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