<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2016-09-07T13:29:08Z" status="active" updated="2024-12-27T08:31:05Z" version="1.2" xmlns:g-colstat="http://dc.g-vo.org/ColStats-1" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:stc="http://www.ivoa.net/xml/STC/stc-v1.30.xsd" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xlink="http://www.w3.org/1999/xlink" 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/STC/stc-v1.30.xsd http://vo.ari.uni-heidelberg.de/docs/schemata/stc-v1.30.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 http://www.w3.org/1999/xlink http://vo.ari.uni-heidelberg.de/docs/schemata/xlink.xsd" xsi:type="vs:CatalogResource"><title>TGAS catalogue</title><shortName>tgas.main</shortName><identifier>ivo://org.gavo.dc/tgas/q/main</identifier><curation><publisher>The GAVO DC team</publisher><creator><name>GAIA Collaboration</name></creator><date role="Updated">2016-09-07T00:00:00Z</date><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>stars</subject><subject>surveys</subject><subject>astrometry</subject><subject>proper-motions</subject><description> This table is a subset of GaiaSource comprising those stars in the
Hipparcos and Tycho-2 Catalogues for which a full 5-parameter
astrometric solution has been possible in Gaia Data Release 1. This is
possible because the early Hipparcos epoch positions break some
degeneracies due to the limited Gaia time coverage. This table
contains a substantial fraction of the around 2.5 million stars in the
Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to
several reasons, such as saturation, cross-match errors or bad
astrometric solution. All rows have Gaia solution id
1635378410781933568.</description><referenceURL>https://dc.g-vo.org/tableinfo/tgas.main</referenceURL><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://org.gavo.dc/tap">GAVO Data Center TAP service</relatedResource></relationship></content><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface role="std" version="1.1" xsi:type="vs:ParamHTTP"><accessURL use="full">http://dc.g-vo.org/tap</accessURL><mirrorURL>https://dc.g-vo.org/tap</mirrorURL></interface></capability><coverage><stc:STCResourceProfile><stc:AstroCoordSystem id="ndhsehghnnha"><stc:SpaceFrame id="ndhulmmpbtha"><stc:ICRS/><stc:UNKNOWNRefPos/><stc:SPHERICAL coord_naxes="2"/></stc:SpaceFrame></stc:AstroCoordSystem><stc:AstroCoordArea coord_system_id="ndhsehghnnha"><stc:AllSky frame_id="ndhulmmpbtha" unit="deg"/></stc:AstroCoordArea></stc:STCResourceProfile><spatial>0/0-11</spatial><spectral>2.721e-19 4.138e-19</spectral><waveband>Optical</waveband></coverage><tableset><schema><name>tgas</name><title>TGAS catalogue</title><description> This table is a subset of GaiaSource comprising those stars in the
Hipparcos and Tycho-2 Catalogues for which a full 5-parameter
astrometric solution has been possible in Gaia Data Release 1. This is
possible because the early Hipparcos epoch positions break some
degeneracies due to the limited Gaia time coverage. This table
contains a substantial fraction of the around 2.5 million stars in the
Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to
several reasons, such as saturation, cross-match errors or bad
astrometric solution. All rows have Gaia solution id
1635378410781933568.</description><table><name>tgas.main</name><description> This table is a subset of GaiaSource comprising those stars in the
Hipparcos and Tycho-2 Catalogues for which a full 5-parameter
astrometric solution has been possible in Gaia Data Release 1. This is
possible because the early Hipparcos epoch positions break some
degeneracies due to the limited Gaia time coverage. This table
contains a substantial fraction of the around 2.5 million stars in the
Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to
several reasons, such as saturation, cross-match errors or bad
astrometric solution. All rows have Gaia solution id
1635378410781933568.</description><nrows>2100000</nrows><column><name>source_id</name><description>Unique source identifier</description><ucd>meta.id;meta.main</ucd><stats><min>7627862074752</min><percentile03>2.7821002160144275e+17</percentile03><median>3.7237859862162985e+18</median><percentile97>6.668831054679873e+18</percentile97><max>6917521537218608640</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">long</dataType><flag>indexed</flag><flag>primary</flag></column><column><name>ra</name><description>Barycentric Right Ascension in ICRS at ref_epoch</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><stats><min>0.000428665</min><percentile03>15.8353</percentile03><median>182.89</median><percentile97>345.991</percentile97><max>360</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>dec</name><description>Barycentric Declination in ICRS at ref_epoch</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><stats><min>-89.8897</min><percentile03>-70.7701</percentile03><median>-4.77104</median><percentile97>69.7306</percentile97><max>89.8323</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag><flag>nullable</flag></column><column><name>ra_error</name><description>Standard error of ra (with cos δ applied).