CFHTLS power spectra

Intro

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:

• z = 0.5 - 0.6
• z = 0.6 - 0.8
• z = 0.8 - 1.0

We provide: the redshift distributions, the measured power spectra, the covariances between measurements and the window functions describing each data point.

z=0.5-0.6: zdisthist_All_5-6_i225.txt
z=0.6-0.8: zdisthist_All_6-8_i225.txt
z=0.8-1.0: zdisthist_All_8-10_i225.txt

cfhtls_pk_est.txt

cfhtls_pk_covariance.txt

cfhtls_pk_windows.txt

cfhtls_cl_est.txt

cfhtls_cl_covariance.txt

cfhtls_cl_windows.txt