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The color-coding in Fig. The TCEs with a period of 0. AU - Kane, Stephen R. Contents move to sidebar hide. Another way to detrend the stellar activity is to fit the correlations between activity indicators as the full width at half maximum FWHM , the bisector or the S-index, and subtract them in order to correct for any long-term effects resulting from a magnetic cycle. The TESS full light curve with the 2 min cadence data is shown in light gray, and the same data binnedto 10 min is in dark gray. More than candidates have been detected and over 80 have been confirmed, expanding the number of small planets around cool stars Guerrero The term "super-Mercury" generally refers to planets that are super-Earth-sized with enhanced uncompressed bulk densities, as compared to Earth-like planets. AU - Nunes, N. Davoult , M. The orbital period of the second planet candidate is at least twice the observing baseline of the PFS RV observations otherwise we would have seen the RV trend turn over before our observations concluded as the potential planet passed through its quadrature phase. Santos , C.

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