The Fermi GBM gamma-ray burst time-resolved spectral catalog: brightest bursts in the first four years

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Table C.1

Best-fit parameters of the identified significant blackbodies of the PLBB model.

GRB name	Spectrum	T_start:T_stop	A_PL	α	A_BB	kT	ΔCSTAT
		(s)	(ph s^-1 cm^-2 keV^-1)		(ph s^-1 cm^-2 keV^-1)	(keV)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)

090618353	46	79.706:80.155	0.0249 ± 0.0061	−1.70 ± 0.06	3.135E−04 ± 1.22E−04	22.12 ± 1.72	57.57
090618353	77	96.641:110.742	0.0051 ± 0.0010	−1.88 ± 0.03	1.333E−04 ± 3.59E−05	15.59 ± 0.81	128.1
090902462^a	10	6.433:6.851	0.0216 ± 0.0021	−1.56 ± 0.05	1.456E−06 ± 1.79E−07	181.20 ± 6.14	12.43
090902462^a	11	6.851:7.218	0.0233 ± 0.0024	−1.58 ± 0.06	1.600E−06 ± 2.08E−07	175.70 ± 6.18	29.47
090902462	12	7.218:7.500	0.0315 ± 0.0031	−1.61 ± 0.05	2.050E−06 ± 2.78E−07	170.50 ± 6.25	82.4
090902462	13	7.500:7.774	0.0387 ± 0.0037	−1.62 ± 0.05	9.601E−07 ± 1.28E−07	222.10 ± 8.40	59.65
090902462	14	7.774:7.958	0.0516 ± 0.0048	−1.63 ± 0.05	9.149E−07 ± 1.48E−07	227.70 ± 10.50	102.04
090902462	15	7.958:8.119	0.0804 ± 0.0069	−1.65 ± 0.04	9.125E−07 ± 1.60E−07	228.50 ± 11.60	67.74
090902462	16	8.119:8.280	0.0635 ± 0.0068	−1.71 ± 0.05	1.179E−06 ± 2.15E−07	204.90 ± 10.40	53.62
090902462	17	8.280:8.424	0.0672 ± 0.0068	−1.76 ± 0.05	8.905E−07 ± 1.53E−07	237.60 ± 11.80	181.34
090902462	18	8.424:8.563	0.0708 ± 0.0065	−1.66 ± 0.04	1.150E−06 ± 2.22E−07	210.40 ± 11.50	125.79
090902462	19	8.563:8.706	0.0681 ± 0.0069	−1.76 ± 0.05	7.986E−07 ± 1.42E−07	240.00 ± 12.30	153.02
090902462	20	8.706:8.874	0.0590 ± 0.0061	−1.75 ± 0.04	5.968E−07 ± 1.13E−07	244.80 ± 13.50	129.94
090902462	21	8.874:9.030	0.0630 ± 0.0063	−1.72 ± 0.05	1.093E−06 ± 1.97E−07	213.70 ± 10.90	148.11
090902462	22	9.030:9.184	0.0772 ± 0.0073	−1.75 ± 0.04	6.380E−07 ± 1.05E−07	264.90 ± 12.90	177.34
090902462	23	9.184:9.315	0.0955 ± 0.0089	−1.71 ± 0.04	1.088E−06 ± 2.37E−07	206.80 ± 12.70	83.87
090902462	24	9.315:9.443	0.0806 ± 0.0088	−1.78 ± 0.05	1.569E−06 ± 3.36E−07	184.40 ± 10.80	536.44
090902462	25	9.443:9.595	0.0890 ± 0.0086	−1.77 ± 0.04	1.567E−06 ± 3.22E−07	184.50 ± 10.40	115.81
090902462	26	9.595:9.721	0.0841 ± 0.0091	−1.78 ± 0.05	3.432E−06 ± 7.35E−07	146.70 ± 8.08	97.97
090902462	27	9.721:9.816	0.1082 ± 0.0117	−1.79 ± 0.05	7.694E−06 ± 1.28E−06	137.40 ± 5.79	110.98
090902462	28	9.816:9.938	0.0940 ± 0.0104	−1.83 ± 0.05	5.745E−06 ± 1.18E−06	128.70 ± 6.56	95.97
090902462	29	9.938:10.059	0.0726 ± 0.0081	−1.73 ± 0.05	3.282E−06 ± 6.22E−07	154.90 ± 7.61	73.25
090902462	30	10.059:10.206	0.0663 ± 0.0076	−1.81 ± 0.06	2.682E−06 ± 4.41E−07	168.50 ± 7.36	126.01
090902462	31	10.206:10.383	0.0550 ± 0.0067	−1.85 ± 0.06	2.792E−06 ± 4.81E−07	155.40 ± 6.97	126.13
090902462	32	10.383:10.561	0.0659 ± 0.0066	−1.78 ± 0.05	8.862E−07 ± 1.40E−07	234.30 ± 10.70	159.15
090902462	33	10.561:10.720	0.0678 ± 0.0068	−1.74 ± 0.05	1.050E−06 ± 1.85E−07	218.80 ± 11.00	136.11
090902462	34	10.720:10.881	0.0826 ± 0.0081	−1.71 ± 0.04	1.020E−06 ± 2.25E−07	199.20 ± 12.30	43.77
090902462	35	10.881:11.011	0.0665 ± 0.0068	−1.71 ± 0.05	2.275E−06 ± 4.08E−07	176.10 ± 8.45	124.71
090902462	36	11.011:11.145	0.0837 ± 0.0080	−1.68 ± 0.04	3.913E−06 ± 7.07E−07	150.70 ± 7.16	54.48
090902462	37	11.145:11.326	0.0505 ± 0.0055	−1.76 ± 0.05	1.764E−06 ± 3.30E−07	171.00 ± 8.50	128.03
090902462	38	11.326:11.521	0.0403 ± 0.0052	−1.83 ± 0.06	2.410E−06 ± 5.04E−07	142.30 ± 7.58	110.62
090902462	39	11.521:11.718	0.0478 ± 0.0051	−1.68 ± 0.05	2.258E−06 ± 3.98E−07	160.60 ± 7.38	83.84
090902462	40	11.718:11.934	0.0448 ± 0.0054	−1.84 ± 0.06	2.277E−06 ± 3.93E−07	158.80 ± 7.21	158.65
090902462	41	11.934:12.204	0.0498 ± 0.0054	−1.72 ± 0.04	2.949E−06 ± 8.41E−07	114.80 ± 8.21	34.59
110622158	13	29.726:31.428	0.0084 ± 0.0024	−1.79 ± 0.07	7.874E−05 ± 3.01E−05	26.23 ± 1.28	155.02
110622158	15	33.430:36.752	0.0046 ± 0.0015	−1.72 ± 0.05	6.697E−05 ± 2.49E−05	21.13 ± 1.10	155.29

Notes. Column (1) lists the GRB names. Column (2) lists the spectrum numbers within individual burst. Column (3) lists the start times T_start and end times T_stop for the time bins. Columns(4)−(7) list the best-fit parameters of the PLBB model. Column (7) lists the values of ΔCSTAT = CSTAT(BEST)−CSTAT(PLBB).

^(a)

We note that for these two spectra the BEST models are SBPL (the rest BEST models from this burst are all COMP), CSTAT values between SBPL and PLBB are directly compared without performing any simulations.

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