Laurence Tresse
Laurence Tresse
Laurence Tresse
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Recap of the VVDS main features<br />
VVDS-CDFS 0.1 deg 2<br />
HST BVIZ<br />
EIS UBVRI<br />
Spectroscopic redshift survey with VIMOS-ESO/VLT<br />
I-band selection VVDS-deep to I AB = 24.0 1.4 deg 2<br />
VVDS-wide to I AB = 22.5 10 deg 2<br />
LRred [5500-9500] Å, R=227, D=7.14 Å/pixel<br />
Exposure ~ 45 mn & 4.5 hours<br />
5 fields<br />
0230-04<br />
CDFS<br />
1000+03<br />
1400+05<br />
2217+00<br />
VVDS-0226-04 1.3 deg 2<br />
Multi-λ<br />
VVDS<br />
U(ESO-WFI) BVRI (CFHT-12K) Jks(ESO-SOFI), VLA 1.4 Ghz<br />
CFTLS Deep ugriz (Y. Mellier)<br />
GALEX NUV, FUV (C.Martin/B.Milliard)<br />
SPITZER-SWIRE NIR, FIR (C. Lonsdale)<br />
XMM (M. Pierre)<br />
4 x 7'x8' ~540 slits<br />
L. <strong>Tresse</strong> NNG Conference, Santa Cruz 10/08/2005<br />
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