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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.