An external-shock model for gamma-ray burst afterglow 130427A
A Panaitescu, WT Vestrand… - Monthly Notices of the …, 2013 - academic.oup.com
The complex multiwavelength emission of gamma-ray burst (GRB) afterglow 130427A
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
An external-shock model for gamma-ray burst afterglow 130427A
A Panaitescu, WT Vestrand… - Monthly Notices of the …, 2013 - ui.adsabs.harvard.edu
The complex multiwavelength emission of gamma-ray burst (GRB) afterglow 130427A
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
[引用][C] An external-shock model for gamma-ray burst afterglow 130427A
A Panaitescu, WT Vestrand, P Woźniak - Monthly Notices of the Royal …, 2013 - cir.nii.ac.jp
An external-shock model for gamma-ray burst afterglow 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 …
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 …
An external-shock model for gamma-ray burst afterglow 130427A
A Panaitescu, WT Vestrand… - Monthly Notices of the …, 2013 - ieeexplore.ieee.org
The complex multiwavelength emission of gamma-ray burst (GRB) afterglow 130427A
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
(monitored in the radio up to 10 d, in the optical and X-ray until 50 d, and at GeV energies …
An external-shock model for GRB afterglow 130427A
A Panaitescu, WT Vestrand, P Wozniak - arXiv preprint arXiv:1311.5867, 2013 - arxiv.org
The complex multiwavelength emission of GRB afterglow 130427A (monitored in the radio
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …
An external-shock model for GRB afterglow 130427A
A Panaitescu, WT Vestrand, P Wozniak - Mon. Not. Roy. Astron. Soc., 2013 - inspirehep.net
The complex multiwavelength emission of GRB afterglow 130427A (monitored in the radio
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …
[PDF][PDF] An external-shock model for GRB afterglow 130427A
A Panaitescu, WT Vestrand, P Wozniak - arXiv preprint arXiv:1311.5867, 2013 - Citeseer
The complex multiwavelength emission of GRB afterglow 130427A (monitored in the radio
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …
up to 10 days, in the optical and X-ray until 50 days, and at GeV energies until 1 day) can be …