2016ApJ...818..110B


Query : 2016ApJ...818..110B

2016ApJ...818..110B - Astrophys. J., 818, 110 (2016/February-3)

Do the Fermi Gamma-ray Burst Monitor and Swift Burst Alert Telescope see the same short gamma-ray bursts?

BURNS E., CONNAUGHTON V., ZHANG B.-B., LIEN A., BRIGGS M.S., GOLDSTEIN A., PELASSA V. and TROJA E.

Abstract (from CDS):

Compact binary system mergers are expected to generate gravitational radiation detectable by ground-based interferometers. A subset of these, the merger of a neutron star with another neutron star or a black hole, are also the most popular model for the production of short gamma-ray bursts (GRBs). The Swift Burst Alert Telescope (BAT) and the Fermi Gamma-ray Burst Monitor (GBM) trigger on short GRBs (SGRBs) at rates that reflect their relative sky exposures, with the BAT detecting 10 per year compared to about 45 for GBM. We examine the SGRB populations detected by Swift BAT and Fermi GBM. We find that the Swift BAT triggers on weaker SGRBs than Fermi GBM, providing they occur close to the center of the BAT field of view, and that the Fermi GBM SGRB detection threshold remains flatter across its field of view. Overall, these effects combine to give the instruments the same average sensitivity, and account for the SGRBs that trigger one instrument but not the other. We do not find any evidence that the BAT and GBM are detecting significantly different populations of SGRBs. Both instruments can detect untriggered SGRBs using ground searches seeded with time and position. The detection of SGRBs below the on-board triggering sensitivities of Swift BAT and Fermi GBM increases the possibility of detecting and localizing the electromagnetic counterparts of gravitational wave (GW) events seen by the new generation of GW detectors.

Abstract Copyright: ∼

Journal keyword(s): gamma-ray burst: general

VizieR on-line data: <Available at CDS (J/ApJ/818/110): table1.dat table2.dat table3.dat table4.dat>

Simbad objects: 54

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Number of rows : 54
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 140930B gB 00 25 23.40 +24 17 41.7           ~ 52 0
2 Fermi bn100117879 G 00 45 04.6610 -01 35 42.020           ~ 155 0
3 Fermi bn111117510 gB 00 50 46.220 +23 00 39.22           ~ 141 0
4 GRB 100625A gB 01 03 10.98 -39 05 18.3           ~ 124 0
5 GRB 120229A gB 01 20 07.90 -35 47 44.0           ~ 22 0
6 Fermi bn081024245 gB 01 51 33.80 +61 21 08.2           ~ 75 0
7 GRB 090417A gB 02 19 59.0 -07 10 51           ~ 36 0
8 GRB 141212A G 02 36 29.9570 +18 08 47.228           ~ 70 0
9 GRB 120403A gB 02 49 49.80 +40 29 21.8           ~ 21 0
10 PSO J047.1631+13.1580 G 03 08 39.14930640 +13 09 29.0253240           ~ 144 0
11 GRB 120305A gB 03 10 08.73 +28 29 30.9           ~ 56 0
12 Fermi bn130912358 gB 03 10 25.60 +13 59 55.7           ~ 57 0
13 GRB 090815C gB 04 17 57 -65 57.0           ~ 19 0
14 GRB 101219A gB 04 58 20.45 -02 32 23.1           ~ 152 0
15 Fermi bn141205337 gB 06 11 26.16 +37 52 33.6           ~ 27 0
16 Fermi bn081101491 gB 06 23 20.70 -00 06 41.5           ~ 39 0
17 GRB 091109B gB 07 30 59.90 -54 05 30.6           ~ 57 0
18 Fermi bn081226044 G 08 02 00.4500 -69 01 49.500           ~ 63 0
19 GRB 120521A gB 09 54 53.91 -49 25 02.4           ~ 41 0
20 Fermi bn101129652 gB 10 23 41 -17 38.7           ~ 34 0
21 GRB 090515 gB 10 56 41.0 +14 27 22           ~ 122 0
22 GRB 121226A G 11 14 34.1210 -30 24 22.840           ~ 44 0
23 SDSS J112848.22+170418.5 G 11 28 48.22989 +17 04 18.5014           ~ 393 0
24 GALEX J123205.0-105600 Bz? 12 32 04.9717245480 -10 56 00.722548932         16.421 ~ 186 0
25 GRB 090426 G 12 36 18.0470 +32 59 09.460           ~ 237 0
26 GRB 100724A gB 12 58 10.38 -11 06 09.3           ~ 198 0
27 GRB 140414A gB 13 01 14 +56 54.1           ~ 18 0
28 GRB 140606A gB 13 27 11.70 +37 35 56.5           ~ 25 0
29 Fermi bn140402007 gB 13 50 23.67 +05 46 28.0           ~ 41 0
30 GRB 100628A gB 15 03 53.59 -31 39 50.4           ~ 50 0
31 GRB 120804A G 15 35 47.5100 -28 46 56.110           ~ 99 0
32 GRB 130313A gB 15 45 38.41 -00 22 08.3           ~ 35 0
33 GRB 140903A G 15 52 03.2650 +27 36 10.710           ~ 138 0
34 GRB 090305 G 16 07 07.5960 -31 33 22.540           ~ 53 0
35 GRB 100702A gB 16 22 47.26 -56 31 53.8           ~ 53 0
36 GRB 140516A gB 16 51 57.40 +39 57 46.3           ~ 38 0
37 GRB 080919 gB 17 40 53.00 -42 22 29.5           ~ 49 0
38 Fermi bn130626452 gB 18 12 30.60 -09 31 29.9           ~ 28 0
39 GRB 111126A gB 18 24 14 +51 27.7           ~ 14 0
40 Fermi bn140320092 gB 18 47 22.40 -11 11 18.5           ~ 29 0
41 Fermi bn130515056 gB 18 53 45.65 -54 16 45.0           ~ 55 0
42 PSO J285.9246+45.7134 G 19 03 41.90914320 +45 42 48.4220520           ~ 63 0
43 GRB 111020A gB 19 08 12.53 -38 00 43.0           ~ 66 0
44 Fermi bn080905499 G 19 10 42.0450 -18 52 54.510           ~ 200 0
45 Fermi bn131004904 gB 19 44 27.20 -02 57 31.0           ~ 113 0
46 Fermi bn150101270 gB 20 50 24.81 +36 43 58.9           ~ 26 0
47 Fermi bn090621922 gB 20 53 49.30 +69 02 02.9           ~ 65 0
48 GRB 140622A gB 21 08 41.56 -14 25 09.5           ~ 61 0
49 Fermi bn110420946 gB 21 20 10.90 -41 16 38.0           ~ 39 0
50 GRB 140129B G 21 47 01.6490 +26 12 23.270           ~ 30 0
51 GRB 110112A gB 21 59 43.77 +26 27 24.4           ~ 47 0
52 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
53 GRB 140611A gB 23 19 40.22 -40 06 16.5           ~ 14 0
54 GRB 120630A gB 23 29 10.75 +42 33 17.4           ~ 19 0

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