Pulsar Timing at Parkes
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Transcript of Pulsar Timing at Parkes
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Purpose of talk
• Highlight some recent results relating to pulsar timing and the Parkes Observatory
• Time constraints => will mainly concentrate on work that I’ve been involved in
CSIRO. Gravitational wave detection
Large number of collaborators including: CASS pulsar group, PPTA team, Chinese pulsar community ….
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CSIRO. Gravitational wave detection
TOA (measured using the observatory clock) Residual
Pulsar timing
Fold Fold
Model
Slide from D. Champion
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CSIRO. Gravitational wave detection
A few simulations
• With one pulsar you cannot (normally) tell what unmodelled physical effect is causing the residuals
GW background Spin-down irregularities Clock noise
Simulated data
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CSIRO. Gravitational wave detection
Spin-down irregularities
No angular signature
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CSIRO. Gravitational wave detection
Terrestrial time standard irregularities
Monopolar signature
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CSIRO. Gravitational wave detection
Errors in the planetary ephemerides - e.g. error in the mass of Jupiter
Dipolar signature
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CSIRO. Gravitational wave detection
What if gravitational waves exist?
Quadrapolar signature
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Studying individual pulsars using Parkes data
• M. Yu et al. (in preparation) – detection of 105 glitches in 36 pulsars observed at Parkes
• X. You et al. (in preparation) – analysis of the Solar Wind magnetic field and electron density using PPTA observations of J1022+1001
• Manchester et al. (2010) – relativistic spin precession in PSR J1141-6545
• Weltevrede et al. (2010) – Pulsar timing for the Fermi mission• Verbiest et al. (2008) - Limits on the variation of the
gravitational “constant” • You et al. (2007) - Studies of the interstellar medium• ….
• - concentrate in this talk on looking for correlations between timing residuals ….
CSIRO. Gravitational wave detection
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Developing a pulsar-based time standardParkes data + Arecibo
CSIRO. Gravitational wave detection
Pulsar time standard w.r.t TT(TAI)
Best time standard w.r.t. TT(TAI)
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Measuring planetary masses
• Use International Pulsar Timing Array data from Parkes, Effelsberg, Nancay and Arecibo.
• Champion et al. 2010, ApJ.• A planetary mass error will lead to incorrect
determination of the Solar System barycentre => correlated pulsar timing residuals
• Can fit to multiple pulsars simultaneously to search for such a signal
CSIRO. Gravitational wave detection
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CSIRO. Gravitational wave detection
Measuring planetary mass
• Champion, Hobbs, Manchester et al. (2010), ApJ, 720, 201• Use data from Parkes, Arecibo, Effelsberg and NancayMSun Best Published This workMercury 1.66013(7)x10-7 1.660(2)x10-7
Venus 2.4478686(4)x10-6 2.44782(10)x10-6
Mars 3.227151(9)x10-7 3.2277(8)x10-7
Jupiter* 9.547919(8)x10-4 9.547916(4)x10-4
Saturn 2.85885670(8)x10-4 2.858858(14)x10-4
9.54791915(11)x10-4
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Published limits on gravitational wave background (95% confidence)
CSIRO. Gravitational wave detection
All use the same Kaspi et al. (1994) data set
Tentative new bound
Poor choice of pulsar?
Incorrect algorithm?
Use same data set
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Pulsar navigation: assume that you are on the Earth’s surface
• PULSE@Parkes observations
CSIRO. Gravitational wave detection
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Pulsar navigation: assume that you are on the Earth’s surface
• Parkes observations
CSIRO. Gravitational wave detection
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Pulsar navigation: assume that you are on the Earth’s surface
• Parkes observations
CSIRO. Gravitational wave detection
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Pulsar navigation: assume that you are on the Earth’s surface
• Parkes observations
CSIRO. Gravitational wave detection
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Pulsar navigation: assume that you are on the Earth’s surface
• Parkes observations … correct to within a few kilometres
CSIRO. Gravitational wave detection
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Pulsar navigation: in 3D
CSIRO. Gravitational wave detection
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Conclusion
• Can distinguish between many phenomena by looking for correlated timing residuals between pulsars
• Have improved understanding of individual pulsars• Have developed a pulsar-based time standard• Have the most precise, published, mass estimate for the Jovian
system• Have not detected gravitational waves, but getting closer• Can reverse the timing procedure to determine our position.
CSIRO. Gravitational wave detection