THE ORIGIN OF THE FE KA LINE IN THE BRIGHT SEYFERT 2 NGC 4507
NCG 4507 is one of the X-ray brightest, but highly obscured, Seyfert 2 galaxies. It has been observed several times in the X-ray band, and it has always shown a strong iron K emission line. NCG 4507 is one of the few Compton thin AGN with a clear detection of the Ni Ka emission line. Iron K absorption lines have also been detected, suggesting the presence of an ionized absorber, possibly outflowing. The proposed 100 ksec XRISM observation will allow us to resolve with unprecedented precision the origin of the Fe K emission and absorption lines. Thanks to the high spectral resolution offered by Resolve any contribution from a BLR-Fe Ka will be fully revealed.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '201067010' / Observation identification string OBJECT = 'NGC4507 ' / Object name OBSERVER= 'VALENTINA BRAITO' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 188.9026 / [deg] Object Right ascension DEC_OBJ = -39.9094 / [deg] Object Declination RA_PNT = 188.90655891107 / Pointing RA DEC_PNT = -39.9080515078193 / Pointing DEC RA_NOM = 188.90388954146 / [deg] Nominal aspect point R.A. DEC_NOM = -39.9096044945271 / [deg] Nominal aspect point Dec. PA_NOM = 283.016839855731 / [deg] Nominal aspect point roll. TELAPSE = 231471 / Elapsed time DATE-OBS= '2025-06-20T09:45:59' / Start date DATE-END= '2025-06-23T02:03:50' / Stop date ONTIME = 109498.77911 / On-source time EXPOSURE= 109498.77911 / 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 = '2025-07-14T21:32:18' / Date and time this file was created or updated SIB2_VER= 'V04.00 ' / SIB2 version JAXA