Optical design of the WFIRST-AFTA wide-field instrument | Zendy

Bert A. Pasquale | Zendy; David A. Content | Zendy; J. Kruk | Zendy; David Vaughnn | Zendy; Qian Gong | Zendy; Joseph Howard | Zendy; Alden S. Jurling | Zendy; Lenward Seals | Zendy; Eric Mentzell | Zendy; Nerses V. Armani | Zendy; Gary Kuan | Zendy

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Optical design of the WFIRST-AFTA wide-field instrument

Author(s) -

Bert A. Pasquale,

David A. Content,

J. Kruk,

David Vaughnn,

Qian Gong,

Joseph Howard,

Alden S. Jurling,

Lenward Seals,

Eric Mentzell,

Nerses V. Armani,

Gary Kuan

Publication year - 2014

Publication title -

proceedings of spie, the international society for optical engineering/proceedings of spie

Language(s) - English

Resource type - Conference proceedings

SCImago Journal Rank - 0.192

H-Index - 176

eISSN - 1996-756X

pISSN - 0277-786X

DOI - 10.1117/12.2177847

Subject(s) - spectrograph , telescope , field of view , pixel , field (mathematics) , sampling (signal processing) , remote sensing , optics , physics , scale (ratio) , mode (computer interface) , computer science , geology , astronomy , detector , mathematics , pure mathematics , quantum mechanics , operating system , spectral line

The WFIRST-AFTA Wide-Field Infrared Survey Telescope TMA optical design provides 0.28-sq°FOV Wide Field Channel at 0.11” pixel scale, operating at wavelengths between 0.76-2.0μm, including a spectrograph mode (1.35-1.95μm.) An Integral Field Channel provides a discrete 3”x3.15” field at 0.15” sampling.

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