<?xml version='1.0'?><?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?><ri:Resource created="2022-06-20T10:00:00Z" 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>Monte Carlo Sampled DR3 XP Spectra with Basic Object Information</title><shortName>gdr3spec.withpos</shortName><identifier>ivo://org.gavo.dc/gaia/s3/withpos</identifier><altIdentifier>doi:10.21938/W:hWbPah3wBabuqewQULTA</altIdentifier><curation><publisher>The GAVO DC team</publisher><creator><name>Demleitner, M.</name></creator><creator><name>Andrae, R.</name></creator><date role="Updated">2022-11-07T08:46:33Z</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>spectroscopy</subject><description>This table contains the data from gdr3spec.spectra plus position and
photometry from gaia.dr3lite. It is a view, and there is generally no
advantage to using it instead of manually performing the join.</description><source format="bibcode">2022arXiv220800211G</source><referenceURL>https://dc.g-vo.org/tableinfo/gdr3spec.withpos</referenceURL></content><facility>Gaia</facility><instrument>Gaia BP/BP Spectrometer</instrument><coverage><spatial>0/0-11</spatial><temporal>56863 57901</temporal><spectral>1.986e-19 4.966e-19</spectral><waveband>Optical</waveband></coverage><tableset><schema><name>gdr3spec</name><title>Gaia DR3 RP/BP (XP) Monte Carlo sampled spectra</title><description>
This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral
Data Model.  It presents the continous spectra in sampled form, using a
Monte Carlo scheme to decorrelate errors, elaborated in this resource's
reference URL.  The underlying tables are also available for querying
through TAP, which opens some powerful methods for mass-analysing the data.</description><table><name>gdr3spec.withpos</name><title>Monte Carlo Sampled DR3 XP Spectra with Basic Object Information</title><description>This table contains the data from gdr3spec.spectra plus position and
photometry from gaia.dr3lite. It is a view, and there is generally no
advantage to using it instead of manually performing the join.</description><nrows>219196404</nrows><column><name>source_id</name><description>Gaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.</description><ucd>meta.id;meta.main</ucd><stats><min>1511828647680</min><percentile03>4.59792466834312e+17</percentile03><median>4.280400489214347e+18</median><percentile97>6.707472532802898e+18</percentile97><max>6917528993283204480</max><fillFactor>1.0</fillFactor></stats><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>ra</name><description>Barycentric Right Ascension in ICRS at epoch J2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><stats><min>1.63271e-06</min><percentile03>44.3559</percentile03><median>260.257</median><percentile97>327.932</percentile97><max>360</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>dec</name><description>Barycentric Declination in ICRS at epoch J2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><stats><min>-89.8559</min><percentile03>-69.306</percentile03><median>-25.658</median><percentile97>58.8287</percentile97><max>89.8089</max><fillFactor>1</fillFactor></stats><dataType xsi:type="vs:VOTableType">double</dataType><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>0.00389233</min><percentile03>0.02618</percentile03><median>0.369316</median><percentile97>12.7472</percentile97><max>99.9676</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>0.00447133</min><percentile03>0.025267</percentile03><median>0.340719</median><percentile97>10.0849</percentile97><max>99.9479</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. To obtain error estimates, see phot_g_mean_flux_over_error.</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.mean</ucd><stats><min>1.77328</min><percentile03>15.5068</percentile03><median>19.7229</median><percentile97>21.0333</percentile97><max>22.7507</max><fillFactor>0.996994</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phot_bp_mean_mag</name><description>Mean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><stats><min>2.398</min><percentile03>15.8911</percentile03><median>20.2943</median><percentile97>21.8565</percentile97><max>25.3161</max><fillFactor>0.851071</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>phot_rp_mean_mag</name><description>Mean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><stats><min>1.96874</min><percentile03>14.5404</percentile03><median>18.6043</median><percentile97>20.2599</percentile97><max>24.6407</max><fillFactor>0.85822</fillFactor></stats><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flux</name><description>mean BP + RP combined spectrum flux</description><unit>W.m**-2.nm**-1</unit><ucd>phot.flux;em.opt</ucd><dataType arraysize="41" xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>flux_error</name><description>mean BP + RP combined spectrum flux error</description><unit>W.m**-2.nm**-1</unit><ucd>stat.error;phot.flux;em.opt</ucd><dataType arraysize="41" xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>