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<ri:Resource created="2026-06-30T16:27:37Z" status="active" updated="2026-07-08T00:00:00Z" 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>Galaxies of Euclid (Q1)</title><shortName>J/A+A/711/A20</shortName><identifier>ivo://CDS.VizieR/J/A+A/711/A20</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Euclid Collaboration: Matamoro Zatarain T.</name></creator><creator><name>Fotopoulou S.</name></creator><creator><name>Ricci F.,Bolzonella M.</name></creator><creator><name>La Franca F.</name></creator><creator><name>Viitanen A.</name></creator><creator><name>Zamorani G.</name></creator><creator><name>Taylor M.B.,Mezcua M.</name></creator><creator><name>Laloux B.</name></creator><creator><name>Bongiorno A.</name></creator><creator><name>Jahnke K.</name></creator><creator><name>Stevens G.</name></creator><creator><name>Shaw R.A.,Bisigello L.</name></creator><creator><name>Roster W.</name></creator><creator><name>Fu Y.</name></creator><creator><name>Margalef-Bentabol B.</name></creator><creator><name>La Marca A.,Tarsitano F.</name></creator><creator><name>Feltre A.</name></creator><creator><name>Calhau J.</name></creator><creator><name>Lopez Lopez X.</name></creator><creator><name>Scialpi M.</name></creator><creator><name>Salvato M.,Allevato V.</name></creator><creator><name>Siudek M.</name></creator><creator><name>Saulder C.</name></creator><creator><name>Vergani D.</name></creator><creator><name>Bremer M.N.</name></creator><creator><name>Wang L.,Giulietti M.</name></creator><creator><name>Alexander D.M.</name></creator><creator><name>Sluse D.</name></creator><creator><name>Shankar F.</name></creator><creator><name>Spinoglio L.</name></creator><creator><name>Scott D.,Shirley R.</name></creator><creator><name>Landt H.</name></creator><creator><name>Selwood M.</name></creator><creator><name>Toba Y.</name></creator><creator><name>Dayal P.</name></creator><creator><name>Aghanim N.</name></creator><creator><name>Altieri B.,Amara A.</name></creator><creator><name>Andreon S.</name></creator><creator><name>Auricchio N.</name></creator><creator><name>Aussel H.</name></creator><creator><name>Baccigalupi C.</name></creator><creator><name>Baldi M.,Bardelli S.</name></creator><creator><name>Basset A.</name></creator><creator><name>Battaglia P.</name></creator><creator><name>Biviano A.</name></creator><creator><name>Bonchi A.</name></creator><creator><name>Branchini E.,Brescia M.</name></creator><creator><name>Brinchmann J.</name></creator><creator><name>Camera S.</name></creator><creator><name>Canas-Herrera G.</name></creator><creator><name>Capobianco V.,Carbone C.</name></creator><creator><name>Carretero J.</name></creator><creator><name>Casas S.</name></creator><creator><name>Castander F.J.</name></creator><creator><name>Castellano M.,Castignani G.</name></creator><creator><name>Cavuoti S.</name></creator><creator><name>Chambers K.C.</name></creator><creator><name>Cimatti A.</name></creator><creator><name>Colodro-Conde C.,Congedo G.</name></creator><creator><name>Conselice C.J.</name></creator><creator><name>Conversi L.</name></creator><creator><name>Copin Y.</name></creator><creator><name>Courbin F.,Courtois H.M.</name></creator><creator><name>Cropper M.</name></creator><creator><name>Da Silva A.</name></creator><creator><name>Degaudenzi H.</name></creator><creator><name>De Lucia G.,Di Giorgio A.M.</name></creator><creator><name>Dolding C.</name></creator><creator><name>Dole H.</name></creator><creator><name>Dubath F.</name></creator><creator><name>Duncan C.A.J.</name></creator><creator><name>Dupac X.,Dusini S.</name></creator><creator><name>Ealet A.</name></creator><creator><name>Escoffier S.</name></creator><creator><name>Fabricius M.</name></creator><creator><name>Farina M.</name></creator><creator><name>Farinelli R.,Faustini F.</name></creator><creator><name>Ferriol S.</name></creator><creator><name>Finelli F.</name></creator><creator><name>Fourmanoit N.</name></creator><creator><name>Frailis M.,Franceschi E.</name></creator><creator><name>Galeotta S.</name></creator><creator><name>George K.</name></creator><creator><name>Gillis B.</name></creator><creator><name>Giocoli C.,Gomez-Alvarez P.</name></creator><creator><name>Gracia-Carpio J.</name></creator><creator><name>Granett B.R.</name></creator><creator><name>Grazian A.</name></creator><creator><name>Grupp F.,Gwyn S.