Add to ORKGBefore contemplating an optical interferometer on the Moon one must first review the accomplishments achieved by this technology in scientific applications for astronomy. This will be done by presenting the technical status of optical interferometry as achieved by the Mount Wilson Optical Interferometer. The further developments needed for a future lunar-based interferometer are discussed
International audienceWe outline a concept for OWL-Moon, a 50-100 m aperture telescope located on th...
In this thesis we have looked at the possibility of using a rover for deployment oflunar interferome...
An array of three radio telescopes on the Moon, separated by 100-1000 km, could measure the position...
Optical interferometric arrays are particularly attractive candidates for a manned lunar base. A per...
Resolution is the greatest constraint in observational astronomy. The Earth's atmosphere causes on o...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Slides of the oral presentation given at the CNES Workshop "Lune 2023", Paris, 28-29 March 2023.Opti...
none8siLunar Laser Ranging (LLR), by providing routine measurements of the distance to retro-reflect...
Optical observations on the Earth must cope with the refractive disturbances of the atmosphere, pert...
The accuracy of Earth-based radio astronomy is limited in a fundamental way by the variable delay of...
The Mark III Interferometer on Mt. Wilson, a long-baseline optical interferometer, was in daily oper...
Previous decade has seen an achievement of large interferometricprojects including 8-10m telescopes ...
Gravitational wave astronomy continues to be one of the exploration concepts under consideration in ...
A Laser‐Interferometer Gravitational‐Wave Observatory (LIGO) is planned for operation in the United ...
The system components, performance, and calibration of two element radio interferometer operating at...
International audienceWe outline a concept for OWL-Moon, a 50-100 m aperture telescope located on th...
In this thesis we have looked at the possibility of using a rover for deployment oflunar interferome...
An array of three radio telescopes on the Moon, separated by 100-1000 km, could measure the position...
Optical interferometric arrays are particularly attractive candidates for a manned lunar base. A per...
Resolution is the greatest constraint in observational astronomy. The Earth's atmosphere causes on o...
A new heterodyne interferometer for the atmospheric window from 9 to 12 microns was developed during...
Slides of the oral presentation given at the CNES Workshop "Lune 2023", Paris, 28-29 March 2023.Opti...
none8siLunar Laser Ranging (LLR), by providing routine measurements of the distance to retro-reflect...
Optical observations on the Earth must cope with the refractive disturbances of the atmosphere, pert...
The accuracy of Earth-based radio astronomy is limited in a fundamental way by the variable delay of...
The Mark III Interferometer on Mt. Wilson, a long-baseline optical interferometer, was in daily oper...
Previous decade has seen an achievement of large interferometricprojects including 8-10m telescopes ...
Gravitational wave astronomy continues to be one of the exploration concepts under consideration in ...
A Laser‐Interferometer Gravitational‐Wave Observatory (LIGO) is planned for operation in the United ...
The system components, performance, and calibration of two element radio interferometer operating at...
International audienceWe outline a concept for OWL-Moon, a 50-100 m aperture telescope located on th...
In this thesis we have looked at the possibility of using a rover for deployment oflunar interferome...
An array of three radio telescopes on the Moon, separated by 100-1000 km, could measure the position...