X-ray Sources in the Dwarf Spheroidal Galaxy Draco
  We present the spectral analysis of an 87~ks \emph{XMM-Newton} observation of
Draco, a nearby dwarf spheroidal galaxy. Of the approximately 35 robust X-ray
source detections, we focus our attention on the brightest of these sources,
for which we report X-ray and multiwavelength parameters. While most of the
sources exhibit properties consistent with AGN, few of them possess
characteristics of LMXBs and CVs. Our analysis puts constraints on population
of X-ray sources with $L_X>3\times10^{33}$~erg~s$^{-1}$ in Draco suggesting
that there are no actively accreting BH and NS binaries. However, we find 4
sources that could be LMXBs/CVs in quiescent state associated with Draco. We
also place constraints on the central black hole luminosity and on a dark
matter decay signal around 3.5~keV.
