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Table 5.

Fit results for the GRB 140629A afterglow SEDs.

Model (a) R-chi. EB − V NH Photon
/d.o.f. (mag) (1021 cm−2) index
775 s

MW×POW 0.94/27
LMC×POW 1.02/27
SMC×POW 1.05/27
MW×BKP 0.94/26
LMC×BKP 0.99/26
SMC×BKP 1.02/26

9350 s

MW×POW 1.92/50
LMC×POW 1.44/50
SMC×POW 1.25/50
MW×BKP 1.95/49
LMC×BKP 1.47/49
SMC×BKP 1.28/49

Notes.

(a)

MW is Milky Way extinction model. LMC is Large Magellanic Cloud extinction model; SMC is Small Magellanic Cloud extinction model; POW is power law model; and BKP is broken power law model.

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