The power spectrum from the angular distribution of galaxies in the CFHTLS‐Wide fields at redshift ∼0.7
2012
We measure the real-space galaxy power spectrum on large scales at redshifts 0.5 to 1.2 using optical colour-selected samples from the CFHT Legacy Survey. With the redshift distributions measured with a preliminary 14000 spectroscopic redshifts from the VIMOS Public Extragalactic Redshift Survey (VIPERS), we deproject the angular distribution and directly estimate the three-dimensional power spectrum. We use a maximum likelihood estimator that is optimal for a Gaussian random eld
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
52
References
19
Citations
NaN
KQI