Meredith L. Rawls edited begin_deluxetable_lccccc_tablecolumns_6__1.tex  over 8 years ago

Commit id: b72550ebaca71c136be1cd67a9f25ef0f4f5e65a

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ELC (Light Curve + RV), Star 2 & $2.14 \pm 0.03$ & $8.33 \pm 0.04$ & $2.927 \pm 0.003$ & $3.702 \pm 0.001$ & $4930 \pm 200$ \\  MOOG Stellar Atmosphere, Star 1 & \nodata & \nodata & $3.21 \pm 0.45$ & \nodata & $4990 \pm 90$ \\  MOOG Stellar Atmosphere, Star 2 & \nodata & \nodata & $3.33 \pm 0.37$ & \nodata & $5030 \pm 80$ \\%  Global Asteroseismology, main \revise{Star 1\tablenotemark{b}} & \nodata & \nodata & \nodata & $4.14 \pm 0.02$ & \nodata \\  Global Asteroseismology, \revise{Star 2\tablenotemark{b}}  & $2.17 \pm 0.13$ & $8.26 \pm 0.16$ & $2.942 \pm 0.007$ & $3.862 \pm 0.009$ & $^{\rm{a}}$\\  Global Asteroseismology, marginal & \nodata & \nodata & \nodata & $4.14 \pm 0.02$ & \nodata  \enddata  \label{table2}  \tablenotetext{a}{A fixed temperature of $5000 \pm 100 \ \rm{K}$ was assumed to calculate the other asteroseismic parameters.}  \tablenotetext{b}{\revise{As discussed in Section \ref{identifying}, we tentatively assign Star 2 to the main set of oscillations and Star 1 to the marginally detected oscillations.}}  \end{deluxetable*}