The relativistic binary programme on MeerKAT: science objectives and first results

Author:

Kramer M12ORCID,Stairs I H3,Venkatraman Krishnan V1ORCID,Freire P C C1ORCID,Abbate F1ORCID,Bailes M45,Burgay M6ORCID,Buchner S7,Champion D J1ORCID,Cognard I89,Gautam T1,Geyer M7ORCID,Guillemot L89,Hu H1ORCID,Janssen G10,Lower M E411ORCID,Parthasarathy A1ORCID,Possenti A612,Ransom S13ORCID,Reardon D J45ORCID,Ridolfi A16ORCID,Serylak M7,Shannon R M45ORCID,Spiewak R24ORCID,Theureau G89,van Straten W14ORCID,Wex N1ORCID,Oswald L S15ORCID,Posselt B1516ORCID,Sobey C17ORCID,Barr E D1ORCID,Camilo F7,Hugo B718,Jameson A45,Johnston S11ORCID,Karastergiou A15,Keith M2,Osłowski S419ORCID

Affiliation:

1. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

2. Jodrell Bank Centre for Astrophysics, University of Manchester, Manchester M13 9PL, UK

3. Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver BC V6T 1Z1, Canada

4. Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn VIC 3122, Australia

5. ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), P.O. Box 218, Hawthorn VIC 3122, Australia

6. INAF – Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius (CA), Italy

7. South African Radio Astronomy Observatory, 2 Fir Street, Black River Park, Observatory 7925, South Africa

8. Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, Université d’Orléans, F-18330 Nançay, France

9. Laboratoire de Physique et Chimie de l’Environnement, CNRS, 3A Avenue de la Recherche Scientifique, F-45071 Orléans Cedex 2, France

10. ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo, the Netherlands

11. CSIRO Astronomy, Space Science, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710, Australia

12. Universitá di Cagliari, Dipartimento di Fisica, S.P. Monserrato-Sestu Km 0,700 – 09042 Monserrato (CA), Italy

13. National Radio Astronomy Observatory, 520 Edgemont Rd., Charlottesville, VA 22903, USA

14. Institute for Radio Astronomy, Space Research, Auckland University of Technology, Private Bag 92006, Auckland 1142, New Zealand

15. Oxford Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK

16. Department of Astronomy, Astrophysics, Pennsylvania State University, 525 Davey Lab, 16802 University Park, PA, USA

17. CSIRO Astronomy and Space Science, PO Box 1130 Bentley, WA 6102, Australia

18. Department of Physics and Electronics, Rhodes University, Artillery Road, Grahamstown, South Africa

19. Gravitational Wave Data Centre, Swinburne University of Technology, P.O. Box 218, Hawthorn, VIC 3122, Australia

Abstract

ABSTRACT We describe the ongoing Relativistic Binary programme (RelBin), a part of the MeerTime large survey project with the MeerKAT radio telescope. RelBin is primarily focused on observations of relativistic effects in binary pulsars to enable measurements of neutron star masses and tests of theories of gravity. We selected 25 pulsars as an initial high priority list of targets based on their characteristics and observational history with other telescopes. In this paper, we provide an outline of the programme, and present polarization calibrated pulse profiles for all selected pulsars as a reference catalogue along with updated dispersion measures. We report Faraday rotation measures for 24 pulsars, twelve of which have been measured for the first time. More than a third of our selected pulsars show a flat position angle swing confirming earlier observations. We demonstrate the ability of the Rotating Vector Model, fitted here to seven binary pulsars, including the Double Pulsar (PSR J0737–3039A), to obtain information about the orbital inclination angle. We present a high time resolution light curve of the eclipse of PSR J0737–3039A by the companion’s magnetosphere, a high-phase-resolution position angle swing for PSR J1141–6545, an improved detection of the Shapiro delay of PSR J1811–2405, and pulse scattering measurements for PSRs J1227–6208, J1757–1854, and J1811–1736. Finally, we demonstrate that timing observations with MeerKAT improve on existing data sets by a factor of, typically, 2–3, sometimes by an order of magnitude.

Funder

INAF

STFC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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