Home > Publications database > Temporal and Spectral Evolution of Gamma-Ray Burst Broad Pulses: Identification of High-latitude Emission in the Prompt Emission > print |
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024 | 7 | _ | |a arXiv:2212.07095 |2 arXiv |
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088 | _ | _ | |a arXiv:2212.07095 |2 arXiv |
100 | 1 | _ | |a Tak, Donggeun |0 P:(DE-H253)PIP1094637 |b 0 |e Corresponding author |
245 | _ | _ | |a Temporal and Spectral Evolution of Gamma-Ray Burst Broad Pulses: Identification of High-latitude Emission in the Prompt Emission |
260 | _ | _ | |a London |c 2023 |b Institute of Physics Publ. |
336 | 7 | _ | |a article |2 DRIVER |
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500 | _ | _ | |a 30 pages, 36 figures, accepted to ApJ |
520 | _ | _ | |a We perform a detailed analysis of broad pulses in bright gamma-ray bursts (GRBs) to understand the evolution of GRB broad pulses. Using the temporal and spectral properties, we test the high-latitude emission (HLE) scenario in the decaying phase of broad pulses. The HLE originates from the curvature effect of a relativistic spherical jet, where higher-latitude photons are delayed and softer than the observer's line-of-sight emission. The signature of HLE has not yet been identified undisputedly during the prompt emission of GRBs. The HLE theory predicts a specific relation, $F_v$,${_E}_p$∝$E^{2}_{p}$, between the peak energy $E_p$ in $νF_ν$ spectra and the spectral flux $F_ν$ measured at $E_p$. . We search for evidence of this relation in 2157 GRBs detected by the Gamma-ray Burst Monitor on board the Fermi Gamma-ray Space Telescope from 2008 to 2017. After imposing unbiased selection criteria in order to minimize contamination in a signal by background and overlaps of pulses, we build a sample of 32 broad pulses in 32 GRBs. We perform a time-resolved spectral analysis on each of these 32 broad pulses and find that the evolution of 18 pulses (56%) is clearly consistent with the HLE relation. For the 18 broad pulses, the exponent δ in the relation of $F_v$,${_E}_p$∝$E^{\delta}_{p}$ is distributed as a Gaussian function with a median and width of 1.99 and 0.34, respectively. This result provides a constraint on the emission radius of GRBs with the HLE signature. |
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700 | 1 | _ | |a Uhm, Z. Lucas |b 1 |
700 | 1 | _ | |a Racusin, Judith |0 0000-0002-4744-9898 |b 2 |
700 | 1 | _ | |a Zhang, Bing |b 3 |
700 | 1 | _ | |a Guiriec, Sylvain |0 0000-0001-5780-8770 |b 4 |
700 | 1 | _ | |a Kocevski, Daniel |0 0000-0001-9201-4706 |b 5 |
700 | 1 | _ | |a Zhang, Bin-Bin |b 6 |
700 | 1 | _ | |a McEnery, Julie |b 7 |
773 | _ | _ | |a 10.3847/1538-4357/acc581 |g Vol. 949, no. 2, p. 110 - |0 PERI:(DE-600)1473835-1 |n 2 |p 110 |t The astrophysical journal / Part 1 |v 949 |y 2023 |x 0004-637X |
856 | 4 | _ | |y OpenAccess |u https://bib-pubdb1.desy.de/record/599254/files/Temporal%20and%20Spectral%20Evolution%20of%20Gamma-Ray%20Burst%20Broad.pdf |
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