All Tables

Table 1: Observed emission line fluxes (unit: 10^-14 W m^-2 $\mu$ m^-1) for the most prominent lines which are well separated (no blends). The fluxes were absolute calibrated with respect to the ASAS-3 photometry ( $m_V = 11\hbox{$.\!\!^{\rm m}$ }34$ ) by folding standard filter curves. The main uncertainty originates from the "definition'' of the continuum around the lines.