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<ri:Resource created="2026-06-12T10:50:35Z" status="active" updated="2026-06-12T10:21:06Z" 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>HSC gLSB galaxies structures and SB properties</title><shortName>J/MNRAS/520/L85</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/520/L85</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Saburova A.S.</name></creator><creator><name>Chilingarian I.V.</name></creator><creator><name>Kulier A.</name></creator><creator><name>Galaz G.</name></creator><creator><name>Grishin K.A.,Kasparova A.V.</name></creator><creator><name>Toptun V.</name></creator><creator><name>Katkov I.Y.</name></creator><date role="Updated">2026-06-12T10:21:06Z</date><date role="Created">2026-06-12T10:50:35Z</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>ring-galaxies</subject><subject>redshifted</subject><subject>galaxy-classification-systems</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>x-ray-sources</subject><subject>active-galactic-nuclei</subject><subject>galaxy-radii</subject><subject>absolute-magnitude</subject><description>Rare giant low surface brightness galaxies (gLSBGs) act as a stress test for the current galaxy formation paradigm. To answer the question 'How rare are they?', we estimate their volume density in the local Universe. A visual inspection of 120 deg^2^ covered by deep Subaru Hyper Suprime-Cam data was performed independently by four team members. We detected 42 giant disky systems (30 of them isolated) at z &lt;= 0.1 with either g-band 27.7 mag arcsec^-2^ isophotal radius or four disc scale lengths 4h =&gt; 50 kpc, 37 of which (including 25 isolated) had low central surface brightness ({mu}_0,g_ =&gt; 22.7 mag arcsec^-2^). This corresponds to volume densities of 4.70*10^-5^ Mpc^-3^ for all galaxies with giant extended discs and 4.04*10^-5^Mpc^-3^ for gLSBGs, which converts to ~12700 such galaxies in the entire sky out to z &lt; 0.1. These estimates agree well with the result of the Evolution and Assembly of GaLaxies and their Environments (EAGLE) cosmological hydrodynamical simulation. Giant disky galaxies represent the large-sized end of the volume density distribution of normal-sized spirals, suggesting the non-exceptional nature of giant discs. We observe a high active galactic nucleus fraction among the newly found gLSBGs.</description><source format="bibcode">2023MNRAS.520L..85S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/520/L85</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/MNRAS/489/4669">J/MNRAS/489/4669 : UGC 1378's giant low surface brightness disc</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/410/166">J/MNRAS/410/166 : Morphological types from Galaxy Zoo 1 (Lintott+, 2011)</relatedResource><relatedResource 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