2006
DOI: 10.1088/1009-9271/6/s2/57
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Pulsar Observations with Radio Telescope FAST

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Cited by 28 publications
(26 citation statements)
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“…While the Square Kilometre Array [154] is not expected to be completed until 2020, a number of pathfinder instruments are now under development. In China, the Five hundred meter Aperture Spherical Telescope [105] is scheduled for completion in 2013 and will provide significant advances for pulsar research [266]. The Australian Square Kilometre Array Pathfinder, will have some applications as a pulsar instrument [164].…”
Section: Pulsar Phenomenologymentioning
confidence: 99%
“…While the Square Kilometre Array [154] is not expected to be completed until 2020, a number of pathfinder instruments are now under development. In China, the Five hundred meter Aperture Spherical Telescope [105] is scheduled for completion in 2013 and will provide significant advances for pulsar research [266]. The Australian Square Kilometre Array Pathfinder, will have some applications as a pulsar instrument [164].…”
Section: Pulsar Phenomenologymentioning
confidence: 99%
“…(9), (10) and (12), we find that the sample detection fraction now depends on the observation frequency and the combined parameter F. We calculate the sample detection fraction under various conditions in the next section.…”
Section: Simulations and Calculationsmentioning
confidence: 97%
“…So we put the known sample in different regions by rotating around the Galactic Center by an angle  of 45°, 90°, 135° and 180°, and we get the samples 1, 2, 3 and 4 as shown in Figure 4. Pulsars in these regions can be observed by the telescopes in the northern hemisphere, such as FAST [10].…”
Section: Simulations and Calculationsmentioning
confidence: 99%
“…当 两个星系并合后, 两个超大质量黑洞会由于引力束 缚而形成双黑洞系统, 并产生引力波辐射 [139] , 现有 的观测也支持这样系统的存在 [140] . 单独的双黑洞系 统并不能够被轻易探测, 但是许多系统混合在一起 [142] , FAST [143] 等都有望提高脉 冲星计时阵列的灵敏度.…”
Section: 脉冲星计时阵列unclassified