Fig. 7.

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Images of the sky around 2S 1845−024 in the K-filter obtained by the UKIRT telescope (GPS/UKIDSS sky survey, left) and in the 3.6μ-band obtained by the Spitzer telescope (right). The red circles indicate an uncertainty for the source position based on the Swift (dashed line) and Chandra (solid line) data, respectively. Cyan contours mark two IR objects closest to the X-ray position.
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