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<ri:Resource created="2009-09-28T21:30:28Z" status="active" updated="2026-03-17T20:06:40Z" 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>Symbiotic stars multi-epoch UBV(RI)c photometry</title><shortName>J/BaltA/17/293</shortName><identifier>ivo://CDS.VizieR/J/BaltA/17/293</identifier><altIdentifier>doi:10.26093/cds/vizier/bm-h-95</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Henden A.</name></creator><creator><name>Munari U.</name></creator><date role="Updated">2026-03-17T20:06:40Z</date><date role="Created">2009-09-28T21:30:28Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>kron-cousins-photometry</subject><description>We present a multi-epoch, accurate UBVRcIc photometric catalog of 83 symbiotic stars and related objects, measured while calibrating the Henden and Munari (2000, Cat. &lt;J/A+AS/143/343&gt;, 2001, Cat. &lt;J/A+A/372/145&gt;, 2006, Cat. &lt;J/A+A/458/339&gt;) photometric sequences around them. The vast majority of the observations where collected in the time interval between October 19, 1998 to April 21, 2002 with the 1.0-m Ritchey-Chretien telescope of the U.S. Naval Observatory, Flagstaff Station (Arizona). On average, UBVRcIc data are given on 3.6 epochs for each program star. The overall budget error of the data is usually better than 0.01mag.</description><source format="bibcode">2008BaltA..17..293H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/BaltA/17/293</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/A+AS/143/343">J/A+AS/143/343 : Symbiotic stars UBV(RI)c photometry. I. (Henden+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/145">J/A+A/372/145 : Symbiotic stars UBV(RI)c photometry. II. (Henden+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/339">J/A+A/458/339 : Symbiotic stars UBV(RI)c photometry. III. 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