[1] 南仁东. 500 m球反射面射电望远镜FAST[J].中国科学G辑:物理学、力学、天文学, 2005, 35(5):3-20.
[2] 南仁东,张海燕,张莹,等. FAST工程建设进展[J].天文学报, 2016, 57(6):623-630.
[3] Qiu Y H. A novel design for a giant Arecibo-type spherical radio telescope with an active main reflector[J]. Monthly Notices of the Royal Astronomical Society, 1998, 301(3):827-830.
[4] 吴鑫基.帕克斯射电望远镜与脉冲星巡天发现:纪念脉冲星发现50年[J].科学, 2017, 69(6):43-49.
[5] Han J L, Wang C, Wang P F, et al. The FAST Galactic Plane Pulsar Snapshot survey:I. Project design and Pulsar discoveries[J]. Research in Astronomy and Astrophysics, 2021, 21(5):107.
[6] Li D, Wang P, Zhu W W, et al. A bimodal burst energy distribution of a repeating fast radio burst source[J]. Nature, 2021, 598(7880):267-271.
[7] Ching T C, Li D, Heiles C, et al. An early transition to magnetic supercriticality in star formation[J]. Nature, 2022, 601:49-52.
[8] Li D, Wang P, Qian L, et al. FAST in space:Considerations for a multibeam, multipurpose survey using China's 500 m aperture spherical radio telescope (FAST)[J]. IEEE Microwave Magazine, 2018, 19(3):112-119.
[9] Jiang P, Tang N Y, Hou L G, et al. The fundamental performance of FAST with 19-beam receiver at L band[J]. Research in Astronomy and Astrophysics, 2020, 20(5):64.
[10] 闫振,沈志强. FAST:脉冲星观测研究的利器[J].科技导报, 2017, 35(24):16-19.
[11] 张承民,崔翔翰,杨佚沿,等.从阿雷西博到中国天眼射电望远镜:工业革命的接力[J].科技导报, 2021, 39(11):9-15.
[12] 张承民,崔翔翰,王德华,等.脉冲星发现55年:中国天眼展望[J].科技导报, 2022, 40(24):72-77.
[13] 彭勃.天眼工程:大射电望远镜FAST追梦实录[M].上海:上海科技教育出版社, 2021.
[14] 吴鑫基.中国天眼和"人民科学家"南仁东[J].科学, 2024, 76(3):47-51.
[15] 朱博勤. FAST工程勘察技术理论与实践[M].武汉:湖北科学技术出版社, 2021.
[16] Li D, Pan Z C. The five-hundred-meter aperture spherical radio telescope project[J]. Radio Science, 2016, 51(7):1060-1064.
[17] Peng B, Nan R, Su Y, et al. Five-hundred-meter aperture spherical telescope project[J]. Astrophysics and Space Science, 2001, 278(1):219-224.
[18] Jiang P, Yao R. The latest progress of Five-hundred-meter Aperture Spherical radio Telescope[J]. Science China Technological Sciences, 2022, 65(4):987-988.
[19] Wang P, Li D, Clark C J, et al. FAST discovery of an extremely radio-faint millisecond pulsar from the FermiLAT unassociated source 3FGL J0318.1+0252[J]. Science China Physics, Mechanics&Astronomy, 2021, 64(12):129562.
[20] The Parkes Pulsar Timing Array[EB/OL].[2024-08-05] . https://www.atnf.csiro.au/research/pulsar/ppta/.
[21] The European Pulsar Timing Array[EB/OL].[2024-08-05] . https://www.epta.eu.org.
[22] The North American Nanohertz Observatory for Gravitational Waves[EB/OL].[2024-08-05] . https://nanograv.org.
[23] Xu H, Chen S Y, Guo Y J, et al. Searching for the nano-hertz stochastic gravitational wave background with the Chinese pulsar timing array data release I[J]. Research in Astronomy and Astrophysics, 2023, 23(7):075024.
[24] Hewish A, Bell S J, Pilkington J D H, et al. Observation of a rapidly pulsating radio source[J]. Nature, 1968, 217:709- 713.
[25] Backer D C, Kulkarni S R, Heiles C, et al. A millisecond pulsar[J]. Nature, 1982, 300(5893):615-618.
[26] Kulkarni S R. Discovery of a millisecond pulsar[C]//Proceedings of AIP Conference Proceedings. AIP, 1983:118-125.
[27] Hessels J W T, Ransom S M, Stairs I H, et al. A radio pulsar spinning at 716 Hz[J]. Science, 2006, 311(5769):1901- 1904.
[28] Manchester R N. Millisecond pulsars, their evolution and applications[J]. Journal of Astrophysics and Astronomy, 2017, 38(3):42.
[29] Bhattacharya D, van den Heuvel E P J. Formation and evolution of binary and millisecond radio pulsars[J]. Physics Reports, 1991, 203(1/2):1-124.
[30] Lorimer D R. Binary and millisecond pulsars[J]. Living Reviews in Relativity, 2008, 11(1):8.
[31] Gotthelf E V, Bogdanov S. NuSTAR hard X-Ray observations of the energetic millisecond pulsars PSR B1821-24, PSR B1937+21, and PSR J0218+4232[J]. The Astrophysical Journal, 2017, 845(2):159.
