2010ApJ...722..862J


Query : 2010ApJ...722..862J

2010ApJ...722..862J - Astrophys. J., 722, 862-870 (2010/October-2)

Very high energy observations of gamma-ray bursts with STACEE.

JARVIS A., ONG R.A., WILLIAMS D.A., AUNE T., BALL J., CARSON J.E., COVAULT C.E., DRISCOLL D.D., FORTIN P., GINGRICH D.M., HANNA D.S., KILDEA J., LINDNER T., MUKHERJEE R., MUELLER C., RAGAN K. and ZWEERINK J.

Abstract (from CDS):

Gamma-ray bursts (GRBs) are the most powerful explosions known in the universe. Sensitive measurements of the high-energy spectra of GRBs can place important constraints on the burst environments and radiation processes. Until recently, there were no observations during the first few minutes of GRB afterglows in the energy range between 30 GeV and ∼1 TeV. With the launch of the Swift GRB Explorer in late 2004, GRB alerts and localizations within seconds of the bursts became available. The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) was a ground-based, gamma-ray telescope with an energy threshold of ∼150 GeV for sources at zenith. At the time of Swift's launch, STACEE was in a rare position to provide >150 GeV follow-up observations of GRBs as fast as three minutes after the burst alert. In addition, STACEE performed follow-up observations of several GRBs that were localized by the HETE-2 and INTEGRAL satellites. Between 2002 June and 2007 July, STACEE made follow-up observations of 23 GRBs. Upper limits are placed on the high-energy gamma-ray fluxes from 21 of these bursts.

Abstract Copyright:

Journal keyword(s): gamma-ray burst: general - gamma-ray burst: individual (GRB 050509B, GRB 050607) - gamma rays: general

Simbad objects: 29

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Number of rows : 29
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 GRB 041016 gB 01 45 24 -04 39.5           ~ 14 0
2 GRB 021112 gB 02 36 52 +48 50.9           ~ 21 0
3 GRB 031220 gB 04 39.6 +07 22           ~ 21 0
4 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4908 1
5 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5765 4
6 GRB 061028 gB 06 28 54.700 +46 17 57.20           ~ 45 0
7 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 326 0
8 GRB 050209 gB 08 26.0 +19 41           ~ 13 0
9 GRB 060121 gB 09 09 51.930 +45 39 45.41           ~ 113 1
10 GRB 070223 gB 10 13 48.390 +43 08 00.71 21.47         ~ 54 0
11 GRB 060323 gB 11 37 44.910 +50 00 33.49           ~ 46 0
12 GRB 050408 gB 12 02 17.320 +10 51 10.00           ~ 144 0
13 GRB 050412 gB 12 04 25.060 -01 12 03.60           ~ 77 0
14 GRB 070419A gB 12 10 58.830 +39 55 34.06 18.52         ~ 111 0
15 GRB 050509B gB 12 36 18.000 +29 01 24.00           ~ 285 1
16 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 290 0
17 GRB 030324 gB 13 37 04.4 -00 15 34           ~ 34 0
18 GRB 060526 gB 15 31 18.360 +00 17 04.90   18.31 17.16     ~ 242 0
19 GRB 090902B gB 17 39 45.26 +27 19 28.1           ~ 340 0
20 2XMM J174931.6-280805 LXB 17 49 31.940 -28 08 05.80           ~ 88 0
21 GRB 040422 gB 18 42 01 +01 58.9           ~ 19 0
22 GRB 030501 gB 19 05 30 +06 18.4           ~ 27 0
23 GRB 070610 X 19 55 09.60 +26 14 06.7           ~ 51 0
24 GRB 050607 gB 20 00 42.790 +09 08 31.50   19.55 18.94     ~ 86 0
25 GRB 050509A gB 20 42 20.000 +54 04 17.30     20.55     ~ 33 0
26 GRB 090510 gB 22 14 12.60 -26 35 51.1           ~ 429 1
27 GRB 040916 gB 23 00 55.1 -05 38 43           ~ 33 0
28 GRB 061222A gB 23 53 03.419 +46 31 58.60           ~ 139 0
29 GRB 050402 gB ~ ~           ~ 4 0

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2021.07.31-07:35:47

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