</description><unit>mas</unit><ucd>stat.error;pos.eq.ra</ucd><stats><min>0.0353231</min><percentile03>0.121808</percentile03><median>0.25414</median><percentile97>1.00204</percentile97><max>19.0627</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dec_error</name><description>Standard error of dec</description><unit>mas</unit><ucd>stat.error;pos.eq.dec</ucd><stats><min>0.0380127</min><percentile03>0.1123</percentile03><median>0.233384</median><percentile97>0.937583</percentile97><max>18.5281</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l</name><description>Galactic longitude (converted from ra, dec)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><stats><min>0.000365459</min><percentile03>15.1964</percentile03><median>197.07</median><percentile97>347.418</percentile97><max>359.999</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b</name><description>Galactic latitude (converted from ra, dec)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><stats><min>-89.7408</min><percentile03>-59.6663</percentile03><median>-0.982201</median><percentile97>58.0646</percentile97><max>89.8997</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pmra</name><description>Proper motion in right ascension of the source in ICRS at ref_epoch. This is the projection of the proper motion vector in the direction of increasing right ascension.</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><stats><min>-3259.36</min><percentile03>-37.9827</percentile03><median>-1.80842</median><percentile97>35.3201</percentile97><max>2890.43</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pmdec</name><description>Proper motion in declination at ref_epoch.</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><stats><min>-3159.34</min><percentile03>-44.9869</percentile03><median>-2.92976</median><percentile97>22.7736</percentile97><max>1858.53</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pmra_error</name><description>Standard error of pmra</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><stats><min>0.0118264</min><percentile03>0.0783715</percentile03><median>1.13309</median><percentile97>3.87223</percentile97><max>18.0084</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmdec_error</name><description>Standard error of pmdec</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><stats><min>0.0126948</min><percentile03>0.0677368</percentile03><median>0.866948</median><percentile97>3.29615</percentile97><max>18.8544</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>parallax</name><description>Absolute barycentric stellar parallax of the source at the reference epoch ref_epoch</description><unit>mas</unit><ucd>pos.parallax</ucd><stats><min>-24.82</min><percentile03>0.20151</percentile03><median>1.77984</median><percentile97>8.26584</percentile97><max>295.804</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>parallax_error</name><description>Standard error of parallax</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><stats><min>0.203974</min><percentile03>0.227369</percentile03><median>0.321973</median><percentile97>0.862496</percentile97><max>0.999998</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phot_g_mean_mag</name><description>Mean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale.</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.mean</ucd><stats><min>4.39512</min><percentile03>8.18077</percentile03><median>11.0353</median><percentile97>12.3765</percentile97><max>19.3079</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phot_g_mean_flux</name><description>G-band mean flux as electrons per second.</description><unit>s**-1</unit><ucd>phot.flux;em.opt;stat.mean</ucd><stats><min>306.736</min><percentile03>181683</percentile03><median>624877</median><percentile97>8.66161e+06</percentile97><max>2.83047e+08</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>phot_g_mean_flux_error</name><description>Error on phot_g_mean_flux</description><unit>s**-1</unit><ucd>stat.error;phot.flux;em.opt;stat.mean</ucd><stats><min>1.04902</min><percentile03>65.6256</percentile03><median>1029.94</median><percentile97>10369</percentile97><max>4.35696e+06</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phot_g_n_obs</name><description>Number of observations contributing to G photometry</description><ucd>meta.number</ucd><stats><min>11</min><percentile03>50.0</percentile03><median>115.0</median><percentile97>269.0</percentile97><max>1866</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>phot_variable_flag</name><description>Photometric variability flag</description><ucd>meta.code;src.var</ucd><dataType arraysize="*" xsi:type="vs:VOTableType">char</dataType><flag>nullable</flag></column><column><name>ref_epoch</name><description>Reference epoch to which the astrometic source parameters are referred, expressed as a Julian Year in TCB.