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N., Pyne S., Legnani E., Ferreira T., 2023, The IA Guide: A Breakdown of Intrinsic Alignment Formalisms ( @eprint arXiv 2309.08605 )

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

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astro-ph.CO 3

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representative citing papers

GI BAO as a cosmological consistency check

astro-ph.CO · 2026-05-12 · unverdicted · novelty 7.0

GI BAO provides a robust consistency check for density BAO and shear data, with the first photometric measurement on DES Y3 showing agreement at α = 0.966 ± 0.252.

Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity

astro-ph.CO · 2025-09-10 · conditional · novelty 6.0

The parity-odd intrinsic alignment power spectrum probes the collapsed limit of the parity-odd primordial trispectrum and can tighten constraints on parity-violating PNG when bias parameters are calibrated from N-body simulations.

Dark Energy Survey Year 3: Blue Shear

astro-ph.CO · 2024-10-29 · unverdicted · novelty 4.0

Blue galaxy selection in DES Y3 cosmic shear mitigates IA effects, producing stable parameters with 1.5x smaller S8 uncertainty and improved CMB agreement versus the full sample.

citing papers explorer

Showing 3 of 3 citing papers.

  • GI BAO as a cosmological consistency check astro-ph.CO · 2026-05-12 · unverdicted · none · ref 41

    GI BAO provides a robust consistency check for density BAO and shear data, with the first photometric measurement on DES Y3 showing agreement at α = 0.966 ± 0.252.

  • Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity astro-ph.CO · 2025-09-10 · conditional · none · ref 45

    The parity-odd intrinsic alignment power spectrum probes the collapsed limit of the parity-odd primordial trispectrum and can tighten constraints on parity-violating PNG when bias parameters are calibrated from N-body simulations.

  • Dark Energy Survey Year 3: Blue Shear astro-ph.CO · 2024-10-29 · unverdicted · none · ref 49

    Blue galaxy selection in DES Y3 cosmic shear mitigates IA effects, producing stable parameters with 1.5x smaller S8 uncertainty and improved CMB agreement versus the full sample.