Table 1
Sample selection.
| VVDS | I AB,lim | Number | Criteria | MASSIV | This |
| Survey fields | of targets | full-filed | sample | work | |
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| Wide | 17.5–22.50 | 24 507 | 224 (183) | 21 (4) | 21 (4) |
| Deep | 17.5–24.00 | 12 668 | 2600 (300) | 29 (1) | 27 (1) |
| Ultra-Deep | 23.0–24.75 | 1200 | 86 (55) | 34 (6) | 2 (2) |
Notes. (1) The fields of the VVDS used in MASSIV. (2) IAB limiting magnitude selection. (3) Total number of spectroscopic targets. (4) Number of targets fulfiling the criteria described in Sect. 2.1. (5) Total number of galaxies in the MASSIV sample at the completion of the survey. (6) Number of galaxies used in this analysis. In Cols. (4) to (6), we indicate in parentheses the numbers of targets observed with adaptive optics in our observing campaign.
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.