Volume 561, January 2014
|Number of page(s)||20|
|Section||Planets and planetary systems|
|Published online||23 December 2013|
Overview of observation nights for OLT and STELLA.
Results of individual transit fits.
Top panels: the 19 primary transits in black points, along with the photometric error bars accounting for correlated noise, cf. Sect. 4.1. Overplotted in continuous red line is the best-fitted primary transit model modulated by the host star pulsations and the low-order normalization polynomial. Bottom panels: residuals.
|Open with DEXTER|
© ESO, 2013
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