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INVESTIGATING THE IMPACT OF OPTICAL SELECTION EFFECTS ON OBSERVED REST-FRAME PROMPT GRB PROPERTIES

  • Authors: D. Turpin, V. Heussaff, J.-P. Dezalay, J-L. Atteia, A. Klotz, and D. Dornic

2016 The Astrophysical Journal 831 28.

  • Provider: AAS Journals

Caption: Figure 8.

Top left: cumulative distribution function (bottom) and histograms (top) of the isotropic γ-ray energy (Eiso) for the three classes of afterglow optical flux and based on a population of 76 GRBs with a redshift. Top right: same caption for the isotropic γ-ray luminosity (Liso) based on a population of 73 GRBs with a redshift. Bottom left: same caption for the intrinsic peak energy (Epi) based on a population of 76 GRBs with a redshift. Bottom right: same caption for the rest-frame burst duration (﹩{T}_{90}^{\mathrm{rest}}﹩) based on a population of 76 GRBs with a redshift. All panels: the faint GRBs are represented with a blue dotted line, the intermediate GRBs with a black dashed line, and the bright GRBs with a red solid line.

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