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

被引:27
|
作者
Cameron, A. D. [1 ,2 ]
Champion, D. J. [1 ]
Bailes, M. [3 ,4 ]
Balakrishnan, V [1 ]
Barr, E. D. [1 ,4 ]
Bassa, C. G. [5 ]
Bates, S. [6 ]
Bhandari, S. [2 ]
Bhat, N. D. R. [7 ]
Burgay, M. [8 ]
Burke-Spolaor, S. [9 ]
Flynn, C. M. L. [3 ]
Jameson, A. [3 ,4 ]
Johnston, S. [2 ]
Keith, M. J. [6 ]
Kramer, M. [1 ,6 ]
Levin, L. [6 ]
Lyne, A. G. [6 ]
Ng, C. [10 ]
Petroff, E. [5 ]
Possenti, A. [8 ,11 ]
Smith, D. A. [12 ]
Stappers, B. W. [6 ]
van Straten, W. [13 ]
Tiburzi, C. [1 ,14 ]
Wu, J. [1 ]
机构
[1] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
[2] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, POB 76, Epping, NSW 1710, Australia
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Mail H39,POB 218, Hawthorn, Vic 3122, Australia
[4] Swinburne Univ Technol, ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Mail H11,POB 218, Hawthorn, Vic 3122, Australia
[5] ASTRON, Netherlands Inst Radio Astron, Postbus 2, NL-7990 AA Dwingeloo, Netherlands
[6] Univ Manchester, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England
[7] Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
[8] INAF, Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy
[9] West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA
[10] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada
[11] Univ Cagliari, Dept Phys, SP Monserrato Sestu Km 0,700, I-09042 Monserrato, Italy
[12] Univ Bordeaux 1, CNRS, IN2P3, Ctr Etud Nucl Bordeaux Gradignan, BP120, F-33175 Gradignan, France
[13] Auckland Univ Technol, Inst Radio Astron & Space Res, Private Bag 92006, Auckland 1142, New Zealand
[14] Univ Bielefeld, Fak Phys, Postfach 100131, D-33501 Bielefeld, Germany
基金
英国科学技术设施理事会; 澳大利亚研究理事会;
关键词
surveys; stars: neutron; pulsars: general; WHITE-DWARF COMPANIONS; YOUNG RADIO PULSAR; MILLISECOND PULSARS; NEUTRON-STAR; POPULATION SYNTHESIS; ACCELERATION SEARCH; BURSTS; MASS; RAY; POLARIMETRY;
D O I
10.1093/mnras/staa039
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We 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.
引用
收藏
页码:1063 / 1087
页数:25
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