[vsnet-grb-info 2860] GRB 060206: Swift-BAT refined analysis
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Tue Feb 7 06:19:31 JST 2006
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 4697
SUBJECT: GRB 060206: Swift-BAT refined analysis
DATE: 06/02/06 21:16:50 GMT
FROM: David Palmer at LANL <palmer at lanl.gov>
D. Palmer (LANL), L. Barbier (GSFC), S. Barthelmy (GSFC),
M. Chester (PSU), J. Cummings (GSFC/ORAU), E. Fenimore (LANL),
N. Gehrels (GSFC), D. Hullinger (UMD), H. Krimm (GSFC/USRA),
C. Markwardt (GSFC/UMD), F. Marshall (GSFC), T. Mitani (ISAS),
A. Parsons (GSFC), T. Sakamoto (GSFC/ORAU), G. Sato (ISAS),
M. Suzuki (Saitama), J. Tueller (GSFC), on behalf of the Swift/BAT team:
Using the data set from T-60 to T+123 sec from the recent telemetry
downlink, we report further analysis of BAT GRB 060206 (trigger
# 180455) (GCN Circ 4682, Morris et al.). The BAT ground-calculated
position is (RA,Dec) = 202.932, 35.050 deg {13h 31m 43.8s, 35d 2' 58.7"}
(J2000) +- 1.0 arcmin, (radius, sys_stat, 90% containment). The partial
coding was 98%.
The 1-second binned light curve shows a single peak which extends out to
around 8 seconds in the two lowest energy bins (15-25 and
25-50 keV), but is shorter in duration in the two highest energy bins
(50-100 and 100-350 keV), extending out to only about 4 seconds. This
could be an indication the burst is softening with time. The highest
energy bin shows a possible double peak structure, with the first peak
at T0-1 second. T90 (15-350 keV) is 7 +- 2 seconds (estimated error
including systematics).
The time-averaged spectrum from T-0.6 to T+13.7 is best fit by a
power law with an exponential cutoff. This fit gives a photon index
1.06 +- 0.34, and Epeak of 75.4 +- 19.5 keV (chi squared 57.88
for 56 d.o.f.). For this model the total fluence in the 15 - 150 keV
band is (8.4 +- 0.4) x 10^-07 erg/cm2 and the 1-sec peak flux
measured form T+2.11 sec in the 15-150 keV band is (2.8 +- 0.2)
ph/cm2/sec. A fit to a simple power law gives a photon index
of 1.69 +- 0.08 (chi squared 69.94 for 57 d.o.f.).
All the quoted errors are at the 90% confidence level.
Using the best fit photon index and Epeak with a Band model with
the high energy photon index fixed at beta = -2.5, and the redshift
of 4.045 (Fynbo et al. GCN 4692), the isotropic-equivalent energy,
Eiso, integrated from 1 to 1000 keV at the GRB rest frame is
5.8 x 10^52 ergs. This Eiso and the Epeak at the GRB rest frame
((1+z)*Epeak = 380 keV) are consistent with the Epeak-Eiso (Amati)
relation (Amati et al, 2002). The Eiso in the BAT observed
energy band (76 - 757 keV in the GRB rest frame) is 3.1 x 10^52 ergs.
The estimated jet break time using the Eiso-Epeak-t_break relation
(Liang & Zhang, ApJ, 633, 611) would be 8.6 days after the burst
at the observer's frame (using the Band model). Using a cutoff
power-law for the analysis (which is also consistent with the
data) gives a 10.4 day estimate for the break time.
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