Breaking the f NL -- b phi degeneracy with the time evolution of tracer number counts

arXiv:2607.18229 · astro-ph.CO · Submitted 2026-07-20 · Read on arXiv

Caio B. de S. Nascimento, Neal Dalal

astro-ph.CO

Submitted: 2026-07-20

Comments: 17 pages, 9 figures. Comments welcome!

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Separate Universe — 36× in this paper
Non-Gaussianity — 31× in this paper · explained in 2 episodes
Primordial non-Gaussianity — 26× in this paper · explained in 2 episodes
Bispectrum — 11× in this paper · explained in 3 episodes
Clustering — 9× in this paper · explained in 2 episodes
Star Formation Rate — 6× in this paper
Abundance — 5× in this paper · explained in 1 episode
Degeneracy — 5× in this paper · explained in 3 episodes
Consistency — 3× in this paper · explained in 3 episodes
Dust Attenuation — 3× in this paper · explained in 2 episodes
Halo Occupation Distribution — 3× in this paper
Metallicity — 3× in this paper · explained in 3 episodes
Population Synthesis — 3× in this paper · explained in 2 episodes
Robustness — 2× in this paper · explained in 5 episodes
Spectral Energy Distribution — 2× in this paper
Star Formation Rate (SFR) — 2× in this paper · explained in 5 episodes
Accuracy — 1× in this paper · explained in 1 episode
Aperture — 1× in this paper · explained in 1 episode
Baryonic Feedback — 1× in this paper · explained in 3 episodes
Core — 1× in this paper · explained in 2 episodes
Cosmic Microwave Background — 1× in this paper
Homogeneity — 1× in this paper · explained in 2 episodes
Matter Power Spectrum — 1× in this paper · explained in 2 episodes
N-body simulations — 1× in this paper · explained in 2 episodes
Selection Bias — 1× in this paper · explained in 4 episodes
Systematic Bias — 1× in this paper · explained in 3 episodes

Terminology

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