Correlation-based Beam Calibration of 21 cm Intensity Mapping
Abstract Foreground removal presents a significant obstacle in both current and forthcoming intensity-mapping surveys. While numerous techniques have been developed that show promise in simulated data sets, their efficacy often diminishes when they are applied to real-world data. A primary issue is the frequency-dependent variations in the instrumental response. In this paper, we propose a novel approach utilizing the internal cross correlation among different frequencies to calibrate the beam’s frequency fluctuations. Using a simulated data set that incorporates frequency-dependent random fluctuations into the beam model, we illustrate that our method can achieve considerable improvements over traditional techniques. Our results represent a step forward in enhancing the precision and reliability of foreground removal in intensity-mapping surveys.
Authors
- Xiao-Dong Li (ORCID: https://orcid.org/0000-0003-3964-0438)
- Ue‐Li Pen (ORCID: https://orcid.org/0000-0003-2155-9578)
- Jiacheng Ding (ORCID: https://orcid.org/0000-0002-8732-5339)
- Xin Wang (ORCID: https://orcid.org/0000-0002-2472-6485)
Publication Details
- Journal
- The Astrophysical Journal Supplement Series
- Published
- 2024-10-01
- DOI
- https://doi.org/10.3847/1538-4365/ad6f0a
- Citations
- 3
- Primary Topic
- Radio Astronomy Observations and Technology
- Type
- article
- Field-Weighted Citation Impact
- 0.99
Funders
- Ontario Research Foundation
- Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada