A Visibility-based 21 cm Bispectrum Estimator for Radio-interferometric Data
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| Format: | Preprint |
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2025
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| author | Gill, Sukhdeep Singh Bharadwaj, Somnath |
| author_facet | Gill, Sukhdeep Singh Bharadwaj, Somnath |
| contents | We present a fast and scalable estimator for the binned multi-frequency angular bispectrum (MABS) and the 3D bispectrum (BS) of the redshifted 21 cm signal from radio interferometric observations. The estimator operates on gridded visibilities and leverages the FFT-based acceleration to efficiently compute the MABS and the 3D BS covering all possible triangle configurations. We present the formalism and validate the estimator using simulated visibility data for a known input model BS, considering the Murchison Widefield Array (MWA) observations with a bandwidth of $30.72$ MHz centered at $154.25$ MHz. We consider two cases, namely, without flagging, and with flagging, which has exactly the same frequency channels flagged as the actual data. We obtain estimates of the BS for a wide range of triangle shapes covering the scales $0.003 ~\mathrm{Mpc}^{-1}\leq k_1 \leq 1.258 ~\mathrm{Mpc}^{-1}$. The estimated BS shows excellent agreement with analytical predictions based on the input model BS. We find that the deviations, which are below 20\% even in the presence of flagging, are mostly consistent with the expected statistical fluctuations. This work paves the way for reliable observational estimates of the 21 cm BS for the epoch of reionization, where the signal is predicted to be highly non-Gaussian. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2506_10526 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | A Visibility-based 21 cm Bispectrum Estimator for Radio-interferometric Data Gill, Sukhdeep Singh Bharadwaj, Somnath Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics We present a fast and scalable estimator for the binned multi-frequency angular bispectrum (MABS) and the 3D bispectrum (BS) of the redshifted 21 cm signal from radio interferometric observations. The estimator operates on gridded visibilities and leverages the FFT-based acceleration to efficiently compute the MABS and the 3D BS covering all possible triangle configurations. We present the formalism and validate the estimator using simulated visibility data for a known input model BS, considering the Murchison Widefield Array (MWA) observations with a bandwidth of $30.72$ MHz centered at $154.25$ MHz. We consider two cases, namely, without flagging, and with flagging, which has exactly the same frequency channels flagged as the actual data. We obtain estimates of the BS for a wide range of triangle shapes covering the scales $0.003 ~\mathrm{Mpc}^{-1}\leq k_1 \leq 1.258 ~\mathrm{Mpc}^{-1}$. The estimated BS shows excellent agreement with analytical predictions based on the input model BS. We find that the deviations, which are below 20\% even in the presence of flagging, are mostly consistent with the expected statistical fluctuations. This work paves the way for reliable observational estimates of the 21 cm BS for the epoch of reionization, where the signal is predicted to be highly non-Gaussian. |
| title | A Visibility-based 21 cm Bispectrum Estimator for Radio-interferometric Data |
| topic | Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2506.10526 |