Table C.3
Parameters of the optical/X-ray SEDs fitted with a broken power-law.
GRB | Host | Part | β op | σ(βop) | β X | σ(βX) | ν br | σ(νbr) | NH | σ(NH) |
|
||||||||||
050319 | MW | P | 0.358 | 0.000 | 0.858 | 0.077 | 1.271 | 1.198 | –0.030 | 0.283 |
050319 | MW | N | 0.607 | 0.000 | 1.107 | 0.045 | 0.545 | 0.118 | 0.114 | 0.437 |
050401 | SMC | P | 0.372 | 0.000 | 0.872 | 0.146 | 0.455 | 87.600 | 1.850 | 2.540 |
050408 | LMC | N | 0.342 | 0.000 | 1.210 | 0.310 | 22.350 | 26.190 | 1.560 | 0.690 |
050416A | SMC | P | 0.619 | 0.000 | 0.951 | 0.156 | 339.900 | 131.310 | 0.398 | 0.097 |
|
||||||||||
E(B − V) | σ(E(B − V)) | N | σ(N) | χ 2 | d.o.f. | p_val | T i | T f | ok | |
0.103 | 0.022 | 0.327 | 0.048 | 4.050e+01 | 40 | 4.467e-01 | 300.000 | 1500.000 | 1 | |
0.165 | 0.034 | 0.021 | 0.005 | 4.050e+01 | 9 | 3.770e-05 | 17 000.000 | 300 000.000 | 1 | |
0.462 | 10.500 | 2.700 | 263.000 | 2.050e+02 | 145 | 7.460e-04 | 200.000 | 2000.000 | 0 | |
0.290 | 0.000 | 0.020 | 0.001 | 2.654e+01 | 27 | 4.885e-01 | 20 000.000 | 40 000.000 | 1 | |
0.321 | 0.044 | 0.060 | 0.005 | 1.890e+01 | 23 | 7.059e-01 | 700.000 | 2000.000 | 1 |
Notes.GRB: GRB name. Host: galaxy chosen as model to fit the SED; Milky Way (MW), Large Magellanic Cloud (LMC), Small Magellanic Cloud (SMC). Part: X-ray LC part considered; “S” steep decay, “P” plateau, “N” normal decay. βop, σ(βop): optical spectral index with error. βX, σ(βX): X-ray spectral index with error. ν, σ(ν): observer frame break frequency (1015 Hz). NH, σ(NH): hydrogen column density with relative error (1022 cm-2). E(B − V), σ(E(B − V)): optical absorption with relative error (mag). N, σ(N): normalization with error (mJy). χ2: chi-square. d.o.f.: degree of freedom. p_val: p_value. Ti, Tf: initial (end) time of the interval of the SED in observer time (s). Ok: “1” if the best fitting function is a broken power-law, otherwise “0”. This table is available in its entirety in a machine-readable form at the CDS (table3c.dat, ReadMe). A portion is shown here for guidance.
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