SCUBA observations of the host galaxies of four dark gamma-ray bursts
Identifieur interne : 000894 ( Main/Corpus ); précédent : 000893; suivant : 000895SCUBA observations of the host galaxies of four dark gamma-ray bursts
Auteurs : V. E. Barnard ; A. W. Blain ; N. R. Tanvir ; P. Natarajan ; I. A. Smith ; R. A. M. J. Wijers ; C. Kouveliotou ; E. Rol ; R. P. J. Tilanus ; P. VreeswijkSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2003-01-01.
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Abstract
We present the results of a search for submillimetre-luminous host galaxies of optically dark gamma-ray bursts (GRBs) using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT). We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. Further observations are required to establish the relationship between the wider GRB host galaxy population and SCUBA galaxies.
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DOI: 10.1046/j.1365-8711.2003.05860.x
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Barnard</name><affiliation><mods:affiliation>Cavendish Astrophysics, University of Cambridge, Cambridge CB3 0HE</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: veb23@mrao.cam.ac.uk</mods:affiliation></affiliation></author><author><name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name><affiliation><mods:affiliation>Department of Astronomy, Caltech 105-24, Pasadena, CA 91125, USA</mods:affiliation></affiliation></author><author><name sortKey="Tanvir, N R" sort="Tanvir, N R" uniqKey="Tanvir N" first="N. R." last="Tanvir">N. R. Tanvir</name><affiliation><mods:affiliation>Department of Physical Sciences, University of Hertfordshire, Hatfield AL10 9AB</mods:affiliation></affiliation></author><author><name sortKey="Natarajan, P" sort="Natarajan, P" uniqKey="Natarajan P" first="P." last="Natarajan">P. 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We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. Further observations are required to establish the relationship between the wider GRB host galaxy population and SCUBA galaxies.</div></front></TEI><istex><corpusName>oup</corpusName><author><json:item><name>V. E. 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We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. 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We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. Further observations are required to establish the relationship between the wider GRB host galaxy population and SCUBA galaxies.</p></abstract><textClass xml:lang="en"><keywords scheme="keyword"><list><head>Key words</head><item><term>stars: evolution</term></item><item><term>dust, extinction</term></item><item><term>cosmology: observations</term></item><item><term>gamma-rays: bursts</term></item><item><term>infrared: galaxies</term></item></list></keywords></textClass></profileDesc><revisionDesc><change when="2003-01-01">Published</change></revisionDesc></teiHeader></istex:fulltextTEI><json:item><original>false</original><mimetype>text/plain</mimetype><extension>txt</extension><uri>https://api.istex.fr/document/0F10167C935EDFD62B90783D89F8B7DAA38CA912/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="corpus oup" wicri:toSee="no header"><istex:xmlDeclaration>version="1.0"</istex:xmlDeclaration><istex:docType PUBLIC="-//NLM//DTD Journal Publishing DTD v2.3 20070202//EN" URI="journalpublishing.dtd" name="istex:docType"></istex:docType><istex:document><article article-type="research-article"><front><journal-meta><journal-id journal-id-type="hwp">mnras</journal-id><journal-id journal-id-type="publisher-id">mnras</journal-id><journal-title>Monthly Notices of the Royal Astronomical Society</journal-title><abbrev-journal-title>Mon. Not. R. Astron. Soc.</abbrev-journal-title><issn pub-type="ppub">0035-8711</issn><issn pub-type="epub">1365-2966</issn><publisher><publisher-name>Blackwell Science Ltd</publisher-name><publisher-loc>Oxford, UK</publisher-loc></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.1046/j.1365-8711.2003.05860.x</article-id><article-categories><subj-group subj-group-type="heading"><subject>Papers</subject></subj-group></article-categories><title-group><article-title>SCUBA observations of the host galaxies of four dark gamma-ray bursts</article-title></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name><surname>Barnard</surname><given-names>V. E.</given-names></name><xref ref-type="aff" rid="a1"><sup>1</sup></xref><xref rid="cor1" ref-type="corresp"><sup>⋆</sup></xref></contrib><contrib contrib-type="author"><name><surname>Blain</surname><given-names>A. W.</given-names></name><xref ref-type="aff" rid="a2"><sup>2</sup></xref></contrib><contrib contrib-type="author"><name><surname>Tanvir</surname><given-names>N. R.