt.V</ucd><stats><min>11.2214</min><percentile03>12.1561</percentile03><median>13.8082</median><percentile97>15.4392</percentile97><max>21.7597</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>g_ext</name><description>Extinction in the g band</description><ucd>phys.absorption;em.opt.V</ucd><stats><min>0</min><percentile03>0.0405472</percentile03><median>0.11492</median><percentile97>0.625451</percentile97><max>0.76382</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_g_min</name><description>3 sigma lower limit of the absolute magnitude in g</description><ucd>phot.mag;em.opt.V;stat.min</ucd><stats><min>-23.538</min><percentile03>-22.5307</percentile03><median>-20.689</median><percentile97>-17.3015</percentile97><max>-13.37</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_g_max</name><description>3 sigma upper limit of the absolute magnitude in g</description><ucd>phot.mag;em.opt.V;stat.max</ucd><stats><min>-23.391</min><percentile03>-22.4436</percentile03><median>-20.621</median><percentile97>-17.2049</percentile97><max>-13.234</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magr</name><description>Magnitude in the r band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id&lt;1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.</description><ucd>phot.mag;em.opt.R</ucd><stats><min>10.5304</min><percentile03>11.3883</percentile03><median>13.1003</median><percentile97>14.7899</percentile97><max>21.0159</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>err_magr</name><description>Error in m_r</description><ucd>stat.error;phot.mag;em.opt.R</ucd><stats><min>10.5304</min><percentile03>11.3883</percentile03><median>13.1003</median><percentile97>14.7899</percentile97><max>21.0159</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_ext</name><description>Extinction in the r band</description><ucd>phys.absorption;em.opt.R</ucd><stats><min>0.0201</min><percentile03>0.0309188</percentile03><median>0.08442</median><percentile97>0.455688</percentile97><max>115</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_r_min</name><description>3 sigma lower limit of the absolute magnitude in r</description><ucd>phot.mag;em.opt.R;stat.min</ucd><stats><min>-24.113</min><percentile03>-23.2408</percentile03><median>-21.289</median><percentile97>-17.721</percentile97><max>-13.592</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_r_max</name><description>3 sigma upper limit of the absolute magnitude in r</description><ucd>phot.mag;em.opt.R;stat.max</ucd><stats><min>-34.95</min><percentile03>-23.2156</percentile03><median>-21.258</median><percentile97>-17.6889</percentile97><max>-13.524</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magi</name><description>Magnitude in the i band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id&lt;1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.</description><ucd>phot.mag;em.opt.I</ucd><stats><min>10.0336</min><percentile03>11.0021</percentile03><median>12.6974</median><percentile97>14.5644</percentile97><max>20.7987</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>err_magi</name><description>Error in m_i</description><ucd>stat.error;phot.mag;em.opt.I</ucd><stats><min>10.0336</min><percentile03>11.0021</percentile03><median>12.6974</median><percentile97>14.5644</percentile97><max>20.7987</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>i_ext</name><description>Extinction in the i band</description><ucd>phys.absorption;em.opt.I</ucd><stats><min>0.01524</min><percentile03>0.0234488</percentile03><median>0.06402</median><percentile97>0.343973</percentile97><max>0.42007</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_i_min</name><description>3 sigma lower limit of the absolute magnitude in i</description><ucd>phot.mag;em.opt.I;stat.min</ucd><stats><min>-24.557</min><percentile03>-23.7231</percentile03><median>-21.681</median><percentile97>-18.0145</percentile97><max>-13.857</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_i_max</name><description>3 sigma upper limit of the absolute magnitude in i</description><ucd>phot.mag;em.opt.I;stat.max</ucd><stats><min>-34.95</min><percentile03>-23.672</percentile03><median>-21.616</median><percentile97>-17.9516</percentile97><max>-13.69</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>magz</name><description>Magnitude in the z band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id&lt;1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.