Free Access

Table 3

Kinematic properties.

Objects υobs,limσint υobs,limσ0,lim
[km s−1] [km s−1] [km s−1]
AS1063-1816 44 ± 3
AS1063-658 62 ± 4 32 ± 9 63 ± 10 1.01 1.97
AS1063-1611 48 ± 2
AS1063-1670 119 ± 27 32 ± 12 80 ± 10 0.67 2.5
AS1063-1152 53 ± 4 40 ± 8 80 ± 11 1.51 2.0
AS1063-1321 52 ± 5 35 ± 7 65 ± 8 1.25 1.86
AS1063-1331 60 ± 5
AS1063-732 79 ± 6 50 ± 10 81 ± 15 1.03 1.62
AS1063-1904 55 ± 4 66 ± 9 22 ± 5 0.39 0.33
AS1063-606_1 40 ± 5 31 ± 6 12 ± 5 0.3 0.39
AS1063-942 40 ± 4 32 ± 6 31 ± 8 0.78 0.97
AS1063-885d 31 ± 11
AS1063-1720 105 ± 54 52 ± 25 37 ± 10 0.35 0.71
MACS1206-2005 104 ± 8 82 ± 15 90 ± 7 0.86 1.1
MACS1206-1123 35 ± 4
MACS1206-1409d 40 ± 22
MACS1206-1235 59 ± 29
MACS1206-445d 71 ± 15
MACS1206-415 78 ± 20
MACS1206-1622 48 ± 5
MACS1206-2372 58 ± 29
MACS1206-1616_1 77 ± 20 79 ± 24 81 ± 7 1.05 1.02
MACS1206-1472 82 ± 7 62 ± 13 63 ± 6 0.77 1.02
MACS1206-820 96 ± 23

Notes. (a) The integrated dispersion σint is the dispersion measured from the integrated spectrum corrected for instrumental broadening (see Eq. (2)). (b) The upper limit dispersion σ0,lim is the dispersion measured in the outer region on the major axis to avoid beam smearing effects and corrected for instrumental broadening. (c) The lower limit velocity υobs,lim is defined as the difference between the maximum and minimum velocity on the major axis divided by two, not corrected for inclination. When both Hα and [OIII] emission lines are detected for the same galaxy, we use Hα only to determine υobs,lim. (d) These three galaxies are unresolved.

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.