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<ri:Resource created="2011-02-14T12:00:00Z" status="active" updated="2026-03-04T11:08:16Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/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/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>HI composite survey survey collection</title><shortName>HI</shortName><identifier>ivo://CDS/P/HI</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>CDS</name></creator><date role="Created">2011-02-14T12:00:00Z</date><date role="Updated">2019-05-05T06:29:00Z</date><contact><name>CDS Helpdesk</name><email>cds-question@unistra.fr</email></contact></curation><content><subject>Sky survey</subject><subject>Radio astronomy</subject><subject>H I line emission</subject><description>Composite all-sky map of neutral hydrogen column density (N_HI), formed from the Leiden/Dwingeloo HI survey data (Hartmann &amp; Burton 1997) and the composite N_HI map of Dickey and Lockman (1990). The two datasets are not matched in sensitivity or resolution: note that discontinuities exist in the constructed composite map. A pixel mask is provided to indicate which dataset was used for each location on the sky. Hartmann &amp; Burton provide a velocity integrated (-450 km/s %3C V_lsr %3C +400 km/s) HI brightness temperature map in Galactic coordinates, sampled every 0.5 degrees. This entire data set was converted to N_HI by multiplying by their factor of 1.8224e18 K km s-1 cm-2 and then interpolated to pixel centers appropriate for HEALPix Nside=512. Since the Leiden/Dwingeloo survey does not have sky coverage for declinations %3C -30 deg., the lower resolution Dickey &amp; Lockman map was also interpolated to HEALPix and used to fill in the coverage gap. The Dickey &amp; Lockman N_HI map is itself a composite of several surveys which had been merged and averaged onto 1 deg. bins in Galactic coordinates. Their map includes emission between -250 km/s %3C V_lsr %3C 250 km/s (excluding the LMC and SMC). The Leiden/Dwingeloo Survey data were obtained from the CDS. The Dickey &amp; Lockman map was obtained from NCSA ADIL. This original HEALPix file is distributed and maintained by LAMBDA.Original acknowledgement for data: We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center.</description><source format="bibcode">1990ARA&amp;A..28..215D</source><referenceURL>https://alasky.cds.unistra.fr/HI</referenceURL><type>Survey</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsDerivedFrom</relationshipType><relatedResource>HEASARC/LAMBDA</relatedResource></relationship></content><rights rightsURI="https://cds.unistra.fr/aladin-org/licences_aladin.html">This HiPS is distributed under ODbL license by Unistra/CNRS</rights><capability standardID="ivo://ivoa.net/std/hips#hips-1.0"><interface role="std" xsi:type="vs:ParamHTTP"><accessURL use="base">https://alasky.cds.unistra.fr/HI</accessURL><mirrorURL>https://alaskybis.cds.unistra.fr/HI</mirrorURL></interface></capability><coverage><temporal>44239 47892</temporal><spectral>9.45926598642347e-25 9.45926598642347e-25</spectral><footprint ivo-id="ivo://mocivod">https://alasky.cds.unistra.fr/HI/Moc.fits</footprint><waveband>Radio</waveband></coverage></ri:Resource>