Image Details
Caption: Figure 6.
Scatter plot of planet radii vs. orbital periods for planet candidates discovered with Kepler data. Black dots are Kepler planet candidates. Red filled circles are planet candidates from this work that are identified by Planet Hunters. Planet candidates with a single transit are marked with red crosses. Yellow filled circles are planet candidates from previous Planet Hunters papers: PH I (Fischer et al. 2012), PH II: (Schwamb et al. 2012), PH III: (Schwamb et al. 2013), PH IV: (Lintott et al. 2013), PH V: (Wang et al. 2013), PH VI: (Schmitt et al. 2014a), PH VII: (Schmitt et al. 2014b). Long-period planet candidates are predominantly discovered by Planet Hunters.
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