A search for Fermi bursts associated with supernovae and their frequency of occurrence

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Volume 569 (September 2014)

A&A, 569 (2014) A108

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Table 3

Main parameters of the Fermi GRB sample presented in this work and of the supernovae associated with these bursts.

GRB	RA	Dec	Error	T ₉₀	Fluence	Peak flux	SN	Date	RA	Dec	z
	GBM	GBM	radius		(0.01–1) MeV	(0.01–1) MeV		discovery	SN	SN
	(deg)	(deg)	(deg)	(s)	(erg cm^-2)	(photon cm^-2)			(deg)	(deg)

090320B	183.4	49.8	9.5	29.2	1.67 × 10^-6	4.35 ± 0.25	2009di	2009 03 21	174.2411	45.0141	0.13
090426B	17.6	–19.2	18.1	16.1	6.77 × 10^-7	2.03 ± 0.18	2009em	2009 05 05	8.6855	–8.3993	0.006
110911A	258.58	–66.98	50.0^*	8.96	5.94 × 10^-7	2.38 ± 0.41	2011gw	2011 09 15	112.0709	–62.3552	0.01
120121B	235.67	–39.34	7.9	18.4	1.95 × 10^-6	2.66 ± 0.21	2012ba	2012 01 21	230.6047	–38.2012	0.017

130702A	228.15	16.58	13.02	59	6.3 × 10^-6	7.03 ± 0.86	2013dx	2013 07 08	217.3116	15.7740	0.145

Notes. We also report the already known GRB-SN connection that we have found with our code in the last row of the table.

^(*)

Nominal maximum value for the error radius of bursts detected by a single GBM detector.

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