</description><unit>yr</unit><ucd>meta.ref;time.epoch</ucd><stats><min>2015</min><percentile03>2015</percentile03><median>2015</median><percentile97>2015</percentile97><max>2015</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>astrometric_delta_q</name><description>Hipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)</description><ucd>stat.value</ucd><stats><min>3.77047e-05</min><percentile03>0.0969304</percentile03><median>2.35784</median><percentile97>39.981</percentile97><max>20437.8</max><fillFactor>0.0456015</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>astrometric_excess_noise</name><description>Excess noise of the source</description><unit>mas</unit><ucd>stat.value</ucd><stats><min>0</min><percentile03>0.241038</percentile03><median>0.478017</median><percentile97>1.28956</percentile97><max>5.29692</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>astrometric_excess_noise_sig</name><description>Significance of excess noise</description><ucd>stat.value</ucd><stats><min>0</min><percentile03>58.6683</percentile03><median>220.223</median><percentile97>1067.43</percentile97><max>1.02922e+24</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>astrometric_n_obs_ac</name><description>Total number of observations AC</description><ucd>meta.number</ucd><stats><min>0</min><percentile03>44.0</percentile03><median>99.0</median><percentile97>252.0</percentile97><max>1871</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_n_obs_al</name><description>Total number of observations AL</description><ucd>meta.number</ucd><stats><min>12</min><percentile03>44.0</percentile03><median>99.0</median><percentile97>254.0</percentile97><max>1878</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_n_bad_obs_ac</name><description>Number of bad observations AC</description><ucd>meta.number</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>4.0</median><percentile97>12.0</percentile97><max>100</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_n_bad_obs_al</name><description>Number of bad observations AL</description><ucd>meta.number</ucd><stats><min>0</min><percentile03>0.0</percentile03><median>0.0</median><percentile97>4.0</percentile97><max>70</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_n_good_obs_ac</name><description>Number of good observations AC</description><ucd>meta.number</ucd><stats><min>0</min><percentile03>42.0</percentile03><median>96.0</median><percentile97>243.0</percentile97><max>1791</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_n_good_obs_al</name><description>Number of good observations AL</description><ucd>meta.number</ucd><stats><min>12</min><percentile03>44.0</percentile03><median>99.0</median><percentile97>252.0</percentile97><max>1866</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_primary_flag</name><description>Only primary sources (for which this flag is True) contribute to the estimation of attitude, calibration, and global parameters. The estimation of source parameters is not affected by primariness.</description><ucd>meta.code</ucd><stats><min>1</min><percentile03>1.0</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>matched_observations</name><description>The number of observations (detection transits) that have been matched to a given source during the last internal crossmatch revision.</description><ucd>meta.number</ucd><stats><min>4</min><percentile03>6.0</percentile03><median>15.0</median><percentile97>33.0</percentile97><max>223</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>astrometric_priors_used</name><description>Type of prior used in in the astrometric solution</description><stats><min>3</min><percentile03>3.0</percentile03><median>5.0</median><percentile97>5.0</percentile97><max>5</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType><flag>nullable</flag></column><column><name>astrometric_relegation_factor</name><description>Relegation factor of the source calculated as per Eq. (118) in 2012A&amp;A...538A..78L used for the primary selection process.</description><ucd>arith.factor</ucd><stats><min>1</min><percentile03>2.44933</percentile03><median>4.70749</median><percentile97>12.4069</percentile97><max>50.0096</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>astrometric_weight_ac</name><description>Mean astrometric weight of the source</description><unit>mas**-2</unit><ucd>stat.weight;stat.mean</ucd><stats><min>1.53261e-06</min><percentile03>1.24645e-05</percentile03><median>2.75841e-05</median><percentile97>3.9385e-05</percentile97><max>0.00871282</max><fillFactor>0.998931</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>astrometric_weight_al</name><description>Mean astrometric weight of the source</description><unit>mas**-2</unit><ucd>stat.weight;stat.mean</ucd><stats><min>0.035149</min><percentile03>0.586919</percentile03><median>4.10138</median><percentile97>14.6345</percentile97><max>205.475</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>duplicated_source</name><description>During data processing, this source happened to been duplicated and one source only has been kept.