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  • Influence
This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron starsExpand
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The High Time Resolution Universe Pulsar Survey - I. System configuration and initial discoveries
We have embarked on a survey for pulsars and fast transients using the 13-beam multibeam receiver on the Parkes Radio Telescope. Installation of a digital backend allows us to record 400 MHz ofExpand
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A high-frequency survey of the southern Galactic plane for pulsars
Results of an HF survey designed to detect young, distant, and short-period pulsars are presented. The survey detected a total of 100 pulsars, 46 of which were previously unknown. The periods of theExpand
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SNR G320.4–01.2 and PSR B1509–58: new radio observations of a complex interacting system
We describe radio continuum and spectral-line observations of the source G320.4–01.2 (MSH 15–52) and the coincident young pulsar B1509–58 made with the Australia Telescope Compact Array. Based on aExpand
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Five new fast radio bursts from the HTRU high-latitude survey at Parkes: First evidence for two-component bursts
The detection of five new fast radio bursts (FRBs) found in the 1.4-GHz High Time Resolution Universe high-latitude survey at Parkes, is presented. The rate implied is 7(-3)(+5) x 10(3) (95 per cent)Expand
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The glitch-induced identity changes of PSR J1119−6127
Rotation-powered radio pulsars are generally observed to pulse regularly in the radio band, but this is not the case for so-called rotating radio transients (RRATs) which emit only sporadic bursts ofExpand
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Precise γ-ray timing and radio observations of 17 Fermi γ-ray pulsars
We present precise phase-connected pulse timing solutions for 16 γ-ray-selected pulsars recently discovered using the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope plus one veryExpand
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XMM–Newton observations of PSR B1259−63 near the 2004 periastron passage
PSR B1259−63 is in a highly eccentric 3.4-yr orbit with a Be star and crosses the Be star disc twice per orbit, just prior to and just after periastron. Unpulsed radio, X-ray and gamma-ray emissionExpand
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