The UKIDSS Ultra-Deep Survey Depths achieved so far: ) (AB, 5 , 2" apertures) 0.88 deg. Year 1: K=23.5, J=23.6 (85 hours) (85 hours) Already IR survey.

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Presentation transcript:

The UKIDSS Ultra-Deep Survey Depths achieved so far: ) (AB, 5 , 2" apertures) 0.88 deg. Year 1: K=23.5, J=23.6 (85 hours) (85 hours) Already IR survey over this area… Already deepest IR survey over this area… Year 2: K=23.7, H=23.5, J=23.7 ( hours) (120 hours) 2012: K=25.0, H=24.8, J=24.7 (1500 hours) (1500 hours)

The Subaru/XMM Deep Field RA = , Dec = Optical: B=28.2, V=27.6, R=27.5, i’=27.2, z’=26.5, U=27.0 X-ray: XMM-Newton 100ks + 6x50ks Radio: VLA 12  Jy rms 1.4Ghz Spitzer: Spitzer SWIRE  m (NEW: Legacy survey to ~24 AB at 3.6, 4.5  m) Submm: SHADES 8mJy ( 850  m)

Lane et al. (2007), Hartley et al. (2008) Univ of Nottingham BzK selection of galaxies at z>1.4 (B-z) AB (z-K) AB Star-forming Passive

Passive galaxies cluster far more strongly at z~2 arXiv: Hartley et al. (2008), MNRAS (in press arXiv: ) Using n(z) + Limbers: r 0 = 15.0  2.2 h -1 Mpc 6.8  0.2 h -1 Mpc

Spectroscopic UDS (‘SUDS’) ESO Large Programme (20% complete) 93 hours VIMOS 142 hours FORS2

Ly-α at z=6.05 (FORS2) Early spectra from SUDS BzK galaxies at 1.4<z<2.5 (VIMOS)