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<ri:Resource created="1998-11-08T11:02:16Z" 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>PHA I observations</title><shortName>J/A+AS/132/233</shortName><identifier>ivo://CDS.VizieR/J/A+AS/132/233</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Xu J.</name></creator><creator><name>Li D.</name></creator><creator><name>Liu J.</name></creator><creator><name>Cheng H.</name></creator><creator><name>Zhang Z.</name></creator><creator><name>Raschotin S.I.,Emeliyanov V.A.</name></creator><creator><name>Kaplenko V.V.</name></creator><creator><name>Zalutsky V.T.</name></creator><date role="Updated">1998-11-08T10:03:59Z</date><date role="Created">1998-11-08T11:02:16Z</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>optical-observation</subject><subject>catalogs</subject><subject>astrometry</subject><description>The Photoelectric Astrolabe Mark I (PHA I) has been revised with a new combined prism which could work as an almucantar with zenith distance of 45 degree, to measure continuous declinations at the latitude of Irkutsk, Russia ({phi}=52 degree). The PHA I has been working at the astronomical base of VS NIIFTRI in Irkutsk since Nov. 1995, based on an international cooperation agreement of near 4 years for star catalogue and EOP measurements. 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