1. Introduction

2. The sample

3. Observations
3.1. ALMA data
3.2. Ancillary data

4. Continuum maps
4.1. Morphology of the emission
4.2. Decomposition of continuum emission: point sources and extended components
4.3. Spectral index maps
4.4. Masses of the extended components
4.5. Orientation of the extended components: equatorial (torus-like) or polar?

5. Molecular line emission
5.1. The ∼ kiloparsec scale region
5.2. The circumnuclear disk (CND) and tori scales: $r\leq200\,pc$ and $r\leq50\,pc$

6. The many faces of dusty molecular tori: dust, CO and $\mathtt{HCO^{+}}$ emission

7. Dusty molecular tori and the processing of $\mathbf{x}$-rays
7.1. Dusty molecular tori and $X$-ray absorption
7.2. Dusty molecular tori and X-ray reflection

8. The radial distribution of molecular gas: the imprint of feedback?
8.2. The dusty molecular tori scales
8.3. A scenario describing the imprint of AGN feedback in Seyfert galaxies

9. Summary and outlook