ESTIMATING THE MASS OF THE WHITE DWARF IN THE INTERMEDIATE POLAR V2400 OPH USING XRISM OBSERVATIONS
Masses of white dwarfs (WDs) play an important role in understanding their formation and evolution. A unique way to estimate the mass of a WD in an Intermediate Polar (IP) is to estimate the gravitational redshift of emission lines. We propose 200 kilosec XRISM observations to carry out accurate estimation of the gravitational redshift of emission lines in an IP V2400 Oph and use these measurements to accurately estimate the mass of the WD. The proposed XRISM observation would also serve as a benchmark for carrying out similar investigations for several other moderately bright IPs in future cycles and to estimate the mass of the WDs.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201111010' / Observation identification string OBJECT = 'V2400_OPH' / Object name OBSERVER= 'NAZMA ISLAM' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 258.1518 / [deg] Object Right ascension DEC_OBJ = -24.2458 / [deg] Object Declination RA_PNT = 258.153308133636 / Pointing RA DEC_PNT = -24.2440470850213 / Pointing DEC RA_NOM = 258.151352707561 / [deg] Nominal aspect point R.A. DEC_NOM = -24.2458978799446 / [deg] Nominal aspect point Dec. PA_NOM = 274.125256704238 / [deg] Nominal aspect point roll. TELAPSE = 397345.963135988 / Elapsed time DATE-OBS= '2025-08-15T14:31:26.036864' / Start date DATE-END= '2025-08-20T04:53:52' / Stop date ONTIME = 224235.3079 / On-source time EXPOSURE= 224235.3079 / Exposure time PROCVER = '03.02.014.010' / Processing script version MKFFF = 'ISAS/JAXA' / Origin of First FITS file ORIGIN = 'GSFC/NASA' / Origin of Processed FITS file SOFTVER = 'Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002' / Version of HEADAS used CALDBVER= 'gen20241115_xtd20241115_rsl20241115' / Version of CALDB used DATE = '2025-08-30T03:09:20' / Date and time this file was created or updated SIB2_VER= 'V04.00 ' / SIB2 version JAXA