[32] Guillot S, Kerr M, Ray P S, et al. NICER X-ray observations of seven nearby rotation-powered millisecond pulsars[J]. The Astrophysical Journal Letters, 2019, 887(1):L27.
[33] Lyne A, Graham-Smith F, Stappers B. Pulsar astronomy[M]. Cambridge, UK:Cambridge University Press, 2022.
[34] Manchester R N, Hobbs G B, Teoh A, et al. The Australia telescope national facility pulsar catalogue[J]. The Astronomical Journal, 2005, 129(4):1993-2006.
[35] 张承民,潘元月,王德华,等.中子星与脉冲星天体物理[M].北京:科学出版社, 2019.
[36] Sun Y H, Wang D H, Zhang C M, et al. Exploring the statistical properties of gamma-ray normal pulsars[J]. Astrophysics and Space Science, 2024, 369(1):4.
[37] Archibald A M, Stairs I H, Ransom S M, et al. A radio pulsar/x-ray binary link[J]. Science, 2009, 324(5933):1411- 1414.
[38] Bhattacharyya S. The permanent ellipticity of the neutron star in PSR J1023+0038[J]. Monthly Notices of the Royal Astronomical Society, 2020, 498(1):728-736.
[39] Yang Z L, Li B D, Misra P, et al. Properties of PSR J1023+0038 based on Kepler, tess, and fast[J]. The Astrophysical Journal, 2024, 960(1):20.
[40] Lorimer D R, Kramer M. Handbook of pulsar astronomy[M]. Cambridge, UK:Cambridge University Press, 2012.
[41] Zhang C M, Kojima Y. The bottom magnetic field and magnetosphere evolution of neutron star in low-mass X-ray binary[J]. Monthly Notices of the Royal Astronomical Society, 2006, 366(1):137-143.
[42] Kiziltan B, Thorsett S E. Millisecond pulsar ages:Implications of binary evolution and a maximum spin limit[J]. The Astrophysical Journal, 2010, 715(1):335-341.
[43] McLaughlin M A, Lyne A G, Lorimer D R, et al. Transient radio bursts from rotating neutron stars[J]. Nature, 2006, 439:817-820.
[44] 王双强,王娜,张承民,等.特殊类型脉冲星的研究进展[J].天文学进展, 2018, 36(1):1-16.
[45] Shapiro S L, Teukolsky S A. Black holes, white dwarfs, and neutron stars[M]. New York:Wiley, 1983.
[46] Bastian N, Lardo C. Multiple stellar populations in globular clusters[J]. Annual Review of Astronomy and Astrophysics, 2018, 56:83-136.
[47] Gratton R, Bragalia A, Carretta E, et al. What is globular cluster?An observation perspective[J]. The Astronomy and Astrophysics Review, 2019, 27(1):8.
[48] Camilo F, Rasio F A. Pulsar in globular cluters[C]//Astrophysice Society of the Pacific Conference Series. US:San Francisco, 2005:147-170.
[49] Freire P C C. The pulsar population in globular clusters and in the galaxy[J]. Proceedings of the International Astronomical Union, 2012, 8(增刊291):243-250.
[50] Ransom S M. Pulsars in globular clusters[J]. Proceedings of the International Astronomical Union, 2007, 3:291-300.
[51] Ransom S M, Hessels J W T, Stairs I H, et al. Twenty-one millisecond pulsars in Terzan 5 using the Green Bank Telescope[J]. Science, 2005, 307(5711):892-896.
[52] Ivanova N, Heinke C O, Rasio F A, et al. Formation and evolution of compact binaries in globular cluster-II. Binaries with neutron stars[J]. Monthly Notices of the Royal Astronomical Society, 2008, 386(1):553-576.
[53] Galactic globular cluster database version 4[EB/OL].[2024-08-31] . https://people.smp.uq.edu.au/HolgerBaumgardt/globular/.
[54] Lyne A G, Brinklow A, Middleditch J, et al. The discovery of a millisecond pulsar in the globular cluster M28[J]. Nature, 1987, 328:399-401.
[55] Lyne A G, Biggs J D, Brinklow A, et al. Discovery of a binary millisecond pulsar in the globular cluster M4[J]. Nature, 1988, 332:45-47.
[56] Loginov A A, Malov I F. Parameters of radio pulsars in binary systems and globular clusters[J]. Astronomy Reports, 2017, 61(2):115-121.
[57] Lee J, Hui C Y, Takata J, et al. A comparison of millisecond pulsar populations between globular clusters and the galactic field[J]. The Astrophysical Journal, 2023, 944(2):225.
[58] Abbott B P, Abbott R, Abbott T D, et al. Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817[J]. The Astrophysical Journal, 2019, 875(2):160.
[59] 李柯伽,徐仁新.脉冲星与脉冲星计时阵[J].物理, 2024, 53(8):507-511.
[60] Miller M C, Miller J M. The masses and spins of neutron stars and stellar-mass black holes[J]. Physics Reports, 2015, 548:1-34.
[61] Miller M C. Astrophysical constraints on dense matter in neutron stars[M]//Belloni T M, Méndez M, Zhang C M, eds. Timing Neutron Stars:Pulsations, Oscillations and Explosions. Berlin:Springer Berlin Heidelberg, 2020:1-51.
