Modeling the Radio Foreground for detection of CMB spectral distortions from Cosmic Dawn and Epoch of Reionization
Mayuri Sathyanarayana Rao, Ravi Subrahmanyan, N Udaya Shankar, Jens, Chluba

TL;DR
This paper introduces a robust foreground modeling method using maximally smooth functions to detect faint CMB spectral distortions from the Cosmic Dawn and Epoch of Reionization, overcoming bright foreground challenges.
Contribution
It demonstrates the effectiveness of MS functions over polynomials for foreground separation and shows that the EoR signal can be detected with high confidence in short integration times.
Findings
MS functions effectively model smooth radio foregrounds.
The EoR signal can be detected with 90% confidence in 10 minutes.
MS functions preserve the EoR signal integrity during fitting.
Abstract
Cosmic baryon evolution during the Cosmic Dawn and Reionization results in redshifted 21-cm spectral distortions in the cosmic microwave background (CMB). These encode information about the nature and timing of first sources over redshifts 30-6 and appear at meter wavelengths as a tiny CMB distortion along with the Galactic and extragalactic radio sky, which is orders of magnitude brighter. Therefore, detection requires precise methods to model foregrounds. We present a method of foreground fitting using maximally smooth (MS) functions. We demonstrate the usefulness of MS functions over traditionally used polynomials to separate foregrounds from the Epoch of Reionization (EoR) signal. We also examine the level of spectral complexity in plausible foregrounds using GMOSS, a physically motivated model of the radio sky, and find that they are indeed smooth and can be modeled by MS functions…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
