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.