Table 4
Variability analysis results according to the V, Vsys3σ, and Vsys2σ indices, divided in to six main source classes.
| Variability | Number of | Source class: Number |
| sources | of variables | |
| Type | (V,Vsys3σ,Vsys2σ) | |
|
|
||
| Variable | 13, 12, 11 | AGN: 7, 8, 8; PSR: 1, 0, 0; |
| PSR∗:1, 1, 1; HMXB: 1, 1, 1; | ||
| CWB: 1, 0, 0; SNR: 0, 0, 0; | ||
| Unidentified: 2, 2, 1 | ||
| Uncertain | 8, 5, 8 | AGN: 2, 1, 3; PSR: 3, 2, 1; |
| HMXB: 1, 0, 1; SNR: 0, 0, 0; | ||
| CWB: 0, 1, 1; Unidentified: 2, 1, 2 | ||
| Non-variable | 21, 25, 34 | AGN: 7, 7, 6; PSR: 4, 6, 8; |
| HMXB: 0, 1, 0; SNR: 2, 2, 2; | ||
| CWB: 0, 0, 0;Unidentified:8, 9, 18 | ||
Notes. The last column lists the number of sources of each variability type found in each source class according to each index, in the same order as in the second column. The PSR∗ source is the Crab pulsar + nebula.
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