The submillimetre properties of gamma‐ray burst host galaxies
Identifieur interne : 000322 ( Main/Exploration ); précédent : 000321; suivant : 000323The submillimetre properties of gamma‐ray burst host galaxies
Auteurs : N. R. Tanvir ; V. E. Barnard [États-Unis] ; A. W. Blain [États-Unis] ; A. S. Fruchter [États-Unis] ; C. Kouveliotou [États-Unis] ; P. Natarajan [États-Unis] ; E. Ramirez-Ruiz [États-Unis] ; E. Rol [Italie] ; I. A. Smith [États-Unis] ; R. P. J. Tilanus [États-Unis] ; R. A. M. J. Wijers [Pays-Bas]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2004-08.
English descriptors
- KwdEn :
Abstract
Long‐duration gamma‐ray bursts (GRBs) accompany the deaths of some massive stars and hence, because massive stars are short‐lived, are a tracer of star formation activity. Given that GRBs are bright enough to be seen to very high redshifts and detected even in dusty environments, they should therefore provide a powerful probe of the global star formation history of the Universe. The potential of this approach can be investigated via submillimetre (submm) photometry of GRB host galaxies. Submm luminosity also correlates with star formation rate, so the distribution of host‐galaxy submm fluxes should allow us to test the two methods for consistency. Here, we report new JCMT/SCUBA 850‐μm measurements for 15 GRB hosts. Combining these data with results from previous studies, we construct a sample of 21 hosts with <1.4 mJy errors. We show that the distribution of apparent 850‐μm flux densities of this sample is reasonably consistent with model predictions, but there is tentative evidence of a dearth of submm‐bright (>4 mJy) galaxies. Furthermore, the optical/infrared properties of the submm‐brightest GRB hosts are not typical of the galaxy population selected in submm surveys, although the sample size is still small. Possible selection effects and physical mechanisms which may explain these discrepancies are discussed.
Url:
DOI: 10.1111/j.1365-2966.2004.08001.x
Affiliations:
Links toward previous steps (curation, corpus...)
Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">The submillimetre properties of gamma‐ray burst host galaxies</title>
<author><name sortKey="Tanvir, N R" sort="Tanvir, N R" uniqKey="Tanvir N" first="N. R." last="Tanvir">N. R. Tanvir</name>
</author>
<author><name sortKey="Barnard, V E" sort="Barnard, V E" uniqKey="Barnard V" first="V. E." last="Barnard">V. E. Barnard</name>
</author>
<author><name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name>
</author>
<author><name sortKey="Fruchter, A S" sort="Fruchter, A S" uniqKey="Fruchter A" first="A. S." last="Fruchter">A. S. Fruchter</name>
</author>
<author><name sortKey="Kouveliotou, C" sort="Kouveliotou, C" uniqKey="Kouveliotou C" first="C." last="Kouveliotou">C. Kouveliotou</name>
</author>
<author><name sortKey="Natarajan, P" sort="Natarajan, P" uniqKey="Natarajan P" first="P." last="Natarajan">P. Natarajan</name>
</author>
<author><name sortKey="Ramirez Uiz, E" sort="Ramirez Uiz, E" uniqKey="Ramirez Uiz E" first="E." last="Ramirez-Ruiz">E. Ramirez-Ruiz</name>
</author>
<author><name sortKey="Rol, E" sort="Rol, E" uniqKey="Rol E" first="E." last="Rol">E. Rol</name>
</author>
<author><name sortKey="Smith, I A" sort="Smith, I A" uniqKey="Smith I" first="I. A." last="Smith">I. A. Smith</name>
</author>
<author><name sortKey="Tilanus, R P J" sort="Tilanus, R P J" uniqKey="Tilanus R" first="R. P. J." last="Tilanus">R. P. J. Tilanus</name>
</author>
<author><name sortKey="Wijers, R A M J" sort="Wijers, R A M J" uniqKey="Wijers R" first="R. A. M. J." last="Wijers">R. A. M. J. Wijers</name>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:E9B600C6D24088A13F1B1D8DB67E61A9D73EB3C9</idno>
<date when="2004" year="2004">2004</date>
<idno type="doi">10.1111/j.1365-2966.2004.08001.x</idno>
<idno type="url">https://api.istex.fr/document/E9B600C6D24088A13F1B1D8DB67E61A9D73EB3C9/fulltext/pdf</idno>
<idno type="wicri:Area/Main/Corpus">000871</idno>
<idno type="wicri:Area/Main/Curation">000871</idno>
<idno type="wicri:Area/Main/Exploration">000322</idno>
<idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000322</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">The submillimetre properties of gamma‐ray burst host galaxies</title>
<author><name sortKey="Tanvir, N R" sort="Tanvir, N R" uniqKey="Tanvir N" first="N. R." last="Tanvir">N. R. Tanvir</name>
<affiliation><wicri:noCountry code="subField">9AB</wicri:noCountry>
</affiliation>
</author>
<author><name sortKey="Barnard, V E" sort="Barnard, V E" uniqKey="Barnard V" first="V. E." last="Barnard">V. E. Barnard</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Joint Astronomy Centre, 660 N, A'ohōkū Place, Hilo, HI 96720</wicri:regionArea>
<wicri:noRegion>HI 96720</wicri:noRegion>
</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 wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Department of Astronomy, Caltech 105‐24, Pasadena, CA 91125</wicri:regionArea>
<wicri:noRegion>CA 91125</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Fruchter, A S" sort="Fruchter, A S" uniqKey="Fruchter A" first="A. S." last="Fruchter">A. S. Fruchter</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD21218</wicri:regionArea>
<wicri:noRegion>MD21218</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Kouveliotou, C" sort="Kouveliotou, C" uniqKey="Kouveliotou C" first="C." last="Kouveliotou">C. Kouveliotou</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>NASA Marshall Space Flight Center, SD‐50, NSSTC, 320 Sparkman Drive, Huntsville, AL 35805</wicri:regionArea>
<wicri:noRegion>AL 35805</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Natarajan, P" sort="Natarajan, P" uniqKey="Natarajan P" first="P." last="Natarajan">P. Natarajan</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Department of Astronomy, Yale University, New Haven, CT 06250‐8181</wicri:regionArea>
<wicri:noRegion>CT 06250‐8181</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Ramirez Uiz, E" sort="Ramirez Uiz, E" uniqKey="Ramirez Uiz E" first="E." last="Ramirez-Ruiz">E. Ramirez-Ruiz</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540</wicri:regionArea>
<wicri:noRegion>NJ 08540</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Rol, E" sort="Rol, E" uniqKey="Rol E" first="E." last="Rol">E. Rol</name>
<affiliation wicri:level="1"><country xml:lang="fr">Italie</country>
<wicri:regionArea>Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122, Padova</wicri:regionArea>
<wicri:noRegion>Padova</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Smith, I A" sort="Smith, I A" uniqKey="Smith I" first="I. A." last="Smith">I. A. Smith</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Department of Physics and Astronomy, Rice University MS 108, Houston, TX 77005‐1892</wicri:regionArea>
<wicri:noRegion>TX 77005‐1892</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Tilanus, R P J" sort="Tilanus, R P J" uniqKey="Tilanus R" first="R. P. J." last="Tilanus">R. P. J. Tilanus</name>
<affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Joint Astronomy Centre, 660 N, A'ohōkū Place, Hilo, HI 96720</wicri:regionArea>
<wicri:noRegion>HI 96720</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Wijers, R A M J" sort="Wijers, R A M J" uniqKey="Wijers R" first="R. A. M. J." last="Wijers">R. A. M. J. Wijers</name>
<affiliation wicri:level="1"><country xml:lang="fr" wicri:curation="lc">Pays-Bas</country>
<wicri:regionArea>Astronomical Insitute ‘Anton Pannekoek’, University of Amsterdam and Center for High‐Energy Astrophysics, Kruislaan 403, 1098 SJ Amsterdam</wicri:regionArea>
<wicri:noRegion>1098 SJ Amsterdam</wicri:noRegion>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series><title level="j">Monthly Notices of the Royal Astronomical Society</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
<imprint><publisher>Blackwell Science Ltd</publisher>
<pubPlace>23 Ainslie Place , Edinburgh EH3 6AJ , UK . Telephone (0131) 226 7232 Fax (0131) 226 3803</pubPlace>
<date type="published" when="2004-08">2004-08</date>
<biblScope unit="volume">352</biblScope>
<biblScope unit="issue">3</biblScope>
<biblScope unit="page" from="1073">1073</biblScope>
