The shallow-decay phase in both optical and x-ray afterglows of Swift GRB 090529A: Energy injection into a wind-type medium?
L.P. Xin, A. Pozanenko, D. A. Kann, D. Xu, J. Gorosabel, G. Leloudas,, J. Y. Wei, M. Andreev, S. F. Qin, M. Ibrahimov, X. H. Han, A. de Ugarte, Postigo, Y. L. Qiu, J. S. Deng, A. Volnova, P. Jakobsson, A. J., Castro-Tirado, F. Aceituno, J. P. U. Fynbo, J. Wang

TL;DR
This study presents optical and X-ray observations of GRB 090529A, analyzing the shallow-decay phase and suggesting energy injection into a wind-type medium, with implications for understanding GRB afterglow physics.
Contribution
It provides simultaneous optical and X-ray data of GRB 090529A, exploring the nature of the shallow-decay phase and testing energy injection models in different media.
Findings
Optical and X-ray afterglows show achromatic decay with a break at ~10^5 sec.
The post-break decay is consistent with a forward shock in an ISM medium without energy injection.
The shallow-decay phase may be due to energy injection in a wind-like medium, but other models are also possible.
Abstract
The energy injection model is usually proposed to interpret the shallow-decay phase in Swift GRB X-ray afterglows. However, very few GRBs have simultaneous signatures of energy injection in their optical and X-ray afterglows. Here, we report optical observations of GRB 090529A from 2000 sec to sec after the burst, in which an achromatic decay is seen at both wavelengths. The optical light curve shows a decay from 0.37 to 0.99 with a break at sec. In the same time interval, the decay indices of the X-ray light curve changed from 0.04 to 1.2. Comparing these values with the closure relations, the segment after 3 sec is consistent with the prediction of the forward shock in an ISM medium without any energy injection. The shallow-decay phase between 2000 to 3 sec could be due to the external shock in a wind-type-like medium with an energy…
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