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Table 1

Log of the long-slit observations with the 6.5 m Baade telescope.

Slit name RA (J2000) Dec (J2000) UT Date Instrument Exp. time (s) PA (a) (°) Slit width (″)
Epoch1(b) 05:24:19.31 −69:38:49.4 2020 March 08 MagE 3 × 180 + 1 × 240 60 1.0
EpochJ 05:24:19.31 −69:38:49.3 2021 January 30 FIRE 4 × 15 13 0.6
Epoch2 05:24:19.24 −69:38:50.2 2022 December 02 MagE 3 × 180 + 1 × 240 17 0.7
Epoch3 05:24:19.29 −69:38:49.4 2023 April 07 MagE 3 × 180 + 1 × 240 90 0.7
Epoch4 05:24:19.29 −69:38:49.7 2023 September 28 MagE 3 × 180 90 0.7

Neb1 05:24:20.22 −69:38:48.2 2022 March 20 MagE 3 × 400 77 0.7
Neb2 05:24:20.06 −69:38:48.1 2022 March 20 MagE 3 × 400 120 0.7
Neb3 05:24:20.00 −69:38:45.4 2022 March 20 MagE 3 × 400 79 0.7
Neb4 05:24:19.60 −69:38:47.0 2022 December 02 MagE 3 × 400 111 0.7
Neb5 05:24:20.00 −69:38:51.8 2022 December 02 MagE 3 × 400 9 0.7
Neb6 05:24:19.94 −69:38:45.0 2023 September 28 MagE 3 × 400 160 0.7

Notes. (a)The position angle PA = 0° refers to the South-to-North direction, while PA = 90° is the West-to-East direction. (b)From de Wit et al. (2023).

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