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<ri:Resource created="2015-07-22T13:07:57Z" 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>BGPS. XI. SHARC-II 350um observations</title><shortName>J/ApJS/218/1</shortName><identifier>ivo://CDS.VizieR/J/ApJS/218/1</identifier><altIdentifier>doi:10.26093/cds/vizier.22180001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Merello M.</name></creator><creator><name>Evans II N.J.</name></creator><creator><name>Shirley Y.L.</name></creator><creator><name>Rosolowsky E.</name></creator><creator><name>Ginsburg A.,Bally J.</name></creator><creator><name>Battersby C.</name></creator><creator><name>Dunham M.M.</name></creator><date role="Updated">2019-06-05T12:14:07Z</date><date role="Created">2015-07-22T13:07:57Z</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>surveys</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We present 107 maps of continuum emission at 350{mu}m from Galactic molecular clumps. Observed sources were mainly selected from the Bolocam Galactic Plane Survey (BGPS) catalog, with three additional maps covering star-forming regions in the outer Galaxy. The higher resolution of the SHARC-II images (8.5" beam) compared with the 1.1mm images from BGPS (33" beam) allowed us to identify a large population of smaller substructures within the clumps. A catalog is presented for the 1386 sources extracted from the 350{mu}m maps. The color temperature distribution of clumps based on the two wavelengths has a median of 13.3K and mean of 16.3+/-0.4K, assuming an opacity law index of 1.7. For the structures with good determination of color temperatures, the mean ratio of gas temperature, determined from NH_3_ observations, to dust color temperature is 0.88 and the median ratio is 0.76. About half the clumps have more than 2 substructures and 22 clumps have more than 10. The fraction of the mass in dense substructures seen at 350{mu}m compared to the mass of their parental clump is ~0.19, and the surface densities of these substructures are, on average, 2.2 times those seen in the clumps identified at 1.1mm. For a well-characterized sample, 88 structures (31%) exceed a surface density of 0.2g/cm2, and 18 (6%) exceed 1.0g/cm2, thresholds for massive star formation suggested by theorists.</description><source format="bibcode">2015ApJS..218....1M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/218/1</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/ApJ/799/29">J/ApJ/799/29 : BGPS. XII. DR2 distance catalog (Ellsworth-Bowers+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/2">J/ApJS/209/2 : The BGPS. X. 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Error in S40</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S</name><description>[0.5/4331] Integrated 350um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.mm.750-1500GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S</name><description>? 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