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From the 1 of 577 papers with an AI index.

output
20082024
most citedEntanglement detection

2.4k citations

Showing 2014 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE201411 cited

Another short-burst host galaxy with an optically obscured high star formation rate: The case of GRB 071227

A. Nicuesa Guelbenzu, S. Klose, M. J. Michalowski +9

We report on radio continuum observations of the host galaxy of the short gamma-ray burst 071227 (z=0.381) with the Australia Telescope Compact Array (ATCA). We detect the galaxy i…

astro-ph.HE201441 cited

A Trio of GRB-SNe: GRB 120729A, GRB 130215A / SN 2013ez and GRB 130831A / SN 2013fu

Z. Cano, A. de Ugarte Postigo, A. Pozanenko +62

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. In the case…

astro-ph.HE201413 cited

Broad band polarimetric follow-up of Type IIP SN 2012aw

Brajesh Kumar, S. B. Pandey, C. Eswaraiah +1

We present the results based on R-band polarimetric follow-up observations of the nearby (~10 Mpc) Type II-plateau SN 2012aw. Starting from ~10 days after the SN explosion, these p…

astro-ph.HE201447 cited

The host of the SN-less GRB 060505 in high resolution

C. C. Thöne, L. Christensen, J. X. Prochaska +5

The spiral host galaxy of GRB 060505 at z=0.089 was the site of a puzzling long duration burst without an accompanying supernova. Studies of the burst environment by Thöne et al. (…

astro-ph.HE201412 cited

The dark nature of GRB 130528A and its host galaxy

S. Jeong, A. J. Castro-Tirado, M. Bremer +18

We study the dark nature of GRB 130528A through multi-wavelength observations and conclude that the main reason for the optical darkness is local extinction inside of the host gala…

astro-ph.HE201481 cited

GRB 130925A: an ultra-long Gamma Ray Burst with a dust-echo afterglow, and implications for the origin of the ultra-long GRBs

P. A. Evans, R. Willingale, J. P. Osborne +24

GRB 130925A was an unusual GRB, consisting of 3 distinct episodes of high-energy emission spanning 20 ks, making it a member of the proposed category of `ultra-long' bursts.…