English

The Application of Continuous Wavelet Transform Based Foreground Subtraction Method in 21 cm Sky Surveys

Cosmology and Nongalactic Astrophysics 2015-06-16 v1 Instrumentation and Methods for Astrophysics

Abstract

We propose a continuous wavelet transform based non-parametric foreground subtraction method for the detection of redshifted 21 cm signal from the epoch of reionization. This method works based on the assumption that the foreground spectra are smooth in frequency domain, while the 21 cm signal spectrum is full of saw-tooth-like structures, thus their characteristic scales are significantly different. We can distinguish them in the wavelet coefficient space easily and perform the foreground subtraction. Compared with the traditional spectral fitting based method, our method is more tolerant to complex foregrounds. Furthermore, we also find that when the instrument has uncorrected response error, our method can also work significantly better than the spectral fitting based method. Our method can obtain similar results with the Wp smoothing method, which is also a non-parametric method, but our method consumes much less computing time.

Keywords

Cite

@article{arxiv.1306.5378,
  title  = {The Application of Continuous Wavelet Transform Based Foreground Subtraction Method in 21 cm Sky Surveys},
  author = {Junhua Gu and Haiguang Xu and Jingying Wang and Tao An and Wen Chen},
  journal= {arXiv preprint arXiv:1306.5378},
  year   = {2015}
}

Comments

Accepted by ApJ

R2 v1 2026-06-22T00:38:41.528Z