2017
DOI: 10.1038/srep39891
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Method for Removing Spectral Contaminants to Improve Analysis of Raman Imaging Data

Abstract: The spectral contaminants are inevitable during micro-Raman measurements. A key challenge is how to remove them from the original imaging data, since they can distort further results of data analysis. Here, we propose a method named “automatic pre-processing method for Raman imaging data set (APRI)”, which includes the adaptive iteratively reweighted penalized least-squares (airPLS) algorithm and the principal component analysis (PCA). It eliminates the baseline drifts and cosmic spikes by using the spectral f… Show more

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Cited by 20 publications
(23 citation statements)
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“…Therefore, in order to extract Raman signal from the raw acquired spectrum, it was necessary to pre-process the acquired spectrum (Hosseini et al, 2002). Furthermore, cosmic ray spikes, randomly generated due to cosmic radiation, which affected different wavenumbers each time, needed to be removed (Hosseini et al, 2002;Zhang et al, 2017). For the latter, there are two approaches described in the literature (Zhang et al, 2017;Li and Dai, 2011).…”
Section: Discussionmentioning
confidence: 99%
See 2 more Smart Citations
“…Therefore, in order to extract Raman signal from the raw acquired spectrum, it was necessary to pre-process the acquired spectrum (Hosseini et al, 2002). Furthermore, cosmic ray spikes, randomly generated due to cosmic radiation, which affected different wavenumbers each time, needed to be removed (Hosseini et al, 2002;Zhang et al, 2017). For the latter, there are two approaches described in the literature (Zhang et al, 2017;Li and Dai, 2011).…”
Section: Discussionmentioning
confidence: 99%
“…Furthermore, cosmic ray spikes, randomly generated due to cosmic radiation, which affected different wavenumbers each time, needed to be removed (Hosseini et al, 2002;Zhang et al, 2017). For the latter, there are two approaches described in the literature (Zhang et al, 2017;Li and Dai, 2011). In this study, we went for the easiest method, by replacing the intensities of the cosmic peaks with the average from the neighboring frames (left and right from the ray) as suggested by Zhang et al (2017).…”
Section: Discussionmentioning
confidence: 99%
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“…The spectrum may be complicated by instrumental noise, complex chemical composition of products, environmental factors and other sources of variability [19]. As a consequence, spectral and image preprocessing and correction are necessary to improve the quality of the data before data analysis [29]. Moreover, the chemometrics is crucial for information extraction and better interpretation of the acquired data.…”
Section: Nondestructive Assessment Methodsmentioning
confidence: 99%
“…Labspec, includes real-time spikes correction, enabling visual inspection of the spectra, and/or manual spike removal when very few spikes are present. Some algorithms have been developed to perform automated spike removal in the case of a large dataset, for which manual correction is not possible [72][73][74][75][76]. The most commonly used smoothing algorithm for de-noising the spectra without losing much information is that of Savitzky-Golay [77].…”
Section: Data Preprocessingmentioning
confidence: 99%