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<ri:Resource created="2022-03-31T07:42:46Z" status="active" updated="2025-05-19T09:50:00Z" 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>The SCOPE 850um compact source catalogue</title><shortName>J/MNRAS/485/2895</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/485/2895</identifier><altIdentifier>doi:10.26093/cds/vizier.74852895</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Eden D.J.</name></creator><creator><name>Liu T.</name></creator><creator><name>Kim K.-T.</name></creator><creator><name>Juvela M.</name></creator><creator><name>Liu S.-Y.</name></creator><creator><name>Tatematsu K.,Di Francesco J.</name></creator><creator><name>Wang K.</name></creator><creator><name>Wu Y.</name></creator><creator><name>Thompson M.A.</name></creator><creator><name>Fuller G.A.</name></creator><creator><name>Li D.,Ristorcelli I.</name></creator><creator><name>Kang S.-J.</name></creator><creator><name>Hirano N.</name></creator><creator><name>Johnstone D.</name></creator><creator><name>Lin Y.</name></creator><creator><name>He J.H.,Koch P.M.</name></creator><creator><name>Sanhueza P.</name></creator><creator><name>Qin S.-L.</name></creator><creator><name>Zhang Q.</name></creator><creator><name>Goldsmith P.F.</name></creator><creator><name>Evans N.J.,Yuan J.</name></creator><creator><name>Zhang C.-P.</name></creator><creator><name>White G.J.</name></creator><creator><name>Choi M.</name></creator><creator><name>Lee C.W.</name></creator><creator><name>Toth L.V.</name></creator><creator><name>Mairs S.,Yi H.-W.</name></creator><creator><name>Tang M.</name></creator><creator><name>Soam A.</name></creator><creator><name>Peretto N.</name></creator><creator><name>Samal M.R.</name></creator><creator><name>Fich M.</name></creator><creator><name>Parsons H.,Malinen J.</name></creator><creator><name>Bendo G.J.</name></creator><creator><name>Rivera-ingraham A.</name></creator><creator><name>Liu H.-L.</name></creator><creator><name>Wouterloot J.,Li P.S.</name></creator><creator><name>Qian L.</name></creator><creator><name>Rawlings J.</name></creator><creator><name>Rawlings M.G.</name></creator><creator><name>Feng S.</name></creator><creator><name>Wang B.</name></creator><creator><name>Li D.,Liu M.</name></creator><creator><name>Luo G.</name></creator><creator><name>Marston A.P.</name></creator><creator><name>Pattle K.M.</name></creator><creator><name>Pelkonen V.-M.</name></creator><creator><name>Rigby A.J.,Zahorecz S.</name></creator><creator><name>Zhang G.</name></creator><creator><name>Bogner R.</name></creator><creator><name>Aikawa Y.</name></creator><creator><name>Akhter S.</name></creator><creator><name>Alina D.</name></creator><creator><name>Bell G.,Bernard J.-P.</name></creator><creator><name>Blain A.</name></creator><creator><name>Bronfman L.</name></creator><creator><name>Byun D.-Y.</name></creator><creator><name>Chapman S.</name></creator><creator><name>Chen H.-R.,Chen M.</name></creator><creator><name>Chen W.-P.</name></creator><creator><name>Chen X.</name></creator><creator><name>Chen X.</name></creator><creator><name>Chrysostomou A.</name></creator><creator><name>Chu Y.-H.,Chung E.J.</name></creator><creator><name>Cornu D.</name></creator><creator><name>Cosentino G.</name></creator><creator><name>Cunningham M.R.</name></creator><creator><name>Demyk K.,Drabek-maunder E.</name></creator><creator><name>Doi Y.</name></creator><creator><name>Eswaraiah C.</name></creator><creator><name>Falgarone E.</name></creator><creator><name>Feher O.</name></creator><creator><name>Fraser H.,Friberg P.</name></creator><creator><name>Garay G.</name></creator><creator><name>Ge J.X.</name></creator><creator><name>Gear W.K.</name></creator><creator><name>Greaves J.</name></creator><creator><name>Guan X.,Harvey-smith L.</name></creator><creator><name>Hasegawa T.</name></creator><creator><name>He Y.</name></creator><creator><name>Henkel C.</name></creator><creator><name>Hirota T.</name></creator><creator><name>Holland W.,Hughes A.</name></creator><creator><name>Jarken E.</name></creator><creator><name>Ji T.-G.</name></creator><creator><name>Jimenez-serra I.</name></creator><creator><name>Kang M.</name></creator><creator><name>Kawabata K.S.,Kim G.</name></creator><creator><name>Kim J.</name></creator><creator><name>Kim J.</name></creator><creator><name>Kim S.</name></creator><creator><name>Koo B.-C.</name></creator><creator><name>Kwon W.</name></creator><creator><name>Kuan Y.-J.,Lacaille K.M.</name></creator><creator><name>Lai S.-P.</name></creator><creator><name>Lee C.F.</name></creator><creator><name>Lee J.-E.</name></creator><creator><name>Lee Y.-U.</name></creator><creator><name>Li H.</name></creator><creator><name>Lo N.,Lopez J.A.P.</name></creator><creator><name>Lu X.</name></creator><creator><name>Lyo A.-R.</name></creator><creator><name>Mardones D.</name></creator><creator><name>Mcgehee P.</name></creator><creator><name>Meng F.,Montier L.</name></creator><creator><name>Montillaud J.</name></creator><creator><name>Moore T.J.T.</name></creator><creator><name>Morata O.</name></creator><creator><name>Moriarty-schieven G.H.,Ohashi S.</name></creator><creator><name>Pak S.</name></creator><creator><name>Park G.</name></creator><creator><name>Paladini R.