EDP Sciences
Free Access
Issue
A&A
Volume 561, January 2014
Article Number A48
Number of page(s) 20
Section Planets and planetary systems
DOI https://doi.org/10.1051/0004-6361/201322453
Published online 23 December 2013

Online material

Table 1

Overview of observation nights for OLT and STELLA.

Table 10

Results of individual transit fits.

thumbnail Fig. 8

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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