A reverse shock in GRB 130427A
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67–12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67–12 days after the burst. We combine these data with …
A reverse shock in GRB 130427A
T Laskar, E Berger, BA Zauderer… - Astrophysical …, 2013 - scholars.northwestern.edu
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
[PDF][PDF] A Reverse Shock in GRB 130427A
T Laskar, E Berger, BA Zauderer, R Margutti… - arXiv preprint arXiv …, 2013 - Citeseer
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
[PDF][PDF] A Reverse Shock in GRB 130427A
T Laskar, E Berger, BA Zauderer… - arXiv preprint arXiv …, 2013 - researchgate.net
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
A Reverse Shock in GRB 130427A
T Laskar, E Berger, BA Zauderer… - The Astrophysical …, 2013 - ui.adsabs.harvard.edu
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
[引用][C] A REVERSE SHOCK IN GRB 130427A
T Laskar, E Berger, BA Zauderer, R Margutti… - The Astrophysical …, 2013 - cir.nii.ac.jp
A REVERSE SHOCK IN GRB 130427A | CiNii Research CiNii 国立情報学研究所 学術情報
ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学図書館の本を …
ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学図書館の本を …
A Reverse Shock in GRB 130427A
T Laskar, E Berger, BA Zauderer… - The Astrophysical …, 2013 - dash.harvard.edu
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
130427A at z= 0.340, spanning 0.67 to 12 d after the burst. Taken in conjunction with …
A REVERSE SHOCK IN GRB 130427A
T Laskar, E Berger, BA Zauderer… - The Astrophysical …, 2013 - repository.ias.ac.in
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67–12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67–12 days after the burst. We combine these data with …
A REVERSE SHOCK IN GRB 130427A
T Laskar, E Berger, BA Zauderer, R Margutti… - Astrophysical …, 2013 - inis.iaea.org
[en] We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
A Reverse Shock in GRB 130427A
T Laskar, E Berger, BA Zauderer, R Margutti… - Astrophys. J., 2013 - inspirehep.net
We present extensive radio and millimeter observations of the unusually bright GRB
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …
130427A at z= 0.340, spanning 0.67-12 days after the burst. We combine these data with …