The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interf
erometer located at Palomar Observatory, California. It was built as a test
bed for interferometric techniques applicable to the Keck Interferometer. F
irst fringes were obtained in 1995 July. PTI implements a dual-star archite
cture, tracking two stars simultaneously for phase referencing and narrow-a
ngle astrometry. The three fixed 40 cm apertures can be combined pairwise t
o provide baselines to 110 m. The interferometer actively tracks the white-
light fringe using an array detector at 2.2 mu m and active delay lines wit
h a range of +/-38 m. Laser metrology of the delay lines allows for servo c
ontrol, and laser metrology of the complete optical path enables narrow-ang
le astrometric measurements. The instrument is highly automated, using a mu
ltiprocessing computer system for instrument control and sequencing.