2019
DOI: 10.1007/s11433-019-1453-2
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Advancing pulsar science with the FAST

Abstract: The authors discuss potential remarkable achievements for pulsar science with the FAST (pulsar monitoring, timing and searching, as well as others related), and expect a FAST era of pulsar science to come. FAST, pulsarPACS number(s):

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Cited by 25 publications
(17 citation statements)
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“…The tests are to be sharpened to a new level with new instruments and continued observations, in particular, with the demonstrated capability of the South African MeerKAT radio telescope (Bailes et al 2018) and the Chinese Five‐hundred‐meter Aperture Spherical Telescope (FAST; Jiang et al 2019; Lu et al 2020), and ultimately with the Square Kilometre Array (SKA; Kramer et al 2004; Shao et al 2015; Weltman et al 2020). Radio pulsars will continue to provide interesting gravity tests, in complement to tests from other fields (Sathyaprakash 2019; Shao et al 2017; Wex 2014; Yunes et al 2016).…”
Section: Discussionmentioning
confidence: 99%
“…The tests are to be sharpened to a new level with new instruments and continued observations, in particular, with the demonstrated capability of the South African MeerKAT radio telescope (Bailes et al 2018) and the Chinese Five‐hundred‐meter Aperture Spherical Telescope (FAST; Jiang et al 2019; Lu et al 2020), and ultimately with the Square Kilometre Array (SKA; Kramer et al 2004; Shao et al 2015; Weltman et al 2020). Radio pulsars will continue to provide interesting gravity tests, in complement to tests from other fields (Sathyaprakash 2019; Shao et al 2017; Wex 2014; Yunes et al 2016).…”
Section: Discussionmentioning
confidence: 99%
“…China's Five-hundred-meter Aperture Spherical radio Telescope (FAST), is dedicated to observe the sky in the frequency range 70 MHz − 3 GHz. Among others, one of the important missions of FAST is the SETI project (Lu et al 2020) and, recently, the collaboration has announced the first SETI observations (Zhang et al 2020, Li et al 2020. The aim of the present paper is to reexamine the results obtained by Osmanov (2020a,b) to consider the radio characteristics of the extraterrestrial von-Neumann self-replicators and discuss the problem in the context of observations performed by FAST.…”
Section: Introductionmentioning
confidence: 91%
“…The Canadian Hydrogen Intensity Mapping Experiment (CHIME, detailed in CHIME/Pulsar Collaboration et al 2021) observes almost every known pulsar in the Northern sky with an approximately daily cadence, in the 400 -800 MHz band, making it an ideal instrument for measuring temporal variations in ISM properties. The Five-Hundred-Metre Aperture Spherical Radio Telescope (FAST, detailed in Lu et al 2019) has recently been used to measure scattering screens in PSR B1929+10 and PSR B1842+14, which was not possible with the previous generation of radio telescopes (Yao et al 2020). MeerKAT (Bailes et al 2020), the precursor to the Square Kilometre Array (SKA), has recently been utilized in making scattering measurements of a small number of pulsars in the Southern sky (Oswald et al 2021) and will be further improved with the completion of the full SKA (Keane 2018).…”
Section: Future Prospectsmentioning
confidence: 99%