dc.contributor.author |
Maclachlan, GA |
|
dc.contributor.author |
Shenoy, Aditi |
|
dc.contributor.author |
Sonbaş, Eda |
|
dc.contributor.author |
Dhuga, K. S. |
|
dc.contributor.author |
Eskandarian, Azim |
|
dc.contributor.author |
Maximon, LC |
|
dc.contributor.author |
Parke, WC |
|
dc.date.accessioned |
2022-05-31T08:22:06Z |
|
dc.date.available |
2022-05-31T08:22:06Z |
|
dc.date.issued |
2012 |
|
dc.identifier.issn |
0035-8711 |
|
dc.identifier.uri |
http://dspace.adiyaman.edu.tr:8080/xmlui/handle/20.500.12414/3060 |
|
dc.description.abstract |
We present a direct link between the minimum variability time-scales extracted through a wavelet decomposition and the rise times of the shortest pulses extracted via fits of 34 Fermi Gamma-ray Burst Monitor (GBM) Gamma-Ray Burst (GRB) light curves comprised of 379 pulses. Pulses used in this study were fitted with lognormal functions, whereas the wavelet technique used employs a multiresolution analysis that does not rely on identifying distinct pulses. By applying a corrective filter to published data fitted with pulses, we demonstrate agreement between these two independent techniques and offer a method for distinguishing signal from noise. |
tr |
dc.language.iso |
en |
tr |
dc.publisher |
Oxford Unıv Press |
tr |
dc.subject |
Methods: data analysis |
tr |
dc.subject |
Gamma-ray burst: general |
tr |
dc.title |
The minimum variability time-scale and its relation to pulse profiles of Fermi GRBs |
tr |
dc.type |
Article |
tr |
dc.contributor.authorID |
0000-0002-6909-192X |
tr |
dc.contributor.department |
George Washington Univ, Dept Phys |
tr |
dc.contributor.department |
Adiyaman Univ, Dept Phys, |
tr |
dc.contributor.department |
NASA Goddard Space Flight Ctr |
tr |
dc.identifier.endpage |
L35 |
tr |
dc.identifier.issue |
1 |
tr |
dc.identifier.startpage |
L32 |
tr |
dc.identifier.volume |
425 |
tr |
dc.source.title |
Monthly Notices Of The Royal Astronomical Society |
tr |