1. Cosmological parameters estimated from peculiar velocity–density comparisons: calibrating 2M++.
- Author
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Hollinger, Amber M and Hudson, Michael J
- Subjects
- *
COSMIC background radiation , *DARK matter , *LARGE scale structure (Astronomy) , *MICROWAVE measurements - Abstract
Cosmological parameters can be measured by comparing peculiar velocities with those predicted from a galaxy density field. Previous work has tested the accuracy of this approach with N -body simulations, but generally on idealized mock galaxy surveys. However, systematic biases may arise solely due to survey selection effects such as flux-limited samples, edge-effects, and complications due to the obscuration of the Galactic plane. In this work, we explore the impact of each of these effects individually as well as collectively using the semi-analytic models from numerical simulations to generate mock catalogues that mimic the 2M++ density field. We find the reconstruction and analysis methods used for our 2M++ mocks produce a value of f σ8 that is biased high by a factor 1.04 ± 0.01 compared to the true value. Moreover, a cosmic volume matching that of 2M++ has a cosmic variance uncertainty in f σ8 of |$\sim 5~{{\ \rm per\ cent}}$|. The systematic bias is a function of distance: it is unbiased close to the origin but is biased slightly high for distances in the range 100–180 h −1 Mpc. Correcting for this small bias, we find that recent peculiar velocity samples yield |$f\sigma _8^{\textrm {lin}} = 0.362\pm 0.023$| , a value that is in tension with the extrapolations from cosmic microwave background measurements. The predicted peculiar velocities from 2M++ have an error of 170 km s−1 that slowly increases with distance, exceeding 200 km s−1 only at distances of 180–200 h −1Mpc. Finally, the residual bulk flow speeds found in previous work are shown to be not in conflict with those expected in the Λ cold dark matter model. [ABSTRACT FROM AUTHOR]
- Published
- 2024
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