Detection of Neptune-size planetary candidates with CoRoT data - Comparison with the planet occurrence rate derived from Kepler

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Fig. 4

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Top panel: the same as Fig. 3 after filtering the 12 h instrumental signal (see Sect. 3.1.h). The planetary signal is now correctly detected as the most significant peak. Bottom panel: phase-folded light curve at the period and epoch found by the BLS, distinctly showing the transit signature.

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