Data

Parkes observations for project P361 semester 2007APRS

Commonwealth Scientific and Industrial Research Organisation
Bailes, Matthew ; Ord, S ; Verbiest, Joris P.W. ; Bhat, Ramesh ; Hotan, Aidan
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/51E7F73858A65&rft.title=Parkes observations for project P361 semester 2007APRS&rft.identifier=https://doi.org/10.4225/08/51E7F73858A65&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose to continue our studies of Southern relativistic binary pulsarsto place stringent limits on General Relativity, pulsar masses, and to map out the emission cone of PSR J1141--6545, which we have established is undergoing rapid profile evolution. In light of our recent results, we would like to continue our current, 2-monthly rate of observations of this pulsar. Our instrumentation is the most sensitive to the evolution of complex features in the double pulsar's profile at 50cm wavelength which we aim to monitor on an annual basis.&rft.creator=Bailes, Matthew &rft.creator=Ord, S &rft.creator=Verbiest, Joris P.W. &rft.creator=Bhat, Ramesh &rft.creator=Hotan, Aidan &rft.date=2013&rft.edition=v2&rft_rights=Creative Commons Attribution 3.0 Unported Licence https://creativecommons.org/licenses/by/3.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO Australia 2011.&rft_subject=Galactic&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO Australia 2011.

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We propose to continue our studies of Southern relativistic binary pulsars
to place stringent limits on General Relativity, pulsar masses, and to map
out the emission cone of PSR J1141--6545, which we have established is
undergoing rapid profile evolution. In light of our recent results, we
would like to continue our current, 2-monthly rate of observations of
this pulsar. Our instrumentation is the most sensitive to the evolution of
complex features in the double pulsar's profile at 50cm wavelength which
we aim to monitor on an annual basis.

Available: 2013-07-19

Data time period: 2007-04-01 to 2007-09-30

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Galactic | Physical Sciences |

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Identifiers
ACN 633 798 857