Fig. 21
Download original image
Simulated observed spectrum by the Ariel mission of TOI-5375 b generated from a PHOENIX/BT-SETTL atmospheric model. The grey line shows the spectra degraded to a resolution of R = 50, while the blue circles indicate the expected fluxes at Ariel wavelengths. Some characteristic spectral features of a brown dwarf are indicated (see e.g. Burrows et al. 2002; Burgasser et al. 2006; Sorahana & Yamamura 2012).
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.