A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors – I. Mathematical formalism

Author:

Sims Peter H12ORCID,Bowman Judd D2,Mahesh Nivedita2,Murray Steven G2ORCID,Barrett John P3,Cappallo Rigel3,Monsalve Raul A245,Rogers Alan E E3,Samson Titu2,Vydula Akshatha K2

Affiliation:

1. Department of Physics & Trottier Space Institute, McGill University , Montreal, QC H3A 2T8, Canada

2. School of Earth and Space Exploration, Arizona State University , Tempe, AZ 85287, USA

3. MIT Haystack Observatory , Westford, MA 01886, USA

4. Space Sciences Laboratory, University of California Berkeley , Berkeley, CA 94720, USA

5. Facultad de Ingeniería, Universidad Católica de la Santísima Concepción , Alonso de Ribera 2850, Concepción, Chile

Abstract

ABSTRACT Accurately accounting for spectral structure in spectrometer data induced by instrumental chromaticity on scales relevant for detection of the 21-cm signal is among the most significant challenges in global 21-cm signal analysis. In the publicly available Experiment to Detect the Global Epoch of Reionization Signature low-band data set, this complicating structure is suppressed using beam-factor-based chromaticity correction (BFCC), which works by dividing the data by a sky-map-weighted model of the spectral structure of the instrument beam. Several analyses of these data have employed models that start with the assumption that this correction is complete. However, while BFCC mitigates the impact of instrumental chromaticity on the data, given realistic assumptions regarding the spectral structure of the foregrounds, the correction is only partial. This complicates the interpretation of fits to the data with intrinsic sky models (models that assume no instrumental contribution to the spectral structure of the data). In this paper, we derive a BFCC data model from an analytical treatment of BFCC and demonstrate using simulated observations that, in contrast to using an intrinsic sky model for the data, the BFCC data model enables unbiased recovery of a simulated global 21-cm signal from beam-factor chromaticity-corrected data in the limit that the data are corrected with an error-free beam-factor model.

Funder

NSF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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