ORIGIN OF THE FE K REPROCESSOR IN SEYFERT 1 GALAXY, IC 4329A
Various structures within AGNs emit Fe K lines. IC 4329A, a prominent Seyfert 1 galaxy in X-rays with minimal absorption in its spectrum, is ideal for studying Fe K emission origins. Line width analysis suggests a radius of about 60 light-days, possibly representing an outer broad line region. We propose using a 130 ks observation with XRISM to constrain the ionization degree of this Fe K reprocessor, enabling the calculation of its number density and a deeper understanding of its properties. Anticipated log ionization parameter falls between 1 and 2, with Fe Kalpha and Kbeta lines exhibiting energy shifts of several eV within this range. XRISM is uniquely equipped to detect this energy shift within a reasonable exposure time.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201044010' / Observation identification string OBJECT = 'IC4329A ' / Object name OBSERVER= 'MISAKI MIZUMOTO' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 207.3303 / [deg] Object Right ascension DEC_OBJ = -30.3095 / [deg] Object Declination RA_PNT = 207.333690614216 / Pointing RA DEC_PNT = -30.3080217360162 / Pointing DEC RA_NOM = 207.33117155779 / [deg] Nominal aspect point R.A. DEC_NOM = -30.3093909813728 / [deg] Nominal aspect point Dec. PA_NOM = 288.000104629399 / [deg] Nominal aspect point roll. TELAPSE = 234921.963135988 / Elapsed time DATE-OBS= '2025-08-07T23:22:05.036864' / Start date DATE-END= '2025-08-10T16:37:27' / Stop date ONTIME = 106650.28434 / On-source time EXPOSURE= 106650.28434 / Exposure time PROCVER = '03.03.015.012' / Processing script version MKFFF = 'ISAS/JAXA' / Origin of First FITS file ORIGIN = 'GSFC/NASA' / Origin of Processed FITS file SOFTVER = 'Hea_26Sep2025_V6.36_XRISM_12Sep2025_V003' / Version of HEADAS used CALDBVER= 'gen20241115_xtd20250915_rsl20250915' / Version of CALDB used DATE = '2025-10-08T16:13:24' / Date and time this file was created or updated SIB2_VER= 'V04.00 ' / SIB2 version JAXA