Back to Search
Start Over
Focal Plane Alignment and Detector Characterization for the Subaru Prime Focus Spectrograph
- Publication Year :
- 2014
- Publisher :
- arXiv, 2014.
-
Abstract
- We describe the infrastructure being developed to align and characterize the detectors for the Subaru Measurement of Images and Redshifts (SuMIRe) Prime Focus Spectrograph (PFS). PFS will employ four three-channel spectrographs with an operating wavelength range of 3800 $\AA$ to 12600 $\AA$. Each spectrograph will be comprised of two visible channels and one near infrared (NIR) channel, where each channel will use a separate Schmidt camera to image the captured spectra onto their respective detectors. In the visible channels, Hamamatsu 2k x 4k CCDs will be mounted in pairs to create a single 4k x 4k detector, while the NIR channel will use a single Teledyne 4k x 4k H4RG HgCdTe device.<br />Comment: 16 pages, 27 figures, SPIE ATI Montreal 2014
- Subjects :
- Physics
Depth of focus
Physics::Instrumentation and Detectors
business.industry
Flatness (systems theory)
Detector
Astrophysics::Instrumentation and Methods for Astrophysics
FOS: Physical sciences
Coplanarity
chemistry.chemical_compound
Optics
Cardinal point
chemistry
Mercury cadmium telluride
Astrophysics - Instrumentation and Methods for Astrophysics
business
Subaru Telescope
Spectrograph
Instrumentation and Methods for Astrophysics (astro-ph.IM)
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....aa7deb1e4d5a1a7d3a0f506f9f7440e7
- Full Text :
- https://doi.org/10.48550/arxiv.1408.2822