Unclustered tracers remain unclustered: the lack of primordial non-Gaussianity response of bias-zero tracers
Celia Merino, Santiago Avila, A. G. Adame, A. Anguren, V. Gonzalez-Perez, J. Meneses-Rizo

TL;DR
This study tests whether unclustered tracers with zero bias can effectively constrain primordial non-Gaussianities, finding that their PNG response is effectively zero and their clustering behavior complicates such analyses.
Contribution
The paper provides a detailed simulation-based analysis showing that bias-zero tracers do not exhibit the expected PNG response, challenging previous assumptions about their utility.
Findings
Most bias-zero tracers have PNG response compatible with zero.
High-mass halos show some trend but still have negligible PNG response.
Selection based on local density complicates clustering and PNG constraints.
Abstract
Constraining primordial non-Gaussianities (PNG) is one of the main goals of new-generation large-scale galaxy surveys. It had been proposed that unclustered tracers (with bias ) could be optimal for PNG studies, and that these could be found by selecting galaxies in bins of their local density. Here, we test this hypothesis in state-of-the-art simulations from the PNG-UNITsim suite with local and . We consider different parent tracer catalogues: all halos together, halos in large mass bins, and HOD models for LRGs and QSO. We then classify these tracers by their local density () and measure the linear bias () and PNG-response (). Most bins show a PNG-response compatible with for all halos or the low-mass bin (log). For high-mass halos (log12), QSO or LRG, we recover a trend closer to…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Statistical Mechanics and Entropy
