The Observer’s Guide to the Gamma-Ray Burst Supernova Connection
Table 1
Average Bolometric properties of GRB-SNe.
()
()
(d, rest)
(mag)
(km )
GRB
19
26.0
18.3
19
5.8
4.0
20
0.38
0.13
2
1.26
0.35
2
12.28
0.67
2
0.85
0.21
6
18400
9700
INT
1
8.2
—
1
3.1
—
1
0.37
—
1
1.08
—
1
12.94
—
1
0.85
—
1
21300
—
LL
6
27.8
19.6
6
6.5
4.0
6
0.35
0.19
5
0.94
0.41
5
13.22
3.53
5
0.75
0.12
4
22800
8200
ULGRB
2
18.8
18.7
2
6.1
2.9
1
0.41
—
1
2.91
—
1
14.80
—
1
0.78
—
1
21000
—
Rel IcBL
2
13.5
6.4
2
3.4
1.0
2
0.16
0.05
2
0.35
0.50
2
12.78
0.84
2
0.90
0.21
2
14000
1400
GRB ALL
28
25.2
17.9
28
5.9
3.8
28
0.37
0.20
9
1.24
0.71
9
13.16
2.61
9
0.79
0.12
12
20300
8100
GRB
27
25.9
17.9
27
5.9
3.9
28
0.37
0.20
8
1.03
0.36
8
12.95
2.72
8
0.79
0.13
11
20200
8500
Ib
19
3.3
2.6
19
4.7
2.8
12
0.21
0.22
—
—
—
—
—
—
—
—
—
11
8000
1700
Ic
13
3.3
3.3
13
4.6
4.5
7
0.23
0.19
—
—
—
—
—
—
—
—
—
10
8500
1800
(Section 3): GRBs: GRB-SNe associated with low-luminosity GRBs ( erg ); INT-GRBs: GRB-SNe associated with intermediate-luminosity GRBs ( erg ); GRBs: GRB-SNe associated with high-luminosity GRBs ( erg ); ULGRBs: GRB-SNe associated with ultra-long-duration GRBs (see Section 3). SN 2011kl. : erg. : erg . Note: average bolometric properties of SNe Ib and Ic are from [18].
