The Symbiotic Relationship Between Infrared Imaging Arrays And A New Type Of Blackbody Simulator

1984 ◽  
Author(s):  
Frederick O. Bartell
Keyword(s):  
Infrared Imaging ◽  
Symbiotic Relationship ◽  
Imaging Arrays ◽  
New Type

High-sensitivity uncooled microcantilever infrared imaging arrays

2006 ◽  
Author(s):  
Scott R. Hunter ◽  
Gregory Maurer ◽  
Lijun Jiang ◽  
Gregory Simelgor
Keyword(s):  
Infrared Imaging ◽  
High Sensitivity ◽  
Imaging Arrays

Infrared imaging arrays using advanced III-V materials and technology

2002 ◽  
Author(s):  
M. Razeghi ◽  
J.D. Kim ◽  
C. Jelen ◽  
S. Slivken ◽  
E. Michel ◽  
...  
Keyword(s):  
Infrared Imaging ◽  
Imaging Arrays

Infrared imaging arrays based on superlattice photodiodes

2008 ◽  
Author(s):  
Cory J. Hill ◽  
Alexander Soibel ◽  
Sam A. Keo ◽  
Jason M. Mumolo ◽  
Sarath D. Gunapala ◽  
...  
Keyword(s):  
Infrared Imaging ◽  
Imaging Arrays

scholarly journals Tracing Molecular Emission in Spiral Galaxies: The Near Infrared Correspondence

1994 ◽  
Vol 140 ◽  
pp. 370-371
Author(s):  
R. L. Hurt ◽  
J. L. Turner ◽  
D. Levine ◽  
K. M. Merrill ◽  
I. Gatley
Keyword(s):  
Large Scale ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Spiral Galaxies ◽  
Molecular Structures ◽  
Optical Observations ◽  
Near Infrared Imaging ◽  
Imaging Arrays ◽  
Molecular Emission ◽  
Infrared Extinction

Near infrared imaging can be a powerful tool in tracing the densest molecular structures in galaxies. The observable molecular emission originates in large molecular cloud complexes which are also subject to significant extinctions caused by the associated dust. It can be difficult to distinguish between regions of moderate and large molecular density with optical observations as both will appear optically thick. Since extinction in the near infrared is only about a tenth of the corresponding visual extinction, multi-band near infrared imaging will trace the regions of the highest optical depths much more effectively. With the advent of large format infrared imaging arrays it is now possible to use infrared extinction maps as a probe of the large scale distribution of molecular emission in extragalactic sources.

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