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Table 1

Overview of the BRITE, HIPPARCOS, and SMEI observations.

Satellite name (acronym) Porbit (min) Year (s) JD-2400000 (start-end) CCDT (°C) Contig. time (min) No. of setups texp (s) No. of observ. No. of TSA data points
HIPPARCOS 637.2 1989–1993 47 860–49 051 N/A N/A N/A ∼20 115 115
SMEI 101.5 2003–2011 52 673–55 833 N/A N/A N/A ∼900 38 617 31 707
BRITE-Heweliusz 97.1 2015 57 098–57 176 9.3–18.8 2.6–29.8 3 1 47 816 487
(BHr) 2017 57 760–57 784 13.3–22.2 4.7–20.1 1 4 15 542 257
2017/18 58 066–58 222 0.9–23.8 3.0–21.4 7 4 63 886 1433
BRITE-Lem 99.6 2016/17 57 738–57 910 18.2–34.6 4.0–13.9 5 2 82 516 1382
(BLb)
BRITE-Toronto 98.2 2016/17 57 697–57 877 2.9–20.4 3.7–15.7 6 4 65 260 1822
(BTr)

Notes. Information not available for HIPPARCOS and SMEI is flagged as “N/A”. Suffixes “b” and “r” in the acronyms of BRITE satellites identify the spectral passband (blue and red). “CCDT” is the detector temperature range. “Contig. time” denotes the typical time interval per satellite orbit during which exposures were made. “No. of TSA data points” is the number of data points (in the case of BRITE formed as orbital averages from the elementary measurements) and used for time-series analysis. Intervals between start and end dates include gaps.

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