XRISM xtend observation 300074010

Object

COMA_OFFSET

Abstract

We propose the first direct measurement of the power spectrum of turbulence in the intracluster medium. The spectrum determines the flow of kinetic energy down the turbulent cascade and the amount that dissipates into heat and feeds cosmic ray acceleration and magnetic field amplification. The nearby Coma cluster is the best system for such a measurement

Summary of xrismmastr

      obsid   = 300074010 / Unique Observation/Sequence Number
      object  = COMA_OFFSET / Object name
      pi_name = Collaboration XRISM / Proposal Principal Investigator Name
      ra  = 194.94118098214 / Right Ascension (Pointing Position) (deg)
      dec = 27.846933593426 / Declination (Pointing Position) (deg)
      roll_angle = 313.826174779643 / Roll Angle (deg)
      start_time = 2024-05-20T12:05:04 / Start Time of the Observation
      stop_time  = 2024-05-22T11:46:04 / Stop Time of the Observation
      exposure   = 89818.63900293 / Effective Total Observation Exposure (s)
      public_date= 2099-12-31 / Public Date

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