All Tables

Table 1: Emission line fluxes in units of 10^-17 erg s^-1 cm^-2. Note that both lines in the [O III] and [N II] doublets were fitted together.
Table 2: Cluster data. Photometry is corrected for foreground reddening only. $\Delta A_B$ is the additional amount of reddening required to best match the SSP model colours. The ranges of turn-off and total cluster masses reflect the differences between spectroscopic and photometric age estimates. The masses are for a Salpeter-like IMF with a lower mass limit of $0.1~M_\odot$
Table 3: Derived nebular properties. $L_{\rm cs}$ is the luminosity of the central star. Note that H $\beta$ fluxes are derived from the H $\alpha$ fluxes assuming standard case B recombination.