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Figure 4: A SPI 100-200 keV image of GRS 1915+105. GRS 1915+105 is clearly visible at the center of the image (marked). The three other sources seen in Fig. 2 are much fainter in this energy range and not visible. |
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Figure 5: The JEM X-2 lightcurves. Top: the whole 100 ks observation showing strong variability. Middle: a zoom covering 1.2 hours. The bin size is 8 s. Bottom: RXTE/PCA color-color diagram. The time bin is 1 s. The scale allows for a direct comparison with Figs. 2a and 2b in Belloni et al. (2000). |
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Figure 6: The JEM X-2 power spectrum. |