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Table 2.

Results of the analysis of the host galaxies.

SN/GRB RAhost Dechost mR (mag) MR/(1+z) (mag) r50 (kpc) r90 (kpc) Offsetcentre (kpc) Offsetbp (kpc)
SN2005ks 21:37:56.54 −00:01:57.84 18.48 ± 0.17 −19.92 ± 0.17 2.26 ± 0.09 4.76 ± 0.19 1.88 1.74
SN2005nba 12:13:37.65 +16:07:10.29 14.66 ± 0.01 −20.58 ± 0.01 5.13 10.84 2.99 2.97
SDSS-IISN14475 22:24:30.87 +00:12:12.22 20.93 ± 0.12 −18.36 ± 0.12 1.97 ± 0.21 5.59 ± 0.71 3.54 3.33
SN2006nx 03:33:30.47 −00:40:37.81 19.96 ± 0.06 −19.11 ± 0.06 3.00 ± 0.14 5.07 ± 0.37 5.80 6.22
SN2007bg 11:49:26.24 +51:49:22.71 >22.4 >−13.6
SN2007ceb 12:10:18.02 +48:43:31.87 20.85 ± 0.24 −15.78 ± 0.24 0.34 ± 0.02 0.65 ± 0.23 0.65 0.63c
12:10:18.19 +48:43:34.69 19.33 ± 0.14 −17.30 ± 0.14 2.48 ± 0.24 5.10 ± 0.67 3.67
SN2007I 11:59:13.13 −01:36:15.88 17.40 ± 0.02 −17.59 ± 0.02 1.79 ± 0.03 4.08 ± 0.08 1.38 1.09
PTF10aavz 11:20:13.38 +03:44:42.63 19.24 ± 0.04 −18.13 ± 0.04 1.49 ± 0.07 3.51 ± 0.21 3.17 3.55
SN2010ah 11:44:02.98 +55:41:22.34 19.07 ± 0.18 −17.71 ± 0.18 2.21 ± 0.06 5.21 ± 0.16 5.32 5.34
SN2010ay 12:35:27.20 +27:04:02.76 19.05 ± 0.03 −18.40 ± 0.30 0.33 ± 0.01 1.07 ± 0.16 0.17 0.25
PTF10qts 16:41:37.53 +28:58:20.36 21.23 ± 0.21 −16.91 ± 0.21 1.28 ± 0.26 3.07 ± 0.81 2.07 1.51
PTF10vgv 22:16:01.59 +40:52:06.07 15.29 ± 0.04 −19.21 ± 0.04 1.81 ± 0.05 4.75 ± 0.19 1.75 1.64
PTF10xem 01:47:07.06 +13:56:29.48 18.60 ± 0.03 −18.57 ± 0.03 1.26 ± 0.06 3.75 ± 0.17 3.18 2.66
PTF11cmh 13:10:21.73 +37:52:57.33 19.89 ± 0.33 −18.55 ± 0.33 5.79 ± 0.56 12.25 ± 1.59 4.54 3.84
PTF11img >22.5 >−16.9
PTF11lbm 23:48:03.18 +26:44:30.05 17.95 ± 0.03 −18.42 ± 0.03 1.79 ± 0.06 4.18 ± 0.22 3.62 3.36
PTF12as 10:01:33.78 +00:26:56.04 16.47 ± 0.01 −19.44 ± 0.01 2.14 ± 0.01 3.95 ± 0.03 3.25 3.90
PTF13alq 11:48:02.12 +54:34:38.87 19.97 ± 0.10 −17.00 ± 0.10 0.26 ± 0.04 0.84 ± 0.04 0.86 0.74
PTF13ebw 08:17:15.32 +56:34:46.12 16.27 ± 0.06 −21.35 ± 0.06 3.66 ± 0.19 9.33 ± 0.74 8.83 9.08
PTF13u 15:58:51.42 +18:13:59.60 17.02 ± 0.02 −21.38 ± 0.02 4.83 ± 0.10 10.84 ± 0.21 13.56 14.0
LSQ14bef 14:27:42.24 −08:36:46.45 17.52 ± 0.02 −19.35 ± 0.01 3.34 ± 0.03 8.94 ± 0.80 7.14 6.69
PTF14dby 15:17:06.28 +25:21:11.90 22.14 ± 0.08 −15.61 ± 0.08 1.23 ± 0.23 1.91 ± 0.35 0.76 0.69
PTF14gaq 21:32:54.05 +17:44:33.50 19.33 ± 0.20 −18.80 ± 0.20 3.50 ± 0.25 7.66 ± 0.58 3.62 4.30
iPTF15dldb 00:58:13.27 −03:39:50.14 18.27 ± 0.12 −18.43 ± 0.12 1.76 ± 0.07 4.07 ± 0.24 0.20 0.12c
00:58:12.95 −03:39:46.15 16.67 ± 0.07 −20.03 ± 0.07 3.49 ± 0.14 7.57 ± 0.32 6.17
SN2016dst 04:55:54.68 −29:34:12.99 18.55 ± 0.04 −19.11 ± 0.04 3.07 ± 0.07 6.33 ± 0.17 1.08 1.94
SN2016coi 21:59:04.69 +18:10:36.67 12.95 ± 0.06 −18.30 ± 0.06 2.00 ± 0.16 4.41 ± 0.40 2.70 2.72
SN2017dcc 12:49:05.34 −12:12:25.91 15.90 ± 0.01 −19.40 ± 0.01 2.79 ± 0.02 5.27 ± 0.07 3.72 3.77
SN2017fgk 17:47:49.25 +16:08:05.79 17.33 ± 0.03 −18.81 ± 0.03 1.08 ± 0.03 2.80 ± 0.07 0.75 0.62

