Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data

碩士 === 國立清華大學 === 通訊工程研究所 === 100 === MUSE (Multi-Unit Spectroscopic Explorer) is a wide-field integral field spectrograph at the Very Large Telescope (VLT) for the European Southern Observatory (ESO) under construction and it is an optical instrument to be used to obtain spectra of astronomical obj...

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Main Authors: Shen, Yu-Shiuan, 沈郁瑄
Other Authors: Chi, Chong-Yung
Format: Others
Language:en_US
Published: 2012
Online Access:http://ndltd.ncl.edu.tw/handle/16912914962294854389
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spelling ndltd-TW-100NTHU56501182015-10-13T21:27:24Z http://ndltd.ncl.edu.tw/handle/16912914962294854389 Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data 以MUSE高光譜影像之空間-頻譜分離法於偵測與分析天體物理訊號源 Shen, Yu-Shiuan 沈郁瑄 碩士 國立清華大學 通訊工程研究所 100 MUSE (Multi-Unit Spectroscopic Explorer) is a wide-field integral field spectrograph at the Very Large Telescope (VLT) for the European Southern Observatory (ESO) under construction and it is an optical instrument to be used to obtain spectra of astronomical objects over a two-dimensional field of view. Hence, MUSE will provide three-dimensional hyperspectral data cube with two spatial axes and a wavelength axis. However, due to the high noise level and the three-dimensional translation variant blur function, detection and analysis of astrophysical sources from the forthcoming MUSE instrument is of greatest challenge. In this thesis, we tackle this challenging task by studying how to accurately estimate the spectra of very distant galaxies and the corresponding abundance maps (or proportional contribution of each galaxy over the field of view affected by spatial blur). We first use some realistic hypotheses of MUSE to reformulate the data convolution model into a set of linear mixing models corresponding to different, disjoint spectral frames. Based on the linear mixing models, we propose a spatial-spectral unmixing (SSU) algorithm to detect and characterize the galaxy spectra. In each spectral frame, the SSU algorithm identifies the pure galaxy regions with a theoretical guarantee, and estimate galaxy spectra based on a sparse approximation assumption. Then, the inversion process is applied to estimate the abundances associated with the spectra estimates. The full galaxy spectra can finally be recovered by concatenating the spectra estimates associated with all the spectral frames through an advisable permutation. Some computer simulations are performed to demonstrate the efficacy of the proposed SSU algorithm. Chi, Chong-Yung Chan, Tsung-Han 祁忠勇 詹宗翰 2012 學位論文 ; thesis 37 en_US
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description 碩士 === 國立清華大學 === 通訊工程研究所 === 100 === MUSE (Multi-Unit Spectroscopic Explorer) is a wide-field integral field spectrograph at the Very Large Telescope (VLT) for the European Southern Observatory (ESO) under construction and it is an optical instrument to be used to obtain spectra of astronomical objects over a two-dimensional field of view. Hence, MUSE will provide three-dimensional hyperspectral data cube with two spatial axes and a wavelength axis. However, due to the high noise level and the three-dimensional translation variant blur function, detection and analysis of astrophysical sources from the forthcoming MUSE instrument is of greatest challenge. In this thesis, we tackle this challenging task by studying how to accurately estimate the spectra of very distant galaxies and the corresponding abundance maps (or proportional contribution of each galaxy over the field of view affected by spatial blur). We first use some realistic hypotheses of MUSE to reformulate the data convolution model into a set of linear mixing models corresponding to different, disjoint spectral frames. Based on the linear mixing models, we propose a spatial-spectral unmixing (SSU) algorithm to detect and characterize the galaxy spectra. In each spectral frame, the SSU algorithm identifies the pure galaxy regions with a theoretical guarantee, and estimate galaxy spectra based on a sparse approximation assumption. Then, the inversion process is applied to estimate the abundances associated with the spectra estimates. The full galaxy spectra can finally be recovered by concatenating the spectra estimates associated with all the spectral frames through an advisable permutation. Some computer simulations are performed to demonstrate the efficacy of the proposed SSU algorithm.
author2 Chi, Chong-Yung
author_facet Chi, Chong-Yung
Shen, Yu-Shiuan
沈郁瑄
author Shen, Yu-Shiuan
沈郁瑄
spellingShingle Shen, Yu-Shiuan
沈郁瑄
Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
author_sort Shen, Yu-Shiuan
title Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
title_short Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
title_full Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
title_fullStr Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
title_full_unstemmed Detection and Analysis of Astrophysical Sources via Spatial-spectral Unmixing of MUSE Hyperspectral Data
title_sort detection and analysis of astrophysical sources via spatial-spectral unmixing of muse hyperspectral data
publishDate 2012
url http://ndltd.ncl.edu.tw/handle/16912914962294854389
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