Table 2.
Best-fit parameters of the Ep, i − L correlation (90% confidence) for the overall sample 𝒮 and for the sub-samples 𝒮(ISM) and 𝒮(W) of time-resolved spectra of GRBs with available information on 
and on 
, respectively.
| Set | Nint | NGRB | mt | qt | σint, t | |
|---|---|---|---|---|---|---|
| Ep, i–Liso | 𝒮 | 793 | 20 |
 |
 |
 |
| Ep, i–Liso | 𝒮(ISM) | 421 | 11 |
 |
 |
 |
| Ep, i–Liso | 𝒮(W) | 390 | 10 |
 |
 |
 |
 |
 |
 |
||||
| Ep, i–Liso | 𝒮 | 793 | 20 | 0.53 ± 0.17 | −25 ± 9 | 0.19 ± 0.09 |
| mcoll | qcoll | σcoll | ||||
Ep, i– |
𝒮(ISM) | 421 | 11 |
 |
 |
 |
Ep, i– |
𝒮(W) | 390 | 10 |
 |
 |
 |
Notes. We note that Nint and NGRB are the total number of intervals and the number of GRBs, respectively, while 
, 
, and 
are the mean values and standard deviations of the distributions of the best-fit parameters of individual GRBs reported in Table 1. The luminosity is either isotropic-equivalent (iso) or collimation-corrected (coll).
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