An infrared imaging technique based on the nonlinear interaction known as upconversion was used to obtain images of several astronomical objects in the 10 micrometer spectral region, and to demonstrate quantitatively the sharper images allowed for wavelengths beyond the visible region. The deleterious effects of atmospheric inhomogeneities on telescope resolution were studied in the infrared region using the technique developed. The low quantum efficiency of the device employed severely limited its usefulness as an astronomical detector
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...
We study the sensitivities of space infrared interferometers. We formulate the signal-to-noise ratio...
The experimental development and evaluation of infrared vidicons for use in solving high precision h...
The basic theory of upconversion is presented, along with a brief historical summary of upconversion...
The performance of an upconversion system is examined for observation of astronomical sources in the...
International audienceHigh resolution stellar interferometers are very powerful efficient instrument...
Far-infrared continuum studies from the Kuiper Airborne Observatory are described that are designed ...
Infrared interferometry promises to be a useful astrometric technique. Preliminary measurements of t...
International audienceThis paper demonstrates the use of a nonlinear upconversion process to observe...
Infrared detector arrays are becoming increasingly available to the astronomy community, with a numb...
International audienceThe Astronomical Light Optical Hybrid Analysis (ALOHA) project investigates th...
Observing in the infrared (IR) part of the electromagnetic spectrum is now an established tool of a...
Contains research objectives and summary of research on two research projects and a report on one re...
Up-conversion sensing based on optical heterodyning of an IR (infrared) image with a local oscillato...
International audienceIn the context of new generation instruments for astronomical interferometer, ...
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...
We study the sensitivities of space infrared interferometers. We formulate the signal-to-noise ratio...
The experimental development and evaluation of infrared vidicons for use in solving high precision h...
The basic theory of upconversion is presented, along with a brief historical summary of upconversion...
The performance of an upconversion system is examined for observation of astronomical sources in the...
International audienceHigh resolution stellar interferometers are very powerful efficient instrument...
Far-infrared continuum studies from the Kuiper Airborne Observatory are described that are designed ...
Infrared interferometry promises to be a useful astrometric technique. Preliminary measurements of t...
International audienceThis paper demonstrates the use of a nonlinear upconversion process to observe...
Infrared detector arrays are becoming increasingly available to the astronomy community, with a numb...
International audienceThe Astronomical Light Optical Hybrid Analysis (ALOHA) project investigates th...
Observing in the infrared (IR) part of the electromagnetic spectrum is now an established tool of a...
Contains research objectives and summary of research on two research projects and a report on one re...
Up-conversion sensing based on optical heterodyning of an IR (infrared) image with a local oscillato...
International audienceIn the context of new generation instruments for astronomical interferometer, ...
Over the last 10 years infrared astronomy from 2 µm to 1000 µm has blossomed into a major field of o...
We study the sensitivities of space infrared interferometers. We formulate the signal-to-noise ratio...
The experimental development and evaluation of infrared vidicons for use in solving high precision h...