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<ri:Resource created="2012-05-03T15:07:34Z" 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>Mira variables om ROTSE-IIId</title><shortName>J/other/NewA/17.</shortName><identifier>ivo://CDS.VizieR/J/other/NewA/17.504</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yesilyaprak C.</name></creator><creator><name>Yerli S.K.</name></creator><creator><name>Gucsav B.B.</name></creator><creator><name>Aksaker N.</name></creator><creator><name>Dikicioglu E.,Helvaci M.</name></creator><creator><name>Coker D.</name></creator><creator><name>Aydin M.E.</name></creator><creator><name>Dincel B.</name></creator><creator><name>Uzun N.</name></creator><date role="Updated">2017-12-15T10:54:59Z</date><date role="Created">2012-05-03T15:07:34Z</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>photometry</subject><description>We have studied the long-term variations of Mira type variables observed with Robotic Optical Transient Search Experiment telescope (ROTSE-IIId) between 2004 and 2009 located at TUBITAK National Observatory (TUG) in Antalya, Turkey. The actual pulsation periods, variability amplitudes, epochs of maximums and light curves of selected 70 Mira type variables already defined in the SIMBAD database were investigated. 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