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<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-10-14T17:58:36Z</responseDate><request identifier="oai:gaia.aip.de:tables/gaiadr3.mcmc_samples_gsp_phot" metadataPrefix="oai_dc">https://gaia.aip.de/oai/</request><GetRecord><record><header><identifier>oai:gaia.aip.de:tables/gaiadr3.mcmc_samples_gsp_phot</identifier><datestamp>2022-06-13</datestamp><setSpec>tables</setSpec></header><metadata><oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>10.17876/gaia/dr.3/45</dc:identifier><dc:title>MCMC samples for GSP from Photometry</dc:title><dc:creator>European Space Agency (ESA)</dc:creator><dc:creator>DPAC Consortium</dc:creator><dc:subject>Astronomy</dc:subject><dc:publisher>Leibniz Institute for Astrophysics Potsdam (AIP)</dc:publisher><dc:description>&lt;p&gt;This is the DataLink table hosting Monte-Carlo Markov Chain (MCMC) samples for the posterior probability distribution of all parameters derived from the General Stellar Parametrizer from Photometry (GSP-Phot, see Section&amp;nbsp;&lt;a href="ssec:cu8par_apsis_gspphot"&gt;cu8par_apsis_gspphot&lt;/a&gt; in the online documentation). 2000 MCMC samples are provided for 1) all sources brighter than G=12, 2) a random subset of 0.1% of the sources fainter than G=12. For all other sources fainter than G=12, the sample size is 100 (the last 100 samples in the MCMC).The table considers the following parameters:&lt;ul&gt; &lt;li&gt; effective temperature T&lt;sub&gt;eff&lt;/sub&gt; in K &lt;li&gt; monochromatic extinction at 547.7~nm A&lt;sub&gt;0&lt;/sub&gt; in mag &lt;li&gt; surface gravity log g &lt;li&gt; metallicity [M/H] &lt;li&gt; G-band extinction in mag &lt;li&gt; absolute magnitude M&lt;sub&gt;G&lt;/sub&gt; in mag &lt;li&gt; distance in pc &lt;li&gt; G&lt;sub&gt;BP&lt;/sub&gt; band extinction A&lt;sub&gt;BP&lt;/sub&gt; in mag &lt;li&gt; G&lt;sub&gt;RP&lt;/sub&gt; band extinction A&lt;sub&gt;RP&lt;/sub&gt; in mag &lt;li&gt; reddening E(G&lt;sub&gt;BP&lt;/sub&gt; - G&lt;sub&gt;RP&lt;/sub&gt;) = A&lt;sub&gt;BP&lt;/sub&gt; - A&lt;sub&gt;RP&lt;/sub&gt; in mag &lt;li&gt; logarithmic posterior probability &lt;li&gt; logarithmic likelihood &lt;li&gt; stellar radius in R&lt;sub&gt;&amp;#8857;&lt;/sub&gt; &lt;/ul&gt;&lt;/p&gt;</dc:description><dc:date>2022-06-13</dc:date><dc:rights>BY_NC_IG</dc:rights><dc:type>Dataset</dc:type></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>