SAGITTARIUS_A_N2
The objective of the observation is to get the direct evidence of the past outflow of Sgr A*. The key information is the bulk motions of the plasmas of not only the Sgr A bipolar but also the Galactic Center X-ray emission, which may have been created or affected by the Sgr A* outflow. We propose to observe four regions (region N1,N2, S1, S2), which cover the Sgr A bipolar, with 50 ks exposure respectively (total 200 ks).
obsid = 201029010 / Unique Observation/Sequence Number
object = SAGITTARIUS_A_N2 / Object name
pi_name = UCHIYAMA HIDEKI / Proposal Principal Investigator Name
ra = 266.327370139265 / Right Ascension (Pointing Position) (deg)
dec = -28.9679202043023 / Declination (Pointing Position) (deg)
roll_angle = 269.997109518746 / Roll Angle (deg)
start_time = 2025-08-24T06:19:04 / Start Time of the Observation
stop_time = 2025-08-25T14:32:04 / Stop Time of the Observation
exposure = 58638.900426 / Effective Total Observation Exposure (s)
public_date= 2026-09-06 / Public Date