MUSE datacubes

Here I am uploading the links to the reduced datacubes that I have used in the following papers:

A monolithic collapse origin for the thin and thick disc structure of ESO 243-49 (Comerón et al. 2016)

The kinematics of local thick discs do not support an accretion origin (Comerón et al. 2019)

The complex multi-component outflow of the Seyfert galaxy NGC 7130 (Comerón et al. 2021)

I am also uploading the links to the information necessary to build the kinematic and stellar population maps appearing in the papers. For details on the reduction, please take a look to the papers. In brief, the cubes were reduced with the Reflex environment. The alignment of the different exposures was done manually instead of relying on the MUSE pipeline. Residual sky features were removed with ZAP in the case of Comerón et al. (2019).

Reduced datacube and material to build stellar kinematics and stellar population maps

ESO 243-49 (Comerón et al. 2016)

Reduced datacubes and material to build kinematic and stellar and ionised gas population maps

ESO 157-49 (Comerón et al. 2019)

ESO 443-21 (Comerón et al. 2019)

ESO 469-15 (Comerón et al. 2019)

ESO 544-27 (Comerón et al. 2019)

IC 217 (Comerón et al. 2019)

IC 1553 (Comerón et al. 2019)

PGC 28308 (Comerón et al. 2019)

PGC 30591 (Comerón et al. 2019)

Reduced datacubes in ESO's Phase3

Reduced datacubes from Comerón et al. (2019)

Reduced datacube from Comerón et al. (2021)