Online material
Table 1
Overview of observation nights for OLT and STELLA.
Table 10
Results of individual transit fits.
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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 | |
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Fig. 8
continued. |
| Open with DEXTER | |
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Fig. 8
continued. |
| Open with DEXTER | |
© ESO, 2013