AGN feeding and feedback in Fornax A - Kinematical analysis of the multi-phase ISM

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Table 1.

Main properties of the observations of the multi-phase gas in NGC 1316.

Telescope	Observing time	Bandwidth	Spatial resolution	Spectral resolution
MeerKAT	8+7 h	1.402–1.420 GHz	22″ × 18″	209 kHz (∼44 km s⁻¹)
ALMA	5.7 h	112.8–114.7 GHz	22″ × 18″	3.8 kHz (∼9.9 km s⁻¹)
MUSE wide-field ^(⋆)	333 s	4650–9300 Å	2.1″ (seeing)	2.3 Å (∼68 km s⁻¹)
MUSE centre-field ^(⋆)	2178 s	4650–9300 Å	2.3″ (seeing)	2.3 Å (∼68 km s⁻¹)

Notes.

^(⋆)

Surface brightness limit after Galactic extinction correction for Hβ and Hα lines. The MUSE spectral resolution (σ) is given at the [N II]λ6583 line.

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