XRISM xtend observation 300075010

Object

NGC1365

Abstract

NGC 1365 is a Seyfert 1.8 galaxy with a rich spectrum of narrow emission and absorption lines. It shows the most robust evidence for four Fe XXV/Fe XXVI K-alpha/K-beta absorption lines from a highly ionised outflow. It shows variable obscuration on timescales as short as days

Summary of xrismmastr

      obsid   = 300075010 / Unique Observation/Sequence Number
      object  = NGC1365 / Object name
      pi_name = Collaboration XRISM / Proposal Principal Investigator Name
      ra  = 53.402567295582 / Right Ascension (Pointing Position) (deg)
      dec = -36.1399005657718 / Declination (Pointing Position) (deg)
      roll_angle = 268.778223200723 / Roll Angle (deg)
      start_time = 2024-02-20T12:23:04 / Start Time of the Observation
      stop_time  = 2024-02-25T01:11:04 / Stop Time of the Observation
      exposure   = 213073.859373 / Effective Total Observation Exposure (s)
      public_date= 2099-12-31 / Public Date

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