Open Access

Table 1.

Results of the kinematical fitting for our sample of galaxies.

Name Line Beam Method z rD inc PA Vmax σgas Vmax/σgas
(arcsec) (kpc) (degree) (degree) (km s−1) (km s−1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
DLA0817g (b) [C II] 0.21×0.15 I 4.249 1.13 108 ± 2 358 5.04
ALESS 073.1 (b) [C II] 0.17×0.14 I 4.746 1.209 32 45 324 54 6.00
HZ7 [C II] 0.35×0.32 I 5.245 1.6 < 47 81 0.95
HZ9 [C II] 0.30×0.25 II 5.529 ... ... 10.8 ± 0.4
HZ4 [C II] 0.39×0.36 I 5.534 108 1.64
J1211 [C II] 0.80×0.57 I 6.019 149 2.57
[O III] 0.76×0.57 I 6.029 1.1 3.12
J0235 [C II] 0.88×0.70 II 6.076 ... ... 10.6 ± 0.3
[O III] 0.69×0.63 II 6.090 ... ... 10.6 ± 0.3
CLM1 [C II] 0.32×0.29 II 6.153 ... ... 10.3 ± 0.3
J0217 [C II] 0.75×0.66 II 6.191 ... ... 10.7 ± 0.3 > 83 < 1.63
[O III] 0.68×0.56 I 6.203 0.8 < 60 < 10.4 < 227 < 2.8
VR7 [C II] 0.56×0.52 II 6.517 ... ... 10.5 ± 0.3
UVISTA-Z-349 [C II] 1.65×1.17 I 6.564 81 1.05
UVISTA-Z-004 [C II] 1.36×1.15 II 6.669 ... ... 10.4 ± 0.3
UVISTA-Z-049 [C II] 1.45×1.16 II 6.716 ... ... 10.4 ± 0.3
UVISTA-Z-019 [C II] 1.39×1.21 II 6.740 ... ... 10.5 ± 0.3
COS-29 [C II] 0.45×0.34 I 6.794 < 60 1.89
COS-30 [C II] 0.43×0.34 I 6.840 73 ± 5 264 3.88
[O III] 0.89×0.60 II 6.851 ... ... 10.2 ± 0.3 > 125 < 1.16
UVISTA-Z-001 [C II] 1.40×1.14 I 7.057 1.3 < 65 201 3.94
UVISTA-Y-004 [C II] 1.37×1.25 I 7.077 < 63 124 2.03
UVISTA-Y-003 [C II] 1.64×1.31 II 7.293 ... ... 10.7 ± 0.3
UVISTA-Y-879 [C II] 1.44×1.25 I 7.357 3.3 < 65 212
SUPER8 [C II] 1.44×1.27 II 7.351 ... ... 10.2 ± 0.3
UVISTA-Y-001 [C II] 1.57×1.28 I 7.660 < 60 90 1.14

Notes. (1) target name; (2) observed line; (3) beam FWHM; (4) best-fitting method; (5) redshift of the FIR line; (6) scale radius of the exponential disk; (7) disk inclination in degrees; (8) position angle of the galaxy; (9) logarithm of the dynamical mass in solar masses; (10) maximum rotational velocity as computed for an exponential disk with the dynamical mass and the scale radius obtained from the fitting; (11) best-fit velocity dispersion; (12) ratio of the maximum rotational velocity and the velocity dispersion.

(b)

Best-fit results with the model exponential disk + stellar bulge.

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.