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<ri:Resource created="2007-09-03T18:08:16Z" 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>ASCA Large Sky Survey</title><shortName>J/ApJ/518/656</shortName><identifier>ivo://CDS.VizieR/J/ApJ/518/656</identifier><altIdentifier>doi:10.26093/cds/vizier.15180656</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ueda Y.</name></creator><creator><name>Takahashi T.</name></creator><creator><name>Inoue H.</name></creator><creator><name>Tsuru T.</name></creator><creator><name>Sakano M.</name></creator><creator><name>Ishisaki Y.,Ogasaka Y.</name></creator><creator><name>Makishima K.</name></creator><creator><name>Yamada T.</name></creator><creator><name>Akiyama M.</name></creator><creator><name>Ohta K.</name></creator><date role="Updated">2007-09-03T18:11:28Z</date><date role="Created">2007-09-03T18:08:16Z</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>galaxies</subject><subject>catalogs</subject><subject>x-ray-sources</subject><description>We carried out the first wide-area unbiased survey with the ASCA satellite in the 0.7-10keV band around a north Galactic-pole region covering a continuous area of 7deg^2^ (Large Sky Survey; LSS). To make the best use of ASCA's capabilities, we developed a new source-detection method in which the complicated detector responses are fully taken into account. Applying this method to the entire LSS data independently in the total (0.7-7keV), hard (2-10keV), and soft (0.7-2keV) bands, we detected 107 sources altogether, with sensitivity limits of 6x10^-14^ (0.7-7keV), 1x10^-13^ (2-10keV), and 2x10^-14^ergs/s/cm^2^ (0.7-2keV), respectively. 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