2019
DOI: 10.1088/1674-4527/19/10/145
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The Richardson-Lucy deconvolution method to extract LAMOST 1D spectra

Abstract: We use the Richardson-Lucy deconvolution algorithm to extract one dimensional (1D) spectra from LAMOST spectrum images. Compared with other deconvolution algorithms, this algorithm is much more fast. The practice on a real LAMOST image illustrates that the 1D resulting spectrum of this method has a higher SNR and resolution than those extracted by the LAMOST pipeline. Furthermore, our algorithm can effectively depress the ringings that are often shown in the 1D resulting spectra of other deconvolution methods.

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Cited by 7 publications
(3 citation statements)
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“…Richardson-Lucy direct demodulation (LucyDDM) [32] with a non-linear iteration to calculate deconvolution has a wide application in astronomy [33]…”
Section: Richardson-lucy Direct Demodulationmentioning
confidence: 99%
“…Richardson-Lucy direct demodulation (LucyDDM) [32] with a non-linear iteration to calculate deconvolution has a wide application in astronomy [33]…”
Section: Richardson-lucy Direct Demodulationmentioning
confidence: 99%
“…Richardson-Lucy direct demodulation (LucyDDM) [15] with a non-linear iteration to calculate deconvolution has a wide application in astronomy [16] and image processing. We view V PE * (t − s) as a conditional probability distribution p(t|s) where t denotes PMT amplified electron time, and s represents the given PE time.…”
Section: Richardson-lucy Direct Demodulationmentioning
confidence: 99%
“…The Richardson-Lucy (R-L) algorithm was initially proposed by Richardson based on the Bayes formula [12]. It was further developed by Lucy using the Lagrange multiplier method for the log-likelihood function maximization problem [13], which has been used in various domains, including image processing and astronomy [14,15]. However, noise amplification and ringing effects will occur in the iterative process of the algorithm, and the convergence speed is slow [16].…”
Section: Introductionmentioning
confidence: 99%