R.J. Harris
Photonic spatial reformatting of stellar light for diffraction-limited spectroscopy
Harris, R.J.; MacLachlan, D.G.; Choudhury, D.; Morris, T.J.; Gendron, E.; Basden, A.G.; Brown, G.; Allington-Smith, J.R.; Thomson, R.R.
Authors
D.G. MacLachlan
D. Choudhury
Professor Timothy Morris t.j.morris@durham.ac.uk
Professor
E. Gendron
A.G. Basden
G. Brown
J.R. Allington-Smith
R.R. Thomson
Abstract
The spectral resolution of a dispersive spectrograph is dependent on the width of the entrance slit. This means that astronomical spectrographs trade-off throughput with spectral resolving power. Recently, optical guided-wave transitions known as photonic lanterns have been proposed to circumvent this trade-off, by enabling the efficient reformatting of multimode light into a pseudo-slit which is highly multimode in one axis, but diffraction-limited in the other. Here, we demonstrate the successful reformatting of a telescope point spread function into such a slit using a three-dimensional integrated optical waveguide device, which we name the photonic dicer. Using the CANARY adaptive optics (AO) demonstrator on the William Herschel Telescope, and light centred at 1530 nm with a 160 nm full width at half-maximum, the device shows a transmission of between 10 and 20 per cent depending upon the type of AO correction applied. Most of the loss is due to the overfilling of the input aperture in poor and moderate seeing. Taking this into account, the photonic device itself has a transmission of 57 ± 4 per cent. We show how a fully-optimized device can be used with AO to provide efficient spectroscopy at high spectral resolution.
Citation
Harris, R., MacLachlan, D., Choudhury, D., Morris, T., Gendron, E., Basden, A., …Thomson, R. (2015). Photonic spatial reformatting of stellar light for diffraction-limited spectroscopy. Monthly Notices of the Royal Astronomical Society, 450(1), 428-434. https://doi.org/10.1093/mnras/stv410
Journal Article Type | Article |
---|---|
Acceptance Date | Feb 20, 2015 |
Online Publication Date | Apr 16, 2015 |
Publication Date | Jun 11, 2015 |
Deposit Date | Nov 29, 2016 |
Publicly Available Date | Dec 14, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 450 |
Issue | 1 |
Pages | 428-434 |
DOI | https://doi.org/10.1093/mnras/stv410 |
Public URL | https://durham-repository.worktribe.com/output/1392062 |
Related Public URLs | http://arxiv.org/pdf/1402.2547 |
Files
Published Journal Article
(1.8 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2015 The Authors. Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved.
You might also like
Adaptive optics telemetry standard: Design and specification of a novel data exchange format
(2024)
Journal Article
On-sky results for the integrated microlens ring tip-tilt sensor
(2021)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search