Volume 566, June 2014
|Number of page(s)||32|
|Section||Planets and planetary systems|
|Published online||23 June 2014|
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).
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.
Sensitivity limit results (at 5σ level) for all observed targets (230 KOIs) in the 2011, 2012, and 2013 observing seasons.
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).
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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