@booklet {41837,
	title = {Following the spectral and spin evolution of the longest-lived post-nova SSS},
	year = {2020},
	month = {2020/10/1},
	pages = {129},
	abstract = {1RXS J050526.3-684628 is a super soft source in the Large Magellanic Cloud(LMC). A recent study reported the discovery of coherent pulsations,and identified the system as an accreting White Dwarf (WD). Moreover, thestudy of historic X-ray and optical properties of J050526 have revealedit to be a remarkably long-lived post-nova SSS (~30 year duration),reaching its peak flux around 2013. Nevertheless, the lack of multipledeep X-ray observations hampers the study of the system and prohibitsfurther testing of theoretical models. We request a 60 ks XMM-Newtonobservation to study the evolution of its spectral and temporal propertiesduring the decay of its flux.},
	url = {https://ui.adsabs.harvard.edu/abs/2020xmm..prop..129V},
	author = {Vasilopoulos, Georgios}
}
