XRISM resolve observation 300018010

Object

M81

Abstract

Up to 40% of all galaxies may harbor low-ionization nuclear emission region (LINERs) and low-luminosity AGN (LLAGN). Well-developed theory suggests that the inner flow should be advective and radiatively inefficient

Summary of xrismmastr

      obsid   = 300018010 / Unique Observation/Sequence Number
      object  = M81 / Object name
      pi_name = Collaboration XRISM / Proposal Principal Investigator Name
      ra  = 148.89023034779 / Right Ascension (Pointing Position) (deg)
      dec = 69.0648665379458 / Declination (Pointing Position) (deg)
      roll_angle = 286.836712693117 / Roll Angle (deg)
      start_time = 2024-05-08T08:43:04 / Start Time of the Observation
      stop_time  = 2024-05-12T00:05:04 / Stop Time of the Observation
      exposure   = 268779.3924019 / Effective Total Observation Exposure (s)
      public_date= 2099-12-31 / Public Date

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