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Parkes observations for project P957 semester 2017OCTS

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Title Parkes observations for project P957 semester 2017OCTS
 
Creator Matthew Kerr
 
Subject Astronomical and Space Sciences not elsewhere classified
 
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.
 
Publisher CSIRO
 
Contributor George Hobbs
Scott Ransom
Andrea Lommen
Paul Ray
Ryan Shannon
Shi Dai
Julia Deneva
 
Date 2018-04-22
 
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Identifier csiro:P957-2017OCTS
 
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