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<ri:Resource created="2022-08-08T08:16:40Z" 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>HOPS: Herschel/PACS 70 and 160um obs.</title><shortName>J/ApJ/905/119</shortName><identifier>ivo://CDS.VizieR/J/ApJ/905/119</identifier><altIdentifier>doi:10.26093/cds/vizier.19050119</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fischer W.J.</name></creator><creator><name>Megeath S.T.</name></creator><creator><name>Furlan E.</name></creator><creator><name>Stutz A.M.</name></creator><creator><name>Stanke T.</name></creator><creator><name>Tobin J.J.,Osorio M.</name></creator><creator><name>Manoj P.</name></creator><creator><name>Di Francesco J.</name></creator><creator><name>Allen L.E.</name></creator><creator><name>Watson D.M.</name></creator><creator><name>Wilson T.L.,Henning T.</name></creator><date role="Updated">2022-08-26T13:25:30Z</date><date role="Created">2022-08-08T08:16:40Z</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>young-stellar-objects</subject><subject>infrared-photometry</subject><subject>molecular-clouds</subject><description>The degree to which the properties of protostars are affected by environment remains an open question. To investigate this, we look at the Orion A and B molecular clouds, home to most of the protostars within 500pc. At ~400pc, Orion is close enough to distinguish individual protostars across a range of environments in terms of both the stellar and gas projected densities. As part of the Herschel Orion Protostar Survey (HOPS), we used the Photodetector Array Camera and Spectrometer to map 108 partially overlapping square fields with edge lengths of 5' or 8' and measure the 70 and 160{mu}m flux densities of 338 protostars within them. In this paper we examine how these flux densities and their ratio depend on evolutionary state and environment within the Orion complex. We show that Class 0 protostars occupy a region of the 70{mu}m flux density versus 160{mu}m/70{mu}m flux density ratio diagram that is distinct from their more evolved counterparts. We then present evidence that the Integral-Shaped Filament (ISF) and Orion B contain protostars with more massive inner envelopes than those in the more sparsely populated LDN 1641 region. This can be interpreted as evidence for increasing star formation rates in the ISF and Orion B or as a tendency for more massive inner envelopes to be inherited from denser birth environments. We also provide technical details about the mapmaking and photometric procedures used in the HOPS program.</description><source format="bibcode">2020ApJ...905..119F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/905/119</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/139">VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/289/101">J/A+A/289/101 : Orion OB1 association. I. (Brown+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/674/336">J/ApJ/674/336 : Spitzer observations of NGC 1333 (Gutermuth+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/31">J/AJ/144/31 : Spitzer+2MASS phot. of protostar candidates (Kryukova+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/192">J/AJ/144/192 : Spitzer survey of Orion A &amp; B. I. YSO catalog (Megeath+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/94">J/AJ/145/94 : Luminosities of protostars from Spitzer (Dunham+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/36">J/ApJ/767/36 : APEX observations of HOPS protostars (Stutz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/11">J/AJ/148/11 : Infrared photometry in Cygnus-X (Kryukova+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/5">J/ApJS/224/5 : Herschel Orion Protostar Survey (HOPS): SEDs (Furlan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/596/A26">J/A+A/596/A26 : OMC-2 FIR 3 and FIR 4 [OI] maps (Gonzalez-Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/52">J/ApJ/821/52 : NIR survey of Spitzer YSOs in Orion (Kounkel+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A106">J/A+A/619/A106 : 3D shape of Orion A from Gaia DR2 (Grossschedl+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/84">J/AJ/156/84 : APOGEE-2 survey of Orion Complex. II. (Kounkel+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A51">J/A+A/633/A51 : Distances to molecular clouds in SFR (Zucker+, 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/ApJ/905/119</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/905/119</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/905/119</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/905/119</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/905/119</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/905/119</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/905/119/table2 (HOPS sources)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/905/119/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/905/119/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/905/119/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>88.6171</ra><dec>1.6264</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/21403 21425 21427-21428 21430 21433 21435-21436 21438-21439 22804-22805 22854-22855 22861 22873 22876 23560</spatial><spectral>9.699422546568423e-22 3.243176138527326e-21</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/905/119?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/905/119/table2</name><description>HOPS sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HOPS</name><description>[0/409] HOPS identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_HOPS</name><description>Duplication flag on identifiers (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>[83.34/88.74]? Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DEJ2000</name><description>[-8.84/1.9]? 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