NGC1365
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
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