@conference {23944,
	title = {XMM-Newton survey of the Local Group galaxy M33 bright individual sources},
	volume = {230},
	year = {2006},
	month = {2006/01/1},
	pages = {162 - 163},
	abstract = {As shown in our first poster, in a recent survey of M33 with XMM-Newton we detected the X-ray source population of this nearby spiral galaxy down to the (0.2-4.5) keV luminosity of 10<SUP>35</SUP> erg s<SUP>-1</SUP>, a factor of 10 deeper than in previous observations. The majority of the detected sources was classified using, in many cases, only their X-ray properties. In particular, 8 new X-ray binary (XRB) candidates were selected, based on their long-term X-ray light curves. We also classified supernova remnants (SNRs), super-soft sources (SSS), AGN, foreground stars and a population of {\textquoteleft}hard{\textquoteright} sources using the hardness ratio (HR) method. A detailed spectral and timing analysis of the brightest sources is in progress. We present a few examples of spectra for particular source classes. We find that bright {\textquoteleft}hard{\textquoteright} sources can be divided into two broad families: one best modelled by a powerlaw with photon index in the range of 1.0-2.0, and the other displaying disk blackbody spectra with kT of 0.8 to 1.5 keV.},
	isbn = {1743-9221},
	url = {https://ui.adsabs.harvard.edu/abs/2006IAUS..230..162M},
	author = {Misanovic, Z. and Pietsch, W. and Haberl, F. and Trinchieri, G. and Ehle, M. and Hatzidimitriou, D.}
}
