We performed photometry on the list provided by `wavedetect` using the the `ACIS Extract` (AE) package [@Broos:2010aa]. AE permits an optimal determination of the local background and the best flux extraction apertures based on the PSF of the image. Photometry is then extracted on selected energy bands and a list of source properties, statistics and best fit spectral models is produced. We used three energy bands: Soft, from 0.2 to 2.0 keV, Medium, from 2.0 to 4.0 keV and Hard, from 4.0 to 7.0 keV. From the final list of sources produced by `ACIS Extract` we rejected those with a probability of 1$\%$ or higher of being a background fluctuation $P_B>0.01$). Our final lists contains a total of 131 X-ray sources. From these, a total of 109 (83.2%) sources have a counterpart in our IR catalog. In Figure \[fig:chandra\] we show a false color (RGB) map of the ACIS field for DR15 using images from the three energy bands, overlaid with contours of visual extinction from the NICEST extinction map ww constructed from near-IR data. In there, we see how sources with hard X-ray emission are preferently located in regions of high column density. This is because soft X-ray bands 