PMO OpenIR  > 南极天文中心
The afterglow and host galaxy of GRB 090205: evidence of a Ly-alpha emitter at z=4.65
D'Avanzo, P.1; Perri, M.2; Fugazza, D.1; Salvaterra, R.3; Chincarini, G.1,4; Margutti, R.1,4; Wu, X. F.5,6,7; Thoene, C. C.1; Fernandez-Soto, A.8; Ukwatta, T. N.9,10; Burrows, D. N.5; Gehrels, N.10; Meszaros, P.5,6,11; Toma, K.5,6; Zhang, B.12; Covino, S.1; Campana, S.1; D'Elia, V.2,13; Della Valle, M.14,15; Piranomonte, S.13
2010-11-01
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume522Pages:A20
AbstractContext. Gamma-ray bursts (GRBs) have proven to be detectable to distances much larger than any other astrophysical object, providing the most effective way, complementing ordinary surveys of studying the high redshift universe.
KeywordGamma Rays: General
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201014801
WOS KeywordGAMMA-RAY BURSTS ; LYMAN-BREAK GALAXIES ; STAR-FORMATION ; TELESCOPE OBSERVATIONS ; STELLAR POPULATIONS ; HIGH-REDSHIFT ; 1ST SURVEY ; SWIFT ; ORIGIN ; FLARES
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000284153100026
Citation statistics
Cited Times:17[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/1189
Collection南极天文中心
Affiliation1.INAF Osservatorio Astron Brera, I-23807 Merate, Italy
2.ASI Sci Data Ctr, I-00044 Frascati, Italy
3.Univ Insubria, Dipartimento Fis & Matemat, I-22100 Como, Italy
4.Univ Milano Bicocca, Dipartimento Fis, I-20126 Milan, Italy
5.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
6.Penn State Univ, Ctr Particle Astrophys, University Pk, PA 16802 USA
7.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
8.Inst Fis Cantabria CSIC UC, Santander 39005, Spain
9.George Washington Univ, Washington, DC 20052 USA
10.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
11.Penn State Univ, Dept Phys, University Pk, PA 16802 USA
12.Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA
13.INAF Osservatorio Astron Roma, I-00040 Monte Porzio Catone, Italy
14.INAF Osservatorio Astron Capodimonte, I-80131 Naples, Italy
15.Int Ctr Relativist Astrophys, I-65122 Pescara, Italy
Recommended Citation
GB/T 7714
D'Avanzo, P.,Perri, M.,Fugazza, D.,et al. The afterglow and host galaxy of GRB 090205: evidence of a Ly-alpha emitter at z=4.65[J]. ASTRONOMY & ASTROPHYSICS,2010,522:A20.
APA D'Avanzo, P..,Perri, M..,Fugazza, D..,Salvaterra, R..,Chincarini, G..,...&Piranomonte, S..(2010).The afterglow and host galaxy of GRB 090205: evidence of a Ly-alpha emitter at z=4.65.ASTRONOMY & ASTROPHYSICS,522,A20.
MLA D'Avanzo, P.,et al."The afterglow and host galaxy of GRB 090205: evidence of a Ly-alpha emitter at z=4.65".ASTRONOMY & ASTROPHYSICS 522(2010):A20.
Files in This Item:
File Name/Size DocType Version Access License
2010016The afterglow(571KB) 开放获取--View Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[D'Avanzo, P.]'s Articles
[Perri, M.]'s Articles
[Fugazza, D.]'s Articles
Baidu academic
Similar articles in Baidu academic
[D'Avanzo, P.]'s Articles
[Perri, M.]'s Articles
[Fugazza, D.]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[D'Avanzo, P.]'s Articles
[Perri, M.]'s Articles
[Fugazza, D.]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 2010016The afterglow and host galaxy of GRB 090205_ evidence of a Ly-alpha emitter at z=4.65 .pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.