MEASURING THE MASS OF SOLAR SYSTEM PLANETS USING PULSAR TIMING
- 23 August 2010
- journal article
- Published by American Astronomical Society in The Astrophysical Journal Letters
- Vol. 720 (2) , L201-L205
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This publication has 16 references indexed in Scilit:
- The International Pulsar Timing Array project: using pulsars as a gravitational wave detectorClassical and Quantum Gravity, 2010
- Multi-telescope timing of PSR J1518+4904Astronomy & Astrophysics, 2008
- Precision Timing of PSR J0437−4715: An Accurate Pulsar Distance, a High Pulsar Mass, and a Limit on the Variation of Newton’s Gravitational ConstantThe Astrophysical Journal, 2008
- TEMPO2, a new pulsar timing package - II. The timing model and precision estimatesMonthly Notices of the Royal Astronomical Society, 2006
- tempo2, a new pulsar-timing package - I. An overviewMonthly Notices of the Royal Astronomical Society, 2006
- The Gravity Field of the Saturnian System from Satellite Observations and Spacecraft Tracking DataThe Astronomical Journal, 2006
- Constraints on the Acceleration of the Solar System from High-Precision TimingThe Astronomical Journal, 2005
- Venus Gravity: 180th Degree and Order ModelIcarus, 1999
- High-precision timing of millisecond pulsars. 3: Long-term monitoring of PSRs B1855+09 and B1937+21The Astrophysical Journal, 1994
- The mass, gravity field, and ephemeris of MercuryIcarus, 1987