Table 5
Radio continuum properties of GRB hosts.
| GRB | F1.38 | F1.86 | F2.35 | F2.80 | Frest1.4a | αb | SFRradioc | AVd |
| (μJy) | (μJy) | (μJy) | (μJy) | (μJy) | (M⊙yr-1) | (mag) | ||
|
|
||||||||
| 980425 | 840 ± 160 | 1110 ± 210 | 710 ± 190 | 400 ± 200 | 912 ± 263 | −0.58 ± 0.41 | 0.11 ± 0.03 | ~0 |
| 031203 | 383 ± 20 | 324 ± 11 | 319 ± 12 | 324 ± 13 | 363 ± 26 | −0.19 ± 0.09 | 2.83 ± 0.20 | 0.08 |
| 060505 | 76 ± 35 | 67 ± 18 | 45 ± 18 | 47 ± 15 | 85 ± 50 | −0.81 ± 0.72 | 0.69 ± 0.40 | ~0 |
| 100316D | 657 ± 21 | 531 ± 13 | 441 ± 13 | 403 ± 13 | 681 ± 33 | −0.71 ± 0.06 | 1.73 ± 0.08 | 0.86 |
| 111005A | 245 ± 30 | 192 ± 18 | 160 ± 16 | 124 ± 16 | 252 ± 46 | −0.92 ± 0.22 | 0.08 ± 0.02 | ~0 |
Notes. Flux densities are given at the observed frequencies indicated in GHz in the column header.
Using the conversion of Bell (2003).
Visual dust attenuation calculated from the ultraviolet attenuation AUV = 2.5log (SFRradio/SFRUV) assuming an SMC extinction curve, which gives AV = AUV/ 2.2 (Gordon et al. 2003). AV ~ 0 mag is reported if a formal value of SFRUV exceeds the SFRradio.
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