Table 2
Results of the joint optical to gamma-ray spectral fit (~1 eV to ~150 keV).
| # | Optical | XRT-BAT-GBM | E break | ||
| interval | time | interval | time | (keV) | |
|
|
|||||
| 1 | 199.0–219.0 | 208.7 | 202.8–206.9 | 204.8 | 4.30(45) |
| 2 | 219.0–238.0 | 228.7 | 227.5–234.5 | 231.0 | 0.78(39) |
| 3 | 239.0–258.0 | 248.7 | 241.5–249.5 | 245.5 | 0.28(18) |
| 4 | 259.0–278.7 | 268.7 | 259.0–278.7 | 268.7 | – |
| 5 | 285.0–385.0 | 331.3 | 318.5–372.5 | 344.4 | – |
| 6 | 272.7–556.7 | 389.6 | 272.7–477.9 | 361.0 | – |
| 7 | 385.0–478.7 | 429.3 | 385.0–477.9 | 428.9 | – |
Notes. Columns 2 and 3: seven time intervals (in units of seconds) defined by the first seven optical data points (“epochs”; Fig. 4) and their logarithmic mean. Columns 4 and 5: the corresponding time spans when high-energy photons were collected and their logarithmic mean. Column 6: the break energy, including its 1σ error. For further details see Sect. 3.1.2.
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