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Xtend spectrum
p0300: All four CCDs in full window mode
Xtend light curve
Light curve
p0300: All four CCDs in full window mode
Light curve
INVESTIGATING THE COMPLEX IRON EMISSION IN NGC7314
We propose to observe the bright Sy1.9 NGC 7314 as the ideal candidate to unveil the structure and physical conditions through emission lines from cold and ionized material. We will investigate the iron K alpha and K beta narrow and broad emission components and disentangle the contribution to the line of the distant reflector, disk and broad line region. This source is also ideal to study the prominent emission from ionized gas and determine its origin and geometry.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201124010' / Observation identification string OBJECT = 'NGC7314 ' / Object name OBSERVER= 'ELISA COSTANTINI' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 338.9425 / [deg] Object Right ascension DEC_OBJ = -26.0504 / [deg] Object Declination RA_PNT = 338.940943561934 / Pointing RA DEC_PNT = -26.0525806116504 / Pointing DEC RA_NOM = 338.942099196663 / [deg] Nominal aspect point R.A. DEC_NOM = -26.0502297693447 / [deg] Nominal aspect point Dec. PA_NOM = 74.0222785508898 / [deg] Nominal aspect point roll. TELAPSE = 160826 / Elapsed time DATE-OBS= '2025-06-13T20:57:25' / Start date DATE-END= '2025-06-15T17:37:51' / Stop date ONTIME = 87109.802734 / On-source time EXPOSURE= 87109.802734 / 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 = '2025-07-14T13:10:33' / Date and time this file was created or updated SIB2_VER= 'V03.01 ' / SIB2 version JAXA