Data

Parkes observations for project P971 semester 2023OCTS_01

Commonwealth Scientific and Industrial Research Organisation
Venkatraman Krishnan, Vivek ; Bailes, Matthew ; Bhat, Ramesh ; van Straten, Willem ; Flynn, Chris ; Reardon, Daniel John ; Batrakov, Alexander
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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:doi10.25919/gngv-w117&rft.title=Parkes observations for project P971 semester 2023OCTS_01&rft.identifier=https://doi.org/10.25919/gngv-w117&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose timing observations of the relativistic pulsar - white-dwarf binary, PSR J1141$-$6545. This unique system offers access to a wide range of physics, from relativistic phenomena through pulsar emission cone studies, to the structure and distribution of interstellar plasma along our line-of-sight. The Parkes Ultra Wide Band Low Frequency (UWL) receiver has opened up the possibility of performing the first-ever studies of its orbital dynamics at high temporal resolution. Our analysis of data obtained to date suggests that the pulsar will precess away from our line-of-sight before 2023. Hence, regular observations are crucial to maximize science outcomes with this source.&rft.creator=Venkatraman Krishnan, Vivek &rft.creator=Bailes, Matthew &rft.creator=Bhat, Ramesh &rft.creator=van Straten, Willem &rft.creator=Flynn, Chris &rft.creator=Reardon, Daniel John &rft.creator=Batrakov, Alexander &rft.date=2023&rft.edition=v1&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2023.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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We propose timing observations of the relativistic pulsar - white-dwarf binary, PSR J1141$-$6545. This unique system offers access to a wide range of physics, from relativistic phenomena through pulsar emission cone studies, to the structure and distribution of interstellar plasma along our line-of-sight. The Parkes Ultra Wide Band Low Frequency (UWL) receiver has opened up the possibility of performing the first-ever studies of its orbital dynamics at high temporal resolution. Our analysis of data obtained to date suggests that the pulsar will precess away from our line-of-sight before 2023. Hence, regular observations are crucial to maximize science outcomes with this source.

Available: 2023-11-26

Data time period: 2023-10-01 to 2024-03-31

Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | neutron stars | pulsars |

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Identifiers
ACN 633 798 857