scholarly journals An Explanation for the Bimodal Duration Distribution of Gamma-Ray Bursts: Millisecond Pulsars from Accretion-induced Collapse

1998 ◽  
Vol 494 (2) ◽  
pp. L163-L166 ◽  
Author(s):  
Insu Yi ◽  
Eric G. Blackman
2006 ◽  
Vol 365 (3) ◽  
pp. 874-884 ◽  
Author(s):  
A. Janiuk ◽  
B. Czerny ◽  
R. Moderski ◽  
D. B. Cline ◽  
C. Matthey ◽  
...  

2013 ◽  
Vol 436 (2) ◽  
pp. 1867-1872 ◽  
Author(s):  
D. Lazzati ◽  
M. Villeneuve ◽  
D. López-Cámara ◽  
B. J. Morsony ◽  
R. Perna

10.14311/1510 ◽  
2012 ◽  
Vol 52 (1) ◽  
Author(s):  
D. Szécsi ◽  
Z. Bagoly ◽  
I. Horváth ◽  
L. G. Balázs ◽  
P. Veres ◽  
...  

The Fermi satellite has a particular motion during its flight which enables it to catch the gamma-ray bursts mostly well. The side-effect of this favourable feature is that the lightcurves of the GBM detectors are stressed by rapidly and extremely varying background. Before this data is processed, it needs to be separated from the background. The commonly used methods [3,7] were useless for most cases of Fermi, so we developed a new technique based on the motion and orientation of the satellite. The background-free lightcurve can be used to perform statistical surveys, hence we showed the efficiency of our background-filtering method presenting a statistical analysis known from the literature.


1996 ◽  
Vol 166 (7) ◽  
pp. 743-762 ◽  
Author(s):  
B.I. Luchkov ◽  
I.G. Mitrofanov ◽  
I.L. Rozental'
Keyword(s):  

2018 ◽  
Vol 189 (08) ◽  
pp. 785-802 ◽  
Author(s):  
Rafail L. Aptekar ◽  
Andrei M. Bykov ◽  
Sergei V. Golenetskii ◽  
Dmitrii D. Frederiks ◽  
Dmitry S. Svinkin ◽  
...  

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