<biblScope unit="page" to="1080">1080</biblScope>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
<idno type="istex">E9B600C6D24088A13F1B1D8DB67E61A9D73EB3C9</idno>
<idno type="DOI">10.1111/j.1365-2966.2004.08001.x</idno>
<idno type="ArticleID">MNR8001</idno>
</biblStruct>
</sourceDesc>
<seriesStmt><idno type="ISSN">0035-8711</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>cosmology: observations</term>
<term>dust, extinction</term>
<term>galaxies: evolution</term>
<term>gamma‐rays: bursts</term>
<term>infrared: galaxies</term>
<term>stars: evolution</term>
</keywords>
</textClass>
<langUsage><language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">Long‐duration gamma‐ray bursts (GRBs) accompany the deaths of some massive stars and hence, because massive stars are short‐lived, are a tracer of star formation activity. Given that GRBs are bright enough to be seen to very high redshifts and detected even in dusty environments, they should therefore provide a powerful probe of the global star formation history of the Universe. The potential of this approach can be investigated via submillimetre (submm) photometry of GRB host galaxies. Submm luminosity also correlates with star formation rate, so the distribution of host‐galaxy submm fluxes should allow us to test the two methods for consistency. Here, we report new JCMT/SCUBA 850‐μm measurements for 15 GRB hosts. Combining these data with results from previous studies, we construct a sample of 21 hosts with <1.4 mJy errors. We show that the distribution of apparent 850‐μm flux densities of this sample is reasonably consistent with model predictions, but there is tentative evidence of a dearth of submm‐bright (>4 mJy) galaxies. Furthermore, the optical/infrared properties of the submm‐brightest GRB hosts are not typical of the galaxy population selected in submm surveys, although the sample size is still small. Possible selection effects and physical mechanisms which may explain these discrepancies are discussed.</div>
</front>
</TEI>
<affiliations><list><country><li>Italie</li>
<li>Pays-Bas</li>
<li>États-Unis</li>
</country>
</list>
<tree><noCountry><name sortKey="Tanvir, N R" sort="Tanvir, N R" uniqKey="Tanvir N" first="N. R." last="Tanvir">N. R. Tanvir</name>
</noCountry>
<country name="États-Unis"><noRegion><name sortKey="Barnard, V E" sort="Barnard, V E" uniqKey="Barnard V" first="V. E." last="Barnard">V. E. Barnard</name>
</noRegion>
<name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name>
<name sortKey="Fruchter, A S" sort="Fruchter, A S" uniqKey="Fruchter A" first="A. S." last="Fruchter">A. S. Fruchter</name>
<name sortKey="Kouveliotou, C" sort="Kouveliotou, C" uniqKey="Kouveliotou C" first="C." last="Kouveliotou">C. Kouveliotou</name>
<name sortKey="Natarajan, P" sort="Natarajan, P" uniqKey="Natarajan P" first="P." last="Natarajan">P. Natarajan</name>
<name sortKey="Ramirez Uiz, E" sort="Ramirez Uiz, E" uniqKey="Ramirez Uiz E" first="E." last="Ramirez-Ruiz">E. Ramirez-Ruiz</name>
<name sortKey="Smith, I A" sort="Smith, I A" uniqKey="Smith I" first="I. A." last="Smith">I. A. Smith</name>
<name sortKey="Tilanus, R P J" sort="Tilanus, R P J" uniqKey="Tilanus R" first="R. P. J." last="Tilanus">R. P. J. Tilanus</name>
</country>
<country name="Italie"><noRegion><name sortKey="Rol, E" sort="Rol, E" uniqKey="Rol E" first="E." last="Rol">E. Rol</name>
</noRegion>
</country>
<country name="Pays-Bas"><noRegion><name sortKey="Wijers, R A M J" sort="Wijers, R A M J" uniqKey="Wijers R" first="R. A. M. J." last="Wijers">R. A. M. J. Wijers</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>
Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Amerique/explor/CaltechV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000322 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000322 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien |wiki= Wicri/Amerique |area= CaltechV1 |flux= Main |étape= Exploration |type= RBID |clé= ISTEX:E9B600C6D24088A13F1B1D8DB67E61A9D73EB3C9 |texte= The submillimetre properties of gamma‐ray burst host galaxies }}
This area was generated with Dilib version V0.6.32. |