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Bayesian Blocks: A New Method to Analyze Photon Counting DataA Bayesian analysis of photon-counting data leads to a new time-domain algorithm for detecting localized structures (bursts), revealing pulse shapes, and generally characterizing intensity variations. The raw counting data -- time-tag events (TTE), time-to-spill (TTS) data, or binned counts -- is converted to a maximum likelihood segmentation of the observation into time intervals during which the photon arrival rate is perceptibly constant -- i.e. has a fixed intensity without statistically significant variations. The resulting structures, Bayesian Blocks, can be thought of as bins with arbitrary spacing determined by the data. The method itself sets no lower limit to the time scale on which variability can be detected. We have applied the method to RXTE data on Cyg X-1, yielding information on this source's short-time-scale variability.
Document ID
20020054342
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Scargle, Jeffrey D.
(NASA Ames Research Center Moffett Field, CA United States)
Bloom, Elliott D.
(Stanford Linear Accelerator Center Stanford, CA United States)
Young, Richard E.
Date Acquired
August 20, 2013
Publication Date
January 1, 1997
Subject Category
Atomic And Molecular Physics
Meeting Information
Meeting: American Astronomical Society High Energy Astrophysics Division Meeting
Country: United States
Start Date: November 3, 1997
End Date: November 7, 1997
Sponsors: American Astronomical Society
Funding Number(s)
PROJECT: RTOP 274-52-71-40
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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