System parameterization of K2-32 and its planets and comparison to literature values.
|Star||Planet e||Planet b||Planet c||Planet d||Ref.|
|R||5.62 R⊕||3.32 R⊕||3.77 R⊕||C16 (a)|
|M||<8.1 M⊕ (95% conf.)||<35.0 M⊕ (95% conf.)||D16|
|<12.1 M⊕ (95% conf.)||P17|
|a (AU)||0.0811||0.14120||0.1879||C16 (a)|
|FPP (d)||0||5 × 10−4||5.4 × 10−6||C16 (a)|
|<1 × 10−3||2.2 × 10−2||<1 × 10−3||S16|
|<1 × 10−4||<1 × 10−4||<1 × 10−4||M18|
|3.1 × 10−3||5.2 × 10−3||4.9 × 10−3||7.2 × 10−3||H19|
Notes. (a) Based on stellar classification (0.92 ± 0.07 R⊙, 0.88 ± 0.03 M⊙) by Huber et al. (2016). (b)Planetary radii and 68.3% confidence intervals based on our measured planet-to-star radius ratio and stellar radius estimates from P17. (c) Semimajor axes and 68.3% confidence intervals based on our measurements of the orbital periods and stellar mass estimates from P17. (d) FPP = false-positive probability. Values do not contain the “multiplicity boost” (reduction in FPP) but are detailed in S16.
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