2024ApJ...972...83B


Query : 2024ApJ...972...83B

2024ApJ...972...83B - Astrophys. J., 972, 83 (2024/September-1)

Single-pulse Gamma-Ray Bursts Have Prevalent Hard-to-soft Spectral Evolution.

BUSBY I. and LAZZATI D.

Abstract (from CDS):

We analyze the spectral evolution of 62 bright Fermi gamma-ray bursts with large enough signal-to-noise to allow for time-resolved spectral analysis. We develop a new algorithm to test for single-pulse morphology that is insensitive to the specific shape of pulses. Instead, it only checks whether or not there are multiple, isolated, or statistical significant peaks in the light curve. In addition, we carry out a citizen science test to assess light-curve morphology and spectral evolution. We find that, no matter the adopted assessment method, bursts characterized by single-peaked prompt emission light curves have a greater tendency to also have a consistently decaying peak energy or hard-to-soft spectral evolution. This contrasts with the behavior of multipeaked bursts, for which the tendency is to have a peak frequency that is not monotonically decreasing. We discuss this finding in the theoretical framework of internal/external shocks and find it to be consistent with at least some single-pulse bursts associated with particularly high-density environments.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gamma-ray bursts - Spectral energy distribution

Simbad objects: 24

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Number of rows : 24
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Fermi bn110428388 gB 00 22 22.89 +64 50 56.8           ~ 26 0
2 Fermi bn081221681 gB 01 03 10.2 -24 32 53           ~ 186 0
3 Fermi bn110213220 gB 02 51 51.37 +49 16 21.2           ~ 175 0
4 Fermi bn100122616 gB 05 16.8 -02 43           ~ 26 0
5 Fermi bn100829876 gB 06 02 +30.3           ~ 20 0
6 Fermi bn110407998 gB 06 30 -11.9           ~ 10 0
7 GRB 111127A gB 06 55 +03.5           ~ 10 0
8 GRB 100511A gB 07 17.2 -04 39           ~ 28 0
9 Fermi bn090804940 gB 08 42 -11.3           ~ 21 0
10 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 201 0
11 Fermi bn110903009 gB 10 57 +42.1           ~ 13 0
12 Fermi bn120624933 gB 11 23 31.98 +08 55 42.1           ~ 100 0
13 Fermi bn101231067 gB 12 47 +17.6           ~ 14 0
14 Fermi bn100910818 gB 15 52.4 -34 37           ~ 17 0
15 GRB 100722A gB 15 55.1 -15 37           ~ 13 0
16 Fermi bn081009140 gB 16 42 +18.4           ~ 40 0
17 GRB 120707A gB 19 24 -34.4           ~ 21 0
18 GRB 110721A gB 22 10 -38.6           ~ 155 0
19 Fermi bn110817191 gB 22 24 -45.8           ~ 17 0
20 GRB 191019A gB 22 40 05.87 -17 19 40.8           ~ 55 0
21 Fermi bn081124060 gB 22 40 -14.6           ~ 13 0
22 Fermi bn120323507 gB 22 42 +29.7           ~ 60 0
23 GRB 100612B gB 23 28 -01.8           ~ 23 0
24 GRB 110729A gB 23 34 +05.0           ~ 15 0

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