标题： 费米大面积望远镜的脉冲星结果 显示英文标题

标题： Pulsar Results with the Fermi Large Area Telescope

摘要： 费米伽马射线空间望远镜的发射标志着脉冲星伽马射线研究新时代的到来。已确认的伽马射线脉冲星数量从6-7个增加到60多个，而费米上的大视场望远镜（LAT）的卓越灵敏度使得对其能谱和光变曲线的详细研究成为可能。其中24个脉冲星是在伽马射线数据的盲搜索中发现的，目前有21个是无线电宁静态的，尽管进行了深入的无线电后续观测。此外，毫秒脉冲星已被确认为一类伽马射线发射体，无论是单个还是作为球状星团中的集体存在。最近，在没有可能对应源的方向上针对LAT源进行的无线电搜索非常成功，导致大量新毫秒脉冲星的发现。综合这些发现，有望大大改善我们对脉冲星伽马射线辐射特性和银河系脉冲星群体的理解。我们总结了这些新探测到的脉冲星及其定时和多波段后续观测的一些结果。 显示英文摘要

摘要： The launch of the Fermi Gamma-ray Space Telescope has heralded a new era in the study of gamma-ray pulsars. The population of confirmed gamma-ray pulsars has gone from 6-7 to more than 60, and the superb sensitivity of the Large Area Telescope (LAT) on Fermi has allowed the detailed study of their spectra and light curves. Twenty-four of these pulsars were discovered in blind searches of the gamma-ray data, and twenty-one of these are, at present, radio quiet, despite deep radio follow-up observations. In addition, millisecond pulsars have been confirmed as a class of gamma-ray emitters, both individually and collectively in globular clusters. Recently, radio searches in the direction of LAT sources with no likely counterparts have been highly productive, leading to the discovery of a large number of new millisecond pulsars. Taken together, these discoveries promise a great improvement in the understanding of the gamma-ray emission properties and Galactic population of pulsars. We summarize some of the results stemming from these newly-detected pulsars and their timing and multi-wavelength follow-up observations.