Characterizing New X-ray Sources in the Swift Galactic Plane Survey

The Swift Galactic Plane Survey is a simultaneous Xray UV survey, tiling theGalactic plane from 60 leq l leq 60 to 1 leq b leq 1 through a series ofshallow 500s exposures, that will obtain complete coverage in the 0.3 10 keVband in addition to simultaneous imaging at UV wavelengths (virgul 2200AA). Here, wepropose to observe a sample of 10 newly discovered Xray sources. None of theproposed fields have previously been observed by either Chandra or XMMNewton.The order of magnitude improvement in sensitivity provided by the proposedobservations will allow us to characterize these new sources based on theirobserved Xray spectral properties. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]