YNAO OpenIR  > 丽江天文观测站(南方基地)
Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts
Bi, Xiongwei1,2; Mao JR(毛基荣)2,3,4; Liu CX(刘传玺)3,4,5; Bai JM(白金明)2,3,4
Source PublicationASTROPHYSICAL JOURNAL
2018-10-20
Volume866Issue:2Pages:15
DOI10.3847/1538-4357/aadcf8
Contribution Rank第3完成单位
Indexed BySCI
Keywordgamma rays: general radiation mechanisms: non-thermal
Abstract

We build a comprehensive sample to statistically describe the properties of X-ray flashes (XRFs) and X-ray riches (XRRs) from the third Swift Burst Alert Telescope (BAT3) catalog of Gamma-ray bursts (GRBs). We obtain 81 XRFs, 540 XRRs, and 394 classical GRBs (C-GRBs). We statistically explore the different properties of the.-ray prompt emission, the X-ray emission, the X-ray light-curve type, the association with supernovae (SNe), and the host galaxy properties for these sources. We confirm that most XRFs/XRRs are long GRBs with low values of peak energy Epeak obs and they are low-luminosity GRBs. XRFs, XRRs, and C-GRBs follow the same EX, iso-E., iso-Epeak, z correlations. Compared to the classical GRBs, XRFs are favorable to have the association with SN explosions. We do not find any significant differences of redshift distribution and host galaxy properties among XRFs, XRRs, and C-GRBs. We also discuss some observational biases and selection effects that may affect our statistical results. The GRB detectors with wide energy range and low energy threshold are expected for the XRF/XRR research in the future.

Funding ProjectOpen Project Program of the Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201501] ; Scientific Research Foundation of the Education Department of Yunnan Province[2014Y463] ; National Natural Science Foundation of China[11433004] ; National Natural Science Foundation of China[11404103] ; National Natural Science Foundation of China[11673062] ; National Natural Science Foundation of China[11661161010] ; Hundred Talent Program ; Major Program of the Chinese Academy of Sciences[KJZD-EW-M06] ; Oversea Talent Program of Yunnan Province ; Ministry of Science and Technology of China[2016YFA0400700]
Funding OrganizationOpen Project Program of the Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences[OP201501] ; Scientific Research Foundation of the Education Department of Yunnan Province[2014Y463] ; National Natural Science Foundation of China[11433004, 11404103, 11673062, 11661161010] ; Hundred Talent Program ; Major Program of the Chinese Academy of Sciences[KJZD-EW-M06] ; Oversea Talent Program of Yunnan Province ; Ministry of Science and Technology of China[2016YFA0400700]
Language英语
Subject Area天文学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeArticle
PublisherIOP PUBLISHING LTD
Publication PlaceTEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS IDWOS:000448150800011
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordOFF-AXIS ; HOST GALAXIES ; E-P,E-I-E-ISO CORRELATION ; LIGHT CURVES ; GRB 130427A ; JET MODELS ; AFTERGLOW ; SUPERNOVAE ; UNIVERSAL ; EMISSION
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/18041
Collection丽江天文观测站(南方基地)
中国科学院天体结构与演化重点实验室
Corresponding AuthorMao JR(毛基荣)
Affiliation1.Department of Physics, Honghe University, 661199 Mengzi, People's Republic of China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, People's Republic of China
3.Yunnan Observatories, Chinese Academy of Sciences, 650011 Kunming, Yunnan Province, People's Republic of China
4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, 100012 Beijing, People's Republic of China
5.University of Chinese Academy of Sciences, 100049 Beijing, People's Republic of China
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Bi, Xiongwei,Mao JR,Liu CX,et al. Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts[J]. ASTROPHYSICAL JOURNAL,2018,866(2):15.
APA Bi, Xiongwei,Mao JR,Liu CX,&Bai JM.(2018).Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts.ASTROPHYSICAL JOURNAL,866(2),15.
MLA Bi, Xiongwei,et al."Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts".ASTROPHYSICAL JOURNAL 866.2(2018):15.
Files in This Item:
File Name/Size DocType Version Access License
Statistical Study of(6715KB)期刊论文出版稿开放获取CC BY-NC-SAView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Bi, Xiongwei]'s Articles
[Mao JR(毛基荣)]'s Articles
[Liu CX(刘传玺)]'s Articles
Baidu academic
Similar articles in Baidu academic
[Bi, Xiongwei]'s Articles
[Mao JR(毛基荣)]'s Articles
[Liu CX(刘传玺)]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Bi, Xiongwei]'s Articles
[Mao JR(毛基荣)]'s Articles
[Liu CX(刘传玺)]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: Statistical Study of the Swift X-Ray Flash and X-Ray Rich Gamma-Ray Bursts.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

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