Add to ORKGInfrared interferometry promises to be a useful astrometric technique. Preliminary measurements of the star alpha Orionis made with a heterodyne interferometer exhibit phase coherence over a period of at least 1000 seconds. The measurements were equivalent to a positional determination of 60 milliarcsecond accuracy every 5 seconds of integration
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Context. Stellar activity causes difficulties in the characterization of transiting exoplanets. In p...
The role of infrared sensing in atmospheric science is discussed and existing infrared measurement t...
Infrared interferometric demonstrations with the University of California, Berkeley's infrared spati...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Ce travail de thèse porte sur l'étude des étoiles jeunes et de leur disque protoplanétaire à l'échel...
Large ground-based telescopes equipped with adaptive optics (AO) systems have ushered in a new era...
The Infrared Spatial Interferometer (ISI) has been conducting mid-IR measurements of red supergiant ...
Imaging of stellar surfaces in visible wavelengths is one of the current frontiers in astronomy. Wit...
Observing in the infrared (IR) part of the electromagnetic spectrum is now an established tool of a...
Using the technique of heterodyne interferometry, measurements were made of the spatial distribution...
This thesis work focuses on the study at the astronomical scale of young stars and their protoplanet...
The Infrared Spatial Interferometer (ISI) is a three telescope interferometer system that operates n...
An infrared imaging technique based on the nonlinear interaction known as upconversion was used to o...
Mars surface and atmosphere characteristics from thermal emission spectrum measurement by infrared i...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Context. Stellar activity causes difficulties in the characterization of transiting exoplanets. In p...
The role of infrared sensing in atmospheric science is discussed and existing infrared measurement t...
Infrared interferometric demonstrations with the University of California, Berkeley's infrared spati...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Ce travail de thèse porte sur l'étude des étoiles jeunes et de leur disque protoplanétaire à l'échel...
Large ground-based telescopes equipped with adaptive optics (AO) systems have ushered in a new era...
The Infrared Spatial Interferometer (ISI) has been conducting mid-IR measurements of red supergiant ...
Imaging of stellar surfaces in visible wavelengths is one of the current frontiers in astronomy. Wit...
Observing in the infrared (IR) part of the electromagnetic spectrum is now an established tool of a...
Using the technique of heterodyne interferometry, measurements were made of the spatial distribution...
This thesis work focuses on the study at the astronomical scale of young stars and their protoplanet...
The Infrared Spatial Interferometer (ISI) is a three telescope interferometer system that operates n...
An infrared imaging technique based on the nonlinear interaction known as upconversion was used to o...
Mars surface and atmosphere characteristics from thermal emission spectrum measurement by infrared i...
The infrared research was divided into two related subjects, observations at wavelengths less than 3...
Context. Stellar activity causes difficulties in the characterization of transiting exoplanets. In p...
The role of infrared sensing in atmospheric science is discussed and existing infrared measurement t...