SPD/AAS Poster 094.16 27-31 May 2007 Mark Weber Smithsonian Astrophysical Observatory On-Orbit Measurement of the Hinode / XRT Point Response Function.
Noise Budget Development for the LIGO 40 Meter Prototype
Optical-Sensors. Wavelength nm Visible Light Near Infrared 4505506507508509501050 0.250.50 % Reflectance.
Optical-Sensors
On-Orbit Measurement of the Hinode / XRT Point Response Function
