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<ri:Resource created="2026-08-19T14:40:29Z" status="active" updated="2026-08-19T14:33:11Z" 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>N(HI) in the local interstellar medium</title><shortName>J/AJ/170/342</shortName><identifier>ivo://CDS.VizieR/J/AJ/170/342</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Youngblood A.</name></creator><creator><name>France K.</name></creator><creator><name>Koskinen T.</name></creator><creator><name>Mason J.P.</name></creator><creator><name>Redfield S.</name></creator><creator><name>Wood B.E.,Bourrier V.</name></creator><creator><name>dos Santos L.</name></creator><creator><name>Johns-Krull C.</name></creator><creator><name>King G.W.</name></creator><creator><name>Linsky J.L.,Peacock S.</name></creator><date role="Updated">2026-08-19T14:33:11Z</date><date role="Created">2026-08-19T14:40:29Z</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>interstellar-medium</subject><subject>h-i-line-emission</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><subject>ultraviolet-sources</subject><subject>x-ray-sources</subject><description>Obtaining a complete census of gas in the local interstellar medium (LISM; &lt;100pc) is challenging given the limited available tracers of the warm, partially ionized medium. Medium- to high-resolution UV absorption spectroscopy toward individual nearby stars is the primary method used, and incomplete spatial sampling of this complex medium makes a global map of the material difficult. Using HI column density measurements derived from HI Ly{alpha} spectroscopy toward 164 stars inside 100pc, we have generated 2D spatially interpolated N(HI) maps for different distance shells. Based on the area-weighted sky averages, we find that sight lines inside 10pc typically have log_10_(N(HI)/cm^-2^)~17.9. For greater distance shells, log_10_(N(HI)/cm^-2^) increases to 18.3 (10-20pc), then to 18.4 (20-70pc), and finally to 18.6 (70-100pc). This last increase is likely associated with the detection of the Local Bubble boundary, thus making the plateau of column density from 20 to 70pc notable and suggestive of the rarity of warm LISM material beyond ~10-20pc. We estimate that the uncertainties associated with N(HI) values inferred from the interpolated sky maps are approximately inversely correlated with the number of samples in each distance shell, and are in the range of 0.20-0.48dex, compared to the 0.01-0.30dex typically determined from direct Ly{alpha} observations. We discuss the impact of these uncertainties on interstellar medium corrections of extreme-UV and Ly{alpha} observations for nearby stars. Denser spatial sampling of the sky via UV absorption spectroscopy of nearby stars is required to improve the accuracy of these N(HI) estimates.</description><source format="bibcode">2025AJ....170..342Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/170/342</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/II/203A">II/203A : Second Extreme Ultra-Violet Explorer Catalog (2EUVE, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/135A">III/135A : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/39">IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/35">IX/35 : Second EUVE Catalogues (Bowyer+, 1996-99)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/274/1165">J/MNRAS/274/1165 : The 2RE Source Catalogue (Pye+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/510/A54">J/A+A/510/A54 : NaI and CaII interstellar absorption (Welsh+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/615/A117">J/A+A/615/A117 : 55 Cnc geocoronal emission lines template (Bourrier+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/886/19">J/ApJ/886/19 : Lya obs. of low-mass stars Ross 825 &amp; 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