XRISM xtend observation 300007010

Object

MRK766

Abstract

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.

Summary of xrismmastr

      obsid   = 300007010 / Unique Observation/Sequence Number
      object  = MRK766 / Object name
      pi_name = Collaboration XRISM / Proposal Principal Investigator Name
      ra  = 184.610684304485 / Right Ascension (Pointing Position) (deg)
      dec = 29.8131086989368 / Declination (Pointing Position) (deg)
      roll_angle = 290.324706294189 / Roll Angle (deg)
      start_time = 2024-06-24T13:19:04 / Start Time of the Observation
      stop_time  = 2024-06-27T00:04:04 / Stop Time of the Observation
      exposure   = 111753.1249996 / Effective Total Observation Exposure (s)
      public_date= 2025-08-31 / Public Date

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