The Parkes Multibeam Pulsar Survey - V. Finding binary and millisecond pulsars

被引:132
作者
Faulkner, AJ [1 ]
Stairs, IH
Kramer, M
Lyne, AG
Hobbs, G
Possenti, A
Lorimer, DR
Manchester, RN
McLaughlin, MA
D'Amico, N
Camilo, F
Burgay, M
机构
[1] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[3] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[4] Osservatorio Astron Cagliari, INAF, I-09012 Capoterra, CA, Italy
[5] Univ Cagliari, Dipartimento Fis, I-90042 Monserrato, CA, Italy
[6] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
关键词
surveys; pulsars : general; pulsars : individual : PSR J1744-3922; pulsars : individual : PSR J1801-1417; pulsars : individual : PSR J1802-2124;
D O I
10.1111/j.1365-2966.2004.08310.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Parkes Multibeam Pulsar Survey is the most successful survey of the Galactic plane ever performed, finding over 600 pulsars in the initial processing. We report on a reprocessing of all 40 000 beams with a number of algorithms, including conventional frequency-domain searches and an acceleration search for fast binary pulsars. The very large volume of results coupled with the need to distinguish new candidates from known pulsars and their many harmonics, often with multiple detections from different search algorithms, necessitated the development of a new graphical selection tool tightly linked to a web-based results data base. We discuss and demonstrate the benefits of these software systems, which are specifically designed for large survey projects. The results of this processing have been encouraging. We have discovered 128 new pulsars, including 11 binary and 15 millisecond pulsars; in addition to those previously found in the survey, we have thus far discovered 737 pulsars. In this paper, we discuss the discoveries of PSR J1744-3922 (a 172-ms mildly recycled pulsar in a 4.6-h orbit that exhibits nulling behaviour, not previously observed in recycled or binary objects), PSR J1802-2124 (an intermediate mass binary pulsar) and PSR J1801-1417 (a solitary millisecond pulsar).
引用
收藏
页码:147 / 158
页数:12
相关论文
共 45 条
[41]  
TAYLOR JH, 1993, PARTICLE ASTROPHYSICS, P367
[42]   FURTHER EXPERIMENTAL TESTS OF RELATIVISTIC GRAVITY USING THE BINARY PULSAR PSR 1913+16 [J].
TAYLOR, JH ;
WEISBERG, JM .
ASTROPHYSICAL JOURNAL, 1989, 345 (01) :434-450
[43]   PULSAR DISTANCES AND THE GALACTIC DISTRIBUTION OF FREE-ELECTRONS [J].
TAYLOR, JH ;
CORDES, JM .
ASTROPHYSICAL JOURNAL, 1993, 411 (02) :674-684
[44]   SEARCHES FOR MILLISECOND PULSATIONS IN LOW-MASS X-RAY BINARIES [J].
WOOD, KS ;
NORRIS, JP ;
HERTZ, P ;
VAUGHAN, BA ;
MICHELSON, PF ;
MITSUDA, K ;
LEWIN, WHG ;
VANPARADIJS, J ;
PENNINX, W ;
VANDERKLIS, M .
ASTROPHYSICAL JOURNAL, 1991, 379 (01) :295-309
[45]  
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