Table E.1.
Comparison with literature values.
| Reference | NGC 5139 | NGC 6715 | NGC 0104 | NGC 5272 | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Arot | PA0 | Arot | PA0 | Arot | PA0 | Arot | PA0 | |||||
| Lane et al. 2010b | - | - | - | - | 2.2±0.2 | - | - | - | ||||
| Bellazzini et al. 2012 | 6.0±1.0 | - | 2.0±0.5 | - | 4.4±0.4 | - | - | - | ||||
| Bianchini et al. 2013 | 6.79 | 12±1 | - | - | 4.00 | 136±1 | - | - | ||||
| Fabricius et al. 2014 | - | - | - | - | - | - | - | 192.2±11.8 | ||||
| Kimmig et al. 2015 | - | - | 1.6±2.9 | - | 4.0±0.3 | - | 0.6±1.0 | - | ||||
| Ferraro et al. 2018 | - | - | - | - | - | - | 1.0 | 151 | ||||
| Kamann et al. 2018 | - | 9.9±4.3 | - | - | - | 134.1±3.6 | - | - | ||||
| Sollima et al. 2019 | 4.27±0.52 | 9.8±7.6 | 0.57±1.11 | - | 5.00±0.32 | 135.7±4.6 | 1.75±0.42 | - | ||||
| Szigeti et al. 2021 | - | - | - | - | - | - | 1.19±0.3 | 164±15 | ||||
| This work | 13.85±0.25 | 162 | 6.01±0.18 | 252 | 9.16±0.50 | 216 | 2.46±0.12 | 162 | ||||
| Reference | NGC 6656 | NGC 3201 | NGC 5904 | NGC 6121 | ||||||||
| Arot | PA0 | Arot | PA0 | Arot | PA0 | Arot | PA0 | |||||
| Lane et al. 2010b | 1.5±0.4 | - | - | - | - | - | 0.9±0.1 | 70−250 | ||||
| Bellazzini et al. 2012 | 1.5±0.4 | - | 1.2±0.3 | - | 2.6±0.5 | 157 | 1.8±0.2 | - | ||||
| Fabricius et al. 2014 | - | - | - | - | - | 148.5±5.6 | - | - | ||||
| Kimmig et al. 2015 | 2.5±2.3 | - | - | - | 2.1±0.7 | - | 1.3±0.5 | - | ||||
| Lee 2017 | - | - | - | - | 3.36±0.7 | 128 | - | - | ||||
| Ferraro et al. 2018 | - | - | 1.3 | 215 | - | - | - | - | ||||
| Lanzoni et al. 2018 | - | - | - | - | 4.0 | 145 | - | - | ||||
| Kamann et al. 2018 | - | 280.9±23.9 | - | 244.3±188.9 | - | 305.7±20.3 | - | 214.5±9.4 | ||||
| Sollima et al. 2019 | 3.38±0.71 | 107.2±9.2 | 0.80±0.41 | - | 4.11±0.42 | 138.4±6.0 | 0.22±0.17 | - | ||||
| Szigeti et al. 2021 | - | - | - | - | 3.45±0.4 | 148±6 | - | - | ||||
| This work | 5.75±0.06 | 252 | 3.37±0.10 | 324 | 8.03±0.14 | 198 | 2.70±0.08 | 234 | ||||
| Reference | NGC 2808 | NGC 6205 | NGC 6752 | NGC 6397 | ||||||||
| Arot | PA0 | Arot | PA0 | Arot | PA0 | Arot | PA0 | |||||
| Lane et al. 2010b | - | - | - | - | ≤0.2 | - | - | - | ||||
| Bellazzini et al. 2012 | 3.3±0.5 | 152 | - | - | 0.0±0.0 | - | 0.2±0.5 | - | ||||
| Fabricius et al. 2014 | - | - | - | 196.5±7.8 | - | - | - | - | ||||
| Lardo et al. 2015 | 4.72±0.2 | 270 | - | - | 0.67±0.2 | 200 | - | - | ||||
| Kimmig et al. 2015 | 3.1±3.8 | - | - | - | 0.3±0.5 | - | - | - | ||||
| Cordero et al. 2017 | - | - | 2.7±0.9 | 14±19 | - | - | - | - | ||||
