The reviewed record of science sign in
Pith

arxiv: 2111.00246 · v1 · pith:KNERIC6I · submitted 2021-10-30 · astro-ph.IM · astro-ph.CO

BISOU: a balloon project to measure the CMB spectral distortions

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 kernel pith:KNERIC6Irecord.jsonopen to challenge →

classification astro-ph.IM astro-ph.CO
keywords spectralballoonbisoudistortionsmissionprojectspaceachievable
0
0 comments X
read the original abstract

The BISOU (Balloon Interferometer for Spectral Observations of the Universe) project aims to study the viability and prospects of a balloon-borne spectrometer, pathfinder of a future space mission dedicated to the measurements of the CMB spectral distortions. We present here a preliminary concept based on previous space mission proposals, together with some sensitivity calculation results for the observation goals, showing that a 5-sigma measurement of the y-distortions is achievable.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Spectral distortion anisotropies from photon to dark photon conversions

    astro-ph.CO 2026-06 unverdicted novelty 7.0

    Computes anisotropic CMB spectral distortion power spectra from photon-dark photon conversions, finding that mass controls multipole shape and mixing sets amplitude, then places Planck limits on the minimal model.

  2. spectroxide: A code package for computing cosmic microwave background spectral distortions

    astro-ph.CO 2026-04 conditional novelty 7.0

    Spectroxide is a publicly available code package that evolves the photon Boltzmann equation from z ~ 5e6 to today to calculate CMB spectral distortions caused by heat or photon injection, with all code and tests gener...

  3. FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics

    astro-ph.CO 2026-05 unverdicted novelty 6.0

    FLAMINGO simulations show tSZ cross-correlations scale as S8 to the power of about 3 and favor low S8=0.72 with strong feedback when compared to SDSS, BOSS, DES, and Planck data.

  4. FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics

    astro-ph.CO 2026-05 conditional novelty 6.0

    tSZ cross-correlations with large-scale structure tracers prefer low S8 and strong baryonic feedback, yielding S8 = 0.72 and low group baryon fraction in FLAMINGO simulations.

  5. Joint probes of dark matter annihilation from neutrino detectors and CMB targets

    hep-ph 2026-06 unverdicted novelty 4.0

    Joint analysis of neutrino detectors and CMB observables can constrain dark matter annihilation into neutrinos for MeV-GeV masses.