@booklet {23784,
	title = {Determining How X-ray Binary Populations Vary Through Time},
	year = {2019},
	month = {2019/08/1},
	pages = {15990},
	abstract = {We propose 200 ks total ACIS-S observations of the spiral galaxy NGC 2336, one of the most actively star-forming galaxies in the local Universe. The proposed observations will reach Lx 7 x 10^{37} erg/s, yielding over 40 high-mass X-ray binaries (XRBs). Archival UV data and supporting Hubble Space Telescope observations fully leverage our proposed Chandra observations by allowing us to: (a) measure the age and metallicity distribution of young XRBs; (b) measure the formation efficiency of young XRBs as a function of the age of their parent stellar populations; (c) constrain XRB formation models; (d) characterize the ultra-luminous XRB population; (e) explore the role of star formation in energizing the ISM; and (f) identify the nature of the nuclear source.},
	url = {https://ui.adsabs.harvard.edu/abs/2019hst..prop15990A},
	author = {Antoniou, Vallia and Anastasopoulou, K. and Andrews, Jeff and Drake, Jeremy J. and Fabbiano, Giuseppina and Hatzidimitriou, Despina and Hong, Jae Sub and Kouroumpatzakis, Konstantinos and Kovlakas, Konstantinos and Maccarone, Thomas J. and Maravelias, Grigoris and Sasaki, Manami and Sell, Paul H. and Swartz, Doug and Williams, Stephen and Zezas, Andreas}
}
