2011ApJ...738..138R

Query : 2011ApJ...738..138R

2011ApJ...738..138R - Astrophys. J., 738, 138 (2011/September-2)

Fermi and Swift gamma-ray burst afterglow population studies.

RACUSIN J.L., OATES S.R., SCHADY P., BURROWS D.N., DE PASQUALE M., DONATO D., GEHRELS N., KOCH S., McENERY J., PIRAN T., ROMING P., SAKAMOTO T., SWENSON C., TROJA E., VASILEIOU V., VIRGILI F., WANDERMAN D. and ZHANG B.

Abstract (from CDS):

The new and extreme population of gamma-ray bursts (GRBs) detected by the Fermi Large Area Telescope (LAT) shows several new features in high-energy gamma rays that are providing interesting and unexpected clues into GRB prompt and afterglow emission mechanisms. Over the last six years, it has been Swift that has provided the robust data set of UV/optical and X-ray afterglow observations that opened many windows into components of GRB emission structure. The relationship between the LAT-detected GRBs and the well-studied, fainter, and less energetic GRBs detected by the Swift Burst Alert Telescope is only beginning to be explored by multi-wavelength studies. We explore the large sample of GRBs detected by BAT only, BAT and the Fermi Gamma-ray Burst Monitor (GBM), and GBM and LAT, focusing on these samples separately in order to search for statistically significant differences between the populations, using only those GRBs with measured redshifts in order to physically characterize these objects. We disentangle which differences are instrumental selection effects versus intrinsic properties in order to better understand the nature of the special characteristics of the LAT bursts.

Abstract Copyright: ∼

Journal keyword(s): gamma-ray burst: general - gamma rays: general - X-rays: bursts

Simbad objects: 42

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Number of rows : 42
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 GRB 060912A gB 00 21 08.11 +20 58 18.9           ~ 116 1
2 GRB 060708 gB 00 31 13.850 -33 45 32.40 19.07 19.79 17.37     ~ 109 0
3 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
4 GRB 081222 gB 01 30 57.76 -34 05 44.0           ~ 199 0
5 Fermi bn091208410 gB 01 57 38.50 +16 52 50.7           ~ 220 0
6 GRB 091018 gB 02 08 46 -57 33.0           ~ 169 0
7 GRB 061007 gB 03 05 19.510 -50 30 02.50 14.28 14.40 12.95     ~ 315 1
8 GRB 070318 gB 03 13 56.830 -42 56 46.30 18.27 16.23 15.49     ~ 170 0
9 GRB 091029 gB 04 00 40.00 -55 57 12.7           ~ 168 0
10 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
11 GRB 090328 gB 06 02 39.69 -41 52 55.1           ~ 194 1
12 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
13 GRB 090102 gB 08 32 59.50 +33 06 25.7           ~ 253 0
14 GRB 061021 gB 09 40 36.120 -21 57 05.40 18.21 19.20 16.82     ~ 160 0
15 GRB 080430 gB 11 01 14.63 +51 41 07.8           ~ 157 0
16 GRB 090426 G 12 36 18.0470 +32 59 09.460           ~ 237 0
17 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
18 Fermi bn090323002 gB 12 42 50.28 +17 03 11.9           ~ 244 1
19 Fermi bn100414097 gB 12 48 30.0 +08 41 35           ~ 136 0
20 GRB 050801 gB 13 36 35.000 -21 55 41.00 15.03 15.82 15.46     ~ 164 0
21 GRB 080319B gB 14 31 41.04 +36 18 09.2           ~ 508 0
22 GRB 080310 gB 14 40 13.89 -00 10 30.4           ~ 214 0
23 GRB 060714 gB 15 11 26.450 -06 33 58.30   20.21 18.54     ~ 209 0
24 GRB 080906 gB 15 12 13 -80 32.4           ~ 63 0
25 GRB 060502A gB 16 03 42.480 +66 36 02.49     18.65     ~ 143 0
26 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
27 GRB 091003A gB 16 46 04.680 +36 37 31.08           ~ 135 0
28 GRB 060926 gB 17 35 43.660 +13 02 18.60     19.36     ~ 135 0
29 Fermi bn090902462 gB 17 39 45.26 +27 19 28.1           ~ 440 0
30 GRB 090618 gB 19 36 01.80 +78 21 07.1           ~ 358 0
31 4B 941017 gB 20 06.2 +09 49           ~ 93 0
32 GRB 050922C gB 21 09 33.000 -08 45 30.10 15.15 15.86 14.69     ~ 301 0
33 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
34 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0
35 GRB 090809 gB 21 54 43.2 -00 05 02           ~ 90 0
36 GRB 051221 G 21 54 48.626 +16 53 27.16 19.49         ~ 377 0
37 GRB 060607 gB 21 58 50.400 -22 29 46.70 18.49 16.67 15.09     ~ 318 0
38 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
39 Fermi bn080916406 gB 22 25 09.30 -57 01 33.7           ~ 177 0
40 GRB 060604 gB 22 28 55.010 -10 54 55.80 20.34 20.31       ~ 134 0
41 SN 2008hw SN* 22 39 50.39 -40 08 49.1           SNIc 197 1
42 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0

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