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<ri:Resource created="2022-05-18T13:46:12Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.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:CatalogService"><title>Exoplanet X-ray irradiation and evaporation rates</title><shortName>J/A+A/661/A23</shortName><identifier>ivo://CDS.VizieR/J/A+A/661/A23</identifier><altIdentifier>doi:10.26093/cds/vizier.36610023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Foster G.</name></creator><creator><name>Poppenhaeger K.</name></creator><creator><name>Ilic N.</name></creator><creator><name>Schwope A.</name></creator><date role="Updated">2022-10-14T13:42:35Z</date><date role="Created">2022-05-18T13:46:12Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>multiple-stars</subject><subject>x-ray-sources</subject><subject>exoplanets</subject><description>High-energy irradiation is a driver for atmospheric evaporation and mass loss in exoplanets. This work is based on data from eROSITA, the soft X-ray instrument on board the Spectrum Roentgen Gamma (SRG) mission, as well as on archival data from other missions. We aim to characterise the high-energy environment of known exoplanets and estimate their mass-loss rates. We use X-ray source catalogues from eROSITA, XMM-Newton, Chandra, and ROSAT to derive X-ray luminosities of exoplanet host stars in the 0.2-2 keV energy band with an underlying coronal, that is, optically thin thermal spectrum. We present a catalogue of stellar X-ray and EUV luminosities, exoplanetary X-ray and EUV irradiation fluxes, and estimated mass-loss rates for total of 287 exoplanets, 96 of which are characterised for the first time based on new eROSITA detections. We identify 14 first-time X-ray detections of transiting exoplanets that are subject to irradiation levels known to cause observable evaporation signatures in other exoplanets. This makes them suitable targets for follow-up observations.</description><source format="bibcode">2022A&amp;A...661A..23F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/661/A23</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/17">J/ApJ/834/17 : Mass + radius of planets, moons, low mass stars (Chen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A1">J/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/661/A2">J/A+A/661/A2 : Galaxy 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