Experimental progress in deep and broadband infrared nulling for TPF-I
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Engineering topics
Publications and source records attributed to Wallace, J..
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We report on the determination of the visual orbit of the double-lined spectroscopic binary system 64 Piscum with data obtained by the Palomar Testbed Interferometer in 1997 and 1998.
The Keck Interferometer is being developed by JPL and CARA as one of the ground-based components of NASA's Origins Program.
Deep nulling of both laser and thermal radiation has been demonstrated in the laboratory at visible wavelengths, by means of a rotational shearing interferometer (RSI) coupled to single-mode input and output fibers.
The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palomar Observatory, California.
A key thrust of NASA's Origins program is the search for and detection of planetary systems about other stars.
Pegasi (HR 8430, HD 210027) is a nearby, short-period (10.2 d) binary system with a F5V primary and a ~ G8V secondary in a circular orbit.
The ASEPS-0 Testbed Interferometer is a long-baseline infrared interferometer optimized for high-accuracy narrow-angle astrometry.