Citation notice #1837 · 2026-07-11 03:18:56.597112+00:00

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO

cites 10.1103/physrevd.106.063501, which carries a correction notice dated 2022-09-06. One-hop deterministic notice: the citation edge exists in the Pith bibliography graph; no model judged whether the citation was load-bearing.

This is not a judgment on the citing paper.

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01Evidence

Raw extraction · citation context · bibliography index 90

cially, while the monopole (all-sky-average) of this chiral V-mode may be difficult to measure, the anisotropies of the stochastic GWB are shown to be a sensitive to it (see, for instance Belgacem and Kamionkowski (2020); Sato-Polito and Kamionkowski (2022); Cruz et al. (2024)). This effect can be leveraged to impose constraints on˜𝑔NL, thereby offering complementary constraint on the parameter over the scales probed by surveys of LSS Philcox (2022); Hou et al. (2023). Section 4 addresses the transition from the theoretical prediction of the GWB to its observational characterization, focusing on its anisotropic component. In the nano-Hertz frequency band, the GWB is primarily sourced by the cosmic population of inspiraling Supermassive Black Hole Binaries(SMBHBs)Sesanaetal.(2008);Casey-Clydeetal.

Parser render (TeX stripped for reading; raw above is the evidence)

cially, while the monopole (all-sky-average) of this chiral V-mode may be difficult to measure, the anisotropies of the stochastic GWB are shown to be a sensitive to it (see, for instance Belgacem and Kamionkowski (2020); Sato-Polito and Kamionkowski (2022); Cruz et al. (2024)). This effect can be leveraged to impose constraints on˜𝑔NL, thereby offering complementary constraint on the parameter over the scales probed by surveys of LSS Philcox (2022); Hou et al. (2023). Section 4 addresses the transition from the theoretical prediction of the GWB to its observational characterization, focusing on its anisotropic component. In the nano-Hertz frequency band, the GWB is primarily sourced by the cosmic population of inspiraling Supermassive Black Hole Binaries(SMBHBs)Sesanaetal.(2008);Casey-Clydeetal

02Event

Type

Correction

Source

Crossref

Original DOI

10.1103/physrevd.106.063501

Notice DOI

10.1103/physrevd.106.063501

Date

2022-09-06

Title

Probing parity violation with the four-point correlation function of BOSS galaxies

Reasons

['Correction']

Work

- (2022) Physical review. D/Physical review. D.

Schema constants (for re-runners): correction · crossref

03Dispute this notice

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