Vievard, S. and Ahn, Kyohoon and Arriola, Alexander and Barjot, Kevin and Cvetojevic, Nick and Deo, Vincent and Duchène, G. and Gretzinger, Thomas and Gross, Simon and Guyon, Olivier and Huby, Elsa and Jovanovic, N. and Kotani, Takayuki and Lacour, Sylvestre and Lagadec, Tiphaine and Lallement, Manon and Lapeyrere, Vincent and Lozi, Julien and Marchis, Franck and Martin, Guillermo and Martinod, Marc-Antoine and Norris, Barnaby and Perrin, Guy and Rouan, Daniel and Skaf, Nour and Tuthill, Peter and Withford, Michael (2021) Very high resolution spectro-interferometry with wavefront sensing capabilities on Subaru/SCExAO using photonics. In: Techniques and Instrumentation for Detection of Exoplanets X. Proceedings of SPIE. No.11823. Society of Photo-Optical Instrumentation Engineers , Bellingham, WA, Art. No. 118230C. ISBN 9781510644847. https://resolver.caltech.edu/CaltechAUTHORS:20220621-36508000
![[img]](https://authors.library.caltech.edu/style/images/fileicons/application_pdf.png) |
PDF
- Published Version
See Usage Policy. 11MB |
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20220621-36508000
Abstract
Post Extreme Adaptive-Optics (ExAO) spectro-interferometers design allows high contrast imaging with an inner working angle down to half the theoretical angular resolution of the telescope. This regime, out of reach for conventional ExAO imaging systems, is obtained thanks to the interferometric recombination of multiple sub-apertures of a single telescope, using single mode waveguides to remove speckle noise. The SCExAO platform at the Subaru telescope hosts two instruments with such design, coupled with a spectrograph. The FIRST instrument operates in the Visible (600-800nm, R~400) and is based on pupil remapping using single-mode fibers. The GLINT instrument works in the NIR (1450-1650nm, R~160) and is based on nulling interferometry. We present here how these photonic instruments have the unique capability to simultaneously do high contrast imaging and be included in the wavefront sensing architecture of SCExAO.
| Item Type: | Book Section | ||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Related URLs: |
| ||||||||||||||||||||||||||||||
| ORCID: |
| ||||||||||||||||||||||||||||||
| Additional Information: | © 2021 Society of Photo-Optical Instrumentation Engineers (SPIE). The development of FIRST was supported by Centre National de la Recherche Scientifique CNRS (Grant ERC LITHIUM - STG - 639248). The development of SCExAO was supported by the Japan Society for the Promotion of Science (Grant-in-Aid for Research #23340051, #26220704, #23103002, #19H00703 & #19H00695), the Astrobiology Center of the National Institutes of Natural Sciences, Japan, the Mt Cuba Foundation and the director’s contingency fund at Subaru Telescope. GLINT work was supported by the Australian Research Council Discovery Project DP180103413. Critical fabrication for GLINT was performed in part at the OptoFab node of the Australian National Fabrication Facility utilising Commonwealth as well as NSW state government funding. S. Gross acknowledges funding through a Macquarie University Research Fellowship (9201300682) and the Australian Research Council Discovery Program (DE160100714). N. Cvetojevic acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement CoG - 683029). The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. | ||||||||||||||||||||||||||||||
| Funders: |
| ||||||||||||||||||||||||||||||
| Subject Keywords: | Interferometry, Pupil remapping, Single-mode fibers, photonics, high contrast imaging, high angular resolution, wavefront sensing, island effect | ||||||||||||||||||||||||||||||
| Series Name: | Proceedings of SPIE | ||||||||||||||||||||||||||||||
| Issue or Number: | 11823 | ||||||||||||||||||||||||||||||
| DOI: | 10.1117/12.2594840 | ||||||||||||||||||||||||||||||
| Record Number: | CaltechAUTHORS:20220621-36508000 | ||||||||||||||||||||||||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20220621-36508000 | ||||||||||||||||||||||||||||||
| Official Citation: | S. Vievard, K. Ahn, A. Arriola, K. Barjot, N. Cvetojevic, V. Deo, T. Gretzinger, S. Gross, O. Guyon, E. Huby, N. Jovanovic, T. Kotani, S. Lacour, T. Lagadec, M. Lallement, V. Lapeyrere, J. Lozi, F. Marchis, G. Martin, M.-A. Martinod, B. Norris, G. Perrin, D. Rouan, N. Skaf, P. Tuthill, M. Withford, and G. Duchêne "Very high resolution spectro-interferometry with wavefront sensing capabilities on Subaru/SCExAO using photonics", Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 118230C (1 September 2021); https://doi.org/10.1117/12.2594840 | ||||||||||||||||||||||||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||||||||||||||||||||||||||
| ID Code: | 115209 | ||||||||||||||||||||||||||||||
| Collection: | CaltechAUTHORS | ||||||||||||||||||||||||||||||
| Deposited By: | Tony Diaz | ||||||||||||||||||||||||||||||
| Deposited On: | 21 Jun 2022 18:30 | ||||||||||||||||||||||||||||||
| Last Modified: | 21 Jun 2022 18:30 |
Repository Staff Only: item control page
