无线电干扰和瞬变的盲测
Blind surveys for radio pulsars and transients
摘要：
寻找中子星的主要目的是：（i）准确地普查中子星的星族及其起源和演化;（ii）将中子星与银河系中的其他恒星星族和球状星团联系起来;（iii）研究银河系天文学（星际介质和磁场）;（iv）发现和研究新的令人感兴趣的单个物体;（v）研究脉冲星现象学;（六）寻找能提高脉冲星定时阵列灵敏度的脉冲星。这篇评论的重点是盲目的（即大面积）搜索无线电信标。我将总结我们使用的方法，他们提出的一些挑战，看看一些最近和目前正在进行的努力，我也将看看这个领域的扩展到传统的脉冲星研究领域以外的团体，突出无线电瞬变的发现，并展望未来。在其他波长上发现的脉冲星将在本卷的其他地方进行评述。
英文摘要：
The main reasons for searching for pulsars are to: (i) get an accurate census of the neutron star population and its origin and evolution; (ii) connect neutron stars to other stellar populations in the Galaxy and globular clusters; (iii) study Galactic astronomy (the interstellar medium and magnetic field); (iv) find and study new interesting individual objects; (v) study pulsar phenomenology; (vi) find pulsars to add to the sensitivity of pulsar timing arrays. This review focuses on blind (i.e. large area) searches for radio pulsars. I'll summarize the methods we use, some of the challenges they present, look at some of the recent and current efforts going on. I will also look at outreach of this area to groups outside the traditional area of pulsar research, highlight the discoveries of radio transients and look ahead to the future. Pulsars found at other wavelengths will be reviewed elsewhere in this volume.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
