The GAPS programme at TNG - LXVI. A homogeneous search for Na I and its possible variability in ten gas giant exoplanets

Open Access

Fig. 2

Final transmission spectrum (left) and relative TLC (right) of GJ 436 b without the correction of the CLV and RM effects (upper panels) and after their correction (bottom panels). The green background marks the exposures taken out-of-transit. For graphic purposes only, we fixed the FWHM of the Gaussian fit (red line) at zero being equal to ${0.94}_{- 0.31}^{+ 0.41}$ $0.94_{ - 0.31}^{ + 0.41}$ km s⁻¹.

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.