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Table A.1

Photometry used in SED fitting.

GRBH A V a Wavelength Fluxb Uncertainty Reference
(galactic) (μm) (μJy) (μJy)
(1) (2) (3) (4) (5) (6)
970828 0.12 0.640 0.28 0.08 1
2.160 1.7 0.5 1
4.501 <3.9 − This paper
7.905 10. 4. This paper
23.680 44. 2. This paper
100. <7000. − This paper
160. <15 400. − This paper
250. <18 900. − This paper
350. <21 900. − This paper
500. <29 100. − This paper
865.5 <7080. − 2
34 860. <27. − 2
980613 0.28 0.434 0.4 0.1 3
0.545 0.8 0.1 3
0.640 0.94 0.05 4
0.760 1.15 0.1 4
2.214 1.4 0.3 4
4.501 43. 3. This paper
7.905 55. 10. This paper
23.680 259. 11. This paper
100. 3500. 800. This paper
160. <20 300. − This paper
447.5 <52 800. − 2
856.5 <2760. − 2
980703 0.18 0.445 2.1 0.3 5
0.557 2.6 0.2 5
0.639 3.3 0.2 5
0.801 4. 1. 5
1.254 7.7 1. 5
1.651 8.2 2. 5
2.161 9.6 1. 5
4.501 6. 2. This paper
7.905 <26. − This paper
23.680 70. 3. This paper
250. <20 100. − This paper
350. <20 400. − This paper
447.5 <32 100. − 2
500. <27 300. − This paper
856.5 <4300. − 6
1344.2 <7551. − 7
34 700. 39. 4. 7
62 500. 42. 8. 7
209 154. 69. 5. 7
990705 0.24 0.545 2.8 0.5 8
0.640 4.9 0.5 9
4.501 16. 2. This paper
7.905 <16. − This paper
23.680 <58. − This paper
100. <5800. − This paper
160. <20 300. − This paper
250. <19 200. − This paper
350. <15 600. − This paper
500. <24 000. − This paper
143 000. <26. − 10
020127 0.15 0.480 <0.178 − 11
0.626 <1.48 − 11
0.659 0.44 0.06 11
0.771 1.2 0.1 11
0.790 0.94 0.09 11
1.252 11 1 11
1.253 10 2 This paper
1.631 20 4 This paper
2.146 18 6 This paper
2.162 26 3 11
3.543 50 1 This paper
5.711 46 7 This paper
23.680 160 32 This paper
100. <5000 − This paper
160. <17 700 − This paper
250. <17 700 − This paper
350. <21 000 − This paper
500. <18 300 − This paper
020819B 0.20 0.436 7. 4. 12
0.459 27.2 0.5 13
0.622 61.6 3.6 13
0.660 51. 1. 12
0.764 83.3 5.2 13
0.899 117. 2.2 13
1.240 150. 5.8 13
1.647 185. 7.7 13
2.170 150. 15. 13
3.543 101. 1. This paper
4.501 94. 2. This paper
5.711 75. 10. This paper
7.905 177. 15. This paper
23.680 389. 22. This paper
100. 19 000. 2000. This paper
160. 27 500. 3500. This paper
250. 24 000. 12 000. This paper
350. <16 800. − This paper
500. <24 300. − This paper
30 000. <138. − 14
60 000. <33. − 14
030115 0.06 0.435 0.15 0.02 15
0.606 0.22 0.01 15
0.814 0.43 0.02 15
1.100 0.9 0.1 15
1.600 3.2 0.2 15
2.200 4.9 0.7 15
3.543 6.8 0.7 This paper
4.501 12.0 1.0 This paper
100. <3900. − This paper
160. <18 600. − This paper
450. <33 000. − 16
850. <2400. − 16
1200. <1800. − 16
050219A 0.51 0.152 <23. − 17
0.193 <7.2 − 18
0.225 <18.9 − 18
0.227 <21. − 17
0.260 <7.4 − 18
0.347 <8.6 − 18
0.430 <16.9 − 18
0.459 16.9 0.6 18
0.543 28. 3. 18
0.622 46. 2.0 18
0.764 65. 2.0 18
0.899 79. 3.0 18
1.240 145. 5.0 18
1.647 179. 17.0 18
2.170 156. 19. 18
3.543 85. 2. This paper
5.711 58. 8. This paper
23.680 19. 5. This paper
100. <5400. − This paper
160. <15 600. − This paper
250. <16 500. − This paper
350. <21 000. − This paper
500. <24 600. − This paper
050223 0.28 0.459 5.9 0.5 This paper
0.622 9.5 0.6 This paper
0.660 7.5 0.3 19
0.764 14.5 1. This paper
0.899 9.2 0.9 This paper
1.256 11.0 2. This paper
1.647 12.0 5. This paper
2.159 19.3 0.4 19
3.543 14.1 0.6 This paper
5.711 11. 3. This paper
23.680 16. 4. This paper
100. <4900. − This paper
160. <21 400. − This paper
250. <22 200. − This paper
350. <15 900. − This paper
500. <25 500. − This paper
051022 0.18 0.365 1.7 0.3 20
0.460 3.7 0.1 20
0.540 4.9 0.2 21
0.629 6.3 0.5 21
0.650 6.14 0.05 21
0.770 7.66 0.07 21
0.876 10.5 0.5 21
0.890 11.6 0.4 21
1.220 17.7 0.8 21
1.630 18. 2. 21
2.159 31. 3. 21
2.210 29. 1. 21
3.543 25. 1. This paper
4.501 19. 1. This paper
100. 6500. 1000. This paper
160. <21 400. − This paper
250. <17 700. − This paper
350. <15 600. − This paper
500. <19 500. − This paper
57 321.7 13.3 3.6 22
160 000. <17. − 10
060904Ac 0.06 0.547 <0.15 − 24
0.760 <0.59 − 24
1.250 <6.6 − 25
2.160 <5.9 − 25
3.543 1.5 0.1 This paper
4.501 2.0 0.2 This paper
5.711 2.1 0.8 This paper
7.905 <3.5 − This paper
100. <5000. − This paper
160. <12 200. − This paper
070306 0.08 0.352 2.2 0.9 26
0.459 2.8 0.2 27
0.622 2.3 0.2 27
0.655 2.2 0.2 23
0.764 2.9 0.3 27
0.790 3.4 0.6 26
0.899 2.7 0.5 27
1.240 7. 3. 27
1.647 10. 3. 27
2.160 5.7 0.6 23
3.543 8.7 0.9 This paper
4.501 15. 2. This paper
100. 4900. 700. This paper
160. 10 700. 2000. This paper
071021 0.21 0.550 0.24 0.07 This paper
0.660 0.17 0.03 This paper
0.760 0.71 0.14 28
0.890 0.49 0.16 28
0.898 0.6 0.3 This paper
1.230 2.5 1. This paper
2.160 5. 1. This paper
3.543 12.9 0.7 This paper
4.501 16. 1. This paper
100. <6000. − This paper
160. <19 700. − This paper
250. <19 800. − This paper
350. <16 200. − This paper
500. <21 900. − This paper
2860. <510. − 29
3485. <450. − 29
57 321.7 <32.1 − 22
080207 0.07 0.473 0.04 0.01 30
0.660 0.10 0.4 31
0.790 0.17 0.05 30
0.925 0.35 0.05 31
1.250 1.6 0.3 31
1.607 2.3 0.4 31
2.160 7. 1. 31
3.543 14.4 0.4 31
4.501 15.5 0.4 31
5.711 18.5 1.5 31
7.905 12.5 2. 31
23.680 92. 7. 31
100. 2200. 600. This paper
160. 5900. 1400. This paper
250. <19 500. − This paper
350. <20 400. − This paper
449. <53 220. − 30
500. <21 900. − This paper
825. <13 120. − 30
57 321.7 17.1 2.5 22
080325 0.20 0.450 0.19 0.02 32
0.660 0.23 0.03 32
0.780 0.41 0.06 32
0.918 0.59 0.04 32
1.199 2.3 0.4 32
2.198 7.7 0.4 32
3.543 15.3 0.8 This paper
4.501 13.9 0.8 This paper
100. 1400. 400. This paper
160. 5000. 800. This paper
250. <18 000. − This paper
350. <16 800. − This paper
500. <26 700. − This paper
57 321.7 <15.4 – 22
090404 0.07 0.437 0.02 0.01 28
0.473 0.14 0.03 28
0.760 0.19 0.04 28
1.050 0.29 0.07 28
1.246 0.59 0.13 28
1.541 0.95 0.19 28
2.200 2.44 0.36 28
3.543 4. 1. This paper
4.501 5. 1. This paper
100. <5000. − This paper
160. <18 200. − This paper
250. <21 600. − This paper
350. <22 800. − This paper
500. <26 100. − This paper
57 321.7 10.9 2.7 22
090417B 0.05 0.193 0.7 0.1 33
0.225 0.9 0.2 33
0.260 0.6 0.4 33
0.347 0.9 0.4 33
0.431 2.1 0.3 33
0.477 2.5 0.3 34
0.623 8. 1. 34
0.660 9.2 0.3 33
0.763 10. 1. 34
0.913 19. 4. 34
1.250 <16. − 35
2.160 <27. − 35
3.543 16. 1. This paper
4.501 13. 1. This paper
100. 1200. 600. This paper
160. 3900. 1600. This paper
250. <16 800. − This paper
350. <19 800. − This paper
500. <23 400. − This paper
3477. <510. − 28
57 321.7 <21.4 − 22

