{
  "bibcode": "2020GCN.28668....1M",
  "body": "P. Minaev (IKI) and A. Pozanenko (IKI)  report on behalf of larger GRB \nfollow-up collaboration:\n\nWe analyzed GRB 201015A detected by Swift (D'Elia et al., GCN 28632) \nusing GBM/Fermi spectral data  (Fletcher et al., GCN 28663) and redshift \nof z = 0.426 (de Ugarte Postigo et al., GCN 28649; Izzo et al., GCN \n28661). GRB 201015A has a low luminosity, Eiso = (1.1 +/- 0.2)*10^50 \nerg, and well consistent with the Ep,i ��� Eiso correlation (Amati \nrelation) for type II (long) bursts, see [1] for details and Figure at\n\nhttp://grb.rssi.ru/GRB201015A/GRB201015A_Epi_Eiso.png\n\nThe position of the burst is within 1-sigma confidence area of the \ncluster of type II (long) bursts on the EH ��� T90,i diagram (see [2] for \ndetails), indicating strong association with type II bursts, see Figure at\n\nhttp://grb.rssi.ru/GRB201015A/GRB201015A_EH_T90i.png\n\nWe encourage follow-up optical observations to search for associated \nsupernova.\n\n[1] - Minaev et al., MNRAS, 492, 1919, 2020\n[2] - Minaev et al., arXiv:2008.12752",
  "circularId": 28668,
  "createdOn": 1602939323000,
  "email": "apozanen@iki.rssi.ru",
  "subject": "GRB 201015A: classification as long GRB",
  "submitter": "Alexei Pozanenko at IKI, Moscow  <apozanen@iki.rssi.ru>",
  "eventId": "GRB 201015A"
}