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<ri:Resource created="2026-05-07T16:03:36Z" status="active" updated="2026-05-18T11:40:52Z" 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>INT monitoring of Local Grp. VII. IC 10 photometry</title><shortName>J/AJ/170/54</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/54</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gholami M.</name></creator><creator><name>Javadi A.</name></creator><creator><name>Mahani H.</name></creator><creator><name>van Loon J.T.</name></creator><creator><name>Khosroshahi H.,Saremi E.</name></creator><creator><name>McDonald I.</name></creator><creator><name>Eftekhari S.</name></creator><creator><name>Ren Yi</name></creator><creator><name>Altafi H.</name></creator><date role="Updated">2026-05-18T11:40:52Z</date><date role="Created">2026-05-07T16:03:36Z</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>variable-stars</subject><subject>dwarf-galaxies</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>galaxies</subject><subject>local-group</subject><description>To identify long-period variable (LPV) stars in IC 10-the nearest starburst galaxy of the Local Group-we conducted an optical monitoring survey using the 2.5m Isaac Newton Telescope with the wide-field camera (WFC) in the i band and V band from 2015 to 2017. We created a photometric catalog for 53,579 stars within the area of CCD4 of WFC (~0.07deg^2^ corresponding to 13.5kpc^2^ at the distance of IC 10), of which we classified 536 and 380 stars as LPV candidates, mostly asymptotic giant branch (AGBs) stars and red supergiants, within CCD4 and two half-light radii of IC 10, respectively. By comparing our output catalog to the catalogs from Pan-STARRS, Spitzer Space Telescope, Hubble Space Telescope (HST), and carbon stars from the Canada- France-Hawai'i Telescope survey, we determined the success of our detection method. We recovered ~73% of Spitzer's sources in our catalog and demonstrated that our survey successfully identified 43% of the variable stars found with Spitzer, and also retrieved 40% of the extremely dusty AGB stars among the Spitzer variables. In addition, we successfully identified ~70% of HST variables in our catalog. Furthermore, we found all the confirmed LPVs that Gaia DR3 detected in IC 10 among our identified LPVs. This paper is the first in a series on IC 10, presenting the variable star survey methodology and the photometric catalog, available to the public through the Centre de Donnees Astronomiques de Strasbourg.</description><source format="bibcode">2025AJ....170...54G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/54</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/355">I/355 : Gaia DR3 Part 1. 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