Table 2.
Results of the analysis for the MUSE central and halo pointings of the sample galaxies.
| Galaxy | Region | PNe detected per region | N2.5 | Lbol (L⊙) | α2.5
 |
[Z/H]SSP (dex) | [Z/H]SFH (dex) |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| Central pointing | |||||||
| FCC 153 | in-plane | 29 |
 |
 |
 |
−0.13 | 0.008 |
| off-plane | 16 |
 |
 |
 |
−0.645 | −0.617 | |
| FCC 170 | in-plane | 38 |
 |
 |
 |
−0.188 | −0.11 |
| off-plane | 4 |
 |
 |
 |
−0.595 | −0.63 | |
| FCC 177 | in-plane | 46 |
 |
 |
 |
−0.173 | −0.057 |
| off-plane | 10 |
 |
 |
 |
−0.135 | −0.556 | |
| Halo pointing | |||||||
| FCC 153 | in-plane | 24 |
 |
 |
 |
−0.049 | 0.016 |
| off-plane | 14 |
 |
 |
 |
−0.554 | −0.483 | |
| FCC 170 | in-plane | 35 |
 |
 |
 |
−0.51 | −0.07 |
| off-plane | 4 |
 |
 |
 |
−0.048 | 0.32 | |
| FCC 177 | in-plane | 12 |
 |
 |
 |
−0.158 | −0.168 |
| off-plane | 7 |
 |
 |
 |
−0.47 | −0.894 | |
Notes. (1) Target galaxy. (2) Studied region. (3) Number of observed PNe. (4) Theoretical expected number of PNe down to 2.5 magnitudes. (5) Bolometric luminosity. (6) Luminosity specific PNe number. (7) Light-weighted metallicity derived from SSP index measurements. (8) Light-weighted metallicity obtained from the analysis of full spectral fitting.
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