XRISM XTEND observation 201064010

Title

TOWARD IDENTIFYING 4U~1700-377 AS NEUTRON STAR OR BLACK HOLE

Abstract

We aim to study 4U 1700-377, a high-mass X-ray binary system, to better understand how matter behaves around its bright companion star and address the ``mass-gap'' mystery. Depending on its true nature, 4U 1700-377 could either be the heaviest neutron star without detected pulsations or the smallest black hole ever found. Using XRISM's detailed spectral analysis, we plan to measure the central energies and the profiles of the neutral and ionized iron lines with unprecedented accuracy.

FITS header

TELESCOP= 'XRISM   '           / Mission name
INSTRUME= 'XTEND   '           / Instrument name
OBS_ID  = '201064010'          / Observation identification string
OBJECT  = '4U1700-37'          / Object name
OBSERVER= 'SHINYA YAMADA'      / PI name
OBS_MODE= 'POINTING'           / POINTING or SLEW or ALL
RA_OBJ  =             255.9865 / [deg] Object Right ascension
DEC_OBJ =             -37.8441 / [deg] Object Declination
RA_PNT  =     255.985114581194 / Pointing RA
DEC_PNT =    -37.8456662412695 / Pointing DEC
RA_NOM  =     255.987135717979 / [deg] Nominal aspect point R.A.
DEC_NOM =    -37.8436520403796 / [deg] Nominal aspect point Dec.
PA_NOM  =     88.5869835772094 / [deg] Nominal aspect point roll.
TELAPSE =        117359.963101 / Elapsed time
DATE-OBS= '2025-02-10T12:55:52.036829' / Start date
DATE-END= '2025-02-11T21:31:51.999930' / Stop date
ONTIME  =         49984.416256 / On-source time
EXPOSURE=         49984.416256 / Exposure time
PROCVER = '03.00.013.010'      / Processing script version
MKFFF   = 'ISAS/JAXA'          / Origin of First FITS file
ORIGIN  = 'GSFC/NASA'          / Origin of Processed FITS file
SOFTVER = 'Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001' / Version of HEADAS used
CALDBVER= 'gen20241115_xtd20241115_rsl20241115' / Version of CALDB used
DATE    = '2025-02-18T06:06:18' / Date and time this file was created or updated
SIB2_VER= 'V03.01  '           / SIB2 version JAXA

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