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The High Time Resolution Universe Pulsar Survey – XVI. Discovery and timing of 40 pulsars from the southern Galactic plane

dc.contributor.authorCAMERON, A.D.
dc.contributor.authorCHAMPION, D.J.
dc.contributor.authorBAILES, M.
dc.contributor.authorBALAKRISHNAN, V.
dc.contributor.authorBARR, E.D.
dc.contributor.authorBASSA, C.G.
dc.contributor.authorBATES, S.
dc.contributor.authorBHANDARI, S.
dc.contributor.authorBHAT, N.D.R.
dc.contributor.authorBURGAY, M.
dc.contributor.authorBURKE-SPOLAOR, S.
dc.contributor.authorFLYNN, C.M.L.
dc.contributor.authorJAMESON, A.
dc.contributor.authorJOHNSTON, S.
dc.contributor.authorKEITH, M.J.
dc.contributor.authorKRAMER, M.
dc.contributor.authorLEVIN, L.
dc.contributor.authorLYNE, A.G.
dc.contributor.authorNG, C.
dc.contributor.authorPETROFF, E.
dc.contributor.authorPOSSENTI, A.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorSMITH, D.A.
dc.contributor.authorSTAPPERS, B.W.
dc.contributor.authorVAN STRATEN, W.
dc.contributor.authorTIBURZI, C.
dc.contributor.authorWU, J.
dc.date.issued2020
dc.description.abstractEnWe present the results of processing an additional 44  per cent of the High Time Resolution Universe South Low Latitude (HTRU-S LowLat) pulsar survey, the most sensitive blind pulsar survey of the southern Galactic plane to date. Our partially coherent segmented acceleration search pipeline is designed to enable the discovery of pulsars in short, highly accelerated orbits, while our 72-min integration lengths will allow us to discover pulsars at the lower end of the pulsar luminosity distribution. We report the discovery of 40 pulsars, including three millisecond pulsar-white dwarf binary systems (PSRs J1537−5312, J1547−5709, and J1618−4624), a black-widow binary system (PSR J1745−23) and a candidate black-widow binary system (PSR J1727−2951), a glitching pulsar (PSR J1706−4434), an eclipsing binary pulsar with a 1.5-yr orbital period (PSR J1653−45), and a pair of long spin-period binary pulsars which display either nulling or intermittent behaviour (PSRs J1812−15 and J1831−04). We show that the total population of 100 pulsars discovered in the HTRU-S LowLat survey to date represents both an older and lower luminosity population, and indicates that we have yet to reach the bottom of the luminosity distribution function. We present evaluations of the performance of our search technique and of the overall yield of the survey, considering the 94  per cent of the survey which we have processed to date. We show that our pulsar yield falls below earlier predictions by approximately 25  per cent (especially in the case of millisecond pulsars), and discuss explanations for this discrepancy as well as future adaptations in RFI mitigation and searching techniques which may address these shortfalls.
dc.language.isoen
dc.subject.ensurveys
dc.subject.enpulsars: general
dc.subject.enstars: neutron
dc.title.enThe High Time Resolution Universe Pulsar Survey – XVI. Discovery and timing of 40 pulsars from the southern Galactic plane
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/staa039
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv2001.01823
bordeaux.journalMon.Not.Roy.Astron.Soc.
bordeaux.page1063-1087
bordeaux.volume493
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-02497785
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02497785v1
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