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<ri:Resource created="2026-05-22T09:51:43Z" status="active" updated="2026-05-22T08:54:59Z" 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>JADES and FRESCO Ha-emitting galaxies at z=5.1-5.5</title><shortName>J/ApJ/961/69</shortName><identifier>ivo://CDS.VizieR/J/ApJ/961/69</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sun F.</name></creator><creator><name>Helton J.M.</name></creator><creator><name>Egami E.</name></creator><creator><name>Hainline K.N.</name></creator><creator><name>Rieke G.H.</name></creator><creator><name>Willmer C.N.A.,Eisenstein D.J.</name></creator><creator><name>Johnson B.D.</name></creator><creator><name>Rieke M.J.</name></creator><creator><name>Robertson B.</name></creator><creator><name>Tacchella S.,Alberts S.</name></creator><creator><name>Baker W.M.</name></creator><creator><name>Bhatawdekar R.</name></creator><creator><name>Boyett K.</name></creator><creator><name>Bunker A.J.,Charlot S.</name></creator><creator><name>Chen Z.</name></creator><creator><name>Chevallard J.</name></creator><creator><name>Curtis-Lake E.</name></creator><creator><name>Danhaive A.L.,DeCoursey C.</name></creator><creator><name>Ji Z.</name></creator><creator><name>Lyu J.</name></creator><creator><name>Maiolino R.</name></creator><creator><name>Rujopakarn W.</name></creator><creator><name>Sandles L.,Shivaei I.</name></creator><creator><name>Ubler H.</name></creator><creator><name>Willott C.</name></creator><creator><name>Witstok J.</name></creator><date role="Updated">2026-05-22T08:54:59Z</date><date role="Created">2026-05-22T09:51:43Z</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>galaxies</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>infrared-photometry</subject><subject>absolute-magnitude</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><subject>surveys</subject><description>HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at z=5.18. With nine-band NIRCam images at 0.8-5.0{mu}m obtained through the JWST Advanced Deep Extragalactic Survey, we detect and resolve the rest-frame UV-optical counterpart of HDF850.1, which splits into two components because of heavy dust obscuration in the center. The southern component leaks UV and H{alpha} photons, bringing the galaxy ~100 times above the empirical relation between infrared excess and UV continuum slope (IRX-{beta}UV). The northern component is higher in dust attenuation and thus fainter in UV and H{alpha} surface brightness. We construct a spatially resolved dust-attenuation map from the NIRCam images, well matched with the dust continuum emission obtained through millimeter interferometry. The whole system hosts a stellar mass of 10^10.8{\pm}0.1^M_{sun}_ and star formation rate (SFR) of 10^2.8{\pm}0.2^M_{sun}_/yr, placing the galaxy at the massive end of the star-forming main sequence at this epoch. We further confirm that HDF850.1 resides in a complex overdense environment at z=5.17-5.30, which hosts another luminous SMG at z=5.30 (GN10). The filamentary structures of the overdensity are characterized by 109 H{alpha}-emitting galaxies confirmed through NIRCam slitless spectroscopy at 3.9-5{mu}m, of which only eight were known before the JWST observations. Given the existence of a similar galaxy overdensity in the GOODS-S field, our results suggest that 50%{\pm}20% of the cosmic star formation at z=5.1-5.5 occur in protocluster environments.</description><source format="bibcode">2024ApJ...961...69S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/961/69</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/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/159">V/159 : JADES NIRCam &amp; NIRSpec phot. &amp; line fluxes (DR1-DR3) (Rieke+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/513/34">J/ApJ/513/34 : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/358/149">J/MNRAS/358/149 : HDFN SCUBA Super-map. 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