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Table 1

Scattered-light observations used in this work.

Instrument UT date Program Bands Coronagraph ε (″) texp (s) ∆PA (°) Reference star
NACO 2013-03-23 090.C-0443(B) Lp / 0.83 10 676 133 HD 134555
2017-05-07 099.C-0883(A) Lp AGPM 1.42 4763 32 /
2017-05-23 099.C-0883(B) Lp AGPM 1.13 5517 33 /
2018-06-01 0101.C-0924(A) Lp AGPM 0.40 3705 54 /
2018-06-02 0101.C-0924(A) Lp AGPM 0.37 3890 128 IRAS 15097-3636
2018-06-29 0101.C-0924(C) Lp AGPM 2.48 2593 105 IRAS 15097-3636

SPHERE 2015-05-14(a) 095.C-0298(A) YJH ALC_YJH_S 0.50 4096 63 HIP 98470
K 12 4096
2018-03-26 2100.C-5045(B) YJH / 0.53 2688 63 /
K 12 1876
2023-05-11 109.23HK.001 YJH / 0.65 1856 12 HD 136533
K 12 1232
2023-07-23 109.23HK.001 YJH / 0.53 1856 60 HD 136533
K 12 1232
2023-07-24 109.23HK.001 YJH / 0.63 1840 12 HD 136533
K 12 1180
2024-03-05 111.24HH.001 YJH / 0.35 1856 58 HD 136533
K 12 1232
2024-03-06 111.24HH.001 YJH / 0.58 1856 58 HD 136533
K 12 1232

NIRCam 2023-02-16(b) GTO 1179 187N+200W
405N+410M
/ / 2674 10 /

ERIS 2024-04-18(c) 113.26B2.001 Lp AGPM 0.52 4963 55 /

Notes. The columns provide the instrument used for the observation, the observing night, the program ID, the spectral bands, the coronagraph used, the average seeing, the total integration time (DIT × Nint), the amount of field rotation (for total intensity observations), and the name of a reference star if one was used. (a) Published in Maire et al. (2017). (b) Published in Cugno et al. (2024). (c) Published in Maio et al. (2025).

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