Paper
12 October 2004 Wide Field Camera 3 optical bench integration, alignment, and test
Joseph Sullivan, George F. Hartig, Mark Martella, Jon Seerveld, Jennifer A. Turner-Valle, Kim I. MacFeely, Stew Willis, Laurie Seide, Greg Moore, Guy Young
Author Affiliations +
Abstract
The Wide Field Camera 3 (WFC3) instrument was designed and built to replace the Hubble Space Telescope (HST) instrument Wide Field and Planetary Camera 2 (WF/PC2) and to provide improved ultra-violet through near infrared imaging capability over the extended HST mission. We describe the optical component integration, alignment, and performance testing of the optical bench assembly.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Joseph Sullivan, George F. Hartig, Mark Martella, Jon Seerveld, Jennifer A. Turner-Valle, Kim I. MacFeely, Stew Willis, Laurie Seide, Greg Moore, and Guy Young "Wide Field Camera 3 optical bench integration, alignment, and test", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.550902
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Cameras

Optical alignment

Optical benches

Infrared telescopes

Hubble Space Telescope

Infrared radiation

Near infrared

Back to Top