Extended Data Fig. 1: Multi-band light curve observed by HiPERCAM on 05 June 2019.
From: A dense ring of the trans-Neptunian object Quaoar outside its Roche limit
The flux observed in the gs, rs, is and zs bands (black points) and the models (red line) vs. time relative to the observer’s closest approach time (03:00:31.858 utc). The blue shaded regions are enlarged in the side panels. Only one common model (the one obtained for is) is plotted as no statistically significant differences are observed between filters (Table 1). Note the increase of the light curve quality with wavelength.