</given-names></name><xref ref-type="aff" rid="a3"><sup>3</sup></xref></contrib><contrib contrib-type="author"><name><surname>Natarajan</surname><given-names>P.</given-names></name><xref ref-type="aff" rid="a4"><sup>4</sup></xref></contrib><contrib contrib-type="author"><name><surname>Smith</surname><given-names>I. A.</given-names></name><xref ref-type="aff" rid="a5"><sup>5</sup></xref></contrib><contrib contrib-type="author"><name><surname>Wijers</surname><given-names>R. A. M. J.</given-names></name><xref ref-type="aff" rid="a6"><sup>6</sup></xref></contrib><contrib contrib-type="author"><name><surname>Kouveliotou</surname><given-names>C.</given-names></name><xref ref-type="aff" rid="a7"><sup>7</sup></xref></contrib><contrib contrib-type="author"><name><surname>Rol</surname><given-names>E.</given-names></name><xref ref-type="aff" rid="a8"><sup>8</sup></xref></contrib><contrib contrib-type="author"><name><surname>Tilanus</surname><given-names>R. P. J.</given-names></name><xref ref-type="aff" rid="a9"><sup>9</sup></xref></contrib><contrib contrib-type="author"><name><surname>Vreeswijk</surname><given-names>P.</given-names></name><xref ref-type="aff" rid="a8"><sup>8</sup></xref></contrib><aff id="a1"><label>1</label>Cavendish Astrophysics, University of Cambridge, Cambridge CB3 0HE</aff><aff id="a2"><label>2</label>Department of Astronomy, Caltech 105-24, Pasadena, CA 91125, USA</aff><aff id="a3"><label>3</label>Department of Physical Sciences, University of Hertfordshire, Hatfield AL10 9AB</aff><aff id="a4"><label>4</label>Department of Astronomy, Yale University, New Haven, CT 06250-8181, USA</aff><aff id="a5"><label>5</label>Department of Physics and Astronomy, Rice University MS 108, Houston, TX 77005-1892, USA</aff><aff id="a6"><label>6</label>Department of Physics and Astronomy, SUNY, Stony Brook, NY 11794-3800, USA</aff><aff id="a7"><label>7</label>NASA Marshall Space Flight Center, SD-50, NSSTC, 320 Sparkman Drive, Huntsville, AL 35805, USA</aff><aff id="a8"><label>8</label>Astronomical Insitute ‘Anton Pannekoek’, University of Amsterdam and Centre for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands</aff><aff id="a9"><label>9</label>Joint Astronomy Centre, 660 N. A‘ohōkū Place, Hilo, HI 96720, USA</aff></contrib-group><author-notes><corresp id="cor1"><label>⋆</label>E-mail: <email>veb23@mrao.cam.ac.uk</email></corresp></author-notes><pub-date pub-type="ppub"><day>1</day><month>1</month><year>2003</year></pub-date><volume>338</volume><issue>1</issue><fpage>1</fpage><lpage>6</lpage><history><date date-type="received"><day>28</day><month>6</month><year>2002</year></date><date date-type="accepted"><day>8</day><month>7</month><year>2002</year></date></history><permissions><copyright-statement>© 2003 RAS</copyright-statement><copyright-year>2003</copyright-year></permissions><abstract><p>We present the results of a search for submillimetre-luminous host galaxies of optically dark gamma-ray bursts (GRBs) using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT). We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. Further observations are required to establish the relationship between the wider GRB host galaxy population and SCUBA galaxies.</p></abstract><kwd-group xml:lang="en"><title>Key words</title><kwd>stars: evolution</kwd><kwd>dust, extinction</kwd><kwd>cosmology: observations</kwd><kwd>gamma-rays: bursts</kwd><kwd>infrared: galaxies</kwd></kwd-group></article-meta></front></article></istex:document></istex:metadataXml><mods version="3.6"><titleInfo><title>SCUBA observations of the host galaxies of four dark gamma-ray bursts</title></titleInfo><titleInfo type="alternative" contentType="CDATA"><title>SCUBA observations of the host galaxies of four dark gamma-ray bursts</title></titleInfo><name type="personal" displayLabel="corresp"><namePart type="given">V. E.</namePart><namePart type="family">Barnard</namePart><affiliation>Cavendish Astrophysics, University of Cambridge, Cambridge CB3 0HE</affiliation><affiliation>E-mail: veb23@mrao.cam.ac.uk</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">A. W.</namePart><namePart type="family">Blain</namePart><affiliation>Department of Astronomy, Caltech 105-24, Pasadena, CA 91125, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">N. R.</namePart><namePart type="family">Tanvir</namePart><affiliation>Department of Physical Sciences, University of Hertfordshire, Hatfield AL10 9AB</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">P.</namePart><namePart type="family">Natarajan</namePart><affiliation>Department of Astronomy, Yale University, New Haven, CT 06250-8181, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">I. A.