Table 1
Overview of BRITE observations.
| Satellite name | Orbital period | Year | Contig. time | JD start | JD end | Range in CCDT | No. of 1-s | No. of TSA |
|---|---|---|---|---|---|---|---|---|
| (acronym) | [min] | [min] | −2 450 000 | [° C] | exposures | data points | ||
| BRITE-Lem | 99.7 | 2014 | 7–10 | 6852 | 6867 | 13.7–22.5 | 3059 | 111 |
| (BLb) | 2015 | 10–15 | 7274 | 7287 | 28.7–38.8 | 1781 | 41 | |
| 2016 | 9–14 | 7634 | 7636 | 25.2–26.6 | 727 | 20 | ||
| BRITE-Toronto | 98.2 | 2014 | 10–16 | 6850 | 6890 | 7.7–20.3 | 9654 | 251 |
| (BTr) | 2015 | 5–27 | 7185 | 7341 | 7.4–22.3 | 105 675 | 2098 | |
| 2016 | 4–27 | 7513 | 7665 | 7.4–20.4 | 65 454 | 1747 | ||
| UniBRITE | 100.4 | 2015 | 7–16 | 7186 | 7204 | 27.2–29.9 | 7681 | 175 |
| (UBr) | ||||||||
Notes. Suffixes “b” and “r” indicate the passband (blue/red). “Contig. time” denotes the typical contiguous time interval per orbit duringwhich exposures were made. CCDT is the temperature of the detector. The BTr observations after JD 2 456 877 suffered from excess noise and reduced instrumental throughput and were discarded.
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