The JPL deep-well mid-infrared array camera

1994 ◽  
Vol 3 (1-4) ◽  
pp. 277-280 ◽  
Author(s):  
Michael E. Ressler ◽  
Michael W. Werner ◽  
Jeff Van Cleve ◽  
Helen A. Chou
Keyword(s):  
Mid Infrared ◽  
Deep Well ◽  
Array Camera ◽  
Infrared Array

The JPL Deep-Well Mid-Infrared Array Camera

1994 ◽  
pp. 429-432 ◽  
Author(s):  
Michael E. Ressler ◽  
Michael W. Werner ◽  
Jeff Van Cleve ◽  
Helen A. Chou
Keyword(s):  
Mid Infrared ◽  
Deep Well ◽  
Array Camera ◽  
Infrared Array

scholarly journals MIRAC: a mid-infrared array camera for astronomy

1993 ◽  
Author(s):  
William F. Hoffmann ◽  
Giovanni G. Fazio ◽  
Kandiah Shivanandan ◽  
Joseph L. Hora ◽  
Lynne K. Deutsch
Keyword(s):  
Mid Infrared ◽  
Array Camera ◽  
Infrared Array

Astronomical observations with the Mid-Infrared Array Camera, MIRAC

1994 ◽  
Vol 35 (2-3) ◽  
pp. 175-194 ◽  
Author(s):  
William F. Hoffmann ◽  
Giovanni G. Fazio ◽  
Kandiah Shivanandan ◽  
Joseph L. Hora ◽  
Lynne K. Deutsch
Keyword(s):  
Mid Infrared ◽  
Astronomical Observations ◽  
Array Camera ◽  
Infrared Array

scholarly journals MIRAC2: a mid-infrared array camera for astronomy

1998 ◽  
Author(s):  
William F. Hoffmann ◽  
Joseph L. Hora ◽  
Giovanni G. Fazio ◽  
Lynne K. Deutsch ◽  
Aditya Dayal
Keyword(s):  
Mid Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals The Morphology of MID-Infrared UIR Feature Emission in the PPN M 2–9 and IRAS 21282+5050

1993 ◽  
Vol 155 ◽  
pp. 344-344
Author(s):  
L. K. Deutsch ◽  
J. L. Hora ◽  
W. F. Hoffmann ◽  
G. G. Fazio ◽  
K. Shivanandan
Keyword(s):  
Near Infrared ◽  
Infrared Images ◽  
Mid Infrared ◽  
Nicmos 3 ◽  
Array Camera ◽  
Infrared Array

The carbon-rich PPN M 2–9 and IRAS 21282+5050 are known to exhibit UIR feature emission at 7.7, 8.6, and 11.22 μm. The two nebulae have been imaged in the mid-IR with the UA/SAO/NRL Mid-Infrared Array Camera (MIRAC) in bandpasses which include UIR feature emission (8.8 and 11.22 μm). Near-infrared images of the nebulae have also been taken with the NICMOS 3 Hg:Cd:Te array camera at J, H, and K for M 2–9 and at K for IRAS 21282+5050.

scholarly journals The Applicability of a 5–18 μm Array Camera to Solar Imaging

1994 ◽  
Vol 154 ◽  
pp. 595-601
Author(s):  
Daniel Y. Gezari
Keyword(s):  
Narrow Band ◽  
Optical Design ◽  
Operating Conditions ◽  
Camera System ◽  
High Background ◽  
Mid Infrared ◽  
Low Background ◽  
Astronomical Imaging ◽  
Array Camera ◽  
Infrared Array

The anticipated requirements and operating conditions are considered for using a mid-infrared array camera in broad- and narrow-band solar imaging observations. The array camera system was designed for high-background 5–18 μm general astronomical imaging observations. The electronic and optical design of the camera, its photometric characteristics, examples of observational results, and the requirements for imaging in both high- and low-background solar applications are discussed.

scholarly journals KWIC: a widefield mid-infrared array camera/spectrometer for the KAO

1993 ◽  
Author(s):  
Gordon J. Stacey ◽  
Thomas L. Hayward ◽  
Harri M. Latvakoski ◽  
George E. Gull
Keyword(s):  
Mid Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals Near- and Mid-Infrared Imaging of the PN IC 418

1993 ◽  
Vol 155 ◽  
pp. 210-210
Author(s):  
J. L. Hora ◽  
L. K. Deutsch ◽  
W. F. Hoffmann ◽  
G. G. Fazio ◽  
K. Shivanandan
Keyword(s):  
High Resolution ◽  
Planetary Nebula ◽  
Infrared Imaging ◽  
Central Star ◽  
Infrared Images ◽  
Mid Infrared ◽  
Near Ir ◽  
Ir Emission ◽  
Array Camera ◽  
Infrared Array

We present high-resolution near- and mid-infrared images of the planetary nebula IC 418 at 1.2 (J), 1.6 (H), 2.2 (K), 9.8, and 11.7 μm. The near-IR images were obtained with a 64×64 pixel Hg:Cd:Te array camera, and the mid-IR images were obtained using the new 20×64 pixel Mid-Infrared Array Camera (MIRAC). The size of IC 418 in the near-IR is seen to vary with wavelength, being largest at K and smallest at J. Differences in the morphology of the nebula are seen between the J and K images. There is excess near-IR emission in the center of the nebula, after subtracting out the emission from the central star. Faint halo emission is detected at H and K, extending to a total diameter of approximately 40″. The 9.8 μm emission is distributed nonsymmetrically, with the peak in the NE lobe.

Characterization of a megapixel mid-infrared array for high background applications

2008 ◽  
Author(s):  
A. K. Mainzer ◽  
Henry Hogue ◽  
Maryn Stapelbroek ◽  
Dale Molyneux ◽  
John Hong ◽  
...  
Keyword(s):  
High Background ◽  
Mid Infrared ◽  
Infrared Array

scholarly journals Mid-Infrared (4.8–12.4 and 20.0 μm) Imaging of the Galactic Center: Modeling the Dust Emission and Energetics of the Central Parsec

1996 ◽  
Vol 169 ◽  
pp. 231-240 ◽  
Author(s):  
Dan Gezari ◽  
Eli Dwek ◽  
Frank Varosi
Keyword(s):  
Galactic Center ◽  
Dust Emission ◽  
Infrared Emission ◽  
Mid Infrared ◽  
New Model ◽  
Central Engine ◽  
Direct Indication ◽  
Sgr A ◽  
Central Parsec ◽  
Array Camera

We have modeled the mid-infrared emission from the Galactic Center using our array camera images at eight wavelengths. The results suggest that the high infrared luminosity of the region is provided by a cluster of luminous stars. There is no direct indication in the new model results of a very luminous object or “central engine” near Sgr A∗.

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