All Tables

Table 1: The sample. $P_{\rm 178}$ in Col. (3) is total radio power (W Hz^-1sr ^-1) at rest-frame 178 MHz. Column (4) lists spectral index between 178 and 750 MHz, and Cols. (5) and (6) the radio morphology and emission-line type. Apparent magnitude in rest-frame $R_{\rm C}$ -filter and corresponding references are listed in Cols. (7) and (8). Columns (9) and (10) show velocity dispersion measurements from the literature (km s^-1) and corresponding references. The last three columns list emission line fluxes in units of 10^-15 erg s^-1 cm^-2, both from the literature and as determined from our wide slit spectrophotometry, and references.
Table 2: Table of observations. For each galaxy, the slit position angle and exposure time is shown.
Table 3: Results from the fitting. The fitting regions and signal-to-noise per pixel in the continuum is listed. Best-fit velocity dispersions normalized to the same physical aperture ( $r_{\rm ap} = 0.595~h^{-1}$ kpc) and their confidence intervals are shown. "AGN cont.'' indicates that there is too much AGN contamination in the spectrum to obtain a reliable fit.