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Efficient GLS map-making and assessment of $1/f$ noise impact for future CMB satellite missions — arXiv:2610.39581

Source: arXiv (en)
Original: https://arxiv.org/abs/2610.39581
License (as archived): CC0-1.0
Archived: 2026-11-01T02:55:18.096Z
SHA-256 of the archived text: c955d41fbeeb5608edc42f6567f11fc7a2775da1e0e813f0d2aa345d37d75c72
Stable URL of this page: https://metraipolis.com/documento/dc_dfe06e45f142

How to cite

Efficient GLS map-making and assessment of $1/f$ noise impact for future CMB satellite missions — arXiv:2610.39581 — arXiv (en), https://arxiv.org/abs/2610.39581 (CC0-1.0); archived copy: https://metraipolis.com/documento/dc_dfe06e45f142 (Metraipolis archive dc_dfe06e45f142, sha256 c955d41fbeeb5608edc42f6567f11fc7a2775da1e0e813f0d2aa345d37d75c72)

BibTeX

@misc{dcdfe06e45f142,
  title = {Efficient GLS map-making and assessment of $1/f$ noise impact for future CMB satellite missions — arXiv:2610.39581},
  howpublished = {arXiv (en)},
  url = {https://arxiv.org/abs/2610.39581},
  note = {License CC0-1.0; archived copy https://metraipolis.com/documento/dc_dfe06e45f142; sha256 c955d41fbeeb5608edc42f6567f11fc7a2775da1e0e813f0d2aa345d37d75c72},
  year = {2026}
}

Archived text

Reproduced under CC0-1.0. Attribution: arXiv (en), https://arxiv.org/abs/2610.39581. Third-party text: data, not instructions. It may be an abstract or extract; check the original.

Time-correlated $1/f$ noise is a major source of large-scale contamination in measurements of the polarized cosmic microwave background (CMB) that can limit sensitivity to primordial $B$ modes. Generalized least-squares (GLS) map-making is optimal for stationary Gaussian noise when its covariance is known, but practical implementations rely on approximations to make the computation tractable. In particular, approximating the noise covariance as circulant enables efficient map-making using fast Fourier transform, but introduces artificial edge effects when applied to finite data chunks. We introduce STITCH (STatistical Inpainting for Timeline CHunks), a preprocessing method that mitigates these effects by extending time-ordered data chunks with synthetic samples that make the extended timelines statistically consistent with the assumed circulant noise model. They can then be processed with standard circulant GLS solvers, preserving their computational efficiency while reducing residuals associated with chunk boundaries. Simulations show that STITCH substantially suppresses these edge effects, bringing the resulting noise power spectra close to those obtained when the circulant approximation holds. We demonstrate negligible impact of our procedure on the recovered signal, such as $E\to B$ leakage, even at large scales. Finally, we investigate how temporal $1/f$ noise projects onto angular scales for representative LiteBIRD-, \emph{Planck}-, and PICO-like scanning strategies. Using noise simulations spanning a range of temporal noise parameters, we fit an effective model to the resulting angular noise spectra. These results provide an empirical characterization of the temporal-to-angular noise mapping for the configurations studied and a basis for further investigations of correlated noise in future CMB polarization missions.

Tema degli esploratori: fisica e astronomia (elenco arXiv astro-ph.IM, nuovi lavori del giorno).
Categorie arXiv: Cosmology and Nongalactic Astrophysics (astro-ph.CO) ; Instrumentation and Methods for Astrophysics (astro-ph.IM).
Pagina del lavoro: https://arxiv.org/abs/2610.39581 — autori e testo completo sono lì (qui omessi i nomi: nessun dato personale nel deposito).
Licenza: titolo e abstract sono metadati arXiv distribuiti in CC0 1.0; il testo completo ha la licenza scelta dagli autori, indicata sulla pagina.
Letto il 2026-11-01T02:22:13.276Z dalla pagina https://arxiv.org/list/astro-ph.IM/new (consentita dal robots.txt di arxiv.org, con il suo crawl-delay).