Combining high-contrast imaging with high-resolution spectroscopy: Actual on-sky MIRI/MRS results compared to expectations

Open Access

Fig. E.1

Comparison of PSDs of stellar modulation functions when the amplitude of simulated photometric errors is equivalent to that of aliasing artifacts in the data. The modulation amplitude of the resampling noise on 1SHORT measured by Law et al. (2023) implies an error of $σ_{p h - e r r} \approx 10 % / \sqrt{2} \approx 7 %$ $\[\sigma_{\mathrm{ph}-\mathrm{err}} \approx 10 \% / \sqrt{2} \approx 7 \%\]$ . The mean and standard deviation are calculated all over the cubes.

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.