DETECTING CHARGE EXCHANGE X-RAY EMISSION FROM THE N63A SUPERNOVA REMNANT
We propose to observe the middle-aged supernova remnant, N63A, in the Large Magellanic Cloud with an exposure time of 300 ks. Our goals of this observation are (1) to detect signatures of charge-exchange (CX) X-ray emission, and (2) to reveal the origin of the Fe K line emission from this remnant. This observation will provide us with the second solid evidence for CX X-ray emission from SNRs after the first detection in N132D with XRISM (private communication). The line broadening of Fe K lines will clarify if the Fe emission arises from Fe-rich ejecta or swept-up interstellar medium. This study cannot be done without XRISM/Resolve having unprecedented spectral resolution above 2 keV.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201005010' / Observation identification string OBJECT = 'N63A ' / Object name OBSERVER= 'SATORU KATSUDA' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 83.9337 / [deg] Object Right ascension DEC_OBJ = -66.0366 / [deg] Object Declination RA_PNT = 83.9384872882092 / Pointing RA DEC_PNT = -66.0370149036739 / Pointing DEC RA_NOM = 83.9325344886602 / [deg] Nominal aspect point R.A. DEC_NOM = -66.0361437813766 / [deg] Nominal aspect point Dec. PA_NOM = 340.011391584201 / [deg] Nominal aspect point roll. TELAPSE = 728219 / Elapsed time DATE-OBS= '2025-05-23T17:12:34' / Start date DATE-END= '2025-06-01T03:29:33' / Stop date ONTIME = 363004.62043 / On-source time EXPOSURE= 363004.62043 / 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 = '2025-07-15T11:08:38' / Date and time this file was created or updated SIB2_VER= 'V03.01 ' / SIB2 version JAXA