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Constructing a pulsar timing array

Foster, R. S., Backer, D. C.·1990·The Astrophysical Journal

Abstract

Arrival time data from a spatial array of millisecond pulsars can be used (1) to provide a time standard for long time scales, (2) to detect perturbations of the earth's orbit, and (3) to search for a cosmic background of gravitational radiation. A polynomial time series representation for these three effects is first developed that is appropriate for analysis of the present data with its limited degrees of freedom. A pulsar timing array program is then described that has been established at the National Radio Astronomy Observatory 43 m telescope with observations of PSR 1620 - 26, PSR 181 - 24, and PSR 1937 + 21. The results cover a 2 yr period beginning in July 1987. The influence of global parameters - clock, earth location, and effects of gravitational radiation is discussed in the context of the polynomial model.

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Metadata

Authors
Foster, R. S., & Backer, D. C.
Venue
The Astrophysical Journal
Published
1990-09
Volume
361
Pages
300
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2033842403
Cited by
538
References
0
FWCI
4.86
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Constructing a pulsar timing array. https://app.cochat.ai/papers/10.1086/169195
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Foster, R. S., & Backer, D. C. (1990). Constructing a pulsar timing array. The Astrophysical Journal. https://doi.org/10.1086/169195

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