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NASA NTRS · 20020054342

Bayesian Blocks: A New Method to Analyze Photon Counting Data

Abstract

A 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.

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BibTeXRIS

Scargle, Jeffrey D., Bloom, Elliott D., Young, Richard E.. 1997-01-01. Bayesian Blocks: A New Method to Analyze Photon Counting Data. https://ntrs.nasa.gov/citations/20020054342

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