NICER observation list: Target ID 358501

Abstract

The Magellanic Clouds (MCs) harbor a large sample of Be/X-ray binaries at a moderate and well known distance with low Galactic foreground absorption. However, their transient nature complicates observations in X-rays. We propose five triggered NICER observations of new or unexplored high-mass X-ray binaries (HMXBs) in the MCs. Our goal is to study their spectral and temporal properties, and build-up a large sample of pulsars in order to study their demographics in the MC system.
Obsid RA DEC l b Start End Exposure Number of
Modules		 Number of
Processing		 Status of
Processing		 Date of
Processing		 Public
date
3585010101 82.449 -65.946 275.875 -32.881 59012.6124 59012.9486 3518.0 52 3 VALIDATED 59016.7 59026
3585010102 82.449 -65.946 275.875 -32.881 59013.0000 59013.9822 6238.0 52 4 VALIDATED 59018.7 59027
3585010103 82.449 -65.946 275.874 -32.881 59014.0359 59014.1113 489.0 52 3 VALIDATED 59018.8 59028
3585010104 82.450 -65.946 275.874 -32.881 59020.1620 59020.8789 653.0 52 3 VALIDATED 59024.9 59034
3585010105 82.450 -65.945 275.874 -32.881 59022.4160 59022.6866 1129.0 52 3 VALIDATED 59026.9 59036
3585010106 82.450 -65.946 275.874 -32.881 59023.7092 59023.9778 1680.0 52 4 VALIDATED 59028.6 59037
3585010107 82.450 -65.945 275.874 -32.881 59024.0332 59024.5588 2979.0 52 3 VALIDATED 59028.7 59038
3585010108 82.450 -65.945 275.874 -32.881 59044.5910 59044.6046 525.0 52 3 VALIDATED 59050.9 59058
3585010109 82.451 -65.944 275.873 -32.880 59045.1084 59045.8954 10274.2 52 2 VALIDATED 59050.9 59059