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

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

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article

Correlation-based Beam Calibration of 21 cm Intensity Mapping

Xiao-Dong Li, Ue‐Li Pen, Jiacheng Ding, Xin Wang
3 citations
The Astrophysical Journal Supplement Series
Radio Astronomy Observations and Technology
0.99
article

Correlation-based Beam Calibration of 21 cm Intensity Mapping

Xiao-Dong Li, Ue‐Li Pen, Jiacheng Ding, Xin Wang
article en
3 citations

Abstract

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.

The Astrophysical Journal Supplement SeriesVol. 274(2)
Ontario Research Foundation, Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada
Openalex Percentile: Top 23%
Radio Astronomy Observations and Technology
0.99
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