scholarly journals How Temporal Symmetry Defines Morphology in BATSE Gamma-Ray Burst Pulse Light Curves

2021 ◽  
Vol 919 (1) ◽  
pp. 37
Author(s):  
Jon Hakkila
2018 ◽  
Vol 863 (1) ◽  
pp. 77 ◽  
Author(s):  
Jon Hakkila ◽  
Stephen Lesage ◽  
Stanley McAfee ◽  
Eric Hofesmann ◽  
Corinne Maly Taylor ◽  
...  

1999 ◽  
Vol 511 (2) ◽  
pp. 852-861 ◽  
Author(s):  
Andrei Gruzinov ◽  
Eli Waxman

2008 ◽  
Vol 386 (2) ◽  
pp. 859-863 ◽  
Author(s):  
P. A. Curran ◽  
A. J. van der Horst ◽  
R. A. M. J. Wijers
Keyword(s):  

2015 ◽  
Vol 815 (2) ◽  
pp. 134 ◽  
Author(s):  
Jon Hakkila ◽  
Amy Lien ◽  
Takanori Sakamoto ◽  
David Morris ◽  
James E. Neff ◽  
...  

2006 ◽  
Vol 650 (1) ◽  
pp. 252-260 ◽  
Author(s):  
Y. Hirose ◽  
M. Umemura ◽  
A. Yonehara ◽  
J. Sato

2020 ◽  
Vol 493 (3) ◽  
pp. 3379-3397 ◽  
Author(s):  
A Rossi ◽  
G Stratta ◽  
E Maiorano ◽  
D Spighi ◽  
N Masetti ◽  
...  

ABSTRACT Multimessenger astronomy received a great boost following the discovery of kilonova (KN) AT2017gfo, the optical counterpart of the gravitational wave source GW170817 associated with the short gamma-ray burst GRB 170817A. AT2017gfo was the first KN that could be extensively monitored in time using both photometry and spectroscopy. Previously, only few candidates have been observed against the glare of short GRB afterglows. In this work, we aim to search the fingerprints of AT2017gfo-like KN emissions in the optical/NIR light curves of 39 short GRBs with known redshift. For the first time, our results allow us to study separately the range of luminosity of the blue and red components of AT2017gfo-like kilonovae in short GRBs. In particular, the red component is similar in luminosity to AT2017gfo, while the blue KN can be more than 10 times brighter. Finally, we exclude a KN as luminous as AT2017gfo in GRBs 050509B and 061201.


2009 ◽  
Vol 695 (1) ◽  
pp. L10-L14 ◽  
Author(s):  
Ayah Lazar ◽  
Ehud Nakar ◽  
Tsvi Piran

2009 ◽  
Vol 705 (1) ◽  
pp. 372-385 ◽  
Author(s):  
Jon Hakkila ◽  
Robert J. Nemiroff

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