NICER observation list: Target ID 657202

Abstract

Famous for their purely thermal emission, X-ray dim isolated neutron stars (XDINS), while still few in numbers, could be as common as radio pulsars and may play an important evolutionary role among the known Galactic isolated neutron star (INS) population. The wide area and depth of the eROSITA All-Sky Survey (eRASS) enables to detect XDINS beyond the solar vicinity. For two candidates, selected from the eRASS, optical follow-up with the Large Binocular Telescope and the South African Large Telescope make a non-INS nature very unlikely. We thus propose follow-up observations with NICER, to probe the candidates' temporal and spectral properties, with the goal to investigate how well the candidates conform to the XDINS population or other classes of INS.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
6572020101 199.321 -40.446 308.238 22.159 60032.5888 60032.9389 10104.0 51 3 VALIDATED 60042.4 60226
6572020102 199.321 -40.446 308.238 22.159 60032.9725 60033.9713 28147.0 51 8 VALIDATED 60048.0 60227
6572020103 199.321 -40.446 308.237 22.159 60034.0046 60034.9861 26468.0 51 7 VALIDATED 60048.0 60228
6572020104 199.321 -40.446 308.238 22.159 60035.0410 60035.4377 3737.0 51 5 VALIDATED 60048.1 60229