<?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="2026-04-14T11:54:35Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vg="http://www.ivoa.net/xml/VORegistry/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/VORegistry/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VORegistry.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:CatalogService"><title>GAVO CALIFA Cubes</title><identifier>ivo://org.gavo.dc/califa/q3/cubesearch</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>
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><source format="bibcode">2016A&amp;A...594A..36S</source><referenceURL>https://dc.g-vo.org/califa/q3/cubesearch/info</referenceURL><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://org.gavo.dc/__system__/obscore/obscore">GAVO Data Center Obscore</relatedResource></relationship></content><rights>
CALIFA asks you to acknowledge:

"This study uses data provided by the Calar Alto Legacy Integral Field Area
(CALIFA) survey (http://califa.caha.es/)."

"Based on observations collected at the Centro Astronómico Hispano Alemán
(CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut fűr
Astronomie and the Instituto de Astrofísica de Andalucía (CSIC)."

and to cite both of :bibcode:`2014A&amp;A...569A...1W` and
:bibcode:`2012A&amp;A...538A...8S`</rights><capability standardID="ivo://ivoa.net/std/SODA#sync-1.0"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">http://dc.g-vo.org/califa/q3/dl/dlget</accessURL><mirrorURL>https://dc.g-vo.org/califa/q3/dl/dlget</mirrorURL></interface></capability><capability standardID="ivo://ivoa.net/std/SODA#async-1.0"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="full">http://dc.g-vo.org/califa/q3/dl/dlasync</accessURL><mirrorURL>https://dc.g-vo.org/califa/q3/dl/dlasync</mirrorURL></interface></capability><capability standardID="ivo://ivoa.net/std/DataLink#links-1.1"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">http://dc.g-vo.org/califa/q3/dl/dlmeta</accessURL><mirrorURL>https://dc.g-vo.org/califa/q3/dl/dlmeta</mirrorURL><queryType>GET</queryType><resultType>application/x-votable+xml;content=datalink</resultType><param std="true"><name>ID</name><description>The publisher DID of the dataset of interest</description><ucd>meta.id;meta.main</ucd><dataType arraysize="*" xsi:type="vs:SimpleDataType">char</dataType></param><param std="true"><name>responseformat</name><description>File format requested for output.</description><ucd>meta.code.mime</ucd><dataType arraysize="*" xsi:type="vs:SimpleDataType">char</dataType></param><param std="true"><name>maxrec</name><description>Maximum number of records returned. 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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.cubes</name><description> Metadata for the CALIFA data cubes as delivered by the project.</description><nrows>1574</nrows><column><name>accref</name><description>Access key for the data</description><ucd>meta.ref.url</ucd><utype>Access.Reference</utype><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>owner</name><description>Owner of the data</description><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>embargo</name><description>Date the data will become/became public</description><unit>yr</unit><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>mime</name><description>MIME type of the file served</description><ucd>meta.code.mime</ucd><utype>Access.Format</utype><dataType arraysize="*" 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>red_cdisp_rms</name><description>RMS cross-dispersion FWHM band over all pointings</description><unit>pixel</unit><ucd>stat.error;instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_red_cdisp</name><description>Quality flag for cross-dispersion FWHM (determined as the most severe over mean, max, and rms</description><ucd>meta.code.qual;instr.dispersion</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>red_resskyline_min</name><description>Flux residual of a bright skyline (at 557.7 nm for V500, 435.8 nm for V1200), minimum over all pointings</description><unit>count</unit><ucd>stat.fit.residual;spect.line;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>red_resskyline_max</name><description>Flux residual of a bright 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xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>red_maxstraylight_max</name><description>Maximum of maximum straylight intensity over all pointings</description><unit>count</unit><ucd>instr.background;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>red_rmsstraylight_max</name><description>Maximum of RMS straylight intensity over all pointings</description><unit>count</unit><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_red_straylight</name><description>Flag for critical straylight.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>obs_skymag_mean</name><description>Mean V band sky surface brightness over all pointings.</description><unit>mag/arcsec**2</unit><ucd>phot.mag.sb;instr.skyLevel;em.opt.V;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>obs_skymag_rms</name><description>RMS of V band sky surface brightness over all pointings.</description><unit>mag/arcsec**2</unit><ucd>stat.error;phot.mag.sb;instr.skyLevel;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_obs_skymag</name><description>Flag for critical sky surface brightness.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>red_limsb</name><description>3-sigma limiting surface brightness in B band in mag.</description><unit>mag/arcsec**2</unit><ucd>phot.mag.sb;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>red_limsbflux</name><description>3-sigma limiting surface brightness in B band as flux.</description><unit>1e3J.cm**-2.s**-1.m**-1.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_red_limsb</name><description>Flag for critical limiting surface brightness sensitivity.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>red_frac_bigerr</name><description>Fraction of bad pixels (error larger than five times the value) in this cube.</description><ucd>instr.det.noise;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_red_errspec</name><description>Flag indicating excessive bad pixels.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>cal_qflux_g</name><description>Average flux ratio relative to SDSS g mean over all pointings</description><ucd>phot.flux;em.opt.V;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>cal_qflux_r</name><description>Average flux ratio relative to SDSS r mean over all pointings</description><ucd>phot.flux;em.opt.R;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>cal_qflux_rms</name><description>Average flux ratio relative to SDSS g and r RMS over all pointings</description><ucd>stat.error;em.opt;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_cal_specphoto</name><description>Flag for problems with spectro-photometric calibration.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>cal_rmsvelmean</name><description>RMS of radial velocity residuals of estimates based on 3 or 4 spectral subranges wrt the estimates from the full spectrum.</description><unit>km/s</unit><ucd>stat.error;instr.calib</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flag_cal_wl</name><description>Flag for critical wavelength calibration stability.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>flag_cal_imgqual</name><description>Flag for visually evident problems in this cube</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>flag_cal_specqual</name><description>Flag for visually evident problems in a 30''-aperture spectrum generated from this cube</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>cal_flatsdss</name><description>Flag for visually evident problems in the `SDSS flat' (see source paper); NULL here means: no SDSS flat applied.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>flag_cal_registration</name><description>Flag for visually evident problems in the registration of the synthetic broad-band image with SDSS and related procedures.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>flag_cal_v1200v500</name><description>Set if a visual check for the 30''-aperture integrated spectra in V500, V1200, and COMB showed problems.</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>obs_seeing_mean</name><description>Mean FWHM seeing over all pointings</description><unit>arcsec</unit><ucd>instr.obsty.seeing;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>obs_seeing_rms</name><description>RMS of FWHM seeing over all pointings</description><unit>arcsec</unit><ucd>stat.error;instr.obsty.seeing</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>cal_snr1hlr</name><description>Signal to noise ratio at the half-light ratio.</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>notes</name><description>Notes</description><ucd>meta.note</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>setup</name><description>Instrument setup (V500, V1200, or COMBO)</description><ucd>meta.code;instr</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>