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Table 2
Characteristics of the spectroscopic redshift sample.
Spectroscopic |
![]() |
imed |
ℱ%
![]() |
|
survey | ||||
|
||||
VIPERS | 33 896 | 21.7 | 60.5![]() |
|
PRIMUS | 14 725 | 21.7 | 26.3![]() |
|
SDSS-BOSS | 4075 | 19.0 | 7.3![]() |
|
VVDS Wide | 1630 | 21.6 | 2.9![]() |
|
VVDS Deep | 457 | 23.1 | 0.8![]() |
|
UDSz | 1220 | 23.1 | 2.2![]() |
|
|
||||
Total sample | 51 396 | 21.6 | 100![]() |
Notes.We report the number of spectroscopic redshifts (), the median value in the i-band (imed), the contribution of each survey to the total spectroscopic sample (ℱ%), and their relative fraction of galaxies with i < 22.5 and i > 22.5.
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