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DC Field | Value | Language |
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dc.contributor.author | Mary Angelie Alagao | en_US |
dc.contributor.author | Christophe Buisset | en_US |
dc.contributor.author | Adithep Kawinkij | en_US |
dc.contributor.author | Apirat Prasit | en_US |
dc.contributor.author | Thierry Lepine | en_US |
dc.contributor.author | Yves Rabbia | en_US |
dc.contributor.author | Anthony Berdeu | en_US |
dc.contributor.author | Eric Thiebaut | en_US |
dc.contributor.author | Maud Langlois | en_US |
dc.contributor.author | Michel Tallon | en_US |
dc.contributor.author | Supachai Awiphan | en_US |
dc.contributor.author | Eugene Semenko | en_US |
dc.contributor.author | Pakakaew Rittipruk | en_US |
dc.contributor.author | David Mkrtichian | en_US |
dc.contributor.author | Saran Poshyachinda | en_US |
dc.contributor.author | Boonrucksar Soonthornthum | en_US |
dc.date.accessioned | 2022-10-16T07:08:26Z | - |
dc.date.available | 2022-10-16T07:08:26Z | - |
dc.date.issued | 2021-01-01 | en_US |
dc.identifier.issn | 1996756X | en_US |
dc.identifier.issn | 0277786X | en_US |
dc.identifier.other | 2-s2.0-85116045755 | en_US |
dc.identifier.other | 10.1117/12.2599626 | en_US |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85116045755&origin=inward | en_US |
dc.identifier.uri | http://cmuir.cmu.ac.th/jspui/handle/6653943832/76327 | - |
dc.description.abstract | The Center for Optics and Photonics of the National Astronomical Research Institute of Thailand, together with the Institut d’Optique Graduate School and the Centre de Recherche Astrohpysique de Lyon (CRAL), is currently developing the Evanescent Wave Coronagraph (EvWaCo). The coronagraph relies on the tunneling effect to produce a fully achromatic focal plane mask (FPM) with an adjustable size. The full instrument comprises a coronagraph and adaptive optics system that will be mounted on the Thai National Telescope and is specified to reach a raw contrast of 10−4 at an inner working angle of 3 Airy radii. The coronagraph will be used to perform high contrast observations of stellar systems during on-sky observations over the spectral domain [600 nm, 900 nm]. In this paper, we present the opto-mechanical design of the EvWaCo prototype and the performance measured in laboratory conditions. We also discuss the potential applications for space-based observations and the development plan under this project in the next five years. | en_US |
dc.subject | Computer Science | en_US |
dc.subject | Engineering | en_US |
dc.subject | Materials Science | en_US |
dc.subject | Mathematics | en_US |
dc.subject | Physics and Astronomy | en_US |
dc.title | Design, performance, and potential scientific applications of the evanescent wave coronagraph with an adjustable inner working angle | en_US |
dc.type | Conference Proceeding | en_US |
article.title.sourcetitle | Proceedings of SPIE - The International Society for Optical Engineering | en_US |
article.volume | 11852 | en_US |
article.stream.affiliations | Institut d'Optique Graduate School | en_US |
article.stream.affiliations | Chulalongkorn University | en_US |
article.stream.affiliations | Observatoire de la Côte d'Azur | en_US |
article.stream.affiliations | CNRS Centre National de la Recherche Scientifique | en_US |
article.stream.affiliations | Chiang Mai University | en_US |
article.stream.affiliations | National Astronomical Research Institute of Thailand | en_US |
Appears in Collections: | CMUL: Journal Articles |
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