Publikationen (FIS)

The TRAPUM Large Magellanic Cloud pulsar survey with MeerKAT

I. Survey set-up and first seven pulsar discoveries

Verfasst von

V. Prayag, L. Levin, M. Geyer, B. W. Stappers, E. Carli, E. D. Barr, R. P. Breton, S. Buchner, M. Burgay, M. Kramer, A. Possenti, V. Venkatraman Krishnan, C. Venter, J. Behrend, W. Chen, D. M. Horn, P. V. Padmanabh, A. Ridolfi

Abstract

The Large Magellanic Cloud (LMC) presents a unique environment for pulsar population studies due to its distinct star formation characteristics and proximity to the Milky Way. As part of the TRAPUM (TRAnsients and PUlsars with MeerKAT) Large Survey Project, we are using the core array of the MeerKAT radio telescope (MeerKAT) to conduct a targeted search of the LMC for radio pulsars at L-band frequencies, 856–1712 MHz. The excellent sensitivity of MeerKAT, coupled with a 2-h integration time, makes the survey 3 times more sensitive than previous LMC radio pulsar surveys. We report the results from the initial four survey pointings which have resulted in the discovery of seven new radio pulsars, increasing the LMC radio pulsar population by 30 per cent. The pulse periods of these new pulsars range from 278 to 1690 ms, and the highest dispersion measure is 254.20 pc cm⁻³. We searched for, but did not find any significant pulsed radio emission in a beam centred on the SN 1987A remnant, establishing an upper limit of 6.3 μJy on its minimum flux density at 1400 MHz.

Details

Organisationseinheit(en): Institut für Gravitationsphysik
Externe Organisation(en): Universität Kapstadt (UCT)
University of Manchester
Max-Planck-Institut für Radioastronomie (MPIfR)
South African Radio Astronomy Observatory (SARAO)
Istituto Nazionale di Astrofisica (INAF)
North-West University (NWU)
National Institute for Theoretical and Computational Sciences (NITheCS)
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)
Typ: Artikel
Journal: Monthly Notices of the Royal Astronomical Society
Band: 533
Seiten: 2570-2581
Anzahl der Seiten: 12
ISSN: 0035-8711
Publikationsdatum: 09.2024
Publikationsstatus: Veröffentlicht
Peer-reviewed: Ja
ASJC Scopus Sachgebiete: Astronomie und Astrophysik, Astronomie und Planetologie
Elektronische Version(en): https://doi.org/10.1093/mnras/stae1917 (Zugang: Offen )