File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

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
KeywordsDark ages, reionization, first stars
Gamma rays: general
Stars: formation
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
ISSN
2023 Impact Factor: 5.4
2023 SCImago Journal Rankings: 1.896
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.issn0004-6361-
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.subjectDark ages, reionization, first stars-
dc.subjectGamma rays: general-
dc.subjectStars: formation-
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.scopuseid_2-s2.0-84881087908-
dc.identifier.hkuros227768en_US
dc.identifier.volume556en_US
dc.identifier.spageA90:1en_US
dc.identifier.epage7en_US
dc.identifier.eissn1432-0746-
dc.identifier.isiWOS:000323893500090-
dc.identifier.issnl0004-6361-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats