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ivo-id="ivo://CDS">CDS</publisher><creator><name>Lockman F.J.</name></creator><creator><name>Murphy E.M.</name></creator><creator><name>Petty-Powell S.</name></creator><creator><name>Urick V.J.</name></creator><date role="Updated">2018-01-02T13:43:10Z</date><date role="Created">2009-09-06T11:59:26Z</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>h-i-line-emission</subject><subject>surveys</subject><subject>radial-velocity</subject><subject>diffuse-molecular-clouds</subject><description>Very sensitive HI 21cm observations have been made in 860 directions at {delta}&gt;=-43{deg} in search of weak, Galactic, high-velocity HI emission lines at moderate and high Galactic latitudes.</description><source 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