Files in this item
Multi-component decomposition of astronomical spectra by compressed sensing
Item metadata
dc.contributor.author | Cheung, Mark C. M. | |
dc.contributor.author | De Pontieu, Bart | |
dc.contributor.author | MartÍnez-Sykora, Juan | |
dc.contributor.author | Testa, Paola | |
dc.contributor.author | Winebarger, Amy R. | |
dc.contributor.author | Daw, Adrian | |
dc.contributor.author | Hansteen, Viggo | |
dc.contributor.author | Antolin, Patrick | |
dc.contributor.author | Tarbell, Theodore D. | |
dc.contributor.author | Wuelser, Jean-Pierre | |
dc.contributor.author | Young, Peter | |
dc.contributor.author | the MUSE team | |
dc.date.accessioned | 2019-09-09T11:30:06Z | |
dc.date.available | 2019-09-09T11:30:06Z | |
dc.date.issued | 2019-09-01 | |
dc.identifier.citation | Cheung , M C M , De Pontieu , B , MartÍnez-Sykora , J , Testa , P , Winebarger , A R , Daw , A , Hansteen , V , Antolin , P , Tarbell , T D , Wuelser , J-P , Young , P & the MUSE team 2019 , ' Multi-component decomposition of astronomical spectra by compressed sensing ' , Astrophysical Journal , vol. 882 , no. 1 , 13 . https://doi.org/10.3847/1538-4357/ab263d | en |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | PURE: 259229065 | |
dc.identifier.other | PURE UUID: f27d6f05-d3a9-49d3-8161-25c0b248298d | |
dc.identifier.other | BibCode: 2019arXiv190203890C | |
dc.identifier.other | Scopus: 85072337353 | |
dc.identifier.other | WOS: 000483047000002 | |
dc.identifier.uri | https://hdl.handle.net/10023/18435 | |
dc.description | Funding: STFC Ernest Rutherford Fellowship (grant agreement No. ST/R004285/1) (PA). | en |
dc.description.abstract | The signal measured by an astronomical spectrometer may be due to radiation from a multi-component mixture of plasmas with a range of physical properties (e.g., temperature, Doppler velocity). Confusion between multiple components may be exacerbated if the spectrometer sensor is illuminated by overlapping spectra dispersed from different slits, with each slit being exposed to radiation from a different portion of an extended astrophysical object. We use a compressed sensing method to robustly retrieve the different components. This method can be adopted for a variety of spectrometer configurations, including single-slit, multi-slit (e.g., the proposed MUlti-slit Solar Explorer mission), and slot spectrometers (which produce overlappograms). | |
dc.format.extent | 9 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysical Journal | en |
dc.rights | Copyright © 2019. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. | en |
dc.subject | Instrumentation: spectrographs | en |
dc.subject | Line: profiles | en |
dc.subject | Methods: observational | en |
dc.subject | Sun: corona | en |
dc.subject | Techniques: imaging spectroscopy | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | 3rd-DAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | Multi-component decomposition of astronomical spectra by compressed sensing | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. Applied Mathematics | en |
dc.identifier.doi | https://doi.org/10.3847/1538-4357/ab263d | |
dc.description.status | Peer reviewed | en |
dc.identifier.url | http://adsabs.harvard.edu/abs/2019arXiv190203890C | en |
dc.identifier.grantnumber | ST/R004285/1 | en |
This item appears in the following Collection(s)
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.