2012MNRAS.425L..32M


Query : 2012MNRAS.425L..32M

2012MNRAS.425L..32M - Mon. Not. R. Astron. Soc., 425, L32-L35 (2012/September-1)

The minimum variability time-scale and its relation to pulse profiles of Fermi GRBs.

MacLACHLAN G.A., SHENOY A., SONBAS E., DHUGA K.S., ESKANDARIAN A., MAXIMON L.C. and PARKE W.C.

Abstract (from CDS):

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.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): methods: data analysis - gamma-ray burst: general

Simbad objects: 4

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Number of rows : 4
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 bn080925775 gB 06 24.4 +18 12           ~ 28 0
2 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
3 GRB 081215A gB 08 22 +54.0           ~ 57 0
4 GRB 080825C gB 15 28.8 -04 54           ~ 71 0

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