<?xml version="1.0" encoding="utf-8"?>
<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>2026-10-11T05:18:28Z</responseDate><request identifier="oai:gaia.aip.de:tables/gaiadr3.sdssdr13_join" metadataPrefix="oai_dc">https://gaia.aip.de/oai</request><GetRecord><record><header><identifier>oai:gaia.aip.de:tables/gaiadr3.sdssdr13_join</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.3/23</dc:identifier><dc:title>SDSS DR13 Join</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;Convenience table to be used to join SDSS DR13 catalogue with the cross-match results. The table links the external catalogue original &lt;code&gt;source_id&lt;/code&gt; (&lt;code&gt;original_ext_source_id&lt;/code&gt;) to the corresponding additional numerical identifier (&lt;code&gt;clean_sdssdr13_oid&lt;/code&gt;). Both &lt;code&gt;original_ext_source_id&lt;/code&gt; and &lt;code&gt;clean_sdssdr13_oid&lt;/code&gt; are present in the cross-match output tables (&lt;code&gt;sdssdr13_best_neighbour&lt;/code&gt; and &lt;code&gt;sdssdr13_neighbourhood&lt;/code&gt;). However, in case there are suspected duplicates in the external catalogue, different &lt;code&gt;original_ext_source_id&lt;/code&gt; will correspond to the same &lt;code&gt;clean_sdssdr13_oid&lt;/code&gt;. In the cross-match output table only the &lt;code&gt;original_ext_source_id&lt;/code&gt; of the source with the best astrometry among the suspected duplicates will be listed. In practice, users may use the &lt;code&gt;original_ext_source_id&lt;/code&gt; in the original catalogue to find the matching source with the best astrometry. Users interested to find all matching suspected duplicates should instead use the &lt;code&gt;clean_sdssdr13_oid&lt;/code&gt; in the join with the cross-match result tables. See Chapter [chap:crossmatch] for more details on the duplicates in the external catalogues and their treatment in the cross-match computations.&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>