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<ri:Resource created="2025-04-24T15:48:58Z" status="active" updated="2026-07-02T11:59:06Z" 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>GW200224_222234 follow-up survey with Subaru &amp; GTC</title><shortName>J/ApJ/947/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/947/9</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xk-9</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ohgami T.</name></creator><creator><name>Gonzalez J.B.</name></creator><creator><name>Tominaga N.</name></creator><creator><name>Morokuma T.</name></creator><creator><name>Utsumi Y.</name></creator><creator><name>Niino Y.,Tanaka M.</name></creator><creator><name>Banerjee S.</name></creator><creator><name>Poidevin F.</name></creator><creator><name>Acosta-Pulido J.A.</name></creator><creator><name>Perez-Fournon I.,Munoz-Darias T.</name></creator><creator><name>Akitaya H.</name></creator><creator><name>Yanagisawa K.</name></creator><creator><name>Sasada M.</name></creator><creator><name>Yoshida M.,Simunovic M.</name></creator><creator><name>Ohsawa R.</name></creator><creator><name>Tanaka I.</name></creator><creator><name>Terai T.</name></creator><creator><name>Takagi Y.,The J-GEM collaboration</name></creator><date role="Updated">2026-07-02T11:59:06Z</date><date role="Created">2025-04-24T15:48:58Z</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>black-holes</subject><subject>gravitational-waves</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>redshifted</subject><description>The LIGO/Virgo detected a gravitational wave (GW) event, named GW200224_222234 (also known as S200224ca) and classified as a binary-black hole coalescence, on 2020 February 24. Given its relatively small localization skymap (71deg^2^ for a 90% credible region; revised to 50deg^2^ in GWTC-3), we performed target- of-opportunity observations using the Subaru/Hyper Suprime-Cam (HSC) in the r2 and z bands. Observations were conducted on 2020 February 25 and 28 and March 23, with the first epoch beginning 12.3hr after the GW detection. The survey covered the highest-probability sky area of 56.6deg^2^, corresponding to a 91% probability. This was the first deep follow-up (m_r_&gt;~24, m_z_&gt;~23) for a binary-black hole merger covering &gt;90% of the localization. By performing image subtraction and candidate screening including light-curve fitting with transient templates and examples, we found 22 off-nucleus transients that were not ruled out as the counterparts of GW200224_222234 with our Subaru/HSC data alone. We also performed GTC/OSIRIS spectroscopy of the probable host galaxies for five candidates; two are likely to be located within the 3D skymap, whereas the others are not. In conclusion, 19 transients remain as possible optical counterparts of GW200224_222234; but we could not identify a unique promising counterpart. If there are no counterparts in the remaining candidates, the upper limits of the optical luminosity are {nu}L_{nu}_&lt;5.2_-1.9_^+2.4^x10^41^erg/s and {nu}L_{nu}_&lt;1.8_-0.6_^+0.8^x10^42^erg/s in the r2 and z bands, respectively, at ~12hr after GW detection. We also discuss improvements in the strategies of optical follow-ups for future GW events.</description><source format="bibcode">2023ApJ...947....9O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/947/9</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/745/31">J/ApJ/745/31 : HST Cluster Supernova Survey. VI. SNIa rate (Barbary+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/23">J/ApJ/794/23 : Pan-STARRS1 transients optical photometry (Drout+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/L33">J/ApJ/848/L33 : Opt. follow-up of GW events with LCO (Arcavi+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/L29">J/ApJ/848/L29 : Opt. follow-up of GW170817 counterpart (Diaz+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/848/L16">J/ApJ/848/L16 : Counterpart of GW170817. I. DECam obs. 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