NICER observation list: Target ID 356101

Abstract

RX J0648.0-4418 is a peculiar binary consisting of an X-ray pulsar, and a hot subdwarf of O spectral type in a circular orbit. With a dinamically measured mass of 1.28 +/-0.05 M_sun, the nature of the X-ray source is still under debate. It may represent one of the heaviest White Dwarfs known, and also the fastest spinning one. Otherwise, it could represent a very light Neutron Star, with puzzling X-ray properties. Fast spin-up from this object has also been measured recently, interpreted in terms of a young, contracting WD. Here we propose for a NICER investigation of this target to characterize its timing and spectral behaviour.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
3561010101 102.019 -44.317 253.707 -19.141 59185.7294 59185.9380 4681.0 51 3 VALIDATED 59189.7 59379
3561010102 102.019 -44.316 253.706 -19.141 59185.9877 59186.9708 16386.0 51 4 VALIDATED 59191.6 59380
3561010103 102.020 -44.316 253.707 -19.141 59187.0194 59187.9519 15205.0 51 3 VALIDATED 59191.6 59381
3561010104 102.020 -44.316 253.707 -19.141 59187.9928 59188.9076 15176.0 51 3 VALIDATED 59192.8 59382
3561010105 102.019 -44.316 253.707 -19.141 59259.6755 59259.8852 4312.0 52 1 VALIDATED 59268.9 59453
3561010106 102.020 -44.316 253.707 -19.141 59259.9979 59260.9780 17914.0 52 1 VALIDATED 59268.9 59454
3561010107 102.020 -44.316 253.707 -19.141 59261.0167 59261.9979 15435.6 52 2 VALIDATED 59270.9 59455