Pith. sign in

REVIEW 3 cited by

class_sz I: Overview

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 2310.18482 v1 pith:DFRM2CIM submitted 2023-10-27 astro-ph.IM astro-ph.CO

classification astro-ph.IMastro-ph.CO
keywords classclass-szcodegithubhttpsnotebooksoverviewalong
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

class_sz is a versatile and robust code in C and Python that can compute theoretical predictions for a wide range of observables relevant to cross-survey science in the Stage IV era. The code is public at https://github.com/CLASS-SZ/class_sz along with a series of tutorial notebooks (https://github.com/CLASS-SZ/notebooks). It will be presented in full detail in paper II. Here we give a brief overview of key features and usage.

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. Full citation record

  1. Measuring Cosmic Neutrino Masses Independently of Dark Energy

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

    Two dark-energy-robust cosmological routes bound ∑mν to <0.152 eV (marginalized) and <0.41 eV (late-Universe-free), with the latter independent of tested w(a) models by construction.

  2. The Atacama Cosmology Telescope: High-redshift measurement of structure growth from the cross-correlation of Quaia quasars and CMB lensing from ACT DR6 and $\textit{Planck}$ PR4

    astro-ph.CO 2025-07 conditional novelty 6.0 of 10

    Quasar-lensing cross-correlations from ACT and Planck give σ8 = 0.804 ± 0.013 and a 12% constraint on matter fluctuation amplitude at z ≈ 5.1, consistent with ΛCDM.

  3. Cosmological feedback from a halo assembly perspective

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    Baryonic feedback imprints on cosmological observables are governed by halo mass assembly: feedback is most efficient at M200m around 10^12.8 solar masses regardless of redshift.

Pith tools