CFHTLS power spectra

The CFHTLS density field. The area is 133 sqr deg.

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:

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

Downloads

Descriptionfile nameplot
Redshift distributions
Redshift distributions
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
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)