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
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.
Forward citations
Cited by 3 Pith papers
-
Measuring Cosmic Neutrino Masses Independently of Dark Energy
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.
-
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
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.
-
Cosmological feedback from a halo assembly perspective
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.
Discussion (0). Continue with ORCID to comment.