Measured magnitudes versus the associated magnitude uncertainty (σmag) for both stars and lunar impact flashes in the I- and R-bands (left and right, respectively). In both panels the stellar measurements are presented as stars, while the validated impact flashes are shown as circles. For the I-band the suspected impact events (cyan crosses) are also shown. For the stars, the predicted model (Eq. (1)) is also presented (solid line; see Fig. 6). The dashed and dotted lines in each panel indicate the model prediction when the minimum and maximum value, respectively, of the background noise (STDbkg) are considered for the case of the observations of 1 March, 2017 with the lower lunar phase ∼0.1 (Fig. 12) observed.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.