</name></creator><creator><name>Haugan S.V.H.</name></creator><creator><name>Hoekstra H.</name></creator><creator><name>Holmes W.</name></creator><creator><name>Hook I.M.</name></creator><creator><name>Hormuth F.,Hornstrup A.</name></creator><creator><name>Hudelot P.</name></creator><creator><name>Jhabvala M.</name></creator><creator><name>Keihaenen E.</name></creator><creator><name>Kermiche S.,Kiessling A.</name></creator><creator><name>Kubik B.</name></creator><creator><name>Kuemmel M.</name></creator><creator><name>Kunz M.</name></creator><creator><name>Kurki-Suonio H.</name></creator><creator><name>Le Boulc'h Q.,Le Brun A.M.C.</name></creator><creator><name>Le Mignant D.</name></creator><creator><name>Liebing P.</name></creator><creator><name>Ligori S.</name></creator><creator><name>Lilje P.B.,Lindholm V.</name></creator><creator><name>Lloro I.</name></creator><creator><name>Mainetti G.</name></creator><creator><name>Maino D.</name></creator><creator><name>Maiorano E.</name></creator><creator><name>Mansutti O.,Marcin S.</name></creator><creator><name>Marggraf O.</name></creator><creator><name>Martinelli M.</name></creator><creator><name>Martinet N.</name></creator><creator><name>Marulli F.</name></creator><creator><name>Massey R.,Masters D.C.</name></creator><creator><name>Maurogordato S.</name></creator><creator><name>Medinaceli E.</name></creator><creator><name>Mei S.</name></creator><creator><name>Melchior M.,Mellier Y.</name></creator><creator><name>Meneghetti M.</name></creator><creator><name>Merlin E.</name></creator><creator><name>Meylan G.</name></creator><creator><name>Mora A.</name></creator><creator><name>Moresco M.,Moscardini L.</name></creator><creator><name>Nakajima R.</name></creator><creator><name>Neissner C.</name></creator><creator><name>Niemi S.-M.</name></creator><creator><name>Nightingale J.W.,Padilla C.</name></creator><creator><name>Paltani S.</name></creator><creator><name>Pasian F.</name></creator><creator><name>Pedersen K.</name></creator><creator><name>Percival W.J.</name></creator><creator><name>Pettorino V.,Pires S.</name></creator><creator><name>Polenta G.</name></creator><creator><name>Poncet M.</name></creator><creator><name>Popa L.A.</name></creator><creator><name>Pozzetti L.</name></creator><creator><name>Raison F.,Rebolo R.</name></creator><creator><name>Renzi A.</name></creator><creator><name>Rhodes J.</name></creator><creator><name>Riccio G.</name></creator><creator><name>Romelli E.</name></creator><creator><name>Roncarelli M.,Rossetti E.</name></creator><creator><name>Rottgering H.J.A.</name></creator><creator><name>Rusholme B.</name></creator><creator><name>Saglia R.</name></creator><creator><name>Sakr Z.,Sanchez A.G.</name></creator><creator><name>Sapone D.</name></creator><creator><name>Sartoris B.</name></creator><creator><name>Schewtschenko J.A.</name></creator><creator><name>Schneider P.,Schrabback 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A.,Zerbi F.M.</name></creator><creator><name>Zinchenko I.A.</name></creator><creator><name>Zucca E.</name></creator><creator><name>Ballardini M.</name></creator><creator><name>Bozzo E.</name></creator><creator><name>Burigana C.,Cabanac R.</name></creator><creator><name>Cappi A.</name></creator><creator><name>Di Ferdinando D.</name></creator><creator><name>Escartin Vigo J.A.</name></creator><creator><name>Fabbian G.,Gabarra L.</name></creator><creator><name>Martin-Fleitas J.</name></creator><creator><name>Matthew S.</name></creator><creator><name>Mauri N.</name></creator><creator><name>Metcalf R.B.,Pezzotta A.</name></creator><creator><name>Poentinen M.</name></creator><creator><name>Porciani C.</name></creator><creator><name>Risso I.</name></creator><creator><name>Scottez V.</name></creator><creator><name>Sereno M.,Tenti M.</name></creator><creator><name>Viel M.</name></creator><creator><name>Wiesmann M.</name></creator><creator><name>Akrami Y.</name></creator><creator><name>Andika I.T.</name></creator><creator><name>Anselmi S.,Archidiacono M.</name></creator><creator><name>Atrio-Barandela F.</name></creator><creator><name>Benoist C.</name></creator><creator><name>Benson K.</name></creator><creator><name>Bertacca D.,Bethermin M.</name></creator><creator><name>Blanchard A.</name></creator><creator><name>Blot L.</name></creator><creator><name>Boehringer H.</name></creator><creator><name>Brown M.L.