{
  "bibcode": "2006GCN..4544....1P",
  "body": "A. Pelangeon & J-L. Atteia (LATT-OMP) report:\n\nWe have used the spectral parameters of GRB 060117\nprovided by Golenetskii et al. (GCNC 4542) to\ncompute the spectral pseudo-redshift of this burst\ndetected by SWIFT-BAT (Campana et al., GCNC 4533;\nCummings et al., GCNC 4538).\n\nWe find a pseudo-redshift pz= 0.45 +/- 0.2\n\nThis is significantly lower than the pseudo-redshift computed from\nthe lag-luminosity relation (pz=1.3, GCNC 4538, Cummings et al.).\nThis small pseudo-redshift suggests that the supernova associated\nwith GRB 060117 could be detectable.\n\nWe encourage observers to follow-up this GRB at various wavelengths\nto look for the possible emergence of the supernova.",
  "circularId": 4544,
  "createdOn": 1137606303000,
  "email": "atteia@ast.obs-mip.fr",
  "subject": "GRB 060117: pseudo-z from spectral parameters of the prompt emission",
  "submitter": "Jean-Luc Atteia at Lab d Astrophys.,OMP,Toulouse  <atteia@ast.obs-mip.fr>",
  "eventId": "GRB 060117"
}