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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>2026-10-07T06:05:27Z</responseDate><request identifier="oai:gaia.aip.de:tables/gaiadr3.vari_spurious_signals" metadataPrefix="oai_dc">https://gaia.aip.de/oai</request><GetRecord><record><header><identifier>oai:gaia.aip.de:tables/gaiadr3.vari_spurious_signals</identifier><datestamp>2023-02-07</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.3/100</dc:identifier><dc:title>Variable Sources: Spurious Signals</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;Several statistics computed for all sources with published photometric time series which can help in the identification of sources that are affected by calibration issues resulting in, for example, spurious variability signals.&lt;/p&gt; &lt;p&gt;The table has a row for every source with {\tt GaiaSource.hasEpochPhotometry} set to TRUE and is described in detail in \cite{DR3-DPACP-164}.&lt;/p&gt;</dc:description><dc:date>2023-02-07</dc:date><dc:rights>BY_NC_IG</dc:rights><dc:type>Dataset</dc:type></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>