Parkes observations for project P957 semester 2017OCTS
CSIRO RDS Repository
View Archive InfoField | Value | |
Title |
Parkes observations for project P957 semester 2017OCTS
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Creator |
Matthew Kerr
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Subject |
Astronomical and Space Sciences not elsewhere classified
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Description |
Pulse times of arrival are the key to any pulsar timing experiment, but the inferences we make depend critically on removing the effects of the interstellar medium. High-precision pulsar timing is reaching the limits of our ISM models and residuals effects may limit future goals, like the detection of gravitational waves. NICER, the newly-installed X-ray observatory on the International Space Station, provides the first opportunity to perform high-precision timing with X-rays, free from ISM effects. Radio telescopes still offer much greater precision, but NICER will allow us to carefully analyze ISM effects on a few pulsars. NICER will make weekly observations of PSR J1824-2452A, and we propose a high-cadence Parkes campaign to obtain contemporaneous radio TOAs. Since we know the "answer" from X-rays, we'll be able to test our ISM models and apply the results to all pulsar timing efforts.
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Publisher |
CSIRO
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Contributor |
George Hobbs
Scott Ransom Andrea Lommen Paul Ray Ryan Shannon Shi Dai Julia Deneva |
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Date |
2018-04-22
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Type |
—
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Format |
—
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Identifier |
csiro:P957-2017OCTS
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Language |
—
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Coverage |
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Rights |
—
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