Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

LaTeX, 11 pages, 10 figures. Changed to match journal paper. Useful pedagogic appendix added for calculations of biased veloci

Scientific paper

10.1111/j.1365-2966.2005.09804.x

Upcoming surveys for galaxy clusters using the Sunyaev-Zel'dovich effect are potentially sensitive enough to create a peculiar velocity catalog. The statistics of these peculiar velocities are sensitive to cosmological parameters. We develop a method to explore parameter space using N-body simulations in order to quantify dark matter halo velocity statistics which will be useful for cluster peculiar velocity observations. We show that mass selection bias from a kinetic Sunyaev-Zel'dovich velocity catalog forecasts rms peculiar velocities with a much more complicated Omega_m dependency than suggested by linear theory. In addition, we show that both two-point functions for velocities disagree with linear theory predictions out to separations of approx. 40 Mpc/h. A pedagogical appendix is included developing linear theory notation with respect to the two-point peculiar velocity functions.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-292350

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.