Add to ORKGInfrared Computer Generated Holograms (CGHs) were designed, manufactured and used to measure the performance of the grism (grating prism) prototype which includes testing Diffractive Optical Elements (DOE). The grism in the Wide Field Infrared Survey Telescope (WFIRST) will allow the surveying of a large section of the sky to find bright galaxies
The WFIRST Wide-Field Infrared Survey Telescope TMA optical design provides 0.28-sq degrees FOV at 0...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...
Interferometers using computer-generated holograms (CGHs) have become the industry standard to accur...
Interferometers using computer-generated holograms (CGHs) have become the industry standard to accur...
The slitless spectrometer plays an important role in the Wide-Field InfraRed Survey Telescope (WFIRS...
The Wide-Field Infra-Red Survey Telescope (WFIRST) is designed to perform wide-field imaging and sli...
The WFIRST wide field instrument (WFI) includes a slitless spectrometer, which plays an important ro...
We had presented the optical design and early test result of WFIRST grism spectrometer in previous S...
textThe silicon diffractive optics we have been developing over the past 15 years have reached the ...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
An introduction to a series of infrared detector technology workshops is given. The establishment of...
Thesis (Ph. D.)--University of Rochester. The Institute of Optics, 2018.The availability of more aff...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
The WFIRST Wide-Field Infrared Survey Telescope TMA optical design provides 0.28-sq degrees FOV at 0...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...
Interferometers using computer-generated holograms (CGHs) have become the industry standard to accur...
Interferometers using computer-generated holograms (CGHs) have become the industry standard to accur...
The slitless spectrometer plays an important role in the Wide-Field InfraRed Survey Telescope (WFIRS...
The Wide-Field Infra-Red Survey Telescope (WFIRST) is designed to perform wide-field imaging and sli...
The WFIRST wide field instrument (WFI) includes a slitless spectrometer, which plays an important ro...
We had presented the optical design and early test result of WFIRST grism spectrometer in previous S...
textThe silicon diffractive optics we have been developing over the past 15 years have reached the ...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
An introduction to a series of infrared detector technology workshops is given. The establishment of...
Thesis (Ph. D.)--University of Rochester. The Institute of Optics, 2018.The availability of more aff...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imagin...
The WFIRST Wide-Field Infrared Survey Telescope TMA optical design provides 0.28-sq degrees FOV at 0...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...
We present the efficiency of near-infrared reflective ruled diffraction gratings designed for the In...