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Table 2
Characteristics of the sky model components assumed in our analysis.
Comp. | G. Lon. position [deg] | G. Lat. position [deg] | Lon. extent (FWHM) [deg] | Lat. extent (FWHM) [deg] |
|
||||
NB | −1.25 | −0.25 | 5.75 | 5.75 |
BB | 0.00 | 0.00 | 20.55 | 20.55 |
Disk | 0.00 | 0.00 | 141.29 | 24.73 |
GCSab | −0.06 | −0.05 | 0.00 | 0.00 |
Craba | −175.44 | −5.78 | 0.00 | 0.00 |
Cyg X-1a | 71.34 | 3.07 | 0.00 | 0.00 |
Notes. The parameters are similar to those of Skinner et al. (2014), except for the extent of the disk. The disk extent has been chosen according to a 2D gridscan for a total maximum likelihood over all 80 bins (see Sect. 3.1).
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