Unravelling sub-stellar magnetospheres | Astronomy & Astrophysics (A&A)

Open Access

Fig. C.1

Same as Figure 2 except for the best fit to the Aug and Dec. ATCA data. The parameters inferred at these two epochs are listed in Table 2. The top panels show the 1σ ‘noise’ bands in which we do not find any significant emission. The rotation phases shown here are consistent with those in Figure 2.

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.