Fig. 1.
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XMM–Newton EPIC pn (right) and Swift/XRT (left) image of the IGR J16426+6536 sky region with the ISGRI error circle superimposed (90% confidence). Two X-ray sources (n.1 and n.2) are detected inside of it in the XMM–Newton image. Conversely, only X-ray source n.1 is detected in the Swift/XRT image, where the small dashed circle marks the position of the undetected X-ray source n.2.
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