| Kamann et al. 2018 | - | 313.0±2.4 | - | - | - | 139.1±41.8 | - | - | ||||
| Sollima et al. 2019 | 2.25±0.56 | 143.9±8.4 | 1.53±0.61 | 14.5±14.2 | 0.91±0.34 | - | 0.48±0.17 | 171.4±15.6 | ||||
| Szigeti et al. 2021 | - | - | 2.38±0.4 | 26±9 | - | - | - | - | ||||
| This work | 8.42±0.34 | 198 | 5.62±0.17 | 306 | 1.04±0.15 | 162 | 1.39±0.08 | 198 | ||||
| Reference | NGC 7078 | NGC 0362 | NGC 1851 | NGC 6171 | ||||||||
| Arot | PA0 | Arot | PA0 | Arot | PA0 | Arot | PA0 | |||||
| Bellazzini et al. 2012 | 3.8±0.5 | 290 | - | - | 1.6±0.5 | 252 | 2.9±1.0 | 264 | ||||
| Bianchini et al. 2013 | 2.84 | 106±1 | - | - | - | - | - | - | ||||
| Lardo et al. 2015 | 3.63±0.1 | 120 | - | - | 1.65±0.5 | 50 | - | - | ||||
| Kimmig et al. 2015 | 2.5±0.8 | - | 1.6±1.4 | - | - | - | - | - | ||||
| Ferraro et al. 2018 | - | - | 1.1 | 260 | - | - | 1.2 | 167 | ||||
| Kamann et al. 2018 | - | 150.9±10.4 | - | 318.0±117.6 | - | 3.2±3.5 | - | - | ||||
| Sollima et al. 2019 | 3.29±0.51 | 127.4±28.8 | 0.51±0.56 | - | 0.45±0.42 | - | 0.70±0.46 | - | ||||
| Szigeti et al. 2021 | 2.38±0.4 | 120±11 | - | - | - | - | 0.72±0.3 | 168±30 | ||||
| This work | 4.16±0.10 | 234 | 3.57±0.08 | 234 | 5.59±0.13 | 180 | 0.77±0.09 | 234 | ||||
| Lane et al. 2010b | - | - | - | - | - | - | 0.25±0.09 | - | ||||
| Bellazzini et al. 2012 | 0.4±0.5 | 95 | - | - | - | - | 0.5±0.2 | - | ||||
| Fabricius et al. 2014 | - | 153.5±14.7 | - | - | - | 98.9±12.0 | - | - | ||||
| Kimmig et al. 2015 | - | - | - | - | 1.8±0.8 | - | 0.4±0.2 | - | ||||
| Johnson et al. 2017 | - | - | 3.83±0.12 | 126±2 | - | - | - | - | ||||
| Ferraro et al. 2018 | 1.4 | 315 | - | - | - | - | - | - | ||||
| Kamann et al. 2018 | - | 142.8±17.9 | - | - | - | - | - | - | ||||
| Sollima et al. 2019 | 0.26±0.56 | - | 4.19±1.12 | 123.1±13.2 | 1.46±0.61 | - | 0.88±0.38 | - | ||||
| Szigeti et al. 2021 | - | - | - | - | 2.06±0.6 | 154±14 | - | - | ||||
| This work | 2.27±0.16 | 198 | 2.37±0.22 | 270 | 4.18±0.11 | 216 | 3.58±0.10 | 252 | ||||
| Bellazzini et al. 2012 | 3.9±1.0 | 117 | ||||||||||
| Kamann et al. 2018 | - | 318.2±16.8 | ||||||||||
| Sollima et al. 2019 | 1.51±0.65 | - | ||||||||||
| This work | 6.64±0.47 | 270 | ||||||||||
Notes. The first sub-column represents the rotation amplitude in km/s and the second is the position angle of the rotational axis in degrees. The last row contains the values of this analysis, which represent the values of the observed rotation. Since different conventions of PA0 were followed, the published result have been converted to PA 90 = east, anti-clockwise system.
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