VizieR Online Data Catalog: Metal-rich host stars abundances & equivalent widths (Teske+, 2019)

The list of candidate stars hosting relatively cool transiting giant planets was constructed with the same selection criterion as used in Thorngren et al. (2016, J/ApJ/831/64): T_eq<1000 K (incident flux <2x10⁸ erg/s/cm²), 20 M_{Earth}<M<20 M_J, and M_p and R_p measured with errors =<50%. The results presented here are based on the analysis of observations from three echelle spectrographs: the High Resolution Echelle Spectrometer (HIRES; Vogt et al. 1994SPIE.2198..362V) on the 10 m Keck I telescope, the Magellan Inamori Kyocera Echelle (MIKE) spectrograph (Bernstein et al. 2003SPIE.4841.1694B) on the 6.5 m Magellan II Telescope, and the High Dispersion Spectrograph (HDS; Noguchi et al. 2002PASJ...54..855N) on the 8.2 m Subaru Telescope.

(4 data files).