Table 4.
Stellar kinematic properties of NGC 1052 from MUSE and MEGARA.
| IFUFoV | ΔV | PA | σc | σ |
|---|---|---|---|---|
| (km s−1) | (°) | (km s−1) | (km s−1) | |
| MEGARA | 78 ± 3 | 112 ± 6 | 215 ± 13 | 201 ± 16 |
| MUSEMEGARA | 75 ± 9 | 122 ± 5 | – | 180 ± 6 |
| MUSE | 167 ± 19 | 122 ± 10 | 201 ± 10 | 145 ± 22 |
Notes. ΔV is the observed velocity amplitude; PA is the position angle of the major kinematic axis; σc and σ are the central velocity dispersion (at R < Reff/8, i.e. 303 pc) and the mean velocity dispersion, respectively (see Sect. 4.1). For the velocity dispersion measurement the quoted uncertainties are one standard deviation. The MUSEMEGARA line indicates that the values are measured using the MUSE data but over the field of view (FoV) of MEGARA.
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