</description><ucd>phot.mag;em.opt.I</ucd><stats><min>9.93636</min><percentile03>10.6784</percentile03><median>12.4641</median><percentile97>14.4508</percentile97><max>20.6179</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>err_magz</name><description>Error in m_z</description><ucd>stat.error;phot.mag;em.opt.I</ucd><stats><min>9.93636</min><percentile03>10.6784</percentile03><median>12.4641</median><percentile97>14.4508</percentile97><max>20.6179</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>z_ext</name><description>Extinction in the z band</description><ucd>phys.absorption;em.opt.I</ucd><stats><min>0.0108</min><percentile03>0.0166232</percentile03><median>0.04539</median><percentile97>0.243879</percentile97><max>0.29784</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_z_min</name><description>3 sigma lower limit of the absolute magnitude in z</description><ucd>phot.mag;em.opt.I;stat.min</ucd><stats><min>-24.982</min><percentile03>-24.1293</percentile03><median>-22.035</median><percentile97>-18.2764</percentile97><max>-14.111</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>abs_z_max</name><description>3 sigma upper limit of the absolute magnitude in z</description><ucd>phot.mag;em.opt.I;stat.max</ucd><stats><min>-24.732</min><percentile03>-24.0371</percentile03><median>-21.923</median><percentile97>-18.1659</percentile97><max>-13.88</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>hubtyp</name><description>Morphological type from CALIFA's own visual classification (see 2014A&amp;A...569A...1W for details). (M) indicates definite merging going on, (m) indicates likely merging, (i) indicates signs of interaction.</description><ucd>src.morph.type</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>minhubtyp</name><description>Earliest morphological type in CALIFA's estimation</description><ucd>src.morph.type</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>maxhubtyp</name><description>Latest morphological type in CALIFA's estimation</description><ucd>src.morph.type</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType></column><column><name>bar</name><description>Bar strength, A -- strong bar, AB -- intermediate, B -- weak bar; with minimum and maximum estimates.</description><ucd>meta.code;src.morph</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>flag_release_comb</name><description>Cube in setup COMB available?</description><ucd>meta.code;meta.dataset</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>1.0</median><percentile97>1.0</percentile97><max>1</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>flag_release_v1200</name><description>Cube in setup V1200 available?</description><ucd>meta.code;meta.dataset</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>1.0</median><percentile97>1.0</percentile97><max>1</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>flag_release_v500</name><description>Cube in setup V500 available?</description><ucd>meta.code;meta.dataset</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>1.0</median><percentile97>1.0</percentile97><max>1</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>axis_ratio</name><description>b/a axis ratio of a moment-based anaylsis of the SDSS DR7 images (cf. 2014A&amp;A...569A...1W).</description><ucd>phys.angSize;arith.ratio</ucd><stats><min>0.11516</min><percentile03>0.183141</percentile03><median>0.56099</median><percentile97>0.93</percentile97><max>45.09</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>position_angle</name><description>Position angle wrt north.</description><unit>deg</unit><ucd>pos.posAng</ucd><stats><min>-66.5715</min><percentile03>-21.4961</percentile03><median>90.3536</median><percentile97>193.14</percentile97><max>380.432</max><fillFactor>0.997001</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>el_hlr</name><description>Petrosian half-light radius in r band</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><stats><min>0.41539</min><percentile03>4.61405</percentile03><median>16.236</median><percentile97>33.2798</percentile97><max>66.924</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>modmag_r</name><description>Model magnitude in r band</description><unit>mag</unit><ucd>phot.mag;meta.modelled</ucd><stats><min>11.9015</min><percentile03>12.4613</percentile03><median>13.7308</median><percentile97>16.6047</percentile97><max>20.8225</max><fillFactor>0.187406</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><foreignKey><targetTable>califadr3.cubes</targetTable><fkColumn><fromColumn>califaid</fromColumn><targetColumn>califaid</targetColumn></fkColumn></foreignKey></table></schema></tableset></ri:Resource>