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<ri:Resource created="2022-11-28T08:30:26Z" status="active" updated="2025-06-13T15:25:00Z" 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>A CO survey of the entire northern sky</title><shortName>J/ApJS/262/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/262/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22620005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dame T.M.</name></creator><creator><name>Thaddeus P.</name></creator><date role="Updated">2023-01-10T08:25:26Z</date><date role="Created">2022-11-28T08:30:26Z</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>molecular-clouds</subject><subject>co-line-emission</subject><subject>interstellar-medium</subject><subject>molecular-physics</subject><subject>surveys</subject><subject>radio-spectroscopy</subject><description>We present a very large extension of the Galactic plane CO survey of Dame+ (2001ApJ...547..792D) to the entire northern sky ({delta}&gt;-17{deg}). The extension was carried out with the same telescope as was used for the plane survey, the CfA 1.2m, and perfectly meshes with its irregular boundaries in latitude. A total of 382,202 CO(1-0) spectra uniformly sample the high-latitude sky with a true-angle spacing of 0.25{deg} or better. The final reduced and folded spectra have a uniform sensitivity of 0.18K in 0.65km/s channels and provide a velocity coverage of +/-47.1km/s. We describe the observational techniques and the data reduction and provide various summary maps of the spatial and velocity distributions of CO emission over the northern sky, and a catalog of the molecular clouds we found there. We also describe the CO spectral line data cubes that we have made available online.</description><source format="bibcode">2022ApJS..262....5D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/5</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/ApJS/196/18">J/ApJS/196/18 : CO survey of galactic molecular clouds. II. 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