NICER observation list: Target ID 252302

Abstract

With the excellent timing ability, high collecting area in soft X-ray band, and relatively low background below 1 keV, NICER is an ideal telescope for supersoft X-ray sources. We therefore propose 3x50 ksec NICER observations for three supersoft X-ray systems. These observations can be useful in searching for the spin period of the white dwarfs, studying the atmospheric emission, and understanding the supersoft X-ray orbital modulation.
Obsid RA DEC l b Start End Exposure Number of modules Status of Processing Date of Processing Public date
2523020101 9.331 -72.236 304.44948 -44.85105 58707.0794 58707.8662 4160.00000 52 VALIDATED 58711.8 58721
2523020102 9.331 -72.236 304.44970 -44.85100 58708.0470 58708.9618 8475.00000 52 VALIDATED 58715.6 58722
2523020103 9.333 -72.237 304.44876 -44.84968 58709.0139 58709.9928 9148.00000 52 VALIDATED 58715.6 58723
2523020104 9.331 -72.236 304.44960 -44.85059 58710.0387 58710.6903 5223.21407 52 VALIDATED 58715.7 58724
2523020105 9.334 -72.237 304.44800 -44.84947 58757.5317 58757.7380 3963.00000 52 VALIDATED 58764.0 58771
2523020106 9.334 -72.237 304.44841 -44.84969 58758.4936 58758.7697 5861.00000 52 VALIDATED 58764.7 58772