Search for the optimal smoothing method to improve S/N in cosmic maser spectra

In this article, a number of smoothing methods were investigated to enhance the signal-to-noise (S/N) ratio of diverse methanol maser spectral data, encompassing variations in signal strength, multiplicity of peaks, and spectral complexity. The study aimed to improve the accuracy and reliability of...

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Main Authors: Egliene Anete, Aberfelds Artis
Format: Article
Language:English
Published: De Gruyter 2025-06-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2025-0012
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author Egliene Anete
Aberfelds Artis
author_facet Egliene Anete
Aberfelds Artis
author_sort Egliene Anete
collection DOAJ
description In this article, a number of smoothing methods were investigated to enhance the signal-to-noise (S/N) ratio of diverse methanol maser spectral data, encompassing variations in signal strength, multiplicity of peaks, and spectral complexity. The study aimed to improve the accuracy and reliability of astronomical measurements obtained with Irbene radio telescopes RT-16 and RT-32 at the Ventspils International Radio Astronomy Center. Comparing eleven different smoothing techniques, including moving average, Gaussian, Hanning, among others, the Savitzky–Golay smoothing method is identified as the optimal choice. The evaluation criteria included the preservation of spectral features, reduction of noise artifacts, and enhancement of S/N ratio metrics. The Savitzky–Golay method outperformed other techniques by effectively balancing noise reduction with the preservation of spectral details crucial for maser emission analysis.
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publishDate 2025-06-01
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spelling doaj-art-5a54f5034cfa4d67ad8d03a858d5c94c2025-08-20T03:45:45ZengDe GruyterOpen Astronomy2543-63762025-06-013415699571410.1515/astro-2025-0012Search for the optimal smoothing method to improve S/N in cosmic maser spectraEgliene Anete0Aberfelds Artis1Engineering Research Institute “Ventspils International Radio Astronomy Center”, Ventspils University of Applied Sciences, Inzenieru Str. 101, Ventspils LV-3601, LatviaEngineering Research Institute “Ventspils International Radio Astronomy Center”, Ventspils University of Applied Sciences, Inzenieru Str. 101, Ventspils LV-3601, LatviaIn this article, a number of smoothing methods were investigated to enhance the signal-to-noise (S/N) ratio of diverse methanol maser spectral data, encompassing variations in signal strength, multiplicity of peaks, and spectral complexity. The study aimed to improve the accuracy and reliability of astronomical measurements obtained with Irbene radio telescopes RT-16 and RT-32 at the Ventspils International Radio Astronomy Center. Comparing eleven different smoothing techniques, including moving average, Gaussian, Hanning, among others, the Savitzky–Golay smoothing method is identified as the optimal choice. The evaluation criteria included the preservation of spectral features, reduction of noise artifacts, and enhancement of S/N ratio metrics. The Savitzky–Golay method outperformed other techniques by effectively balancing noise reduction with the preservation of spectral details crucial for maser emission analysis.https://doi.org/10.1515/astro-2025-0012smoothingradioastronomyspectraconvolution
spellingShingle Egliene Anete
Aberfelds Artis
Search for the optimal smoothing method to improve S/N in cosmic maser spectra
Open Astronomy
smoothing
radioastronomy
spectra
convolution
title Search for the optimal smoothing method to improve S/N in cosmic maser spectra
title_full Search for the optimal smoothing method to improve S/N in cosmic maser spectra
title_fullStr Search for the optimal smoothing method to improve S/N in cosmic maser spectra
title_full_unstemmed Search for the optimal smoothing method to improve S/N in cosmic maser spectra
title_short Search for the optimal smoothing method to improve S/N in cosmic maser spectra
title_sort search for the optimal smoothing method to improve s n in cosmic maser spectra
topic smoothing
radioastronomy
spectra
convolution
url https://doi.org/10.1515/astro-2025-0012
work_keys_str_mv AT eglieneanete searchfortheoptimalsmoothingmethodtoimprovesnincosmicmaserspectra
AT aberfeldsartis searchfortheoptimalsmoothingmethodtoimprovesnincosmicmaserspectra