主要内容:
做法貌似是通过谱指数将辐射流量换算到同一个能断。
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文章信息:
- · arXiv e-print (arXiv:1008.0478)
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| Title: |
| Gamma-Ray Bursts: Connecting the Prompt Emission with the Afterglow |
| Authors: |
| Veres, P.; Bagoly, Z. |
| Affiliation: |
| AA(Department of Physics of Complex Systems, Eötvös University, H-1117 Budapest, Pázmany P. s. 1/A, Hungary; veresp@elte.hu; Department of Physics, Bolyai Military University, H-1581 Budapest, POB 15, Hungary), AB(Department of Physics of Complex Systems, Eötvös University, H-1117 Budapest, Pázmany P. s. 1/A, Hungary; zsolt.bagoly@elte.hu) |
| Publication: |
| Baltic Astronomy, Vol. 18, p. 284-288 |
| Publication Date: |
| 00/2009 |
| Origin: |
| BALTA |
| Keywords: |
| gamma rays: bursts |
| Bibliographic Code: |
| 2009BaltA..18..284V |
Abstract
With the early afterglow localizations of gamma-ray burst positions made by Swift, the clear delimitation of the prompt phase and the afterglow is not so obvious anymore. It is important to see weather the two phases have the same origin or they stem from different parts of the progenitor system. We will combine the two kinds of gamma-ray burst data from the Swift-XRT instrument (windowed timing and photon counting modes) and from BAT. A thorough desription of the applied procedure is given. We apply various binning techniques to the different data: Bayes blocks, exponential binning and signal-to-noise type of binning. We present a handful of flux curves and their possible applications.
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