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Table 3.

Photometry of ESO580-49, the host galaxy of GRB 111005A.

λobs (μm) Flux (mJy) Filter Reference
0.1516 0.25 ± 0.06 GALEXFUV This paper
0.2267 0.530 ± 0.037 GALEXNUV This paper
0.3442 1.35 ± 0.06 U This paper
0.4390 3.30 ± 0.29 B Lauberts & Valentijn (1989)
0.4770 3.272 ± 0.006 B This paper
0.6231 8.742 ± 0.008 R This paper
0.6390 6.9 ± 0.6 R Lauberts & Valentijn (1989)
0.7625 10.404 ± 0.019 I This paper
0.7900 9.52 ± 0.35 I Springob et al. (2007)
1.25 15.3 ± 0.7 J Skrutskie et al. (2006)
1.64 17.3 ± 1.0 H Skrutskie et al. (2006)
2.17 14.9 ± 1.3 K Skrutskie et al. (2006)
3.6 9.078 ± 0.017 IRAC1 This paper
4.5 6.076 ± 0.017 IRAC2 This paper
60 347 ± 43 IRAS60 Moshir (1990)
90 561 ± 77 AKARI90 Murakami et al. (2007)
100 957 ± 252 IRAS100 Moshir (1990)
140 2016 ± 264 AKARI140 Murakami et al. (2007)
106310 0.124 ± 0.016 2.8 GHz Michałowski (2015)
126490 0.160 ± 0.016 2.35 GHz Michałowski (2015)
160320 0.192 ± 0.018 1.87 GHz Michałowski (2015)
215680 0.245 ± 0.030 1.39 GHz Michałowski (2015)
12 <140 IRAS12 Moshir (1990)
25 < 146 IRAS25 Moshir (1990)
65 <252 AKARI65 Murakami et al. (2007)
160 <1427 AKARI160 Murakami et al. (2007)
870 <40 LAB0CA870 This paper
8817 <1.8 34 GHz This paper
16655 <1.5 18 GHz This paper

Notes. Upper limits are 2σ. The archival data were compiled from the NASA/IPAC Extragalactic Database with the appropriate reference shown in the last column. Radio limits are from our deepest afterglow photometry excluding the data in configurations with overly high resolution, which resolves out the host extended emission.

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