NICER observation list: Target ID 361501

Abstract

We propose to observe a nova in outburst and a flaring nova-like system in the Large Magellanic Cloud, both nuclear burning white dwarfs and very luminous supersoft X-ray sources. Our main aim is to measure pulsations with time scales of a minute, detected in other supersoft sources. The nova-like RX J0513.9-6951 has been observed before, but the timing analysis was not conclusive for short periods. For it and for the next luminous nova, we need good data with high S/N. Together with the results of three previous NICER targets, and with our accompanying proposal on the nuclear burning symbiotic SMC 3, these data will allow connecting the intriguing short time pulsations with binary physical parameters, giving insight on the root cause of the quasi-periodic variability.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
3615010101 59.623 -54.778 265.397 -46.395 59120.6416 59120.9796 7121.0 51 4 VALIDATED 59125.7 59134
3615010102 59.623 -54.778 265.397 -46.395 59121.0289 59121.8833 13961.0 51 3 VALIDATED 59125.7 59135