Pupil functions for Keck-style (left panel) and HDRT (right panel

HDRT-WFM layout, the eeective focal length is EFL=-41838mm resulting in

Roy COULTER, New Jersey Institute of Technology, New Jersey, NJIT, Department of Physics

r_IPgeocode/CRANpkgMaintainers.csv at master · cengel/r_IPgeocode · GitHub

Image Classification in the Dark Using Quanta Image Sensors

14730_TalkFlyer.Pickering.3-5-24.rev.1709830562.png

14396_Science_Communication_Workshop.rev.1707921925.png

D. L. Mickey's research works Honolulu University, Honolulu and other places

Chesapeake Magazine Summer 2016

Pupil functions for Keck-style (left panel) and HDRT (right panel)

4-H Club Projects - Steele County Free Fair

Image Classification in the Dark Using Quanta Image Sensors

Left panel: Model of the Keck II Telescope pupil used for the

Past Events, Carney Institute for Brain Science

D. L. Mickey's research works Honolulu University, Honolulu and other places