Table 3
Properties of the UV pulses.
| Mode | Year | Orbit | Orbital phase | Amplitude (%) |
|---|---|---|---|---|
| High | 2021 | 1 | 0.62–0.74 | <2.3 |
| High | 2021 | 2 | 0.92–1.07 | 2.13(36) |
| Low | 2021 | 1-2 | 0.64–1.12 | <2.7 |
| High | 2021 | 1-2 | 0.62–1.07 | 1.41(23) |
| High | 2017 | 1 | 0.04–0.16 | 1.25(47) (*) |
| High | 2017 | 2 | 0.37–0.50 | <2.4 |
| High | 2017 | 3 | 0.73–0.82 | 1.56(59) |
| High | 2017 | 1-2-3-4 (**) | 0.04–1.08 | 1.06(37) |
| Low | 2017 | 1-2-3 | 0.03–0.82 | <2.0 |
| Flaring | 2017 | 3 | 0.76–0.81 | <1.6 |
| High | 2014 | 1-2-3 | 0.01–0.81 | 0.68(19) (*) |
| Low | 2014 | 1-2-3 | 0.01–0.76 | <1.8 |
Notes. The total rms amplitude is estimated from the rms amplitude of the first and second harmonic (A1 and A2) as 
.Theuncertainties on the rms amplitudes are at a confidence level of 1s, while the upper limits on the rms amplitudes are at a 3s confidence level. (*)The significance of the signal is lower than 3.5s, but the morphology of the pulse profile is similar to the expected one. (**)In the fourth orbit we consider only 50% of the observation, where there is the overlap with the X-ray band.
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