Evolution of GRS 1915+105 before and after H.E.S.S. observations. RXTE PCA intensity and hardness (defined in the caption of Fig. A.1) are plotted on the top and middle panels, respectively. The bottom panel presents contemporaneous 15 GHz radio data obtained using the Ryle Telescope (Pooley 2006). Long-term monitoring data in the 15 GHz radio band are illustrated in the inset. Coloured markers and lines indicate the H.E.S.S.observation epochs.
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