Understand
Published galaxy power spectra from the 2dFGRS and SDSS are not in good agreement.
- We revisit this issue by analyzing both the 2dFGRS and SDSS DR5 catalogues using essentially identical techniques.
- We confirm that the 2dFGRS exhibits relatively more large scale power than the SDSS, or, equivalently, SDSS has more small scale power.
- We demonstrate that this difference is due to the r-band selected SDSS catalogue being dominated by more strongly clustered red galaxies, which have a stronger scale dependent bias.
Reading the bibliography…