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The CFHT- Legacy Survey
Elisabetta SemboloniArgelander Institut für Astronomie
Terapix/Skywatcher : all data 03A-05A : 20000 Megacam images
W2D4
W3 & D3D2
The CFHTLS -Overview
HST Groth strip
GEMINI-N visibility
VLT visibility VLT visibility + XMM fields
VVDS spectro. survey
VLT visibility
+ HST-Cosmos VLT visibility +
Quasar fieldW1 & D1
W4 VVDSUKIDSS DXS
The CFHTL- Survey
u* g r i z
28.20
33h
28.20
33h
28.60
66h
28.30
132h
27.00
66h
4 uncorrelated fields:W1=72 deg²W2=49 deg²W3=49 deg²W4=25 deg²
Depth in the 5 colors:
The CFHTLS Wide
The CFHTLS Deep
4 uncorrelated fields1 degree² each
Depth in the 5 colors:
u* g r i z
26.40 26.60 25.90 25.50 24.80
The CFHTLS Status• First World Wide release on February 2007 ( data between June 1st, 2003 and May, 2005)
• T0004 release completed on June 2007 ( data between June 1st, 2003 and Oct. 24, 2006) Wide fields in the I band:
W1= 44,W2=33,W3= 44,W4=16 Wide fields in all bands:
W1=19, W2=0,W3=5,W4=11
• End of the survey: 2008
u* g r i Z
D1 26.0
30%
25.7
37%
26.2
40%
26.0 42%
25.2 38%
D2 25.7
3%
26.2 55%
26.1
26%
25.8 25%
25.0 23%
D3 26.1
26%
25.7
37%
26.5
42%
26.2 41%
25.3 44%
D4 26.1
38%
25.7
37%
26.4 47%
26.1 43%
25.2 50%
Scientific goals
Cosmic shear at very large scale (Wide) Galaxy-galaxy lensing (Wide) Evolution of shear signal (Deep)
Cluster of galaxies (Deep + Wide) Observation of high redshift Quasar (Deep) Stellar population (Wide) Stars movement (Wide) Morphologic classification of galaxies Galaxy evolution Supernovae Survey (Deep)
The CFHTLS & the cosmic shear
06.089.08
0P
8.00
Hoekstra et al. 2006
Semboloni et al. 2006
Schimd et al. 2006
Latest CFHTLS-Wide shear results
Work based on T0003 Wide release
First Shear measurement up to 4 degrees !!
Fu et al. in prep
CFHTLS Wide T0003 shear Results
Fu et al. in prep
WMAP 3rd year +CFHTLS Wide
llbert et al 2006
A short (incomplete) summary ofthe science possible the CFHTLS
Astier et al 2006
I
Parker et al 2007
….more at https://cfht.hawaii.edu/Science/CFHTLS/cfhtlspupblications.htm
The future of the CFHTLS ?• The CFHTLS will be ended in 2008 Wircam and Megacam shown their performance and
they could be employed for a 3 year new program
Several options possible: - Wide shallow survey i=23.3, A=4600 deg² (no need of
infrared ) - Deep survey i=25.2, A=80 deg² (Wircam follow up ) - Just focus on the follow up on the infra-red follow up of
the CFHTLS-1 Many option but nothing has been still decided