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Article: The high-redshift star formation rate derived from gamma-ray bursts: possible origin and cosmic reionization

TitleThe high-redshift star formation rate derived from gamma-ray bursts: possible origin and cosmic reionization
Authors
Issue Date2013
PublisherEDP Sciences. The Journal's web site is located at http://www.aanda.org
Citation
Astronomy & Astrophysics, 2013, v. 556, p. A90:1-7 How to Cite?
Persistent Identifierhttp://hdl.handle.net/10722/194740
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorWang, Fen_US
dc.date.accessioned2014-02-17T02:05:36Z-
dc.date.available2014-02-17T02:05:36Z-
dc.date.issued2013en_US
dc.identifier.citationAstronomy & Astrophysics, 2013, v. 556, p. A90:1-7en_US
dc.identifier.urihttp://hdl.handle.net/10722/194740-
dc.languageengen_US
dc.publisherEDP Sciences. The Journal's web site is located at http://www.aanda.orgen_US
dc.relation.ispartofAstronomy & Astrophysicsen_US
dc.rightsThe original publication is available at [journal web site]en_US
dc.titleThe high-redshift star formation rate derived from gamma-ray bursts: possible origin and cosmic reionizationen_US
dc.typeArticleen_US
dc.identifier.emailWang, F: fayin@hku.hken_US
dc.identifier.doi10.1051/0004-6361/201321623en_US
dc.identifier.hkuros227768en_US
dc.identifier.volume556en_US
dc.identifier.spageA90:1en_US
dc.identifier.epage7en_US
dc.identifier.isiWOS:000323893500090-

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