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dc.contributor.authorJones, Hugh
dc.contributor.authorMartin, Bill
dc.contributor.authorAnglada, Guillem
dc.contributor.authorErrmann, Ronny
dc.contributor.authorLondon, Queen Mary University
dc.contributor.authorChoochalerm, Piyamas
dc.contributor.authorBoonsri, Chantira
dc.date.accessioned2021-03-16T00:08:15Z
dc.date.available2021-03-16T00:08:15Z
dc.date.issued2021-02-01
dc.identifier.citationJones , H , Martin , B , Anglada , G , Errmann , R , London , Q M U , Choochalerm , P & Boonsri , C 2021 , ' A small actively-controlled high-resolution spectrograph based on off-the-shelf components ' , Publications of the Astronomical Society of the Pacific , vol. 133 , no. 1020 , 025001 . https://doi.org/10.1088/1538-3873/abc7ee
dc.identifier.issn0004-6280
dc.identifier.otherORCID: /0000-0003-0757-6689/work/90910042
dc.identifier.urihttp://hdl.handle.net/2299/24112
dc.description© 2021. The Astronomical Society of the Pacific. The original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. https://creativecommons.org/licenses/by/3.0/
dc.description.abstractWe present the design and testing of a prototype in-plane echelle spectrograph based on an actively controlled fiber-fed double-pass design. This system aims to be small and efficient with the minimum number of optical surfaces—currently a collimator/camera lens, cross-dispersing prism, grating and a reflector to send light to the detector. It is built from catalog optical components and has dimensions of approximately 20 × 30 cm. It works in the optical regime with a resolution of >70,000. The spectrograph is fed by a bifurcated fiber with one fiber to a telescope and the other used to provide simultaneous Thorium Argon light illumination for wavelength calibration. The positions of the arc lines on the detector are processed in real time and commercial auto-guiding software is used to treat the positions of the arc lines as guide stars. The guiding software sends any required adjustments to mechanical piezo-electric actuators which move the mirror sending light to the camera removing any drift in the position of the arc lines. The current configuration using an sCMOS detector provides a precision of 3.5 milli-pixels equivalent to 4 ms −1 in a standard laboratory environment.en
dc.format.extent13
dc.format.extent1808743
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacific
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.titleA small actively-controlled high-resolution spectrograph based on off-the-shelf componentsen
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionCentre of Data Innovation Research
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionCentre for Atmospheric and Climate Physics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85100885559&partnerID=8YFLogxK
rioxxterms.versionofrecord10.1088/1538-3873/abc7ee
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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