The Thousand-Pulsar-Array Programme on MeerKAT IV: Polarization Properties of Young, Energetic Pulsars

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aut.relation.endpage4495
aut.relation.issue3en_NZ
aut.relation.journalMonthly Notices of the Royal Astronomical Societyen_NZ
aut.relation.startpage4483
aut.relation.volume505en_NZ
aut.researcherVan Straten, Willem
dc.contributor.authorSerylak, Men_NZ
dc.contributor.authorJohnston, Sen_NZ
dc.contributor.authorKramer, Men_NZ
dc.contributor.authorBuchner, Sen_NZ
dc.contributor.authorKarastergiou, Aen_NZ
dc.contributor.authorKeith, MJen_NZ
dc.contributor.authorParthasarathy, Aen_NZ
dc.contributor.authorWeltevrede, Pen_NZ
dc.contributor.authorBailes, Men_NZ
dc.contributor.authorBarr, EDen_NZ
dc.contributor.authorCamilo, Fen_NZ
dc.contributor.authorGeyer, Men_NZ
dc.contributor.authorHugo, BVen_NZ
dc.contributor.authorJameson, Aen_NZ
dc.contributor.authorReardon, DJen_NZ
dc.contributor.authorShannon, RMen_NZ
dc.contributor.authorSpiewak, Ren_NZ
dc.contributor.authorvan Straten, Wen_NZ
dc.contributor.authorVenkatraman Krishnan, Ven_NZ
dc.date.accessioned2022-03-03T03:08:43Z
dc.date.available2022-03-03T03:08:43Z
dc.date.copyright2021-06-23en_NZ
dc.date.issued2021-06-23en_NZ
dc.description.abstractWe present observations of 35 high spin-down energy radio pulsars using the MeerKAT telescope. Polarization profiles and associated parameters are also presented. We derive the geometry for a selection of pulsars which show interpulse emission. We point out that, in several cases, these radio pulsars should also be seen in γ-rays but that improved radio timing is required to aid the high-energy detection. We discuss the relationship between the width of the radio profile and its high-energy detectability. Finally, we reflect on the correlation between the spin-down energy and the radio polarization fraction and the implications this may have for γ-ray emission.en_NZ
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volume 505, Issue 3, August 2021, Pages 4483–4495, https://doi.org/10.1093/mnras/staa2811
dc.identifier.doi10.1093/mnras/staa2811en_NZ
dc.identifier.issn0035-8711en_NZ
dc.identifier.issn1365-2966en_NZ
dc.identifier.urihttps://hdl.handle.net/10292/14966
dc.languageenen_NZ
dc.publisherOxford University Press (OUP)en_NZ
dc.relation.urihttps://academic.oup.com/mnras/article-abstract/505/3/4483/6288428
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2021 Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.rights.accessrightsOpenAccessen_NZ
dc.subjectInstrumentation: interferometers; Techniques: polarimetric; Pulsars: general
dc.titleThe Thousand-Pulsar-Array Programme on MeerKAT IV: Polarization Properties of Young, Energetic Pulsarsen_NZ
dc.typeJournal Article
pubs.elements-id447087
pubs.organisational-data/AUT
pubs.organisational-data/AUT/Faculty of Design & Creative Technologies
pubs.organisational-data/AUT/Faculty of Design & Creative Technologies/School of Engineering, Computer & Mathematical Sciences
pubs.organisational-data/AUT/Faculty of Design & Creative Technologies/School of Engineering, Computer & Mathematical Sciences/Centre of Radio Astronomy & Space Research
pubs.organisational-data/AUT/Faculty of Design & Creative Technologies/School of Engineering, Computer & Mathematical Sciences/Science, Technology, Engineering, & Mathematics Tertiary Education Centre
pubs.organisational-data/AUT/PBRF
pubs.organisational-data/AUT/PBRF/PBRF Design and Creative Technologies
pubs.organisational-data/AUT/PBRF/PBRF Design and Creative Technologies/PBRF ECMS
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