Table 3
Afterglow spectral energy distributions of GRB 151027A.
| ν [Hz] | Fν [mJy] | β | tc [s] | Ref. |
|
|
||||
| 5.55 × 1014 | 7.98 ± 0.66 | – | 1109 | 1 |
| 6.93 × 1014 | 5.53 ± 0.25 | – | 1034 | 1 |
| 8.57 × 1014 | 5.28 ± 0.19 | – | 893.4 | 1 |
| 1.14 × 1015 | 2.48 ± 0.18 | – | 1072 | 1 |
| 1.34 × 1015 | 1.66 ± 0.14 | – | 1130 | 1 |
| 1.48 × 1015 | 1.66 ± 0.14 | – | 1086 | 1 |
| XRT | 4.9 × 10-10 |
|
993 | 2 |
|
|
||||
| 3.72 × 1014 | 1.08 ± 0.039 | – | 1.89 × 104 | 3 |
| 4.56 × 1014 | 1.89 ± 0.087 | – | 1.89 × 104 | 3 |
| 6.32 × 1014 | 0.851 ± 0.047 | – | 1.89 × 104 | 3 |
| XRT | 4.3 × 10-11 |
|
1.84 × 104 | 2 |
|
|
||||
| 2.19 × 1010 | 1.7 | – | 6.74 × 104 | 4 |
| 1.37 × 1014 | 0.600 ± 0.055 | – | 6.34 × 104 | 5 |
| 1.84 × 1014 | 0.658 ± 0.061 | – | 6.26 × 104 | 5 |
| 2.46 × 1014 | 0.450 ± 0.042 | – | 6.09 × 104 | 5 |
| 3.72 × 1014 | 0.297 ± 0.027 | – | 6.58 × 104 | 5 |
| 4.56 × 1014 | 0.311 ± 0.034 | – | 6.35 × 104 | 6 |
| 6.74 × 1014 | 0.258 ± 0.024 | – | 6.46 × 104 | 5 |
| XRT | 3.5 × 10-12 |
|
6.35 × 104 | 2 |
|
|
||||
| 5.0 × 109 | 0.29 ± 0.05 | – | 7.69 × 106 | 7 |
| 8.4 × 109 | 0.18 ± 0.03 | – | 7.69 × 106 | 7 |
| 1.5 × 1010 | 0.14 ± 0.03 | – | 7.69 × 106 | 7 |
Notes. For the XRT data the 0.3–10 keV flux in erg/cm2/s is shown in addition to the spectral slope β.
Reference. [1] this work: UVOT observations; [2] XRT automatic analysis (http://www.swift.ac.uk/xrt_products/00661775); [3] Yano et al. (2015); [4] Laskar et al. (2015); [5] Cano (2015); [6] Oksanen et al. (2015); [7] this work: VLBA observations.
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