New transiting planet candidates from Kepler

The search method consists of initial de-trending of the data, applying the trend filtering algorithm, searching for transit signals with the Box Least Squares fitting method in three frequency domains, visual inspection of the potential transit candidates and an in-depth analysis of the shortlisted candidates.

In this paper we present 150 new periodic planet candidates and seven single transit events, 72 of which are in multiple systems. The periods of these planet candidates vary from ~0.17 to ~440d. 124 of the planet candidates have radii smaller than 3R_{earth}_. We recover 82.5 per cent of the Batalha et al. (2012, Cat.