</name></creator><creator><name>Pech G.</name></creator><creator><name>Qiu K.</name></creator><creator><name>Ren Z.-Y.,Richer J.</name></creator><creator><name>Sakai T.</name></creator><creator><name>Shang H.</name></creator><creator><name>Shinnaga H.</name></creator><creator><name>Stamatellos D.</name></creator><creator><name>Tang Y.-W.,Traficante A.</name></creator><creator><name>Vastel C.</name></creator><creator><name>Viti S.</name></creator><creator><name>Walsh A.</name></creator><creator><name>Wang H.</name></creator><creator><name>Wang J.,Ward-thompson D.</name></creator><creator><name>Whitworth A.</name></creator><creator><name>Wilson C.D.</name></creator><creator><name>Xu Y.</name></creator><creator><name>Yang J.</name></creator><creator><name>Yuan Y.-L.,Yuan L.</name></creator><creator><name>Zavagno A.</name></creator><creator><name>Zhang C.</name></creator><creator><name>Zhang G.</name></creator><creator><name>Zhang H.-W.</name></creator><creator><name>Zhou C.</name></creator><creator><name>Zhou J.,Zhu L.</name></creator><creator><name>Zuo P.</name></creator><date role="Updated">2024-08-19T20:17:29Z</date><date role="Created">2022-03-31T07:42:46Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>surveys</subject><subject>interstellar-medium</subject><subject>molecular-clouds</subject><subject>young-stellar-objects</subject><description>We present the first release of the data and compact-source catalogue for the JCMT Large Program SCUBA-2 Continuum Observations of Pre-protostellar Evolution (SCOPE). SCOPE consists of 850um continuum observations of 1235 Planck Galactic Cold Clumps (PGCCs) made with the Submillimetre Common-User Bolometer Array 2 on the James Clerk Maxwell Telescope. These data are at an angular resolution of 14.4", significantly improving upon the 353GHz resolution of Planck at 5', and allowing for a catalogue of 3528 compact sources in 558 PGCCs. We find that the detected PGCCs have significant sub-structure, with 61 per cent of detected PGCCs having three or more compact sources, with filamentary structure also prevalent within the sample. A detection rate of 45 per cent is found across the survey, which is 95% complete to Planck column densities of N_H2_&gt;5x10^21^cm^-2^. By positionally associating the SCOPE compact sources with young stellar objects, the star formation efficiency, as measured by the ratio of luminosity to mass, in nearby clouds is found to be similar to that in the more distant Galactic Plane, with the column density distributions also indistinguishable from each other.</description><source format="bibcode">2019MNRAS.485.2895E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/485/2895</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/327">II/327 : AKARI Far-Infrared Surveyor YSO catalog (Toth+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/275/67">J/A+A/275/67 : Velocity Field of the outer Galaxy (Brand+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/993">J/A+A/487/993 : MAMBO Mapping of c2d Clouds and Cores (Kauffmann+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/1019">J/ApJ/723/1019 : Galactic SFR and gas surface densities (Heiderman+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/422/3178">J/MNRAS/422/3178 : Distances of 793 BGPS sources (Eden+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/76">J/ApJ/756/76 : Planck cold dust clumps CO survey (Wu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/4">J/ApJS/202/4 : Planck cold clumps survey in the Orion complex (Liu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A130">J/A+A/549/A130 : YSOs in Herschel-Hi-GAL survey (Veneziani+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/1587">J/MNRAS/431/1587 : GRS/BGPS sources in Galactic Plane (Eden+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/37">J/ApJS/209/37 : Planck cold clumps in ^12^CO, ^13^CO &amp; C^18^O (Meng+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A125">J/A+A/563/A125 : L1642 Herschel maps (Malinen+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/443/1555">J/MNRAS/443/1555 : ATLASGAL massive star forming clumps (Urquhart+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/64">J/AJ/149/64 : MIPSGAL 24{mu}m point source catalog (Gutermuth+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/448/1551">J/MNRAS/448/1551 : JCMT Gould Belt Survey: Serpens MWC 297 (Rumble+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/453/4264">J/MNRAS/453/4264 : JCMT Plane Survey: l=30{deg} field (Moore+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A91">J/A+A/584/A91 : Cat. of dense cores in Aquila from Herschel (Konyves+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/584/A92">J/A+A/584/A92 : Gal. 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II. 850um (Yi+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/249/33">J/ApJS/249/33 : Nobeyama molecular line survey of SCUBA-2 cores (Kim+, 2020)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/485/2895</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/485/2895</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/485/2895</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/485/2895</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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