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作 者:Xiao-Li Zhang Yong-Feng Huang Ze-Cheng Zou
机构地区:[1]Department of Physics,Nanjing University,Nanjing 210023,China [2]School of Astronomy and Space Science,Nanjing University,Nanjing 210023,China [3]Key Laboratory of Modern Astronomy and Astrophysics(Nanjing University),Ministry of Education,Nanjing 210023,China [4]Xinjiang Astronomical Observatory,Chinese Academy of Sciences,Urumqi 830011,China
出 处:《Research in Astronomy and Astrophysics》2023年第12期57-62,共6页天文和天体物理学研究(英文版)
基 金:supported by the National Natural Science Foundation of China(grant Nos.12233002,12041306,12147103,U1938201);by the National SKA Program of China(No.2020SKA0120300);by the National Key R&D Program of China(2021YFA0718500);by the Youth Innovations and Talents Project of Shandong Provincial Colleges and Universities(grant No.201909118)。
摘 要:A negative correlation was found to exist between the low-energy spectral index and the redshift of gamma-ray bursts(GRBs)by Amati et al.It was later confirmed by Geng&Huang and Gruber et al.,but the correlation was also found to be quite dispersive when the sample size was significantly expanded.In this study,we have established two even larger samples of GRBs to further examine the correlation.One of our samples consists of316 GRBs detected by the Swift satellite,and the other one consists of 80 GRBs detected by the Fermi satellite.It is found that there is no correlation between the two parameters for the Swift sample,but there does exist a weak negative correlation for the Fermi sample.The correlation becomes even more significant when the spectral index at the peak flux is considered.It is argued that the absence of the correlation in the Swift sample may be due to the fact that Swift has a very narrow energy response so that it could not measure the low-energy spectral index accurately enough.Further studies based on even larger GRB samples are solicited.
关 键 词:(stars:)gamma-ray burst general-methods statistical-catalogs
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