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Signal detection amid noise with known statisticsConventional methods of signal detection are based on the comparison of a local signal-to-noise ratio S/N to some threshold value. We present a new method that compares instead the histogram of the data with the one expected for background noise alone. Signals are detected from discrepancies between the two. We expect it to be applicable in the detection of signals from any data whose background statistics is known. To illustrate the method, we apply it to the case of photon-limited imaging data where the underlying background is Poissonian. Numerical simulations are used to check the efficiency of our method, finding that for signals with low S/N (less than 5), it detects signals with a higher degree of reliability than the conventional method.
Document ID
19950034156
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Zepka, A. F.
(Cornell Univ. Ithaca, NY, United States)
Cordes, J. M.
(Cornell Univ. Ithaca, NY, United States)
Wasserman, I.
(Cornell Univ. Ithaca, NY, United States)
Date Acquired
August 16, 2013
Publication Date
May 20, 1994
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 427
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
95A65755
Funding Number(s)
CONTRACT_GRANT: NAGW-666
CONTRACT_GRANT: NSF AST-91-19475
CONTRACT_GRANT: NAG5-1247
CONTRACT_GRANT: NAG5-1563
Distribution Limits
Public
Copyright
Other

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