2013ApJ...774...76A


Query : 2013ApJ...774...76A

2013ApJ...774...76A - Astrophys. J., 774, 76 (2013/September-1)

New Fermi-LAT event reconstruction reveals more high-energy gamma rays from gamma-ray bursts.

ATWOOD W.B., BALDINI L., BREGEON J., BRUEL P., CHEKHTMAN A., COHEN-TANUGI J., DRLICA-WAGNER A., GRANOT J., LONGO F., OMODEI N., PESCE-ROLLINS M., RAZZAQUE S., ROCHESTER L.S., SGRO C., TINIVELLA M., USHER T.L. and ZIMMER S.

Abstract (from CDS):

Based on the experience gained during the four and a half years of the mission, the Fermi-LAT Collaboration has undertaken a comprehensive revision of the event-level analysis going under the name of Pass 8. Although it is not yet finalized, we can test the improvements in the new event reconstruction with the special case of the prompt phase of bright gamma-ray bursts (GRBs), where the signal-to-noise ratio is large enough that loose selection cuts are sufficient to identify gamma rays associated with the source. Using the new event reconstruction, we have re-analyzed 10 GRBs previously detected by the Large Area Telescope (LAT) for which an X-ray/optical follow-up was possible and found four new gamma rays with energies greater than 10 GeV in addition to the seven previously known. Among these four is a 27.4 GeV gamma ray from GRB 080916C, which has a redshift of 4.35, thus making it the gamma ray with the highest intrinsic energy (∼147 GeV) detected from a GRB. We present here the salient aspects of the new event reconstruction and discuss the scientific implications of these new high-energy gamma rays, such as constraining extragalactic background light models, Lorentz invariance violation tests, the prompt emission mechanism, and the bulk Lorentz factor of the emitting region.

Abstract Copyright: ∼

Journal keyword(s): astroparticle physics - cosmology: observations - gamma rays: general - methods: data analysis

Simbad objects: 10

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Number of rows : 10
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 bn091208410 gB 01 57 38.50 +16 52 50.7           ~ 220 0
2 GRB 090328 gB 06 02 39.69 -41 52 55.1           ~ 194 1
3 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
4 Fermi bn090323002 gB 12 42 50.28 +17 03 11.9           ~ 244 1
5 Fermi bn100414097 gB 12 48 30.0 +08 41 35           ~ 136 0
6 GRB 091003A gB 16 46 04.680 +36 37 31.08           ~ 135 0
7 Fermi bn090902462 gB 17 39 45.26 +27 19 28.1           ~ 440 0
8 Fermi bn110731465 gB 18 42 00.99 -28 32 13.8           ~ 193 0
9 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
10 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0

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