The DOI matches its Crossref record.
Arrival-time analysis for a pulsar in a binary system.
Abstract
A method is described for analyzing the arrival times of pulses from the binary pulsar PSR 1913+16, in terms of the orbital elements and their possible secular variations. Estimates are given for the times necessary to measure such secular changes and to detect various relativistic effects. If measurement errors 1 ms are the dominant source of error and 1000 independent observations are made per year, then 5 years of observations are necessary for a dynamical determination of the component masses accurate to 10 percent and 15 years for the possible detection of gravitational radiation. Other sources of error are briefly discussed. Subject headings: pulsars - stars: binaries
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Citations
Cited by
Theory and Experiment in Gravitational Physics
Will, C. M. (2018) · doi:10.1017/9781316338612 · Cited by 3,637
The Australia Telescope National Facility Pulsar Catalogue
Manchester, R. N., Hobbs, G. B., Teoh, A., & Hobbs, M. (2005) · The Astronomical Journal · doi:10.1086/428488 · Cited by 3,442
Tensor-multi-scalar theories of gravitation
Damour, T., & Esposito-Farese, G. (1992) · Classical and Quantum Gravity · doi:10.1088/0264-9381/9/9/015 · Cited by 1,016
Metadata
- Authors
- Blandford, R., & Teukolsky, S. A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1976-04
- Volume
- 205
- Pages
- 580
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2085100657
- Cited by
- 309
- References
- 0
- FWCI
- 3.13
- Type
- journal article
- Language
- en
- Open access
- closed
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- CoChat. (2026). Citation check: Arrival-time analysis for a pulsar in a binary system. https://app.cochat.ai/papers/10.1086/154315
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- Blandford, R., & Teukolsky, S. A. (1976). Arrival-time analysis for a pulsar in a binary system. The Astrophysical Journal. https://doi.org/10.1086/154315
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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