A far infrared monochromator of Czerny- Turner type has been devised which has an output optical system comprising two small spherical mirrors to obtain non-astigmatic image. The far infrared monochromator covers both 50-120 um and 100-240 um wavelengths ranges and can be used to measure spectral response of stressed Ge:Ga photoconductors having response up to 200 um, which we have fabricated to apply them to far infrared astronomical observations by balloons and by sattelites. Experimental performance of the stressed Ge:Ga photoconductors under low photon fluxes conditions also will be given
Contains fulltext : mmubn000001_026603683.pdf (publisher's version ) (Open Access)...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
We have developed an imaging Fourier transform spectrometer (FTS) for space-based far-infrared astro...
A concept of a sensitive cryogenically cooled far infrared detector is presented. The device consist...
Extrinsic photoconductors are favored detectors for infrared photon detection in astronomical instru...
The authors report on Ge:Ga and Ge:Sb photoconductor materials and detectors that are under developm...
The design and construction of a novel heterodyne spectrometer for airborne astronomy in the 50 µm -...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The optimization of far infrared photoconductive detectors for use in balloon-borne or satellite-bor...
Author Institution: Department of Chemistry, Purdue UniversityA small, versatile, infrared spectrome...
$^{\ast}$ Supported in part through a grant from the National Science Foundation and a contract betw...
A portable wavelength tunable light source to calibrate the spectral responsivities of detectors in ...
Efficient long wavelength broadband and spectral imaging on SOFIA and in future FIR/sub-mm missions ...
Highly compensated Ge:Ga photoconductors have been fabricated and evaluated for high bandwidth heter...
The goals of the proposed work were to determine if final steady state current values for Ge:Ga phot...
Contains fulltext : mmubn000001_026603683.pdf (publisher's version ) (Open Access)...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
We have developed an imaging Fourier transform spectrometer (FTS) for space-based far-infrared astro...
A concept of a sensitive cryogenically cooled far infrared detector is presented. The device consist...
Extrinsic photoconductors are favored detectors for infrared photon detection in astronomical instru...
The authors report on Ge:Ga and Ge:Sb photoconductor materials and detectors that are under developm...
The design and construction of a novel heterodyne spectrometer for airborne astronomy in the 50 µm -...
The Long Wavelength Spectrometer (LWS), part of the Infrared Space Observatory (ISO), uses an array ...
The optimization of far infrared photoconductive detectors for use in balloon-borne or satellite-bor...
Author Institution: Department of Chemistry, Purdue UniversityA small, versatile, infrared spectrome...
$^{\ast}$ Supported in part through a grant from the National Science Foundation and a contract betw...
A portable wavelength tunable light source to calibrate the spectral responsivities of detectors in ...
Efficient long wavelength broadband and spectral imaging on SOFIA and in future FIR/sub-mm missions ...
Highly compensated Ge:Ga photoconductors have been fabricated and evaluated for high bandwidth heter...
The goals of the proposed work were to determine if final steady state current values for Ge:Ga phot...
Contains fulltext : mmubn000001_026603683.pdf (publisher's version ) (Open Access)...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
We have developed an imaging Fourier transform spectrometer (FTS) for space-based far-infrared astro...