JWST science instrument pupil alignment measurements
NASA's James Webb Space Telescope (JWST) is a 6.5m diameter, segmented, deployable telescope for cryogenic IR space astronomy (similar to 40K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contain...
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ndltd-arizona.edu-oai-arizona.openrepository.com-10150-6225342017-02-15T03:00:32Z JWST science instrument pupil alignment measurements Kubalak, Dave Sullivan, Joe Ohl, Ray Antonille, Scott Beaton, Alexander Coulter, Phillip Hartig, George Kelly, Doug Lee, David Maszkiewicz, Michael Schweiger, Paul Telfer, Randal Te Plate, Maurice Wells, Martyn Univ Arizona NASA Goddard Space Flight Ctr. (United States) Ball Aerospace & Technologies Corp. (United States) NASA Goddard Space Flight Ctr. (United States) NASA Goddard Space Flight Ctr. (United States) COM DEV International Ltd. (Canada) NASA Goddard Space Flight Ctr. (United States) Space Telescope Science Institute (United States) The Univ. of Arizona (United States) UK Astronomy Technology Ctr. (United Kingdom) Canadian Space Agency (Canada) Lockheed Martin Space Systems Co. (United States) Space Telescope Science Institute (United States) European Space Agency (Netherlands) UK Astronomy Technology Ctr. (United Kingdom) JWST ISIM pupil alignment pupil pupil shear testing verification NASA's James Webb Space Telescope (JWST) is a 6.5m diameter, segmented, deployable telescope for cryogenic IR space astronomy (similar to 40K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SI), including a guider. OSIM is a full field, cryogenic, optical simulator of the JWST OTE. It is the "Master Tool" for verifying the cryogenic alignment and optical performance of ISIM by providing simulated point source/star images to each of the four Science Instruments in ISIM. Included in OSIM is a Pupil Imaging Module (PIM) - a large format CCD used for measuring pupil alignment. Located at a virtual stop location within OSIM, the PIM records superimposed shadow images of pupil alignment reference (PAR) targets located in the OSIM and SI pupils. The OSIM Pupil Imaging Module was described by Brent Bos, et al, at SPIE in 2011 prior to ISIM testing. We have recently completed the third and final ISIM cryogenic performance verification test before ISIM was integrated with the OTE. In this paper, we describe PIM implementation, performance, and measurement results. 2016-09-27 Article Dave Kubalak ; Joe Sullivan ; Ray Ohl ; Scott Antonille ; Alexander Beaton ; Phillip Coulter ; George Hartig ; Doug Kelly ; David Lee ; Michael Maszkiewicz ; Paul Schweiger ; Randal Telfer ; Maurice Te Plate and Martyn Wells " JWST science instrument pupil alignment measurements ", Proc. SPIE 9951, Optical System Alignment, Tolerancing, and Verification X, 99510D (September 27, 2016); doi:10.1117/12.2238830; http://dx.doi.org/10.1117/12.2238830 0277-786X 10.1117/12.2238830 http://hdl.handle.net/10150/622534 http://arizona.openrepository.com/arizona/handle/10150/622534 Optical System Alignment, Tolerancing, and Verification X en http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2238830 © 2016 SPIE SPIE-INT SOC OPTICAL ENGINEERING |
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JWST ISIM pupil alignment pupil pupil shear testing verification |
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JWST ISIM pupil alignment pupil pupil shear testing verification Kubalak, Dave Sullivan, Joe Ohl, Ray Antonille, Scott Beaton, Alexander Coulter, Phillip Hartig, George Kelly, Doug Lee, David Maszkiewicz, Michael Schweiger, Paul Telfer, Randal Te Plate, Maurice Wells, Martyn JWST science instrument pupil alignment measurements |
description |
NASA's James Webb Space Telescope (JWST) is a 6.5m diameter, segmented, deployable telescope for cryogenic IR space astronomy (similar to 40K). The JWST Observatory architecture includes the Optical Telescope Element (OTE) and the Integrated Science Instrument Module (ISIM) element that contains four science instruments (SI), including a guider. OSIM is a full field, cryogenic, optical simulator of the JWST OTE. It is the "Master Tool" for verifying the cryogenic alignment and optical performance of ISIM by providing simulated point source/star images to each of the four Science Instruments in ISIM. Included in OSIM is a Pupil Imaging Module (PIM) - a large format CCD used for measuring pupil alignment. Located at a virtual stop location within OSIM, the PIM records superimposed shadow images of pupil alignment reference (PAR) targets located in the OSIM and SI pupils. The OSIM Pupil Imaging Module was described by Brent Bos, et al, at SPIE in 2011 prior to ISIM testing. We have recently completed the third and final ISIM cryogenic performance verification test before ISIM was integrated with the OTE. In this paper, we describe PIM implementation, performance, and measurement results. |
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Univ Arizona |
author_facet |
Univ Arizona Kubalak, Dave Sullivan, Joe Ohl, Ray Antonille, Scott Beaton, Alexander Coulter, Phillip Hartig, George Kelly, Doug Lee, David Maszkiewicz, Michael Schweiger, Paul Telfer, Randal Te Plate, Maurice Wells, Martyn |
author |
Kubalak, Dave Sullivan, Joe Ohl, Ray Antonille, Scott Beaton, Alexander Coulter, Phillip Hartig, George Kelly, Doug Lee, David Maszkiewicz, Michael Schweiger, Paul Telfer, Randal Te Plate, Maurice Wells, Martyn |
author_sort |
Kubalak, Dave |
title |
JWST science instrument pupil alignment measurements |
title_short |
JWST science instrument pupil alignment measurements |
title_full |
JWST science instrument pupil alignment measurements |
title_fullStr |
JWST science instrument pupil alignment measurements |
title_full_unstemmed |
JWST science instrument pupil alignment measurements |
title_sort |
jwst science instrument pupil alignment measurements |
publisher |
SPIE-INT SOC OPTICAL ENGINEERING |
publishDate |
2016 |
url |
Dave Kubalak ; Joe Sullivan ; Ray Ohl ; Scott Antonille ; Alexander Beaton ; Phillip Coulter ; George Hartig ; Doug Kelly ; David Lee ; Michael Maszkiewicz ; Paul Schweiger ; Randal Telfer ; Maurice Te Plate and Martyn Wells " JWST science instrument pupil alignment measurements ", Proc. SPIE 9951, Optical System Alignment, Tolerancing, and Verification X, 99510D (September 27, 2016); doi:10.1117/12.2238830; http://dx.doi.org/10.1117/12.2238830 http://hdl.handle.net/10150/622534 http://arizona.openrepository.com/arizona/handle/10150/622534 |
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