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<ri:Resource created="2013-01-09T16:04:40Z" 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>Arecibo 1612 MHz survey supplement</title><shortName>J/ApJS/93/549</shortName><identifier>ivo://CDS.VizieR/J/ApJS/93/549</identifier><altIdentifier>doi:10.26093/cds/vizier.20930549</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lewis B.M.</name></creator><date role="Updated">2017-09-22T16:16:22Z</date><date role="Created">2013-01-09T16:04:40Z</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>radio-sources</subject><description>The completeness of the Arecibo 1612 MHz survey of color-selected/IRAS sources (see references) is extended to (25-12){mu}m&gt;-0.7. In addition (1) most IR sources with spectral types normally associated with OH/IR stars and colors outside the coverage of the original survey have been examined; (2) most ambiguous observations during the survey have been reobserved: (3) most single peaked sources have been reexamined, and 17 found with second peaks. We report 39 new 1612MHz detections, of which 34 are original. These are also surveyed in the mainlines. Analysis of the complete flux-limited survey confirms the existence of a longitude sensitivity effect in the detection of sources, which reduces the total number detected by ~4%. This analysis sets an upper limit of 16%, on the proportion of a color-selected sample that may be identified with carbon stars and/or star-formation regions.</description><source format="bibcode">1994ApJS...93..549L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/93/549</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/125">II/125 : IRAS Point Source Catalogue, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/90/327">J/A+AS/90/327 : IRAS Point Source 1612MHz OH survey (te Lintel Hekkert+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/89/189">J/ApJS/89/189 : IRAS PSC new OH/IR stars. III. 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Integrated 1612MHz flux in the high-velocity half of the spectrum</description><unit>mJy.km/s</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DV100</name><description>? Velocity width at 100% of the peak velocity {Delta}V_100_</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_DV100</name><description>[)] Uncertainty flag on DV100</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>DV50</name><description>? Velocity width at 50% of the peak velocity {Delta}V_50_</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_DV50</name><description>[)] Uncertainty flag on DV50</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vl</name><description>LSR velocity of the low-velocity peak</description><unit>km/s</unit><ucd>phys.veloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vh</name><description>? 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III/197, Note 1)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Name</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>PSC</name><description>Details from the IRAS-PSC catalog</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/93/549/table3</name><description>Main line parameters of 1612 MHz detections</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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