The Subaru Coronographic Extreme AO (SCExAO) system: Implementation and performances of the Coronographic Low Order WaveFront Sensor
| dc.contributor.author | Vogt, Frédéric P.A. | |
| dc.contributor.author | Martinache, Frantz | |
| dc.contributor.author | Guyon, Olivier | |
| dc.contributor.author | Yoshikawa, Takashi | |
| dc.contributor.author | Yokochi, Kaito | |
| dc.contributor.author | Garrel, Vincent | |
| dc.contributor.author | Matsuo, Taro | |
| dc.coverage.spatial | San Diego, CA | |
| dc.date.accessioned | 2022-02-09T01:05:33Z | |
| dc.date.available | 2022-02-09T01:05:33Z | |
| dc.date.created | June 27-July 2 2010 | |
| dc.date.issued | 2010 | |
| dc.date.updated | 2020-12-13T07:22:11Z | |
| dc.description.abstract | The Subaru Coronagraphic Extreme AO project (SCExAO) is a high performance coronagraph designed to deliver high contrast at small angular separation. For the detection of structures near the diffraction limit, an accurate control of low order wavefront aberrations - tip-tilt and focus - is essential as these aberrations create light leaks that are the source of confusion in the final science image. To address this major difficulty, we have equipped SCExAO with a specially designed Coronagraphic Low Order WaveFront Sensor (CLOWFS) using defocused images of a reflective ring located in the focal plane, that can track tip-tilt errors as small as 10-3?/D. CLOWFS was originally designed to drive actuators in a closed-loop. Here, we show that it can also be used in post-processing to efficiently subtract the tip-tilt induced coronagraphic leaks in the final science image. | en_AU |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.isbn | 9780819482266 | en_AU |
| dc.identifier.issn | 0277-786X | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/259907 | |
| dc.language.iso | en_AU | en_AU |
| dc.provenance | ttps://v2.sherpa.ac.uk/id/publication/27454..."The Published Version can be archived in a Non-Commercial Institutional Repository" from SHERPA/RoMEO site (as at 09/02/2022). Copyright 2010 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. Hinz, P. M., Bouchez, A., Johns, M., Shectman, S., Hart, M., McLeod, B., & McGregor, P. (2010, July). The GMT adaptive optics system. In Adaptive Optics Systems II (Vol. 7736, pp. 139-150). SPIE. | en_AU |
| dc.publisher | SPIE - The International Society for Optical Engineering | en_AU |
| dc.relation.ispartofseries | Adaptive Optics Systems II | en_AU |
| dc.rights | © 2010 SPIE | en_AU |
| dc.source | Proceedings of SPIE - The International Society for Optical Engineering | en_AU |
| dc.subject | CLOWFS | en_AU |
| dc.subject | Coronography | en_AU |
| dc.subject | Extra solar planets | en_AU |
| dc.subject | PIAA | en_AU |
| dc.subject | SCExAO | en_AU |
| dc.subject | Subaru telescopes | en_AU |
| dc.subject | Adaptive optics | en_AU |
| dc.subject | Optical telescopes | en_AU |
| dc.subject | Sensors | en_AU |
| dc.subject | Wavefronts | en_AU |
| dc.subject | Planets Adaptive optics | en_AU |
| dc.subject | CLOWFS | en_AU |
| dc.subject | Coronography | en_AU |
| dc.subject | Extrasolar planets | en_AU |
| dc.subject | PIAA | en_AU |
| dc.subject | SCExAO | en_AU |
| dc.subject | Subaru telescope | en_AU |
| dc.title | The Subaru Coronographic Extreme AO (SCExAO) system: Implementation and performances of the Coronographic Low Order WaveFront Sensor | en_AU |
| dc.type | Conference paper | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.lastpage | 773612-9 | en_AU |
| local.bibliographicCitation.startpage | 773612-1 | en_AU |
| local.contributor.affiliation | Vogt, Frederic, College of Science, ANU | en_AU |
| local.contributor.affiliation | Martinache, Frantz, National Astronomical Observatory of Japan | en_AU |
| local.contributor.affiliation | Guyon, Olivier, National Astronomical Observatory of Japan | en_AU |
| local.contributor.affiliation | Yoshikawa, Takashi, National Astronomical Observatory of Japan | en_AU |
| local.contributor.affiliation | Yokochi, Kaito, National Astronomical Observatory of Japan | en_AU |
| local.contributor.affiliation | Garrel, Vincent, National Astronomical Observatory of Japan | en_AU |
| local.contributor.affiliation | Matsuo, Taro, National Astronomical Observatory of Japan | en_AU |
| local.contributor.authoruid | Vogt, Frederic, u4873788 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.description.refereed | Yes | |
| local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | en_AU |
| local.identifier.ariespublication | U3488905xPUB19101 | en_AU |
| local.identifier.citationvolume | 7736 | en_AU |
| local.identifier.doi | 10.1117/12.857915 | en_AU |
| local.identifier.essn | 1996-756X | en_AU |
| local.identifier.scopusID | 2-s2.0-77957841710 | |
| local.identifier.thomsonID | 000285506400035 | |
| local.publisher.url | http://spie.org | en_AU |
| local.type.status | Published Version | en_AU |
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