Table 1.
Point-spread function across the MUSE pointings of the sample galaxies, as characterised using a Moffat function fit to either a foreground star or a selection of bright PNe sources.
| Galaxy | Method | Pointing | FWHM | β |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| FCC 153 | PNe | Centre | 3.6 | 1.9 |
| Halo | 3.6 | 4.2 | ||
| FCC 170 | Star | Centre | 4.1 | 2.4 |
| Halo | 3.5 | 1.7 | ||
| FCC 177 | PNe | Centre | 3.8 | 1.8 |
| Halo | 4.1 | 4.4 |
Notes. (1) Galaxy name. (2) Selected object to estimate the PSF. (3) Selected MUSE pointing. (4) FWHM values are in pixels. (5) β parameter of the Moffat profile. The values FWHM and β are taken from Spriggs et al. (in prep.).
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