NICER observation list: Target ID 459201

Abstract

A recently-discovered intermediate polar, CTCV J2056-3014, has the shortest spin period (29.6 sec) among all CVs and white dwarfs. The orbital period of 1.76 hours is below the period gap where the binary orbit decays via gravitational wave radiation. Fast-spinning CVs are extremely rare and unique as manifested by AR Sco (the so-called white dwarf pulsar) and AE Aqr which spins down via the propeller effect. The proposed NICER and NuSTAR observations, motivated by the recent XMM-Newton detection, will fully explore the X-ray properties of this remarkable CV, such as spin-down rate, soft time lag, white dwarf mass measurement and search for non-thermal X-ray pulsation.
Obsid RA DEC l b Start End Exposure Number of modules Status of Processing Date of Processing Public date
4592010101 314.219 -30.246 14.67829 -39.03479 59302.9650 59302.9782 102.00000 49 VALIDATED 59317.8 59496
4592010102 314.217 -30.244 14.67966 -39.03254 59303.0296 59303.8940 286.00000 49 VALIDATED 59317.9 59497
4592010103 314.216 -30.243 14.68064 -39.03211 59304.0162 59304.6687 22.00000 49 VALIDATED 59315.8 59498
4592010104 314.217 -30.244 14.67953 -39.03256 59305.5593 59305.9457 947.00000 49 VALIDATED 59315.9 59499
4592010105 314.217 -30.244 14.67984 -39.03242 59305.9993 59306.9914 4522.00000 52 VALIDATED 59317.9 59500
4592010106 314.217 -30.244 14.67988 -39.03233 59307.0433 59307.9597 1072.00000 52 VALIDATED 59318.0 59501
4592010107 314.217 -30.244 14.67970 -39.03244 59308.0137 59308.3309 76.00000 52 VALIDATED 59318.1 59502