Table 2
Kinematics results.
Field | ID | ϵ | PAphot | PA![]() |
PA![]() |
S / N | Ref. line |
– | – | – | (°) | (°) | (°) | – | – |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|||||||
HDFS | 1 | 0.41 | 31.4±0.1 | 23.5±18.0 | 30.5±15.0 | 15 | [OIII] doublet |
HDFS | 3 | 0.06 | –18.8±3.0 | 50.5±11.5 | 59.5±21.8 | 15 | Balmer series |
HDFS | 4 | 0.44 | 35.8±0.1 | 48.0±7.5 | 48.0±14.5 | 15 | [OIII] doublet |
HDFS | 5 | 0.17 | 6.9±0.2 | 14.0±16.5 | 32.0±35.3 | 15 | Balmer series |
HDFS | 6 | 0.16 | 45.0±2.0 | 102.0±89.8 | 2.5±29.5 | 15 | [OIII] doublet |
HDFS | 7 | 0.20 | 43.0±0.7 | 75.5±24.2 | 49.0±12.8 | 11 | [OIII] doublet |
HDFS | 8 | 0.15 | –29.5±0.4 | –26.5±3.2 | –22.5±5.2 | 12 | Balmer series |
HDFS | 9 | 0.19 | –34.8±0.4 | –36.0±7.5 | –36.0±9.8 | 15 | Balmer series |
HDFS | 11 | 0.08 | 27.3±0.5 | –47.0±75.5 | 21.0±89.5 | 12 | [OIII] doublet |
HDFS | 12 | 0.42 | –144.0±4.9 | –125.5±41.8 | –103.5±89.8 | 12 | [OIII] doublet |
UDF-10 | 1 | 0.09 | –35.7±0.1 | –30.0±6.5 | –28.0±4.8 | 15 | Balmer series |
UDF-10 | 2 | 0.05 | 9.1±0.1 | –9.0±11.7 | –13.0±11.8 | 15 | Balmer series |
UDF-10 | 3 | 0.20 | 52.4±0.1 | 51.0±8.2 | 56.5±6.8 | 12 | Balmer series |
UDF-10 | 4 | 0.18 | 64.2±0.1 | 80.0±12.2 | 81.5±11.5 | 12 | Balmer series |
UDF-10 | 5 | 0.07 | 31.4±0.1 | 17.0±89.8 | – | 12 | – |
UDF-10 | 7 | 0.16 | 43.2±0.1 | –68.0±89.8 | –14.0±89.8 | 12 | [OIII] doublet |
UDF-10 | 10 | 0.19 | –5.8±0.1 | 63.0±10.2 | –8.0±24.3 | 10 | Balmer series |
Notes. Kinematics parameters of the galaxy sample. (1) Field of observations; (2) galaxy’s ID; (3) ellipticity of galaxy measured on the MUSE white light image, at 2 Re, and derived as the first moment of the surface brightness; (4) photometric major-axis position angle (PA); (5) stellar kinematic major-axis PA; (6) gas kinematics major-axis PA; (7) targeted spectral S/N of the stellar continuum of the binned sub-cubes; and (8) brightest emission line detected in the MUSE sub-cubes, used to constrain gas kinematics.
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