English

Bayesian Multi-line Intensity Mapping

Cosmology and Nongalactic Astrophysics 2024-07-22 v2 Astrophysics of Galaxies

Abstract

Line intensity mapping (LIM) has emerged as a promising tool for probing the 3D large-scale structure through the aggregate emission of spectral lines. The presence of interloper lines poses a crucial challenge in extracting the signal from the target line in LIM. In this work, we introduce a novel method for LIM analysis that simultaneously extracts line signals from multiple spectral lines, utilizing the covariance of native LIM data elements defined in the spectral--angular space. We leverage correlated information from different lines to perform joint inference on all lines simultaneously, employing a Bayesian analysis framework. We present the formalism, demonstrate our technique with a mock survey setup resembling the SPHEREx deep field observation, and consider four spectral lines within the SPHEREx spectral coverage in the near infrared: Hα\alpha, [[\ion{O}{3}]], Hβ\beta, and [[\ion{O}{2}]]. We demonstrate that our method can extract the power spectrum of all four lines at the 10σ\gtrsim 10\sigma level at z<2z<2. For the brightest line, Hα\alpha, the 10σ10\sigma sensitivity can be achieved out to z3z\sim3. Our technique offers a flexible framework for LIM analysis, enabling simultaneous inference of signals from multiple line emissions while accommodating diverse modeling constraints and parameterizations.

Keywords

Cite

@article{arxiv.2403.19740,
  title  = {Bayesian Multi-line Intensity Mapping},
  author = {Yun-Ting Cheng and Kailai Wang and Benjamin D. Wandelt and Tzu-Ching Chang and Olivier Doré},
  journal= {arXiv preprint arXiv:2403.19740},
  year   = {2024}
}

Comments

27 pages, 18 figures, accepted by ApJ

R2 v1 2026-06-28T15:37:36.640Z