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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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