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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 6.

Intrinsic optical luminosity density as a function of redshift for 76 GRBs with a redshift and 14 GRBs without a redshift (dashed–dotted lines). Upper limits are plotted as downward triangles. The red dashed lines indicates the iso-magnitude of the optical afterglow as a function of the redshift (up to z = 6.0). They define our three classes of optical afterglow flux (bright are GRBs with ﹩R\,\leqslant ﹩ 17.9, intermediate are GRBs with ﹩17.9\lt R\leqslant 19.1﹩, and faint are GRBs with ﹩R\gt 19.1﹩). As discussed in Section 6, the green circles represent GRBs below the best-fit E﹩{}_{{\rm{pi}}}﹩–E﹩{}_{{\rm{iso}}}﹩ relation while black squares represent GRBs located above the best-fit E﹩{}_{{\rm{pi}}}﹩–E﹩{}_{{\rm{iso}}}﹩ relation. For GRBs without a redshift, the color of the dashed–dotted line indicates whether the GRB is located below the best-fit E﹩{}_{{\rm{pi}}}﹩–E﹩{}_{{\rm{iso}}}﹩ relation (green) or above it (black).

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