</name></creator><creator><name>Bruton S.,Calabro A.</name></creator><creator><name>Camacho Quevedo B.</name></creator><creator><name>Caro F.</name></creator><creator><name>Carvalho C.S.</name></creator><creator><name>Castro T.,Cogato F.</name></creator><creator><name>Contini T.</name></creator><creator><name>Cooray A.R.</name></creator><creator><name>Cucciati O.</name></creator><creator><name>Davini S.</name></creator><creator><name>De Paolis F.,Desprez G.</name></creator><creator><name>Diaz-Sanchez A.</name></creator><creator><name>Diaz J.J.</name></creator><creator><name>Di Domizio S.</name></creator><creator><name>Diego J.M.,Duc P.-A.</name></creator><creator><name>Enia A.</name></creator><creator><name>Fang Y.</name></creator><creator><name>Ferrari A.G.</name></creator><creator><name>Finoguenov A.</name></creator><creator><name>Fontana A.,Fontanot F.</name></creator><creator><name>Franco A.</name></creator><creator><name>Ganga K.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Gasparetto T.,Gautard V.</name></creator><creator><name>Gaztanaga E.</name></creator><creator><name>Giacomini F.</name></creator><creator><name>Gianotti F.</name></creator><creator><name>Gozaliasl G.,Gregorio A.</name></creator><creator><name>Guidi M.</name></creator><creator><name>Gutierrez C.M.</name></creator><creator><name>Hall A.</name></creator><creator><name>Hartley W.G.</name></creator><creator><name>Hemmati S.,Hernandez-Monteagudo C.</name></creator><creator><name>Hildebrandt H.</name></creator><creator><name>Hjorth J.</name></creator><creator><name>Kajava J.J.E.</name></creator><creator><name>Kang Y.,Kansal V.</name></creator><creator><name>Karagiannis D.</name></creator><creator><name>Kiiveri K.</name></creator><creator><name>Kirkpatrick C.C.</name></creator><creator><name>Kruk S.,Legrand L.</name></creator><creator><name>Lembo M.</name></creator><creator><name>Lepori F.</name></creator><creator><name>Leroy G.</name></creator><creator><name>Lesci G.F.</name></creator><creator><name>Lesgourgues J.,Leuzzi L.</name></creator><creator><name>Liaudat T.I.</name></creator><creator><name>Loureiro A.</name></creator><creator><name>Macias-Perez J.</name></creator><creator><name>Maggio G.,Magliocchetti M.</name></creator><creator><name>Magnier E.A.</name></creator><creator><name>Mannucci F.</name></creator><creator><name>Maoli R.</name></creator><creator><name>Martins C.J.A.P.,Maurin L.</name></creator><creator><name>Miluzio M.</name></creator><creator><name>Monaco P.</name></creator><creator><name>Moretti C.</name></creator><creator><name>Morgante G.</name></creator><creator><name>Murray C.,Naidoo K.</name></creator><creator><name>Navarro-Alsina A.</name></creator><creator><name>Nesseris S.</name></creator><creator><name>Passalacqua F.</name></creator><creator><name>Paterson K.,Patrizii L.</name></creator><creator><name>Pisani A.</name></creator><creator><name>Potter D.</name></creator><creator><name>Quai S.</name></creator><creator><name>Radovich M.</name></creator><creator><name>Rocci P.-F.,Rodighiero G.</name></creator><creator><name>Sacquegna S.</name></creator><creator><name>Sahlen M.</name></creator><creator><name>Sanders D.B.</name></creator><creator><name>Sarpa E.,Schneider A.</name></creator><creator><name>Schultheis M.</name></creator><creator><name>Sciotti D.</name></creator><creator><name>Sellentin E.</name></creator><creator><name>Shulevski A.,Smith L.C.</name></creator><creator><name>Stanford S.A.</name></creator><creator><name>Tanidis K.</name></creator><creator><name>Testera G.</name></creator><creator><name>Teyssier R.</name></creator><creator><name>Tosi S.,Troja A.</name></creator><creator><name>Tucci M.</name></creator><creator><name>Valieri C.</name></creator><creator><name>Venhola A.</name></creator><creator><name>Verza G.</name></creator><creator><name>Vielzeuf P.,Walton N.A.</name></creator><creator><name>Soubrie E.