For GRBs detected by Swift-BAT, the coordinates are obtained from https://swift.gsfc.nasa.gov/archive/grb_table/. For those detected by Fermi-GBM, the coordinates are taken from von Kienlin et al. (2020). For GRBs detected by HETE-2, the coordinates are retrieved from the GCN Circulars.

For sources detected by HETE-2, T₉₀ values are taken from H.E.S.S. Collaboration (2009).

R, O, and HE represent radio, optical, and high-energy (100 MeV to 100 GeV) gamma-ray observations. A ✓ indicates a counterpart detection, × indicates no detection, and ⋅ means no information is available via GCN.

This burst is referred to with the suffix “B”, contrary to the name given by the GCN Circulars, to distinguish it from GRB 041211A, which occurred earlier on the same day (Pélangeon, private communication).

GRBs detected by Fermi/GBM are not included in Table A.4. GRBs with an

after the name indicate that the GRB does not appear with a GCN-style name in the literature, adopting the auto-generated name of GCNweb: https://user-web.icecube.wisc.edu/~grbweb_public/index.html.

Stanek et al. (2005)

de Pasquale et al. (2007)

GCN: Ofek et al. (2006)

Thöne et al. (2010)

GCN: Fynbo et al. (2007)

GCN: Berger & Fox (2007)

Xiao & Schaefer (2011)

GCN: Cucchiara et al. (2007)

Perley et al. (2008)

GCN: Thoene et al. (2008)

Krühler et al. (2015)

Krühler et al. (2011)

GCN: Xu et al. (2013)

GCN: de Ugarte Postigo et al. (2014)

Selsing et al. (2019)

GCN: de Ugarte Postigo et al. (2017)

GCN: Malesani et al. (2017)

GCN: Japelj et al. (2019)

GCN: D’Elia et al. (2019)