Selecting samples of galaxies with fewer Fingers-of-God
Ant\'on Baleato Lizancos, Uro\v{s} Seljak, Minas Karamanis, Marco Bonici, Simone Ferraro

TL;DR
This paper proposes data-driven methods to select galaxy samples with fewer Fingers-of-God distortions, improving large-scale structure analysis by reducing non-perturbative effects in redshift-space maps.
Contribution
It introduces new selection techniques based on the power spectrum quadrupole and halo mass to mitigate Fingers-of-God effects in galaxy surveys.
Findings
Quadrupole sign change correlates with satellite fraction and velocity dispersion.
Excluding massive haloes reduces problematic galaxy populations.
Mitigation yields marginal improvements in perturbative modeling fits.
Abstract
The radial positions of galaxies inferred from their measured redshift appear distorted due to their peculiar velocities. We argue that the contribution from stochastic velocities -- which gives rise to Fingers-of-God (FoG) anisotropy in the inferred maps -- does not lend itself to perturbative modelling already on scales targeted by current experiments. To get around this limitation, we propose to remove FoG using data-driven indicators of their abundance that are local in nature and thus avoid selection biases. In particular, we show that the scale where the measured power spectrum quadrupole changes sign is tightly anti-correlated with both the satellite fraction and the velocity dispersion, and can thus be used to select galaxy samples with fewer FoG. In addition, we show that excluding galaxies in haloes more massive than a given mass threshold can help to discard many of the most…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
