<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2018-03-13T13:08:00Z" status="active" updated="2024-02-06T08:59:18Z" 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>Gaia Astrometric Performance, Table 2</title><shortName>gdr2mock.astrome</shortName><identifier>ivo://org.gavo.dc/gdr2mock/q/astrometric_performance2</identifier><altIdentifier>doi:10.21938/SYx.JVejuu66uzDiLcfRlA</altIdentifier><curation><publisher>The GAVO DC team</publisher><creator><name>Rybizki, J.</name></creator><creator><name>Demleitner, M.</name></creator><creator><name>Fouesneau, M.</name></creator><creator><name>Bailer-Jones, C.</name></creator><creator><name>Rix, H.-W.</name></creator><creator><name>Andrae, R.</name></creator><date role="Updated">2020-05-04T09:28:20Z</date><date role="Updated">2018-07-24</date><date role="Updated">2018-05-17</date><date role="Updated">2018-04-25</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>astrostatistics-techniques</subject><subject>milky-way-galaxy</subject><subject>astronomical-simulations</subject><description>This table gives numerical factors to be applied to the sky-averaged
astrometric errors for the different astrometric parameters as
function of ecliptic latitude β, including the effect of the variation
of the number of transits over the sky. Source:
https://www.cosmos.esa.int/web/gaia/table-2</description><source format="bibcode">2018PASP..130g4101R</source><referenceURL>https://dc.g-vo.org/tableinfo/gdr2mock.astrometric_performance2</referenceURL><type>Simulation</type><contentLevel>Research</contentLevel></content><coverage><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>gdr2mock</name><title>A Gaia DR2 mock stellar catalog</title><description> This catalogue is a simulation of the Gaia DR2 stellar content using
Galaxia (a tool to sample stars from a Besancon-like Milky Way model),
3d dust extinction maps and the latest PARSEC Isochrones. It is
mimicking the Gaia DR2 data model and an apparent magnitude limit of
g=20,7. Extinctions and photometry in different bands have also been
included in a supplementary table as well as uncertainty estimates
using a scaled nominal error model.</description><table><name>gdr2mock.astrometric_performance2</name><title>Gaia Astrometric Performance, Table 2</title><description>This table gives numerical factors to be applied to the sky-averaged
astrometric errors for the different astrometric parameters as
function of ecliptic latitude β, including the effect of the variation
of the number of transits over the sky. Source:
https://www.cosmos.esa.int/web/gaia/table-2</description><nrows>20</nrows><column><name>lat_index</name><description>Bin index, starting at 0</description><ucd>meta.id;meta.main</ucd><stats><min>0</min><percentile03>0.57</percentile03><median>9.5</median><percentile97>18.43</percentile97><max>19</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">short</dataType><flag>indexed</flag><flag>primary</flag></column><column><name>n_obs</name><description>The sky averaged number of observations at eom for a specific bin in ecliptic latitude</description><ucd>meta.number;obs</ucd><stats><min>61</min><percentile03>61.0</percentile03><median>75.0</median><percentile97>131.45999999999998</percentile97><max>144</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>alpha_ratio</name><description>The error factor to be multiplied with the nominal parallax error to derive ra error for a specific ecliptic latitude bin</description><ucd>stat.error;arith.ratio</ucd><stats><min>0.646</min><percentile03>0.6517</percentile03><median>0.8</median><percentile97>0.91772</percentile97><max>0.92</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>delta_ratio</name><description>The error factor to be multiplied with the nominal parallax error to derive dec error for a specific ecliptic latitude bin</description><ucd>stat.error;arith.ratio</ucd><stats><min>0.666</min><percentile03>0.66657</percentile03><median>0.6875</median><percentile97>0.79464</percentile97><max>0.822</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>parallax_ratio</name><description>The error factor to be multiplied with the nominal parallax error to derive parallax error for a specific ecliptic latitude bin</description><ucd>stat.error;arith.ratio</ucd><stats><min>0.7</min><percentile03>0.72337</percentile03><median>1.0445</median><percentile97>1.15486</percentile97><max>1.156</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmra_ratio</name><description>The error factor to be multiplied with the nominal parallax error to derive pmra error for a specific ecliptic latitude bin</description><ucd>stat.error;arith.ratio</ucd><stats><min>0.451</min><percentile03>0.45442</percentile03><median>0.572</median><percentile97>0.64929</percentile97><max>0.651</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmdec_ratio</name><description>The error factor to be multiplied with the nominal parallax error to derive pmdec error for a specific ecliptic latitude bin</description><ucd>stat.error;arith.ratio</ucd><stats><min>0.478</min><percentile03>0.478</percentile03><median>0.4885</median><percentile97>0.55704</percentile97><max>0.573</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>