[HTML][HTML] High-redshift cosmology by Gamma-Ray Bursts: An overview
Abstract Several correlations among Gamma-Ray Bursts (GRBs) quantities, both in the
prompt and afterglow emissions, have been established during the last decades, thus …
prompt and afterglow emissions, have been established during the last decades, thus …
Gamma Ray Burst afterglow and prompt-afterglow relations: An overview
MG Dainotti, R Del Vecchio - New Astronomy Reviews, 2017 - Elsevier
The mechanism responsible for the afterglow emission of Gamma Ray Bursts (GRBs) and its
connection to the prompt γ-ray emission is still a debated issue. Relations between intrinsic …
connection to the prompt γ-ray emission is still a debated issue. Relations between intrinsic …
How bad or good are the external forward shock afterglow models of gamma-ray bursts?
The external forward shock models have been the standard paradigm to interpret the
broadband afterglow data of gamma-ray bursts (GRBs). One prediction of the models is that …
broadband afterglow data of gamma-ray bursts (GRBs). One prediction of the models is that …
The optical two-and three-dimensional fundamental plane correlations for nearly 180 gamma-ray burst afterglows with Swift/UVOT, RATIR, and the subaru telescope
Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. We study
optical plateaus in GRB afterglows via an extended search into archival data. We …
optical plateaus in GRB afterglows via an extended search into archival data. We …
X-ray plateaus in gamma-ray bursts' light curves from jets viewed slightly off-axis
P Beniamini, R Duque, F Daigne… - Monthly Notices of the …, 2020 - academic.oup.com
Using multiple observational arguments, recent work has shown that cosmological gamma-
ray bursts (GRBs) are typically viewed at angles within, or close to the cores of their …
ray bursts (GRBs) are typically viewed at angles within, or close to the cores of their …
Synchrotron self-Compton emission from external shocks as the origin of the sub-TeV emission in GRB 180720B and GRB 190114C
XY Wang, RY Liu, HM Zhang, SQ **… - The Astrophysical …, 2019 - iopscience.iop.org
Recently, very high-energy photons above 100 GeV were reported to be detected from GRB
190114C and GRB 180720B at, respectively, 100–1000 s and 10 hr after the burst. We …
190114C and GRB 180720B at, respectively, 100–1000 s and 10 hr after the burst. We …
The optical luminosity–time correlation for more than 100 Gamma-ray burst afterglows
Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. Their
afterglow emission is observed from sub-TeV energies to radio wavelengths. We investigate …
afterglow emission is observed from sub-TeV energies to radio wavelengths. We investigate …
Cosmological fast optical transients with the Zwicky Transient Facility: a search for dirty fireballs
Dirty fireballs are a hypothesized class of relativistic massive-star explosions with an initial
Lorentz factor Γ init below the Γ init∼ 100 required to produce a long-duration gamma-ray …
Lorentz factor Γ init below the Γ init∼ 100 required to produce a long-duration gamma-ray …
Gamma-ray burst jet breaks revisited
XG Wang, B Zhang, EW Liang, RJ Lu… - The Astrophysical …, 2018 - iopscience.iop.org
Gamma-ray Burst (GRB) collimation has been inferred with the observations of achromatic
steepening in GRB light curves, known as jet breaks. Identifying a jet break from a GRB …
steepening in GRB light curves, known as jet breaks. Identifying a jet break from a GRB …
A comprehensive analysis of fermi gamma-ray burst data. III. energy-dependent T90 distributions of GBM GRBs and instrumental selection effect on duration …
Y Qin, EW Liang, YF Liang, SX Yi, L Lin… - The Astrophysical …, 2012 - iopscience.iop.org
ABSTRACT The durations (T 90) of 315 gamma-ray bursts (GRBs) detected with Fermi/GBM
(8–1000 keV) up to 2011 September are calculated using the Bayesian Block method. We …
(8–1000 keV) up to 2011 September are calculated using the Bayesian Block method. We …