Simulation of the Galactic field millisecond pulsar population and its gamma- and X-ray emission

Monte Carlo simulation of the millisecond pulsar population in the Galactic field. The simulation includes four spatial components: the disk; the boxy bulge; the nuclear stellar cluster; the nuclear stellar disk. The last 3 components together form the Galactic bulge. There is one file per component, each containing at least 100 Monte Carlo simulations. Each line contains: the longitude L in deg; the latitude B in deg; the line of sight S in kpc; the 0.1-100 GeV gamma-ray flux in erg/cm^2/s; the X-ray spectral index; the gamma-to-X flux ratio, where the gamma-ray flux is the same as in the fourth column and the X-ray flux is the 2-10 keV unabsorbed one of a simulated MSP. More information about the simulation can be found in the related paper.

银河系场域内毫秒脉冲星（millisecond pulsar）群体的蒙特卡洛（Monte Carlo）模拟。本次模拟包含四类空间成分：银盘、盒状核球、核星团以及核恒星盘。后三类成分共同构成银河系核球。每类成分对应一个数据文件，每个文件至少包含100次蒙特卡洛模拟。每行数据包含以下内容：以度（deg）为单位的银经L、以度为单位的银纬B、以千秒差距（kpc）为单位的视线距离S、0.1~100 GeV能段的γ射线流量（单位：erg/cm²/s）、X射线谱指数、γ射线与X射线流量比值，其中γ射线流量与第四列数值一致，X射线流量为模拟毫秒脉冲星（MSP）未被吸收的2~10 keV能段流量。有关本次模拟的更多信息可参阅相关研究论文。