1 code implementation • 30 Apr 2019 • Srinivasan Raghunathan, Gilbert P. Holder, James G. Bartlett, SanjayKumar Patil, Christian L. Reichardt, Nathan Whitehorn
For the fiducial cluster sample considered in this work, we find that bias is negligible compared to the statistical uncertainties for both the standard and the modified QE even when modes up to $\sim 2700$ are used for the gradient estimation.
Cosmology and Nongalactic Astrophysics
1 code implementation • 1 Nov 2018 • Kevin Aylor, Mackenzie Joy, Lloyd Knox, Marius Millea, Srinivasan Raghunathan, W. L. Kimmy Wu
Assumption of the $\Lambda$CDM model, together with data to constrain its parameters, can also be used to determine the size of the sound horizon.
Cosmology and Nongalactic Astrophysics