</namePart><namePart type="family">Smith</namePart><affiliation>Department of Physics and Astronomy, Rice University MS 108, Houston, TX 77005-1892, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">R. A. M. J.</namePart><namePart type="family">Wijers</namePart><affiliation>Department of Physics and Astronomy, SUNY, Stony Brook, NY 11794-3800, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">C.</namePart><namePart type="family">Kouveliotou</namePart><affiliation>NASA Marshall Space Flight Center, SD-50, NSSTC, 320 Sparkman Drive, Huntsville, AL 35805, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">E.</namePart><namePart type="family">Rol</namePart><affiliation>Astronomical Insitute ‘Anton Pannekoek’, University of Amsterdam and Centre for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">R. P. J.</namePart><namePart type="family">Tilanus</namePart><affiliation>Joint Astronomy Centre, 660 N. A‘ohōkū Place, Hilo, HI 96720, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">P.</namePart><namePart type="family">Vreeswijk</namePart><affiliation>Astronomical Insitute ‘Anton Pannekoek’, University of Amsterdam and Centre for High-Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="research-article" displayLabel="research-article"></genre><originInfo><publisher>Blackwell Science Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2003-01-01</dateIssued><copyrightDate encoding="w3cdtf">2003</copyrightDate></originInfo><language><languageTerm type="code" authority="iso639-2b">eng</languageTerm><languageTerm type="code" authority="rfc3066">en</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType></physicalDescription><abstract>We present the results of a search for submillimetre-luminous host galaxies of optically dark gamma-ray bursts (GRBs) using the Submillimetre Common-User Bolometer Array (SCUBA) on the James Clerk Maxwell Telescope (JCMT). We made photometry measurements of the 850-μm flux at the location of four ‘dark bursts’, which are those with no detected optical afterglow despite rapid deep searches, and which may therefore be within galaxies containing substantial amounts of dust. We were unable to detect any individual source significantly. Our results are consistent with predictions for the host galaxy population as a whole, rather than for a subset of dusty hosts. This indicates that optically dark GRBs are not especially associated with very submillimetre-luminous galaxies and so cannot be used as reliable indicators of dust-enshrouded massive star formation activity. Further observations are required to establish the relationship between the wider GRB host galaxy population and SCUBA galaxies.</abstract><subject lang="en"><genre>Key words</genre><topic>stars: evolution</topic><topic>dust, extinction</topic><topic>cosmology: observations</topic><topic>gamma-rays: bursts</topic><topic>infrared: galaxies</topic></subject><relatedItem type="host"><titleInfo><title>Monthly Notices of the Royal Astronomical Society</title></titleInfo><titleInfo type="abbreviated"><title>Mon. Not. R. Astron. Soc.</title></titleInfo><genre type="journal">journal</genre><identifier type="ISSN">0035-8711</identifier><identifier type="eISSN">1365-2966</identifier><identifier type="PublisherID">mnras</identifier><identifier type="PublisherID-hwp">mnras</identifier><part><date>2003</date><detail type="volume"><caption>vol.</caption><number>338</number></detail><detail type="issue"><caption>no.</caption><number>1</number></detail><extent unit="pages"><start>1</start><end>6</end></extent></part></relatedItem><identifier type="istex">0F10167C935EDFD62B90783D89F8B7DAA38CA912</identifier><identifier type="DOI">10.1046/j.1365-8711.2003.05860.x</identifier><accessCondition type="use and reproduction" contentType="copyright">© 2003 RAS</accessCondition><recordInfo><recordContentSource>OUP</recordContentSource></recordInfo></mods></metadata><annexes><json:item><original>true</original><mimetype>image/jpeg</mimetype><extension>jpeg</extension><uri>https://api.istex.fr/document/0F10167C935EDFD62B90783D89F8B7DAA38CA912/annexes/jpeg</uri></json:item><json:item><original>true</original><mimetype>image/gif</mimetype><extension>gif</extension><uri>https://api.istex.fr/document/0F10167C935EDFD62B90783D89F8B7DAA38CA912/annexes/gif</uri></json:item></annexes><enrichments><istex:catWosTEI uri="https://api.istex.fr/document/0F10167C935EDFD62B90783D89F8B7DAA38CA912/enrichments/catWos"><teiHeader><profileDesc><textClass><classCode scheme="WOS">ASTRONOMY & ASTROPHYSICS</classCode></textClass></profileDesc></teiHeader></istex:catWosTEI></enrichments><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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