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Table 4.
Comparison of the characteristics of light curve rebrightenings seen for other GRB afterglows.
| GRB | αrise | Δmag | trise (day) |
|---|---|---|---|
| 100418A | 5.4 ± 1.1 | 3.4 ± 0.5 | 0.062 ± 0.005 |
| 970508 | 3.93 ± 0.12 | 1.41 ± 0.12 | 1.08 ± 0.03 |
| 020903 | 2.97 ± 0.10 | 1.02 ± 0.10 | 1.10 ± 0.02 |
| 060206 | 5.43 ± 0.20 | 1.27 ± 0.12 | 0.0125 ± 0.0010 |
| 060906 | 2.02 ± 0.28 | 1.28 ± 0.40 | 0.029 ± 0.002 |
| 081029 | 4.33 ± 0.21 | 1.19 ± 0.14 | 0.0165 ± 0.0010 |
| 100621A | 15.8 ± 1.32 | 1.96 ± 0.16 | 0.058 ± 0.002 |
| 100901A | 4.09 ± 0.55 | 1.45 ± 0.25 | 0.110 ± 0.005 |
| 111209A | 3.74 ± 0.18 | 0.90 ± 0.05 | 1.007 ± 0.010 |
| 130831A | 2.83 ± 0.11 | 1.41 ± 0.14 | 0.0082 ± 0.0003 |
Notes. The values have been calculated after shifting all the light curves to z = 1.
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