Data

Parkes observations for project P1054 semester 2025APRS_12

Commonwealth Scientific and Industrial Research Organisation
Burgay, Marta ; Possenti, Andrea ; Kramer, Michael ; Freire, Paulo ; Weltevrede, Patrick ; Stappers, Benjamin ; Levin, Lina ; Champion, David ; Buchner, Sarah ; Barr, Ewan ; Berezina, Marina ; Venkatraman Krishnan, Vivek ; Boettcher, Markus ; Balakrishnan, Vishnu ; Clark, Colin James ; Breton, Rene ; Desvignes, Gregory ; Ridolfi, Alessandro ; Cognard, Ismaë; l ; Grieß; meier, Jean-Mathias ; Colom I Bernadich, Miquel ; Thongmeearkom, Tinn ; Sengupta, Shalini ; Voraganti Padmanabh, Prajwal ; Carli, Emma ; Parthasarathy, Aditya ; Men, Yunpeng ; Turner, James ; Vleeschower, Laila ; Prayag, Venu ; Pillay, Denisha ; Sergio, Belmonte Dì; az ; Hurter, Heinrich
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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/ft2e-j488&rft.title=Parkes observations for project P1054 semester 2025APRS_12&rft.identifier=https://doi.org/10.25919/ft2e-j488&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 19 in the Magellanic Clouds, 105 in Globular Clusters and 81 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including a few relativistic systems and several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing for the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.&rft.creator=Burgay, Marta &rft.creator=Possenti, Andrea &rft.creator=Kramer, Michael &rft.creator=Freire, Paulo &rft.creator=Weltevrede, Patrick &rft.creator=Stappers, Benjamin &rft.creator=Levin, Lina &rft.creator=Champion, David &rft.creator=Buchner, Sarah &rft.creator=Barr, Ewan &rft.creator=Berezina, Marina &rft.creator=Venkatraman Krishnan, Vivek &rft.creator=Boettcher, Markus &rft.creator=Balakrishnan, Vishnu &rft.creator=Clark, Colin James &rft.creator=Breton, Rene &rft.creator=Desvignes, Gregory &rft.creator=Ridolfi, Alessandro &rft.creator=Cognard, Ismaël &rft.creator=Grießmeier, Jean-Mathias &rft.creator=Colom I Bernadich, Miquel &rft.creator=Thongmeearkom, Tinn &rft.creator=Sengupta, Shalini &rft.creator=Voraganti Padmanabh, Prajwal &rft.creator=Carli, Emma &rft.creator=Parthasarathy, Aditya &rft.creator=Men, Yunpeng &rft.creator=Turner, James &rft.creator=Vleeschower, Laila &rft.creator=Prayag, Venu &rft.creator=Pillay, Denisha &rft.creator=Sergio, Belmonte Dìaz &rft.creator=Hurter, Heinrich &rft.date=2025&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 2025.&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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Creative Commons Attribution 4.0 International Licence
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Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO 2025.

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Brief description

With this proposal we ask time to continue our timing follow-up campaign of pulsars discovered with the MeerKAT telescope. Fourtytwo sources have been discovered in targeted observations of Fermi unidentified point sources, two towards Supernova Remnants, 19 in the Magellanic Clouds, 105 in Globular Clusters and 81 in a survey of the Galactic plane. A large fraction of the new discoveries are recycled pulsars (including a few relativistic systems and several 'spider' binaries), or young pulsars. Timing observations have an essential role in exploiting the full potential of any pulsar discovery, allowing for the precise measurement of rotational, astrometric and orbital parameters which, in turn, give us powerful tools to improve our understanding of the physics in extreme environments as well as of the population of neutron stars as a whole. The UWL receiver of the Parkes telescope is a sensitive, versatile instrument that is allowing us to successfully time these new sources, in the bright-end of TRAPUM discoveries.

Available: 2025-08-15

Data time period: 2025-04-01 to 2025-09-30

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

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