2–6 juin 2025
Laboratoire d'Annecy de Physique Théorique (LAPTh)
Fuseau horaire Europe/Paris

Session

Contributed Talks 4: COMAP

3 juin 2025, 09:40
Laboratoire d'Annecy de Physique Théorique (LAPTh)

Laboratoire d'Annecy de Physique Théorique (LAPTh)

9, chemin de Bellevue 74940 ANNECY France

Présidents de session

Contributed Talks 4: COMAP

  • Nils-Ole Stutzer (Institute of Theoretical Astrophysics, University of Oslo)
  • Patrick Breysse (Southern Methodist University)
  • Jonas Lunde
  • Leah Hansen (University of Oslo)

Documents de présentation

  1. Jonas Lunde
    03/06/2025 09:40

    This talk reflects on the present and future of data analysis techniques in line intensity mapping, with examples from COMAP. COMAP continues to integrate down and will soon achieve a sensitivity consistent with the level of our fiducial models, but proper handling of systematics and a robust data model will be vital in this effort. The Season 2 COMAP results utilized PCA filtering in order to...

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  2. Leah Hansen (University of Oslo)
    03/06/2025 09:55

    In this talk we present a physically motivated signal simulation of the most central systematics in the COMAP telescope. While the Season 2 COMAP results provided the strongest constraints on cosmological CO line emission to date, 75% of the data were cut due to systematic errors. Properly understanding, and subsequently mitigating, the systematics are crucial in order to recover the lost...

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  3. Nils-Ole Stutzer (Institute of Theoretical Astrophysics, University of Oslo)
    03/06/2025 10:10

    In this talk, we will present the state-of-the-art COMAP power spectrum methodology, discuss key lessons learned since the COMAP Season 2 release, and mention some advantages of a joint COMAP-Pathfinder and COMAP-Wide analysis. The COMAP power spectrum methodology relies on cross-correlating maps made by specific configurations of detectors and elevations, each with largely independent...

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  4. Patrick Breysse (Southern Methodist University)
    03/06/2025 10:25

    I will introduce COMAP-Wide, an extension to the ongoing CO Mapping Array Project. Currently, COMAP is operating an autocorrelation-focused CO intensity mapping survey targeting ~12 square degrees of total sky area. COMAP-Wide aims to complement this deep survey with a wide-area, cross-correlation-focused measurement of ~400 square degrees. The primary target of COMAP-Wide will be a...

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