Table 2.
Characteristics of the observations.
| Galaxy | Project | PI | ESO project ID | Exp. time (s) | Seeing (arcsec) |
|---|---|---|---|---|---|
| NGC 0863 | The dynamics of the AGN | Sandra Raimundo | 099.B-0294 | 8×1100 | 0.901 |
| fuelling reservoir in MRK 590 | |||||
| NGC 3393 | The MUSE atlas of disks (MAD) | C.M. Carollo | 098.B-0551 | 4×900 | 0.789 |
| NGC 6627 | AMUSING survey IX | J. Anderson | 103.D-0440 | 4×601 | 0.839 |
| NGC 0692 | AMUSING survey VII | Hanindyo Kuncarayakti | 101.D-0748 | 4×599 | 1.403 |
| ESO584-7 | AMUSING survey VII | Hanindyo Kuncarayakti | 101.D-0748 | 4×701 | 0.796 |
| ESO325-43 | AMUSING survey V | L. Galbany | 099.D-0022 | 8×701 | 1.285 |
| IC3476 | MUSE study of nearby CC-SNe host | Hanindyo Kuncarayakti | 095.D-0172 | 4×450 | 0.742 |
| environments and parent stellar populations |
Notes. Second column is the project where the galaxy was observed. Last column is the measured seeing in arcesec (as the TEL.IA.FWHMOBS parameter in the header of the .fits files from the datacubes). All galaxies were observed following the AMUSING survey strategy: non-optimal weather at Paranal, that is, at any seeing and even a bright moon.
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