Free Access

Table 2

Light curves of five transiting exoplanet systems.

WASP- Source Filter Date Δm σ m Flip

119 W WASP 5780.52513 0.0123 0.0163 0
119 W WASP 5780.52557 −0.0135 0.0159 0
119 W WASP 5780.54147 −0.0014 0.0156 0

Notes. This table is available in its entirety at CDS. The first few lines are shown here for guidance as to its contents and format. Column 1 is the WASP identification number of the star. Column 2 indicates the source of the observation as follows: W – WASP-South; T – TRAPPIST; E – EulerCam. Column 3 indicates the filter used for the observations as follows: WASP – 400–700 nm; NIR – Astrodon NIR 700 nm cut-on luminance; Exo – Astrodon ExoPlanet-BB; NGTS – EulerCam NGTS; z_p – z; Gunn – Gunn R; I_C – Cousins IC. Column 4 is the UTC date of the observation given as HJD-2 450 000. Columns 5 and 6 are the apparent magnitude of the star and its standard error relative to the mean out-of-transit apparent magnitude. Column 7 is a flag that is set to the value 1 for the first observation after a meridian flip with the TRAPPIST telescope.

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.