Parkes observations for project P1054 semester 2025APRS_19

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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, Ismaël;Grießmeier, 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 Dìaz;Hurter, Heinrich

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.

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Mentions (0)

Metrics

Dataset Index

0.1

FAIR Score

13%

Citations

0

Mentions

0

Metrics Over Time

Publication Details

DOI

Publisher

CSIRO

License

Creative Commons Attribution 4.0 International

Assigned Domain

Subfield

Astronomy and Astrophysics

Field

Physics and Astronomy

Domain

Physical Sciences

Confidence Score

57%

Source

Scholar Data Model

Normalization Factors

FT

63.46

CTw

1.00

MTw

1.00