The long γ-ray burst rate and the correlation with host galaxy properties

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Volume 539 (March 2012)

A&A, 539 (2012) A113

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Table 3

Properties of the GROND dark burst samples.

Burst	z^a	log ₁₀(E_iso/erg)	T₉₀	Prompt model^b					Sample^c

				Name	α	E_peak	K_A	Δt
			(s)			(keV)	phkeV^-1cm^-2s^-1	(s)

GRB100316B	1.180 (1)	51.57	4.3	...	...	...	...	...	S, P, UL1, UL2
GRB091127	0.490 (2)	52.36	9.6	...	...	...	...	...	S, P, UL1, UL2
GRB091029	2.752 (3)	52.84	40.0	...	...	...	...	...	S, P, UL1, UL2
GRB091018	0.971 (4)	51.88	4.4	...	...	...	...	...	S, P, UL1, UL2
GRB090926B	1.24 (5)	52.52	126.4	...	...	...	...	...	S, P, UL1, UL2
GRB090814A	0.696 (6)	51.30	113.2	...	...	...	...	...	S, P, UL1, UL2
GRB090812	2.452 (7)	53.89	99.8	...	...	...	...	...	S, P, UL1, UL2
GRB090519	3.85 (8)	53.76	81.8	...	...	...	...	...	S, P, UL1, UL2
GRB090313	3.375 (9)	53.11	90.2	...	...	...	...	...	S, P, UL1, UL2
GRB090102	1.547 (10)	53.65	30.7	...	...	...	...	...	S, P, UL1, UL2
GRB081222	2.77 (11)	53.17	33.5	...	...	...	...	...	S, P, UL1, UL2
GRB081121	2.512 (12)	53.08	19.4	...	...	...	...	...	S, P, UL1, UL2
GRB081029	3.848 (13)	53.48	169.1	...	...	...	...	...	S, P, UL1, UL2
GRB081008	1.968 (14)	52.83	199.3	...	...	...	...	...	S, P, UL1, UL2
GRB081007	0.529 (15)	50.89	5.6	...	...	...	...	...	S, P, UL1, UL2
GRB080913	6.7 (16)	52.72	8.2	...	...	...	...	...	S, P, UL1, UL2
GRB080805	1.505 (17, 18)	52.99	111.8	...	...	...	...	...	S, P, UL1, UL2
GRB080804	2.20 (19, 18)	53.94	61.7	...	...	...	...	...	S, P, UL1, UL2
GRB080710	0.845 (20, 18)	52.69	139.1	...	...	...	...	...	S, P, UL1, UL2
GRB080707	1.23 (21, 18)	52.07	30.3	...	...	...	...	...	S, P, UL1, UL2
GRB080605	1.640 (22, 18)	53.31	19.6	...	...	...	...	...	S, P, UL1, UL2
GRB080520	1.545 (23, 18)	52.68	3.0	...	...	...	...	...	S, P, UL1, UL2
GRB080413B	1.1 (24, 18)	52.17	7.0	...	...	...	...	...	S, P, UL1, UL2
GRB080413A	2.433 (25, 18)	53.41	46.7	...	...	...	...	...	S, P, UL1, UL2
GRB080411	1.03 (26, 18)	53.60	58.3	...	...	...	...	...	S, P, UL1, UL2
GRB080330	1.51 (27)	52.13	66.1	...	...	...	...	...	S, P, UL1, UL2
GRB080210	2.641 (28, 18)	53.06	43.9	...	...	...	...	...	S, P, UL1, UL2
GRB080129	4.349 (29)	53.42	45.6	...	...	...	...	...	S, P, UL1, UL2
GRB071031	2.692 (30)	52.91	187.2	...	...	...	...	...	S, P, UL1, UL2
GRB071010A	0.98 (31)	51.56	22.4	...	...	...	...	...	S, P, UL1, UL2
GRB070802	2.45 (32)	52.16	14.7	...	...	...	...	...	S, P, UL1, UL2

GRB090429B	9.2 (33)	53.42	5.8	CPL			0.059	7.55	P, UL1, UL2
GRB081228	3.4 (34)	52.43	3.8	PL		...	0.028	4.44	P, UL1, UL2
GRB080516	3.6 (35)	52.98	6.8	PL		...	0.039	7.83	P, UL1, UL2

GRB091221	<3.3^d	54.21	69.0	PL		...	0.043	101.31	UL1, UL2
GRB090904B	<5.0^d	54.94	58.2	PL		...	0.105	86.40	UL1, UL2

GRB100205A	12.0^e	54.2	32.76	PL		...	0.008	41.40	UL2

Notes.

^(a)

If not mentioned otherwise, the redshift is taken from Greiner et al. (2011a).

^(b)

Both the prompt best-fit model and parameters are taken from NB11. They are only listed if the E_iso was calculated manually.

^(c)

S: Spectroscopic, P: Photometric, UL1: upper limit 1, UL2: upper limit 2.

^(d)

These upper limits are treated as being the actual redshift value.

^(e)

Value taken from between 11 < z < 13.5, (Cucchiara et al. 2010).

References. All references are taken from Greiner et al. (2011a, Table 2). (1) Vergani et al. (2010); (2) Cucchiara et al. (2009); (3) Chornock et al. (2009b); (4) Chen et al. (2009); (5) Fynbo et al. (2009b); (6) Jakobsson et al. (2009); (7) de Ugarte Postigo et al. (2009a); (8) Thoene et al. (2009); (9) Chornock et al. (2009a); de Ugarte Postigo et al. (2010); (10) de Ugarte Postigo et al. (2009b); (11) Cucchiara et al. (2008); (12) Berger & Rauch (2008); (13) D’Elia et al. (2008); (14) D’Avanzo et al. (2008); (15) Berger et al. (2008); (16) Greiner et al. (2009b); (17) Jakobsson et al. (2008b); (18) Fynbo et al. (2009a); (19) Thoene et al. (2008b); (20) Perley et al. (2008); (21) Fynbo et al. (2008a); (22) Jakobsson et al. (2008d); (23) Jakobsson et al. (2008a); (24) Vreeswijk et al. (2008); (25) Thoene et al. (2008c); (26) Thoene et al. (2008a); (27) Malesani et al. (2008); Guidorzi et al. (2009); (28) Jakobsson et al. (2008c); (29) Greiner et al. (2009b); (30) Ledoux et al. (2007); Fox et al. (2008); (31) Prochaska et al. (2007a); (32) Prochaska et al. (2007b); Elíasdóttir et al. (2009); (33) Tanvir (2010); (34) Afonso et al. (2008); Krühler et al. (2011b); (35) Filgas et al. (2008).

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