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<ri:Resource created="2025-01-27T15:01:29Z" 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>High-z protocluster candidates from COSMOS2020</title><shortName>J/ApJ/943/153</shortName><identifier>ivo://CDS.VizieR/J/ApJ/943/153</identifier><altIdentifier>doi:10.26093/cds/vizier.19430153</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brinch M.</name></creator><creator><name>Greve T.R.</name></creator><creator><name>Weaver J.R.</name></creator><creator><name>Brammer G.</name></creator><creator><name>Ilbert O.</name></creator><creator><name>Shuntov M.,Jin S.</name></creator><creator><name>Liu D.</name></creator><creator><name>Gimenez-Arteaga C.</name></creator><creator><name>Casey C.M.</name></creator><creator><name>Davidson I.</name></creator><creator><name>Fujimoto S.,Koekemoer A.M.</name></creator><creator><name>Kokorev V.</name></creator><creator><name>Magdis G.</name></creator><creator><name>McCracken H.J.</name></creator><creator><name>McPartland C.J.R.,Mobasher B.</name></creator><creator><name>Sanders D.B.</name></creator><creator><name>Toft S.</name></creator><creator><name>Valentino F.</name></creator><creator><name>Zamorani G.</name></creator><creator><name>Zavala J.,(The COSMOS Team)</name></creator><date role="Updated">2025-03-03T20:11:16Z</date><date role="Created">2025-01-27T15:01:29Z</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>galaxy-clusters</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>redshifted</subject><subject>infrared-photometry</subject><description>We conduct a systematic search for protocluster candidates at z&gt;=6 in the Cosmic Evolution Survey (COSMOS) field using the recently released COSMOS2020 source catalog. We select galaxies using a number of selection criteria to obtain a sample of galaxies that have a high probability of being inside a given redshift bin. We then apply overdensity analysis to the bins using two density estimators, a Weighted Adaptive Kernel estimator and a Weighted Voronoi Tessellation estimator. We have found 15 significant (&gt;4{sigma}) candidate galaxy overdensities across the redshift range 6&lt;=z&lt;=7.7. The majority of the galaxies appear to be on the galaxy main sequence at their respective epochs. We use multiple stellar-mass-to-halo-mass conversion methods to obtain a range of dark matter halo mass estimates for the overdensities in the range of ~10^11^-10^13^M_{sun}_, at the respective redshifts of the overdensities. The number and the masses of the halos associated with our protocluster candidates are consistent with what is expected from the area of a COSMOS-like survey in a standard {Lambda} cold dark matter cosmology. Through comparison with simulation, we expect that all of the overdensities at z~6 will evolve into Virgo-/Coma-like clusters at present (i.e., with masses ~10^14^-10^15^M_{sun}_). Compared to other overdensities identified at z&gt;=6 via narrowband selection techniques, the overdensities presented appear to have ~10x higher stellar masses and star formation rates (SFRs). We compare the evolution in the total SFR and stellar mass content of the protocluster candidates across the redshift range 6&lt;=z&lt;=7.7 and find agreement with the total average SFR from simulations.</description><source format="bibcode">2023ApJ...943..153B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/943/153</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/373">II/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/301">J/ApJS/176/301 : Subaru/XMM-Newton deep survey IV. 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