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Table 3

Summary of the properties of the various instruments and corresponding light curves.

Observation Wavelength Observation Observation T 1/T fNy. cadence DC
(nm) start end (days) (10−3 day−1) (day−1) (s) (%)
BHr 550–700 16 March 2015 2 June 2015 78.32 12.77 4167 10.37 6.78
BTr + BHr 550–700 4 Nov. 2016 17 June 2017 224.6 4.453 2128 20.30 7.07
BHr 550–700 9 Nov. 2017 25 April 2018 167.3 5.976 2128 20.30 7.48

bRing 463–639 2 Feb. 2017 1 Sept. 2018 575.5 1.738 135.4 319.1 27.0

ASTEP17 695–844 28 March 2017 14 Sept. 2017 170.0 5.881 495.8 87.13 18.9
ASTEP18 695–844 28 March 2018 15 July 2018 109.3 9.150 502.8 85.92 29.2

TESS 600–1000 19 Oct. 2018 1 Feb. 2019 105.2 9.507 360.0 120.0 85.3
TESS 600–1000 20 Nov. 2020 8 Feb. 2021 79.8 12.53 360.0 120.0 90.2

Notes. The term T denotes the time base of the observations, the reciprocal value 1 /T corresponds to the Rayleigh criterion, fNy, is the Nyquist frequency, and DC is the duty cycle. BRITE Lem (BLb) is equipped with a blue filter and observed β Pictoris from December 2016 until June 2017, but due to significantly higher noise in the time series, the data was disregarded from the analysis. See Zwintz et al. (2019) for an analysis of the BLb observations.

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