</description><stats><min>0</min><percentile03>0.0</percentile03><median>0.0</median><percentile97>1.0</percentile97><max>1</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType></column><column><name>ra_dec_corr</name><description>Correlation between right ascension and declination</description><ucd>stat.correlation</ucd><stats><min>-0.999982</min><percentile03>-0.910318</percentile03><median>-0.0237216</median><percentile97>0.9157</percentile97><max>0.999972</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ra_pmra_corr</name><description>Correlation between right ascension and proper motion in right ascension</description><ucd>stat.correlation</ucd><stats><min>-0.999882</min><percentile03>-0.974559</percentile03><median>-0.706246</median><percentile97>0.288975</percentile97><max>0.997909</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ra_pmdec_corr</name><description>Correlation between right ascension and proper motion in declination</description><ucd>stat.correlation</ucd><stats><min>-0.999417</min><percentile03>-0.919702</percentile03><median>-0.0068451</median><percentile97>0.909037</percentile97><max>0.999383</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dec_pmra_corr</name><description>Correlation between declination and proper motion in right ascension</description><ucd>stat.correlation</ucd><stats><min>-0.999119</min><percentile03>-0.895108</percentile03><median>0.000694773</median><percentile97>0.885208</percentile97><max>0.999226</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dec_pmdec_corr</name><description>Correlation between declination and proper motion in declination</description><ucd>stat.correlation</ucd><stats><min>-0.999646</min><percentile03>-0.951697</percentile03><median>-0.585395</median><percentile97>0.486597</percentile97><max>0.998781</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmra_pmdec_corr</name><description>Correlation between proper motion in right ascension and proper motion in declination</description><ucd>stat.correlation</ucd><stats><min>-0.99975</min><percentile03>-0.96263</percentile03><median>0.00728044</median><percentile97>0.963255</percentile97><max>0.999722</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ra_parallax_corr</name><description>Correlation between right ascension and parallax</description><ucd>stat.correlation</ucd><stats><min>-0.998476</min><percentile03>-0.901085</percentile03><median>-0.0440962</median><percentile97>0.905623</percentile97><max>0.997722</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dec_parallax_corr</name><description>Correlation between declination and parallax</description><ucd>stat.correlation</ucd><stats><min>-0.996157</min><percentile03>-0.741047</percentile03><median>0.162042</median><percentile97>0.868581</percentile97><max>0.997952</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>parallax_pmra_corr</name><description>Correlation between parallax and proper motion in right ascension</description><ucd>stat.correlation</ucd><stats><min>-0.99835</min><percentile03>-0.944323</percentile03><median>0.0476041</median><percentile97>0.937921</percentile97><max>0.998762</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>parallax_pmdec_corr</name><description>Correlation between parallax and proper motion in declination</description><ucd>stat.correlation</ucd><stats><min>-0.996898</min><percentile03>-0.913624</percentile03><median>-0.160417</median><percentile97>0.786437</percentile97><max>0.996262</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>scan_direction_mean_k1</name><description>Mean position angle of scan directions across the source</description><unit>deg</unit><stats><min>-180</min><percentile03>-165.847</percentile03><median>-77.5503</median><percentile97>163.398</percentile97><max>179.999</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>scan_direction_strength_k1</name><description>Degree of concentration of scan directions across the source</description><stats><min>0.000191388</min><percentile03>0.0771294</percentile03><median>0.353239</median><percentile97>0.69019</percentile97><max>0.999985</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>scan_direction_mean_k2</name><description>Mean position angle of scan directions across the 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