| Issue |
A&A
Volume 707, March 2026
|
|
|---|---|---|
| Article Number | L15 | |
| Number of page(s) | 5 | |
| Section | Letters to the Editor | |
| DOI | https://doi.org/10.1051/0004-6361/202558825 | |
| Published online | 17 March 2026 | |
Unclustered tracers remain unclustered
The lack of primordial non-Gaussianity response of bias-zero tracers
1
Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain
2
Departamento de Física Teórica, Universidad Autónoma de Madrid, 28049 Madrid, Spain
3
Department of Astrophysics, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
4
Centro de Investigación Avanzada en Física Fundamental (CIAFF), Universidad Autónoma de Madrid, ES-28049 Madrid, Spain
5
Instituto de Física, Universidad Nacional Autónoma de México, Apdo. Postal 20-364 Ciudad de México, Mexico
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
30
December
2025
Accepted:
14
February
2026
Abstract
Constraining primordial non-Gaussianities (PNGs) is one of the main goals of new-generation large-scale galaxy surveys. It had been proposed that unclustered tracers (with bias b1 = 0) could be optimal for PNG studies, and that these could be found by selecting galaxies in bins of their local density. We tested this hypothesis in state-of-the-art simulations from the PNG-UNITsim suite with local fNL = 100 and fNL = −20. We considered different parent tracer catalogues: all haloes together, haloes in broad mass bins, and halo occupation distribution (HOD) models for luminous red galaxies (LRGs) and quasars (QSOs). We then classify these tracers by their local density (δt, R) and measure the linear bias (b1) and PNG response (bϕ). Most δt, R bins show a PNG response compatible with bϕ = 0 for all haloes or the low-mass bin (log M < 11). For high-mass haloes (log M> 12), QSO or LRG, we recover a trend closer to the universality relation (bϕ = 2δcrit(b1 − 1)) for b1 > 1, but the bϕ(b1) curve flattens to 0 below |b1|< 1. Hence, we find bϕ ≈ 0 for all bias-zero tracers considered. The complex δt, R-based selection causes their clustering to strongly deviate from simple assumptions, namely the universality relation and Poisson shot noise, hindering their capability to constrain PNGs.
Key words: early Universe / large-scale structure of Universe / inflation
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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