The development of stressed Ge:Ga detector arrays for far-infrared astronomy from the Kuiper Airborne Observatory (KAO) is discussed. Researchers successfully constructed and used a three channel detector array on five flights from the KAO, and have conducted laboratory tests of a two-dimensional, 25 elements (5x5) detector array. Each element of the three element array performs as well as the researchers' best single channel detector, as do the tested elements of the 25 channel system. Some of the exciting new science possible with far-infrared detector arrays is also discussed
Efficient long wavelength broadband and spectral imaging on SOFIA and in future FIR/sub-mm missions ...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
Infrared detector development and characterization at NASA Langley Research Center will be reviewed....
We are developing two-dimensional 16 x 25 pixel detector arrays of both unstressed and stressed Ge:G...
Two modules of gallium-doped germanium (Ge:Ga) infrared detectors with integrated multiplexing reado...
We are developing two-dimensional 16 x 25 pixel detector arrays of both unstressed and stressed Ge:G...
Seven gallium doped germanium (Ge:Ga) photoconductive infrared detectors were fabricated and mounted...
The performance of two multi-element, multiplexed Ge:Ga linear arrays under low-background condition...
This grant supports the development of a variety of advanced far infrared detection techniques that ...
We have built an array-based camera (FIRARI) for thermal imaging (lambda = 8 to 12 microns). FIRARI ...
The design and construction of a novel heterodyne spectrometer for airborne astronomy in the 50 µm -...
Information is given in viewgraph form. Information is given on the characteristics of stressed Ge:G...
Programs are now underway to develop and demonstrate the detector/array technology needed for the Sp...
The far-IR band is uniquely suited to study the physical conditions in the interstellar medium from ...
The development of doped-germanium detectors which have optimized performance in the 30- to 120-mu m...
Efficient long wavelength broadband and spectral imaging on SOFIA and in future FIR/sub-mm missions ...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
Infrared detector development and characterization at NASA Langley Research Center will be reviewed....
We are developing two-dimensional 16 x 25 pixel detector arrays of both unstressed and stressed Ge:G...
Two modules of gallium-doped germanium (Ge:Ga) infrared detectors with integrated multiplexing reado...
We are developing two-dimensional 16 x 25 pixel detector arrays of both unstressed and stressed Ge:G...
Seven gallium doped germanium (Ge:Ga) photoconductive infrared detectors were fabricated and mounted...
The performance of two multi-element, multiplexed Ge:Ga linear arrays under low-background condition...
This grant supports the development of a variety of advanced far infrared detection techniques that ...
We have built an array-based camera (FIRARI) for thermal imaging (lambda = 8 to 12 microns). FIRARI ...
The design and construction of a novel heterodyne spectrometer for airborne astronomy in the 50 µm -...
Information is given in viewgraph form. Information is given on the characteristics of stressed Ge:G...
Programs are now underway to develop and demonstrate the detector/array technology needed for the Sp...
The far-IR band is uniquely suited to study the physical conditions in the interstellar medium from ...
The development of doped-germanium detectors which have optimized performance in the 30- to 120-mu m...
Efficient long wavelength broadband and spectral imaging on SOFIA and in future FIR/sub-mm missions ...
The SIRTF 32x32 Ge:Ga array is the largest format far-infrared array. It is constructed from a stack...
Infrared detector development and characterization at NASA Langley Research Center will be reviewed....