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public:bggrbinfo [2021/09/27 21:03] bruce [Emission Mechanism Theory] |
public:bggrbinfo [2023/09/12 12:04] (current) bruce [X-rays] |
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| ^GRB^Comment^ | ^GRB^Comment^ | ||
| |080319b| **Prototype? | |080319b| **Prototype? | ||
| - | |11025A|**Prototype? | + | |110205A|**Prototype? |
| |130427A|Largest E_ISO ever measured; 5.65e54 | |130427A|Largest E_ISO ever measured; 5.65e54 | ||
| |130603B| - short, Bright burst| | |130603B| - short, Bright burst| | ||
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| === Alternative Classifications to the Short vs. Long Classification Scheme: === | === Alternative Classifications to the Short vs. Long Classification Scheme: === | ||
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| + | At the GRB50 meeting there was a lot of talk of long GRBs apparently with Knovae, longs with no SNe, etc. So the distinction is not that clear. | ||
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| + | Here is a Girlanda paper asking if they are so different: https:// | ||
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| To understand the various spectral components and the theoretical slopes, please see the section on [[public: | To understand the various spectral components and the theoretical slopes, please see the section on [[public: | ||
| - | GRB 110205A: http:// | + | ==== GRB 110205A |
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| + | GRB 110205A was a 200 s duration GRB from z=2.2 that has really good data. | ||
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| + | http:// | ||
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| + | ==== GROND Prompt Measurement (but long delayed) ==== | ||
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| + | Eliot+13 | ||
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| + | Listen to this incredibly useful summary from abstract, "Only in a handful of cases has it been possible obtain simultaneous coverage of the prompt emission in a multi-wavelength regime (gamma-ray to optical), as a result of: observing the field by chance prior to the GRB (e.g. 080319B/ | ||
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| + | ==== Other Papers ==== | ||
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| + | This oddly short little paper gives a kind of list of " | ||
| - | Other Papers: | ||
| BIggest collected study of prompt is Kopac+13 http:// | BIggest collected study of prompt is Kopac+13 http:// | ||
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| This paper http:// | This paper http:// | ||
| + | Later, however, [[public: | ||