Pith. sign in

REVIEW 3 cited by

Galaxy Bias and $\sigma_8$ from Counts in Cells from the SDSS Main Sample

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2006.01146 v1 pith:JSNU7YZQ submitted 2020-06-01 astro-ph.CO astro-ph.GA

classification astro-ph.COastro-ph.GA
keywords distributiongalaxysigmabiasredshiftdarkdistortionslinear
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
abstract

The counts-in-cells (CIC) galaxy probability distribution depends on both the dark matter clustering amplitude $\sigma_8$ and the galaxy bias $b$. We present a theory for the CIC distribution based on a previous prescription of the underlying dark matter distribution and a linear volume transformation to redshift space. We show that, unlike the power spectrum, the CIC distribution breaks the degeneracy between $\sigma_8$ and $b$ on scales large enough that both bias and redshift distortions are still linear; thus we obtain a simultaneous fit for both parameters. We first validate the technique on the Millennium Simulation and then apply it to the SDSS Main Galaxy Sample. We find $\sigma_8 = 0.94^{+.11}_{-.10}$ and $b = 1.36^{+.14}_{-.11}$, consistent with previous complementary results from redshift distortions and from Planck.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 29 citations worldwide. Full citation record

  1. A theoretical approach to density-split clustering

    astro-ph.CO 2025-01 conditional novelty 7.0 of 10

    Density-split correlation functions can be modeled analytically through the two-point density PDF; a large-deviation-theory version matches N-body simulations on large scales with a single fitted variance parameter.

  2. One with HI: Modelling HI Intensity Mapping one-point statistics including systematics

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    The HI one-point PDF, modelled with large-deviation statistics and validated against simulations including beam and foreground systematics, tightens cosmological constraints and breaks the sigma8-b1 degeneracy beyond ...

  3. Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum

    astro-ph.CO 2024-12 conditional novelty 6.0 of 10

    The inferred initial matter power spectrum from the SELFI algorithm reveals misspecified galaxy bias, selection, mask, redshift, and gravity models, exposing a >2σ cosmological bias before parameter inference.

Pith tools