The DOI matches its Crossref record; 18 of the 18 references it cites were found in a registry or an index.
Precision timing measurements of PSR J1012+5307
Open accessAbstract
We present results and applications of high-precision timing measurements of the binary millisecond pulsar J1012+5307. Combining our radio timing measurements with results based on optical observations, we derive complete 3D velocity information for this system. Correcting for Doppler effects, we derive the intrinsic spin parameters of this pulsar and a characteristic age of 8.6 ± 1.9 Gyr. Our upper limit for the orbital eccentricity of only 8 × 10−7 (68 per cent confidence level) is the smallest ever measured for a binary system. We demonstrate that this makes the pulsar an ideal laboratory in which to test certain aspects of alternative theories of gravitation. Our precision measurements suggest deviations from a simple pulsar spin-down timing model, which are consistent with timing noise and the extrapolation of the known behaviour of slowly rotating pulsars.
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Cites
Pulsar distances and the galactic distribution of free electrons
Taylor, J. H., & Cordes, J. M. (1993) · The Astrophysical Journal · doi:10.1086/172870 · Cited by 1,281
Further experimental tests of relativistic gravity using the binary pulsar PSR 1913 + 16
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Tensor-scalar gravity and binary-pulsar experiments
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High-precision timing of millisecond pulsars. 3: Long-term monitoring of PSRs B1855+09 and B1937+21
Kaspi, V. M., Taylor, J. H., & Ryba, M. F. (1994) · The Astrophysical Journal · doi:10.1086/174280 · Cited by 595 · cited 2×
“In this case, PSR J1012+5307 is only the second Galactic field millisecond pulsar to show a significant second spin frequency derivative, ν̈, the other being PSR B1937+21 (Kaspi et al. 1994)‡.”
BackgroundInfluentialStrong-field tests of relativistic gravity and binary pulsars
Damour, T., & Taylor, J. H. (1992) · Physical Review D · doi:10.1103/physrevd.45.1840 · Cited by 523
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On the orbital period change of the binary pulsar PSR 1913 + 16
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Relativity parameters determined from lunar laser ranging
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Blandford, R., & Teukolsky, S. A. (1976) · The Astrophysical Journal · doi:10.1086/154315 · Cited by 309
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Cited by
Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
Cromartie, H. T., Fonseca, E., Ransom, S. M., Demorest, P. B., Arzoumanian, Z., Blumer, H., Brook, P. R., DeCesar, M. E., Dolch, T., Ellis, J. A., et al. (2019) · Nature Astronomy · doi:10.1038/s41550-019-0880-2 · Cited by 1,615
A statistical study of 233 pulsar proper motions
Hobbs, G., Lorimer, D. R., Lyne, A. G., & Kramer, M. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09087.x · Cited by 1,373
Self-citationThe Nuclear Equation of State and Neutron Star Masses
Lattimer, J. M. (2012) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev-nucl-102711-095018 · Cited by 937
Binary and Millisecond Pulsars
Lorimer, D. R. (2008) · Living Reviews in Relativity · doi:10.12942/lrr-2008-8 · Cited by 616
Freire, P. C. C., Wex, N., Esposito-Farèse, G., Verbiest, J. P. W., Bailes, M., Jacoby, B. A., Kramer, M., Stairs, I. H., Antoniadis, J., & Janssen, G. H. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21253.x · Cited by 543
Self-citation
Metadata
- Authors
- Lange, C., Camilo, F., Wex, N., Kramer, M., Backer, D. C., Lyne, A. G., & Doroshenko, O.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2001-09
- Volume
- 326
- Issue
- 1
- Pages
- 274-282
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2120497457
- Cited by
- 256
- References
- 18
- FWCI
- 4.89
- Type
- journal article
- Language
- en
- Open access
- green
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- Lange, C., Camilo, F., Wex, N., Kramer, M., Backer, D. C., Lyne, A. G., & Doroshenko, O. (2001). Precision timing measurements of PSR J1012+5307. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2001.04606.x
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