</name></creator><date role="Updated">2026-06-30T15:40:05Z</date><date role="Created">2026-06-30T16:27:37Z</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>active-galactic-nuclei</subject><subject>quasars</subject><subject>surveys</subject><description>We present three catalogues of candidate active galactic nuclei (AGN) in the Euclid Quick Release (Q1) fields. For each Euclid source we collect multi-wavelength photometric and spectroscopic information from surveys such as the Galaxy Evolution Explorer (GALEX), Gaia, Dark Energy Survey (DES), Wide-field Infrared Survey Explorer (WISE), Spitzer, Dark Energy Spectroscopic Instrument (DESI), and Sloan Digital Sky Survey (SDSS), including spectroscopic redshifts from public compilations when available. We investigate the AGN content of the Q1 fields using multiple selection methods. Applying Euclid colours and WISE-AllWISE cuts, we identify 292222 and 65131 candidates, respectively. We compile a high-purity QSO catalogue based on Gaia DR3 information, containing 1971 candidates. Using spectroscopic information from DESI, we perform broad-line and narrow-line AGN selections, yielding 4392 AGN candidates across the Q1 fields. We investigate and refine the Euclid Q1 probabilistic random forest QSO population, selecting a refined sample of 180666 candidates. Additionally, we perform SED fitting on sources with available z_spec_ and, utilizing the derived AGN fraction, identify 7766 AGN candidates. To improve selection purity, we define two new colour criteria (JH_IeY and IeH_gz), finding 313714 and 267513 candidates, respectively, across the Q1 fields. We find a total of 229779 AGN candidates equivalent to an AGN surface density of 3641 deg^{-2} for 18&lt;Ie&lt;=24.5, and a subsample of 30422 candidates corresponding to an AGN surface density of 482 deg^{-2} when limiting the depth to 18&lt;Ie&lt;=22. The AGN surface densities recove</description><source format="bibcode">2026A&amp;A...711A..20E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/711/A20</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/II/388">II/388 : Euclid final merged catalog. Q1 data release</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A10">J/A+A/711/A10 : Euclid (Q1). Census of dwarf galaxies (Euclid Coll., 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A16">J/A+A/711/A16 : X-ray point-like sources of Euclid (Q1) (Euclid Coll.+, 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A37">J/A+A/711/A37 : Ultracool dwarfs in Euclid Deep Fields (Zerjal+, 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A38">J/A+A/711/A38 : Euclid Q1. Photometric studies of known transients</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A39">J/A+A/711/A39 : Euclid Q1. Secondary nuclei in ET galaxies (Fabricius+, 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A20">J/A+A/711/A20 : Galaxies of Euclid (Q1) (Euclid Coll.+, 2026)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/711/A24">J/A+A/711/A24 : Euclid Q1. 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WISE-AllWISE declination (J2000.0) (dec_allwise)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>GoodFlags</name><description>[0/1] Cleaning implemented to keep only those sources with `good flags' (good_flags) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BrightVmagbin</name><description>[0/1] Bright Ie magnitude bin: 18&lt;Ie&lt;=21 (bright_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MediumVmagbin</name><description>[0/1] Medium Ie magnitude bin: 21&lt;Ie&lt;=22 (medium_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FaintVmagbin</name><description>[0/1] Faint Ie magnitude bin: 22&lt;Ie&lt;=24.5 (faint_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandGaia</name><description>[0/1] Stellar candidate based on Gaia's proper motion and parallax (star_candidate_gaia) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandPRF</name><description>[0/1] Stellar candidate based on Probabilistic Random Forest (PRF) star probability &gt;0.7 (star_candidate_PRF) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandAll</name><description>[0/1] Stellar candidate based on CandGaia and/or CandPRF (star_candidate_all) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PRFQSOCand</name><description>[0/1] QSO candidate based on PRF QSO probability&gt;0.95 (PRF_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B24aQSOCand</name><description>[0/1] QSO candidate based on B24A (B24a_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>C75AGNCand</name><description>[0/1] AGN candidate based on C75 (C75_agn_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R90AGNCand</name><description>[0/1] AGN candidate based on R90 (R90_agn_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GDR3QSOCand</name><description>[0/1] QSO candidate based on GDR3-QSO (GDR3_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JHIeYQSOCand</name><description>[0/1] QSO candidate based on JH_IeY (JH_IeY_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IeHgzQSOCand</name><description>[0/1] QSO candidate based on IeH_gz (IeH_gz_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/711/A20/edff</name><description>Catalogue of sources for the EDF-F</description><column><name>DE3deg</name><description>? DES declination (J2000.0) (dec_des)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>Allwise</name><description>? WISE-AllWISE unique source identifier (object_id_allwise)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>RA4deg</name><description>? WISE-AllWISE right ascension (J2000.0) (ra_allwise)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Euclid</name><description>Euclid unique source identifier (object_id_euclid)</description><ucd>meta.id;meta.main</ucd></column><column><name>RAJ2000</name><description>Euclid right ascension (J2000.0) (ra_euclid)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Euclid declination (J2000.0) (dec_euclid)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Galex</name><description>? GALEX source identifier (object_id_galex)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>RA1deg</name><description>? GALEX right ascension (J2000.0) (ra_galex)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE1deg</name><description>? GALEX declination (J2000.0) (dec_galex)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>Gaia</name><description>? Gaia unique source identifier (object_id_gaia)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>RA2deg</name><description>? Gaia right ascension (ICRS) at Ep=2016.0 (ra_gaia)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE2deg</name><description>? Gaia declination (ICRS) at Ep=2016.0 (dec_gaia)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>DES</name><description>? DES unique identifier for the coadded objects (object_id_des)</description><ucd>meta.id</ucd><flag>nullable</flag></column><column><name>RA3deg</name><description>? DES right ascension (J2000.0) (ra_des)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DE4deg</name><description>? WISE-AllWISE declination (J2000.0) (dec_allwise)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag></column><column><name>GoodFlags</name><description>[0/1] Cleaning implemented to keep only those sources with `good flags' (good_flags) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BrightVmagbin</name><description>[0/1] Bright Ie magnitude bin: 18&lt;Ie&lt;=21 (bright_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MediumVmagbin</name><description>[0/1] Medium Ie magnitude bin: 21&lt;Ie&lt;=22 (medium_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FaintVmagbin</name><description>[0/1] Faint Ie magnitude bin: 22&lt;Ie&lt;=24.5 (faint_vis_mag_bin) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandGaia</name><description>[0/1] Stellar candidate based on Gaia's proper motion and parallax (star_candidate_gaia) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandPRF</name><description>[0/1] Stellar candidate based on Probabilistic Random Forest (PRF) star probability &gt; 0.7 (star_candidate_PRF) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CandAll</name><description>[0/1] Stellar candidate based on CandGaia and/or CandPRF (star_candidate_all) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PRFQSOCand</name><description>[0/1] QSO candidate based on PRF QSO probability&gt;0.95 (PRF_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B24aQSOCand</name><description>[0/1] QSO candidate based on B24A (B24a_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>C75AGNCand</name><description>[0/1] AGN candidate based on C75 (C75_agn_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R90AGNCand</name><description>[0/1] AGN candidate based on R90 (R90_agn_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GDR3QSOCand</name><description>[0/1] QSO candidate based on GDR3-QSO (GDR3_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JHIeYQSOCand</name><description>[0/1] QSO candidate based on JH_IeY (JH_IeY_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IeHgzQSOCand</name><description>[0/1] QSO candidate based on IeH_gz (IeH_gz_qso_candidate) (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>