- Conference date: 28–2 November 2007
- Location: St. Pete Beach (Florida)
We present an initial matching of the source positions of the Chandra Nuclear Bulge X‐ray sources to the new UKIDSS‐GPS near‐infrared survey of the Nuclear Bulge. This task is made difficult by the extremely crowded nature of the region; despite this, we find candidate counterparts to of the X‐ray sources. We show that detection in the J‐band for a candidate counterpart to an X‐ray source preferentially selects those candidate counterparts in the foreground whereas candidate counterparts with only detections in the H and K‐bands are more likely to be Nuclear Bulge sources. We discuss the planned follow‐up for these candidate counterparts.
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