We present the measurements of P(k) and C_l from Granett et al 2011 http://http://arxiv.org/xxxx (contact: ben.granett@brera.inaf.it). The power spectrum was estimated independentally for three photometric redshift samples selected from CFHTLS:
Description  file name  plot 

Redshift distributions  
Redshift distributions  z=0.50.6: zdisthist_All_56_i225.txt z=0.60.8: zdisthist_All_68_i225.txt z=0.81.0: zdisthist_All_810_i225.txt 

Deprojected power spectra  
power spectra P(k)  cfhtls_pk_est.txt 

Covariance matrix for P(k)  cfhtls_pk_covariance.txt 

Window functions for P(k)  cfhtls_pk_windows.txt 

Angular power spectra  
Angular spectra lC_l  cfhtls_cl_est.txt 

Covariance matrix for lC_l  cfhtls_cl_covariance.txt 

Window functions for lC_l  cfhtls_cl_windows.txt 
contact: Ben Granett (ben.granett@brera.inaf.it)