An Efficient Profile Detection Method for Fiber Spectrum Images with Low SNR Based on Wigner Bispectrum

Details An Efficient Profile Detection Method for Fiber Spectrum Images with Low SNR Based on Wigner Bispectrum An Efficient Profile Detection Method for Fiber Spectrum Images with Low SNR Based on Wigner Bispectrum

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011pasa...28..144z&link_type=abstract

Publications of the Astronomical Society of Australia, Volume 28, Issue 2, pp. 144-149.

Astronomy and Astrophysics

Astronomy

Line: Profiles, Methods: Data Analysis, Techniques: Spectroscopic

Scientific paper

A novel profile detection method is proposed for astronomical fiber spectrum data with low signal-to-noise ratio. This approach can be applied to the pretreatment for 2-D astronomical spectrum data before the extraction of spectra. The Wigner bispectrum, a classical higher-order spectrum analysis method, is introduced and applied to deal with the spectrum signal in this article. After analyzing the Wigner higher-order spectra distribution of the target profile signal, the combination of the Wigner bispectrum algorithm and the fast Fourier transform algorithm is used to weaken the effect of the noise to obtain more accurate information. Both the reconstruction method of the Wigner bispectrum and inverse fast Fourier transform are used to acquire the detection signal. At the end of this paper, experiments with both simulated and observed data based on the Large Sky Area Multi-Object Fiber Spectroscopy Telescope project are presented to demonstrate the effectiveness of the proposed method.

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