The ISO (Infrared Space Observatory) Long Wavelength Spectrometer (LWS) uses an array of ten doped Ge photoconductors to cover the wavelength range 45 to 200 micrometers. Under the low background conditions appropriate to the LWS, these devices are know to exhibit a number of memory effects, such as spontaneous spiking at high signal levels and slow relaxation after a step change in illumination. This type of nonlinear behavior can cause degradation of the excellent instantaneous sensitivity of the LWS detectors, and other calibration problems. These effects were studied and the implications of operation and calibration of the LWS are considered
The detector of the Long Wavelength channel of the ISOCAM camera on-board the Infrared Space Observ...
The ISO (Infrared Space Observatory) Short Wavelength Spectrometer (SWS) employs four different type...
A large number of low background photodetectors were used on the ISO satellite, covering wavelengths...
The ISO (Infrared Space Observatory) Long Wavelength Spectrometer (LWS) uses an array of ten doped G...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The ISO (Infrared Space Observatory) Long Wavelength Spectrometer (LWS) uses an array of ten doped g...
Doped germanium photoconductors are the most sensitive detectors for astronomy in the wavelength ran...
The Long-Wavelength Spectrometer (LWS) onboard the Infrared Space Observatory (ISO) covers the 43197...
The aim of the long wavelength spectrometer (LWS) of the Infrared Space Observatory is to perform sp...
The configuration of the detectors in the Long Wavelength Spectrometer (LWS) flown on the Infrared S...
The wavelength and flux calibration, and the in-orbit performance of the Infrared Space Observatory ...
The detector of the Long Wavelength channel of the ISOCAM camera on-board the Infrared Space Observ...
The ISO (Infrared Space Observatory) Short Wavelength Spectrometer (SWS) employs four different type...
A large number of low background photodetectors were used on the ISO satellite, covering wavelengths...
The ISO (Infrared Space Observatory) Long Wavelength Spectrometer (LWS) uses an array of ten doped G...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The ISO (Infrared Space Observatory) Long Wavelength Spectrometer (LWS) uses an array of ten doped g...
Doped germanium photoconductors are the most sensitive detectors for astronomy in the wavelength ran...
The Long-Wavelength Spectrometer (LWS) onboard the Infrared Space Observatory (ISO) covers the 43197...
The aim of the long wavelength spectrometer (LWS) of the Infrared Space Observatory is to perform sp...
The configuration of the detectors in the Long Wavelength Spectrometer (LWS) flown on the Infrared S...
The wavelength and flux calibration, and the in-orbit performance of the Infrared Space Observatory ...
The detector of the Long Wavelength channel of the ISOCAM camera on-board the Infrared Space Observ...
The ISO (Infrared Space Observatory) Short Wavelength Spectrometer (SWS) employs four different type...
A large number of low background photodetectors were used on the ISO satellite, covering wavelengths...