High resolution near-IR imaging with arrays

Details High resolution near-IR imaging with arrays High resolution near-IR imaging with arrays

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....3..281g&link_type=abstract

Experimental Astronomy, vol. 3, no. 1-4, p. 281-292

Physics

Optics

Adaptive Optics, Galactic Nuclei, Image Enhancement, Image Reconstruction, Image Resolution, Infrared Astronomy, Infrared Imagery, Lunar Occultation, Orion Nebula, Speckle Interferometry, Star Formation, Arrays, Astronomical Photography, Infrared Detectors, Infrared Photography

Scientific paper

The availability of large format, low noise detector arrays has opened the 1 to 20 micrometer region for sub-arcsecond imaging. Using recent results in the investigation of Galactic star forming regions, the Galactic center and external galaxies as exampled, we discuss the various techniques that have been employed. These range from image selection and image sharpening, over speckle techiques and adaptive optics to lunar occultation. These examples demonstrate that sub-arcsecond imaging and spatial interferometry in the near- and mid-infrared has a great future potential.

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