Swift and CBA Observations of TT Ari on 2009 October 16
Swift XRT spectrum of TT Ari, as observed on 2009 October 16 for 4.4 ksec. The best-fit, 2-temperature mekal model is shown in red along with the data. Also shown are the best-fit 2-temperature mekal model for the ASCA high-state observation, folded through the Swift XRT response (in blue).
Swift XRT (top) and CBA (bottom) light curves of TT Ari.
For details, see ATel #2254.