Beardmore, A. P.A. P.BeardmorePage, K. L.K. L.PageO'Brien, P. T.P. T.O'BrienCapalbi, MilviaMilviaCapalbi2020-09-172020-09-172007-02-01https://hdl.handle.net/20.500.13025/920Monthly Notices of the Royal Astronomical Society, Volume 374, Issue 4, pp. 1473-1478.We describe observations of GRB050422, a Swift-discovered gamma-ray burst. The prompt gamma-ray emission had a T<SUB>90</SUB> duration of 59 s and was multipeaked, with the main peak occurring at T + 53 s. Swift was able to follow the X-ray afterglow within 100 s of the burst trigger. The X-ray light curve, which shows a steep early decline, can be described by a broken power law with an initial decay slope of alpha<SUB>1</SUB> ~ 5.0, a break time t<SUB>b</SUB> ~ 270 s and a post-break decay slope of alpha<SUB>2</SUB> ~ 0.9, when the zero time of the X-ray emission is taken to be the burst trigger time. However, if the zero time is shifted to coincide with the onset of main peak in the gamma-ray light curve then the initial decay slope is shallower with alpha<SUB>1</SUB> ~ 3.2. The initial gamma-ray spectrum can be modelled by a power law with a spectral index of beta<SUB>B</SUB> = 0.50 +/- 0.19. However, the early time X-ray spectrum is significantly steeper than this and requires a spectral index of beta<SUB>X</SUB> = 2.33<SUP>+0.58</SUP><SUB>-0.55</SUB>. In comparison with other Swift bursts, GRB050422 was unusually X-ray faint, had a soft X-ray spectrum, and had an unusually steep early X-ray decline. Even so, its behaviour can be accommodated by standard models. The combined BAT/XRT light curve indicates that the initial, steeply declining, X-ray emission is related to the tail of the prompt gamma-ray emission. The shallower decay seen after the break is consistent with the standard afterglow model.gamma-rays bursts10.1111/j.1365-2966.2006.11249.xhttp://adsabs.harvard.edu/abs/2007MNRAS.374.1473B2007MNRAS.374.1473B