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Table 2:

Emission-line properties of the red-sequence galaxies for which the spectra covers both [OII] and H$\beta $. The first two columns indicate whether or not [OII] and H$\beta $ have been detected (at 2-$\sigma $ level). High and low [OII]/H$\beta $ stand for EW([OII])>18EW(H$\beta $)-6 and ${\it EW}{\rm ([OII])}<=18{\it EW}$(H$\beta $)-6, respectively.
[OII] H$\beta $ [OII]/H$\beta $ Fraction
N N   48.5%
N Y uncertain 24%
Y N high 4%
Y Y high 4%
Y Y low 19.5%

Source LaTeX | All tables | In the text

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