Table A.2
Spectral parameters for each component from the alternative bulge emission model.
| Cont. flux dens. | Line Flux | FWHM | ΔE0 | o-Ps Flux | Pos. frac. | χ2/d.o.f. | |
| The bulge | 2.31(91) | 15.1(2.3) | 2.35(34) | 0.24(17) | 82.6(31.6) | 1.05(9) | 61.53/74 |
| Disk (−180°<l< 180°) | 5.76(1.69) | 18.4(6.0) | 3.25(98) | −0.08(36) | 41.8(48.9) | 0.80(39) | 69.48/74 |
| GCS | 0.09(5) | 0.9(2) | 3.04(54) | −0.24(28) | 2.3(1.7) | 0.85(23) | 63.98/74 |
| Craba | 2.20(7) | < 0.7 | −(−) | −(−) | −(−) | −(−) | 66.88/78 |
| Cygnus X-1a | 0.66(6) | < 0.2 | −(−) | −(−) | −(−) | −(−) | 73.38/78 |
| Galaxy (total) | 10.71(1.29) | 34.3(3.9) | 2.77(29) | 0.10(11) | 137.9(44.3) | 0.97(9) | 73.70/74 |
Notes. Continuum flux densities are given as the value at 511 keV in units of 10-5 ph cm-2 s-1 keV-1, line and ortho-positronium fluxes are given in 10-4 ph cm-2 s-1, FWHM of the celestial emission line in keV, and the centroid shift ΔE0 = Epeak−Elab in keV.
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