Table 2
Results of the maximum likelihood analysis.
| Model name | ST1 | ST2 | FG1 | FG2 |
| Spatial distribution | Exp. | Gauss. | Exp. | Gauss. |
|
|
||||
| R0/σr (kpc) |
|
|
|
|
| z0 (kpc) |
|
|
|
|
| Nexp (103) |
|
|
|
|
| S| b | ≤ 10°, | l | ≤ 30° (10-7)* |
|
|
|
|
| S| b | ≥ 40° (10-7)* |
|
|
|
|
Notes.The scaling parameters R0, σ0, and z0 are given in units of kpc. Nexp is the total number of Galactic MSPs in the Milky Way given in units of 103. S| b | ≤ 10°, | l | ≤ 30° are the estimated integrated average intensity above 100 MeV of the undetectable MSPs in units of 10-7 ph cm-2 s-1 sr-1 from the central Galactic radian, defined by | l | ≤ 30° and | b | ≤ 10°. S| b | ≥ 40° gives the integrated average intensity above 100 MeV of the undetectable MSPs in the same units at high Galactic latitudes (| b | ≥ 40°). All uncertainties are only statistical (2σ confidence level).
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