2012MNRAS.421.1256N


Query : 2012MNRAS.421.1256N

2012MNRAS.421.1256N - Mon. Not. R. Astron. Soc., 421, 1256-1264 (2012/April-1)

A complete sample of bright Swift long gamma-ray bursts: testing the spectral-energy correlations.

NAVA L., SALVATERRA R., GHIRLANDA G., GHISELLINI G., CAMPANA S., COVINO S., CUSUMANO G., D'AVANZO P., D'ELIA V., FUGAZZA D., MELANDRI A., SBARUFATTI B., VERGANI S.D. and TAGLIAFERRI G.

Abstract (from CDS):

We use a nearly complete sample of gamma-ray bursts (GRBs) detected by the Swift satellite to study the correlations between the spectral peak energy Epeak of the prompt emission, the isotropic energetics Eiso and the isotropic luminosity Liso. This GRB sample is characterized by a high level of completeness in redshift (90 per cent). This allows us to probe in an unbiased way the issue related to the physical origin of these correlations against selection effects. We find that one burst, GRB 061021, is an outlier to the Epeak–Eisocorrelation. Despite this case, we find strong Epeak–Eiso and Epeak–Liso correlations for the bursts of the complete sample. Their slopes, normalizations and dispersions are consistent with those found with the whole sample of bursts with measured redshift and Epeak. This means that the biases present in the total sample commonly used to study these correlations do not affect their properties. Finally, we also find no evolution with redshift of the Epeak–Eiso and Epeak–Lisocorrelations.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

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

Simbad objects: 60

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Number of rows : 60
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 Fermi bn081221681 gB 01 03 10.2 -24 32 53           ~ 186 0
3 GRB 080602 gB 01 16 42.18 -09 13 55.4           ~ 61 0
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 060908 gB 02 07 18.360 +00 20 31.20 16.99 18.34 16.85     ~ 217 0
7 GRB 091018 gB 02 08 46 -57 33.0           ~ 169 0
8 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
9 GRB 071112C gB 02 36 50.89 +28 22 16.9           ~ 164 0
10 GRB 060306 gB 02 44 22.830 -02 08 55.00           ~ 119 0
11 Fermi bn100728439 gB 02 56 13.44 +00 16 51.6           ~ 142 0
12 Fermi bn090926914 gB 03 05 14.30 -38 59 50.9           ~ 149 1
13 GRB 061007 gB 03 05 19.510 -50 30 02.50 14.28 14.40 12.95     ~ 315 1
14 GRB 050318 gB 03 18 51.000 -46 23 43.61 18.10 18.68 17.58     ~ 189 0
15 GRB 060210 gB 03 50 57.370 +27 01 34.40   20.27       ~ 275 0
16 GRB 070328 gB 04 20 27.680 -34 04 00.60 20.29         ~ 97 0
17 GRB 081121 gB 05 57 07.70 -60 36 42.1           ~ 152 0
18 GRB 090201 gB 06 08 12.30 -46 36 16.1           ~ 68 0
19 GRB 071020 gB 07 58 39.65 +32 51 38.8           ~ 158 0
20 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
21 GRB 090102 gB 08 32 59.50 +33 06 25.7           ~ 253 0
22 GRB 110503A gB 08 51 06.31 +52 12 27.7           ~ 115 0
23 GRB 061021 gB 09 40 36.120 -21 57 05.40 18.21 19.20 16.82     ~ 160 0
24 GRB 061121 gB 09 48 54.570 -13 11 42.68 17.19 17.71 17.02     ~ 350 0
25 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 222 1
26 GRB 110205A gB 10 58 31.12 +67 31 31.2           ~ 213 0
27 GRB 080430 gB 11 01 14.63 +51 41 07.8           ~ 157 0
28 GRB 080613B gB 11 35 11.51 -07 06 17.5           ~ 51 0
29 Fermi bn091020900 gB 11 42 55.20 +50 58 42.0           ~ 188 0
30 GRB 080603B gB 11 46 07.46 +68 03 38.5           ~ 153 0
31 Fermi bn100615083 gB 11 48 49.25 -19 28 52.2           ~ 133 0
32 GRB 050416 gB 12 33 54.600 +21 03 26.69     19.12     ~ 300 1
33 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
34 GRB 080607A gB 12 59 47.14 +15 55 09.6           ~ 257 0
35 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
36 GRB 080319B gB 14 31 41.04 +36 18 09.2           ~ 508 0
37 GRB 050802 gB 14 37 05.820 +27 47 12.62 16.85 17.38 16.97     ~ 186 0
38 GRB 060814 gB 14 45 21.480 +20 35 11.80           ~ 241 0
39 GRB 080721A gB 14 57 55.76 -11 43 24.9           ~ 180 0
40 GRB 081203A gB 15 32 07.6 +63 31 15           ~ 177 0
41 GRB 060904A gB 15 50 54.560 +44 59 10.51           ~ 77 0
42 GRB 070521 gB 16 10 38.600 +30 15 22.70           ~ 164 0
43 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
44 GRB 090715B gB 16 45 21.59 +44 50 20.1           ~ 144 0
45 GRB 080319C gB 17 15 55.48 +55 23 31.7           ~ 174 0
46 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
47 SN 2005nc SN* 18 32 32.560 +26 20 22.34           SNIc: 400 1
48 GRB 090709A gB 19 19 46.70 +60 43 40.8           ~ 125 0
49 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
50 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
51 GRB 050922C gB 21 09 33.000 -08 45 30.10 15.15 15.86 14.69     ~ 301 0
52 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
53 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0
54 Fermi bn080804972 gB 21 54 41.90 -53 11 20.2           ~ 158 0
55 GRB 060927A gB 21 58 11.930 +05 21 50.32           ~ 215 0
56 GRB 071117 gB 22 20 10.40 -63 26 36.6           ~ 112 0
57 Fermi bn080916406 gB 22 25 09.30 -57 01 33.7           ~ 177 0
58 SN 2008hw SN* 22 39 50.39 -40 08 49.1           SNIc 197 1
59 GRB 090812 gB 23 32 48.5 -10 36 17           ~ 165 0
60 GRB 061222A gB 23 53 03.419 +46 31 58.60           ~ 177 0

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