The Infrared Imaging Spectrograph (IRIS) for TMT: The ADC optical design
| dc.contributor.author | Phillips, Andrew C | |
| dc.contributor.author | Suzuki, Ryuji | |
| dc.contributor.author | Larkin, J | |
| dc.contributor.author | Moore, Anna | |
| dc.contributor.author | Hayano, Yutaka | |
| dc.contributor.author | Tsuzuki, Toshihiro | |
| dc.contributor.author | Wright, Shelley A | |
| dc.coverage.spatial | Edinburgh, United Kingdom | |
| dc.date.accessioned | 2018-11-30T01:19:38Z | |
| dc.date.available | 2018-11-30T01:19:38Z | |
| dc.date.created | June 26-30 2016 | |
| dc.date.issued | 2016 | |
| dc.date.updated | 2018-11-29T08:21:45Z | |
| dc.description.abstract | We present the current optical design for the IRIS Atmospheric Dispersion Corrector (ADC). The ADC is designed for residual dispersions less than ~1 mas across a given passband at elevations of 25 degrees. Since the last report, the area of the IRIS Imager has increased by a factor of four, and the pupil size has increased from 75 to 90mm, both of which contribute to challenges with the design. Several considerations have led to the current design: residual dispersion, amount of introduced distortion, glass transmission, glass availability, and pupil displacement. In particular, it was found that there are significant distortions that appear (two different components) that can lead to image blur over long exposures. Also, pupil displacement increases the wave front error at the imager focus. We discuss these considerations, discuss the compromises, and present the final design choice and expected performance | |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.isbn | 9781510601956 | |
| dc.identifier.uri | http://hdl.handle.net/1885/154138 | |
| dc.publisher | SPIE - The International Society for Optical Engineering | |
| dc.relation.ispartofseries | Ground-Based and Airborne Instrumentation for Astronomy VI | |
| dc.source | Proceedings of SPIE - The International Society for Optical Engineering | |
| dc.title | The Infrared Imaging Spectrograph (IRIS) for TMT: The ADC optical design | |
| dc.type | Conference paper | |
| dcterms.accessRights | Open Access | en_AU |
| local.contributor.affiliation | Phillips, Andrew C, University of California Observatories | |
| local.contributor.affiliation | Suzuki, Ryuji, National Astronomical Observatory of Japan | |
| local.contributor.affiliation | Larkin, J, University of California | |
| local.contributor.affiliation | Moore, Anna, College of Science, ANU | |
| local.contributor.affiliation | Hayano, Yutaka, National Astronomical Observatory of Japan | |
| local.contributor.affiliation | Tsuzuki, Toshihiro, National Astronomical Observatory of Japan | |
| local.contributor.affiliation | Wright, Shelley A, University of California | |
| local.contributor.authoruid | Moore, Anna, u1036159 | |
| local.description.notes | Imported from ARIES | |
| local.description.refereed | Yes | |
| local.identifier.absfor | 020102 - Astronomical and Space Instrumentation | |
| local.identifier.ariespublication | a383154xPUB6752 | |
| local.identifier.doi | 10.1117/12.2232952 | |
| local.identifier.scopusID | 2-s2.0-85007236216 | |
| local.type.status | Published Version |
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