Fig. 1
INTEGRAL/ISGRI sky image of the field of view around IGR J17511–3057 (20–70 keV). The size of each pixel in the image corresponds to 3′. Evidently the non-imaging instruments on-board RXTE with a field of view of ~1° (radius) are not be able to separate the emission from the two AMXPs XTE J1751-305 and IGR J17511–3057 when they are both active in X-rays (see Fig. 2).
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