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Table 6.
Spectral slope computed “before” and “after” the Tbreak.
| FXRT | ID | Γbefore(T < Tbreak) | Γafter(T ≥ Tbreak) |
|---|---|---|---|
| (1) | (2) | (3) | (4) |
| Nearby extragalactic FXRT Candidates from CSC2 | |||
| 2 | XRT 010908 | 1.8 ± 0.7 | 2.1 ± 0.7 |
| 3 | XRT 070530 | 6.2 ± 2.6 | 5.9 ± 1.6 |
| Distant extragalactic FXRT Candidates from CSC2 | |||
| 7 | XRT 030511 | 1.8 ± 0.3 | 2.4 ± 0.2 |
| 8 | XRT 041230 | 2.6 ± 1.2 | 3.6 ± 3.5 |
| 9 | XRT 080819 | 2.4 ± 1.2 | 5.9 ± 2.2 |
| 10 | XRT 100831 | 3.7 ± 1.0 | 2.7 ± 1.7 |
| 12 | XRT 110919 | 1.8 ± 0.9 | 2.8 ± 1.1 |
| 14 | XRT 141001 | 1.7 ± 0.8 | 1.7 ± 0.3 |
Notes. Columns 1 and 2: FXRT# and ID of the candidate, respectively. Columns 3 and 4: Spectrum photon index computed before and after the Tbreak for light curves that are well fit with a BPL. Errors are quoted at the 90% confidence level.
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