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Table 1.

Observation log of the VLTI GRAVITY+UT high-resolution (R ∼ 4000) observations of NGC 2024 IRS 2.

Date UT Tot. Int. DIT (a) NDIT (b) Proj. baselines PA (c) Calibrator UD diameter (d)
yyyy-mm-dd hh:mm [s] [s] [s] [m] [°] [mas]
2019-01-21 05:04 900 30 10 45, 45, 56, 72, 101, 119 298, 46, 36, 82, 40, 62 HD 31464, HD 37491 0.186  ±  0.004, 0.464  ±  0.018
2019-01-21 05:27 900 30 10 44, 56, 100 45, 36, 40 HD 31464, HD 37491 0.186  ±  0.004, 0.464  ±  0.018
2019-01-21 06:00 900 30 10 34, 43, 55, 56, 98, 103 309, 43, 35, 80, 39, 53 HD 31464, HD 37491 0.186  ±  0.004, 0.464  ±  0.018

Notes.

(a)

Detector integration time per interferogram.

(b)

Number of interferograms.

(c)

Baseline position angle (PA, from N to E) from the shortest to longest baseline.

(d)

The calibrator uniform-disc (UD) diameter (K band) was taken from Chelli et al. (2016).

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