Table 5
Comparison of VVDS surveys with other spectroscopic redshift surveys, by order of increasing mean redshift (updated from Baldry et al. 2010).
| Survey | Area | Depth iABa | N obj | z range | z mean | Selection | Reference |
|
|
|||||||
| SSRS2 | 5500 | 14.5 | 5369 | 0.0–0.08 | 0.03 | B < 15.5 | da Costa et al. (1998) |
| PSCz | 34 000 | 15.0 | 15 411 | 0.0–0.1 | 0.03 | 60 μAB < 9.5 | Saunders et al. (2000) |
| 2MRS | 37 000 | 15.2 | 23 200 | 0.0–0.08 | 0.03 | K < 15.2 | Erdoğdu et al. (2006) |
| SAPM | 4300 | 15.7 | 1769 | 0.0–0.1 | 0.034 | BJ < 17.1 | Loveday et al. (1992) |
| 6dFGS | 17 000 | 15.7 | 110 256 | 0.0–0.1 | 0.05 | K < 12.7 | Jones et al. (2009) |
| CfA2 | 17 000 | 14.5 | 13 000 | 0.0–0.1 | 0.05 | B < 15.5 | Falco et al. (1999) |
| DURS | 1500 | 15.6 | 2500 | 0.0–0.2 | 0.07 | BJ < 17.0 | Ratcliffe et al. (1996) |
| LCRS | 700 | 17.5 | 26 418 | 0.0–0.25 | 0.1 | R < 17.5 | Shectman et al. (1996) |
| 2dFGRS | 1500 | 18.0 | 250 000 | 0.0–0.3 | 0.11 | BJ < 19.4 | Colless et al. (2001) |
| H-AAO | 8.2 | 18.0 | 1056 | 0.0–0.55 | 0.14 | KAB < 16.8 | Huang et al. (2003) |
| ESP | 23.3 | 18.0 | 3500 | 0.0–0.3 | 0.15 | BJ < 19.4 | Vettolani et al. (1997) |
| AGES | 9.3 | 19.8 | 6500 | 0.0–0.5 | 0.2 | R < 20BW < 20.5 | Watson et al. (2009) |
| GAMA | 144 | 19.8 | 79 599 | 0.0–0.6 | 0.25 | r < 19.8,z < 18.2, KAB < 17.6 | Baldry et al. (2010) |
| CNOC2 | 1.5 | 21.3 | 5000 | 0.12–0.55 | 0.3 | R < 21.5 | Yee et al. (2000) |
| Autofib | 5.5 | 20.5 | 1700 | 0.0–0.75 | 0.3 | BJ < 22 | Ellis et al. (1996) |
| SDSS-LRG | 8000 | 19.5 | 46 748 | 0.16–0.47 | 0.3 | r < 19.5+ CSb | Eisenstein et al. (2005) |
| SDSS-MGS | 9380 | 17.8 | 935 000 | 0.0–0.6 | 0.3 | r < 17.8, DR7 | Abazajian et al. (2009) |
| 2SLAQ-LRG | 180 | 20.3 | 11 000 | 0.45–0.8 | 0.5 | i < 19.8 + CS | Cannon et al. (2006) |
| CFRS | 0.14 | 22.5 | 600 | 0–1.5 | 0.55 | IAB ≤ 22.5 | Lilly et al. (1995) |
| zCosmos-Bright | 1.7 | 22.5 | 20 000 | 0–1.5 | 0.55 | 17.5 ≤ iAB ≤ 22.5 | Lilly et al. (2007) |
| VVDS-Widec | 8.7 | 22.5 | 26 178 | 0–1.5 | 0.55 | 17.5 ≤ IAB ≤ 22.5 | Garilli et al. (2008) |
| PRIMUS | 9.1 | 23.5 | 96 599 | 0.0–1.2 | 0.6 | iAB ≤ 23 | Coil et al. (2011) |
| WiggleZ | 1000 | 21.0 | 100 000 | 0.2–1.0 | 0.6 | NUV < 22.8 + CS | Blake et al. (2011) |
| VVDS-Deep | 0.74 | 24.00 | 11 601 | 0–5 | 0.92 | 17.5 ≤ IAB ≤ 24.0 | Le Fèvre et al. (2005a), this paper |
| DEEP2 | 2.8 | 23.4 | 38 000 | 0.7–1.4 | 1.0 | RAB < 24.1 + CS | Newman et al. (2013) |
| VIPERS | 24 | 22.5 | 100 000 | 0.5–1.5 | 1.0 | 17.5 ≤ iAB ≤ 22.5 + CS | Guzzo et al. (2013) |
| VVDS-UDeep | 0.14 | 24.75 | 941 | 0–4.5 | 1.38 | 23.0 ≤ iAB ≤ 24.75 | This paper |
| zCosmos-Deep | 1 | 23.75 | 2728 | 1.5–2.5 | 2.1 | BAB ≤ 25 + CS | Lilly et al. (2007) |
| LBG-z3 | 0.38 | 24.8 | 1000 | 2.7–3.5 | 3.2 | RAB < 25.5 + CS | Steidel et al. (2003) |
| VUDS | 1 | 25 | 10 000 | 2–6.7 | 3.7 | iAB < 25 + photo-z | Le Fèvre et al. (in prep.) |
| LBG-z4 | 0.38 | 25.0 | 300 | 3.5–4.5 | 4.0 | IAB < 25 +CS | Steidel et al. (1999) |
|
|
|||||||
| VVDS-Alld | 8.7 | 24.75 | 35 016 | 0–5 | 1.2 | Combined VVDS | This paper |
Notes.
includes all objects in the 3 VVDS-Wide fields (1003+01, 1400+05 and 2217+00), in the VVDS-Deep fields (0226 and ECDFS), in the VVDS-Ultra-Deep field (0226-04), and the LAE emitters, as described in Table 1.
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