Free Access
Volume 566, June 2014
Article Number A103
Number of page(s) 32
Section Planets and planetary systems
Published online 23 June 2014

Online material

Table 1

Observational information, completeness, and detectability magnitudes for the isolated KOIs observed with the Calar Alto/AstraLux instrument during the 2011 observational season (62 KOIs in total) and all targets observed during 2012 and 2013 seassons (20 and 57 KOIs, respectively).

Table 1


Table 3

Photometry of the 23 active KOIs (upper part of the table) and 18 demoted KOIs (bottom part of the table) with detected companions that are closer than 6 arcsec in the new sample observed during 2012 and 2013.

Table 4

Sensitivity limit results (at 5σ level) for all observed targets (230 KOIs) in the 2011, 2012, and 2013 observing seasons.

Table 7

Results of the blended source probability prior (PBS,0) and after () the AstraLux images for 222 planet candidates around isolated KOIs from all three observing runs (Type = 0) and KOIs with detected companions at 3–6 arcsec from the 2012 and 2013 observing runs (Type = 1).

Table 11

Comparison between the blended source probabilities (PBS, in %) obtained by using the L13 (Law et al. 2013) and our high-resolution images (LB14) for coincident planet candidates (167 in total).

© ESO, 2014

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