The Fizeau Interferometer Testbed (FIT) is a collaborative effort between NASA's Goddard Space Flight Center, the Naval Research Laboratory, Sigma Space Corporation, and the University of Maryland. The testbed will be used to explore the principles of and the requirements for the full, as well as the pathfinder, Stellar Imager mission concept. It has a long term goal of demonstrating closed-loop control of a sparse array of numerous articulated mirrors to keep optical beams in phase and optimize interferometric synthesis imaging. In this paper we present the optical and data acquisition system design of the testbed, and discuss the wavefront sensing and control algorithms to be used. Currently we have completed the initial design and hardwa...
The MIT Adaptive Reconnaissance Golay-3 Optical Satellite (ARGOS) is a wide-angle Fizeau interferome...
This work demonstrates the use of two different observing modes with the twin apertures of the LBT. ...
Future spaceborne interferometric arrays must meet stringent optical performance and tolerance requi...
Abstract. | Space-based interferometers dedicated to wide-angle astrometry would dramatically increa...
Abstract. We present the design of a Fizeau interferometer to be implemented for the GAME mission. T...
Viewgraphs on optical interferometer testbed presented at the MIT Space Research Engineering Center ...
Several new space science mission concepts under development at NASA-GSFC for astronomy are intended...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
LINC-NIRVANA is the near-infrared Fizeau interferometric imaging camera for the Large Binocular Tele...
The StarLight mission aimed to place the first formation flying optical interferometer into space in...
Space-based interferometers dedicated to wide-angle astrometry would dramatically increase the accu...
International audienceThe Fresnel interferometric imager is a new kind of high angular resolution sp...
The light collecting apertures of space telescopes are currently limited in part by the size and wei...
Numerous space interferometry missions are planned for the next decade to verify different enabling ...
The Northrup-Grummann/Ball/Kodak team is building the James Webb Space Telescope (JWST), scheduled f...
The MIT Adaptive Reconnaissance Golay-3 Optical Satellite (ARGOS) is a wide-angle Fizeau interferome...
This work demonstrates the use of two different observing modes with the twin apertures of the LBT. ...
Future spaceborne interferometric arrays must meet stringent optical performance and tolerance requi...
Abstract. | Space-based interferometers dedicated to wide-angle astrometry would dramatically increa...
Abstract. We present the design of a Fizeau interferometer to be implemented for the GAME mission. T...
Viewgraphs on optical interferometer testbed presented at the MIT Space Research Engineering Center ...
Several new space science mission concepts under development at NASA-GSFC for astronomy are intended...
The laser interferometer space antenna (LISA) is a future space-based interferometric gravitational-...
LINC-NIRVANA is the near-infrared Fizeau interferometric imaging camera for the Large Binocular Tele...
The StarLight mission aimed to place the first formation flying optical interferometer into space in...
Space-based interferometers dedicated to wide-angle astrometry would dramatically increase the accu...
International audienceThe Fresnel interferometric imager is a new kind of high angular resolution sp...
The light collecting apertures of space telescopes are currently limited in part by the size and wei...
Numerous space interferometry missions are planned for the next decade to verify different enabling ...
The Northrup-Grummann/Ball/Kodak team is building the James Webb Space Telescope (JWST), scheduled f...
The MIT Adaptive Reconnaissance Golay-3 Optical Satellite (ARGOS) is a wide-angle Fizeau interferome...
This work demonstrates the use of two different observing modes with the twin apertures of the LBT. ...
Future spaceborne interferometric arrays must meet stringent optical performance and tolerance requi...