NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Shot noise limits to sensitivity of optical interferometryBy arguing that the limiting noise is the photoelectron shot noise, we show that the sensitivity of image synthesis by an ideal optical interferometer is independent of the details of beam-splitting and recombination. The signal-to-noise ratio of the synthesized image is proportional to the square root of the total number of photoelectrons detected by the entire array. For non-ideal interferometers, which are forced to employ a closure-phase method of indirect inference of the visibility data, essentially the same result holds for strong sources, but at weak light levels beam-splitting degrades sensitivity.
Document ID
19930004398
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Prasad, Sudhakar
(New Mexico Univ. Albuquerque, NM, United States)
Date Acquired
September 6, 2013
Publication Date
November 1, 1992
Publication Information
Publication: A Lunar Optical-Ultraviolet-Infrared Synthesis Array (LOUISA)
Subject Category
Astronomy
Accession Number
93N13586
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available