Gamma-ray burst spectral-luminosity correlations in the synchrotron scenario

Open Access

Table A.2.

Bursts in the single-bin sample, Band subsample.

GRB	Redshift	L_iso	E_p, z	α	p value	log B	Best-fit model
		[10⁵¹ erg/s]	[keV]
GRB081221A	2.26	$125 . 09_{- 5.62}^{+ 6.95}$ $125.09_{-5.62}^{+6.95}$	$347_{- 12}^{+ 15}$ $347_{-12}^{+15}$	$- 0 . 12_{- 0.09}^{+ 0.08}$ $-0.12_{-0.09}^{+0.08}$	2.8 × 10⁻⁵	-21.01	B
GRB090102A	1.55	$58 . 69_{- 4.3}^{+ 4.56}$ $58.69_{-4.3}^{+4.56}$	$984_{- 74}^{+ 73}$ $984_{-74}^{+73}$	$- 0 . 13_{- 0.09}^{+ 0.11}$ $-0.13_{-0.09}^{+0.11}$	2.2 × 10⁻²	-15.69	B
GRB090510A	0.9	$248 . 08_{- 15.72}^{+ 16.1}$ $248.08_{-15.72}^{+16.1}$	$7842_{- 546}^{+ 627}$ $7842_{-546}^{+627}$	$- 0 . 69_{- 0.04}^{+ 0.04}$ $-0.69_{-0.04}^{+0.04}$	6.3 × 10⁻⁴	-9.5	B
GRB090902B	1.82	$572 . 25_{- 20.62}^{+ 22.39}$ $572.25_{-20.62}^{+22.39}$	$2117_{- 74}^{+ 83}$ $2117_{-74}^{+83}$	$0 . 18_{- 0.08}^{+ 0.1}$ $0.18_{-0.08}^{+0.1}$	< 10⁻¹⁶	-41.64	B
GRB090926A	2.11	$741 . 84_{- 12.9}^{+ 14.39}$ $741.84_{-12.9}^{+14.39}$	$778_{- 25}^{+ 24}$ $778_{-25}^{+24}$	$- 0 . 4_{- 0.03}^{+ 0.03}$ $-0.4_{-0.03}^{+0.03}$	1.6 × 10⁻¹¹	-36.65	B
GRB140206A	2.73	$177 . 82_{- 11.21}^{+ 12.83}$ $177.82_{-11.21}^{+12.83}$	$450_{- 27}^{+ 27}$ $450_{-27}^{+27}$	$0 . 7_{- 0.19}^{+ 0.22}$ $0.7_{-0.19}^{+0.22}$	1.6 × 10⁻¹¹	-33.19	B
GRB140508A	1.03	$128 . 89_{- 4.0}^{+ 4.49}$ $128.89_{-4.0}^{+4.49}$	$726_{- 35}^{+ 35}$ $726_{-35}^{+35}$	$- 0 . 5_{- 0.03}^{+ 0.03}$ $-0.5_{-0.03}^{+0.03}$	2.3 × 10⁻²	-14.73	B
GRB140801A	1.32	$30 . 65_{- 1.17}^{+ 1.3}$ $30.65_{-1.17}^{+1.3}$	$294_{- 10}^{+ 10}$ $294_{-10}^{+10}$	$- 0 . 01_{- 0.08}^{+ 0.08}$ $-0.01_{-0.08}^{+0.08}$	1.0 × 10⁻⁴	-29.85	B
GRB150314A	1.76	$394 . 64_{- 10.69}^{+ 11.12}$ $394.64_{-10.69}^{+11.12}$	$727_{- 27}^{+ 27}$ $727_{-27}^{+27}$	$- 0 . 3_{- 0.04}^{+ 0.04}$ $-0.3_{-0.04}^{+0.04}$	1.1 × 10⁻¹⁶	-42.04	B
GRB190114C	0.42	$68 . 9_{- 1.48}^{+ 1.56}$ $68.9_{-1.48}^{+1.56}$	$786_{- 14}^{+ 14}$ $786_{-14}^{+14}$	$- 0 . 08_{- 0.03}^{+ 0.03}$ $-0.08_{-0.03}^{+0.03}$	< 10⁻¹⁶	-294.36	B
GRB200826A	0.75	$23 . 76_{- 1.81}^{+ 2.32}$ $23.76_{-1.81}^{+2.32}$	$212_{- 17}^{+ 17}$ $212_{-17}^{+17}$	$- 0 . 27_{- 0.11}^{+ 0.13}$ $-0.27_{-0.11}^{+0.13}$	3.1 × 10⁻³	-7.67	B
GRB200829A	1.25	$724 . 37_{- 12.25}^{+ 13.45}$ $724.37_{-12.25}^{+13.45}$	$730_{- 20}^{+ 24}$ $730_{-20}^{+24}$	$- 0 . 24_{- 0.03}^{+ 0.04}$ $-0.24_{-0.03}^{+0.04}$	< 10⁻¹⁶	-88.57	B
GRB201020B	0.8	$25 . 65_{- 1.62}^{+ 1.5}$ $25.65_{-1.62}^{+1.5}$	$422_{- 22}^{+ 29}$ $422_{-22}^{+29}$	$- 0 . 65_{- 0.05}^{+ 0.04}$ $-0.65_{-0.05}^{+0.04}$	4.0 × 10⁻²	-2.33	B
GRB210619B	1.94	$2678 . 56_{- 42.36}^{+ 40.39}$ $2678.56_{-42.36}^{+40.39}$	$1157_{- 36}^{+ 38}$ $1157_{-36}^{+38}$	$- 0 . 38_{- 0.02}^{+ 0.02}$ $-0.38_{-0.02}^{+0.02}$	< 10⁻¹⁶	-88.54	B
GRB220527A	0.86	$48 . 13_{- 1.18}^{+ 1.28}$ $48.13_{-1.18}^{+1.28}$	$268_{- 6}^{+ 6}$ $268_{-6}^{+6}$	$- 0 . 35_{- 0.03}^{+ 0.03}$ $-0.35_{-0.03}^{+0.03}$	2.5 × 10⁻¹⁴	-52.47	B
GRB230812B	0.36	$50 . 44_{- 0.41}^{+ 0.48}$ $50.44_{-0.41}^{+0.48}$	$323_{- 3}^{+ 3}$ $323_{-3}^{+3}$	$- 0 . 11_{- 0.01}^{+ 0.01}$ $-0.11_{-0.01}^{+0.01}$	< 10⁻¹⁶	< − 10³	B

Notes. The GRBs here listed are the ones which do not meet the condition of Table A.1. Therefore, we report redshifts z (see Sec. 2.1), isotropic-equivalent luminosities L_iso, rest-frame peak energies E_p,z and low energy photon indices α obtained from the Band fit. We report errors at 68 per cent confidence level. We further report the p value returned from the PPC analysis, the Bayes factor log B obtained comparing Band and synchrotron models, and the associated best-fit model: S = synchrotron, B = Band, and ND = not defined; in other words, when |log B|< 0.5

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.