GRB 980425 19:35:04.00 −52:50:37.68 14.37 ± 0.05 −18.66 ± 0.05 2.25 ± 0.03 4.74 ± 0.03 2.25 0.87
GRB 030329 10:44:49.94 +21:31:17.35 23.09 ± 0.02 −16.42 ± 0.02 0.54 ± 0.03 1.37 ± 0.08 0.86 0.59
GRB 031203A 08:02:30.18 −39:51:03.68 20.65 ± 0.03 −20.19 ± 0.03 1.04 ± 0.04 2.79 ± 0.16 0.34 0.64
GRB 060218 03:21:39.69 16:52:01.88 20.30 ± 0.06 −15.88 ± 0.06 0.37 ± 0.01 0.85 ± 0.05 0.08 0.12
GRB 100316D 07:10:30.31 −56:15:20.21 17.80 ± 0.05 −19.61 ± 0.05 2.55 ± 0.02 5.42 ± 0.10 2.48 0.39
GRB 130702A 14:29:14.78 +15:46:26.25 23.34 ± 0.12 −15.88 ± 0.12 1.85 ± 0.16 3.77 ± 0.30 0.49 1.64
GRB 161219B 06:06:51.37 −26:47:30.62 20.67 ± 0.03 −18.56 ± 0.03 3.19 ± 0.16 7.17 ± 0.62 3.45 4.37
GRB 171205A 11:09:39.69 −12:35:11.31 15.33 ± 0.02 −20.90 ± 0.02 4.86 ± 0.03 9.25 ± 0.06 5.77 5.58

Notes. Columns are: barycentre position (RAhost,Dechost) of the host galaxy, apparent and absolute magnitude, radii r50 and r90 (radii containing 50 and 90% of the light from the galaxy) and the projected offset of an explosion from the centre of the galaxy (offsetcentre) and from the brightest pixel (offsetbp). Absolute magnitudes are corrected for Galactic foreground extinction (Schlafly & Finkbeiner 2011), while the apparent magnitudes are not. Systematic errors on measured offsets are discussed in Sect. 3.2.

(a)

The surface brightness of this host can not be modelled with a simple phenomenological model, therefore the results are from photometric analysis and the measured characteristic radii are without errors.

(b)

The first line corresponds to the measurement assuming the host galaxy is only the bright (blue) region near the SN explosion. The second line is obtained in the case the host galaxy is the whole complex.

(c)

The brightest pixel is located in the compact region of the complex.

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