ABSORPTION AND EMISSION UNDER EXTREME CONDITIONS: THE CASE OF MRK766
We propose to observe the highly accreting AGN Mrk 766 in order to characterize its emission spectrum and its peculiar, variable, absorption features. In this source also an ultra-fast outflow was reported. Only XRISM is able to characterize the behaviour of spectral features in a highly accreting object as a function of time.
TELESCOP= 'XRISM ' / Mission name INSTRUME= 'XTEND ' / Instrument name OBS_ID = '300007010' / Observation identification string OBJECT = 'MRK766 ' / Object name OBSERVER= 'XRISM Collaboration' / PI name OBS_MODE= 'POINTING' / POINTING or SLEW or ALL RA_OBJ = 184.61046 / [deg] Object Right ascension DEC_OBJ = 29.81292 / [deg] Object Declination RA_PNT = 184.627508128986 / Pointing RA DEC_PNT = 29.8139592227419 / Pointing DEC RA_NOM = 184.610684304485 / [deg] Nominal aspect point R.A. DEC_NOM = 29.8131086989368 / [deg] Nominal aspect point Dec. PA_NOM = 290.324706294189 / [deg] Nominal aspect point roll. TELAPSE = 208735 / Elapsed time DATE-OBS= '2024-06-24T13:27:47' / Start date DATE-END= '2024-06-26T23:26:42' / Stop date ONTIME = 91167.385761 / On-source time EXPOSURE= 91167.385761 / Exposure time PROCVER = '03.00.013.009' / 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= 'gen20240315_xtd20240815_rsl20240815' / Version of CALDB used DATE = '2024-09-20T16:35:57' / Date and time this file was created or updated SIB2_VER= / SIB2 version JAXA