Notes.

(a)

Taken from Schlegel et al. (1998).

(b)

Fluxes corrected for Galactic extinction as given by Col. (2). Flux upper limits are 3σ.

(c)

The position of the host of GRB 060904A was originally associated with a source which had significantly more IRAC 3.6 μm flux than the current photometry. Recently, however, the coordinates were revised making this source fainter than our original sample requirements. We have retained it in our analysis in any case.

Reference. (1) Djorgovski et al. (2001); (2) Berger et al. (2003); (3) Sokolov et al. (2001); (4) Djorgovski et al. (2003); (5) Christensen et al. (2004); (6) Tanvir et al. (2004); (7) Michałowski et al. (2008); (8) Holland et al. (2000); (9) Bloom et al. (2002); (10) Hatsukade et al. (2012); (11) Berger et al. (2007); (12) Jakobsson et al. (2005); (13) Küpcü Yoldaş et al. (2010); (14) Stanway et al. (2010); (15) Levan et al. (2006); (16) Priddey et al. (2006); (17) http://galex.stsci.edu/GR6/; (18) Rossi et al. (2014); (19) Pellizza et al. (2006); (20) Castro-Tirado et al. (2007); (21) Rol et al. (2007); (22) Perley & Perley (2013); (23) Hjorth et al. (2012); (24) http://www.astro.caltech.edu/grbhosts/; (25) Aoki et al. (2006); (26) Jaunsen et al. (2008); (27) Krühler et al. (2011); (28) Perley et al. (2013); (29) de Ugarte Postigo et al. (2012); (30) Svensson et al. (2012); (31) Hunt et al. (2011); (32) Hashimoto et al. (2010); (33) Holland et al. (2010); (34) http://www.sdss3.org/dr9/; (35) Aoki et al. (2009).

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