Light curves for the right circularly polarized flux at the position of τ Boötis b over the course of the observing campaign. Time series at time resolution of 4 s and 17 minutes are shown in red and blue, respectively, with rms noise of 65 mJy for the 4 s resolution time series and 4 mJy for the 17 minute resolution time series. No evidence for heightened emission is present during any of the observed orbital/rotational phase of the planet.