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Table 1.
Best estimates for the Moffat PSF parameters in our target galaxies, as derived using either foreground stars or PNe.
| Galaxy | Method | α | β | FWHM | FWHMHDR |
|---|---|---|---|---|---|
| (pixels) | (pixels) | ||||
| FCC 167 | PNe | 2.99 | 2.15 | 3.69 | 3.56 |
| FCC 219 | PNe | 4.26 | 3.37 | 4.07 | 3.50 |
| FCC 219 | Star | 4.29 | 3.42 | 4.07 | 3.50 |
Notes. The corresponding FWHM of our Moffat models are also compared to the FWHM measurements from the MUSE data header, as obtained by the MUSE slow-guiding system.
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