A trio of gamma-ray burst supernovae:

Cano, Z.; de Ugarte Postigo, A.; Pozanenko, A.; Butler, N.; C. Thöne, C.; Guidorzi, C.; Krühler, T.; Gorosabel, J.; Jakobsson, P.; Leloudas, G.; Malesani, D.; Hjorth, J.; Melandri, A.; G. Mundell, C.; Wiersema, K.; D’Avanzo, P.; Schulze, S.; Gomboc, A.; Johansson, T.; Zheng, W.; А. Канн, Д.; Knust, F.; Varela, K.; Akerlof, C.; S. Bloom, J.; Бурхонов, О.; A. Cooke, Elizabeth; A. de Diego, J.; Dhungana, G.; Fariña, C.; V. Ferrante, F.; Flewelling, H.; D. Fox, Ori; P. U. Fynbo, J.; Gehrels, N.; Георгиев, Л.; González‐Hernández, J.; Greiner, J.; Güver, Tolga; E. Hartoog, O.; A. Hatch, N.; Jelínek, M.; Kehoe, R.; Klose, S.; Klunko, E.; Kopač, D.; Kutyrev, A.; N. Krugly, Yu.; H. Lee, W.; J. Levan, A.

doi:10.1051/0004-6361/201423920

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A trio of gamma-ray burst supernovae:

Shared by NobleBlocks on Jun 5, 2014 • 12:00 AM UTC

Authors:

Z. Cano

A. de Ugarte Postigo

A. Pozanenko

Abstract

We present optical and near-infrared (NIR) photometry for three gamma-ray burst supernovae (GRB-SNe): GRB 120729A, GRB 130215A/SN 2013ez, and GRB 130831A/SN 2013fu. For GRB 130215A/SN 2013ez, we also present optical spectroscopy at tt 0 = 16.1 d, which covers rest-frame 3000-6250 . Based on Fe 5169 ...

Subject

Gamma-ray burst

Physics

Afterglow

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