Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

The Infrared Imaging Spectrograph (IRIS) for TMT: The ADC optical design

dc.contributor.authorPhillips, Andrew C
dc.contributor.authorSuzuki, Ryuji
dc.contributor.authorLarkin, J
dc.contributor.authorMoore, Anna
dc.contributor.authorHayano, Yutaka
dc.contributor.authorTsuzuki, Toshihiro
dc.contributor.authorWright, Shelley A
dc.coverage.spatialEdinburgh, United Kingdom
dc.date.accessioned2018-11-30T01:19:38Z
dc.date.available2018-11-30T01:19:38Z
dc.date.createdJune 26-30 2016
dc.date.issued2016
dc.date.updated2018-11-29T08:21:45Z
dc.description.abstractWe 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.mimetypeapplication/pdfen_AU
dc.identifier.isbn9781510601956
dc.identifier.urihttp://hdl.handle.net/1885/154138
dc.publisherSPIE - The International Society for Optical Engineering
dc.relation.ispartofseriesGround-Based and Airborne Instrumentation for Astronomy VI
dc.sourceProceedings of SPIE - The International Society for Optical Engineering
dc.titleThe Infrared Imaging Spectrograph (IRIS) for TMT: The ADC optical design
dc.typeConference paper
dcterms.accessRightsOpen Accessen_AU
local.contributor.affiliationPhillips, Andrew C, University of California Observatories
local.contributor.affiliationSuzuki, Ryuji, National Astronomical Observatory of Japan
local.contributor.affiliationLarkin, J, University of California
local.contributor.affiliationMoore, Anna, College of Science, ANU
local.contributor.affiliationHayano, Yutaka, National Astronomical Observatory of Japan
local.contributor.affiliationTsuzuki, Toshihiro, National Astronomical Observatory of Japan
local.contributor.affiliationWright, Shelley A, University of California
local.contributor.authoruidMoore, Anna, u1036159
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020102 - Astronomical and Space Instrumentation
local.identifier.ariespublicationa383154xPUB6752
local.identifier.doi10.1117/12.2232952
local.identifier.scopusID2-s2.0-85007236216
local.type.statusPublished Version

Downloads

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
01_Phillips_The_Infrared_Imaging_2016.pdf
Size:
494.3 KB
Format:
Adobe Portable Document Format
abcd