COMA_OFFSET
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
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