Fig. 1

INTEGRAL/ISGRI sky image of the field of view around IGR J17498–2921 in the 20–100 keV band for an effective exposure of 210 ks. The size of each pixel in the image corresponds to 3′. As the ~1°-radius RXTE/PCA field of view also includes 1A 1742-294 ( from IGR J17498 − 2921) and SLX 1744 − 300 (
), the data from that instrument also has contributions from those sources, as well as the diffuse emission from the Galactic center, in particular the non-imaging PCA instrument was unable to associate the detected bursts with the three burster sources.
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