Table A.3
Results of the spectral analysis of the most significant sources detected with AGILE in this analysis.
| ID | TeV Source | Type | AGILE power-law | AGILE | Fermi | 3FGL power-law |
| spectral index21 | association | association | spectral index22 | |||
|
|
||||||
| 1 | TeVJ0006+727 | PWN | 1.91 ± 0.05 | 1AGLR J0007+7307 | 3FGL J0007.0+7302 | 1.88 |
| 12 | TeVJ0222+430 | IBL | 2.04 ± 0.10 | 1AGLR J0222+4305 | 3FGL J0222.6+4301 | 1.94 |
| 15 | TeVJ0240+612 | XRB | 2.19 ± 0.04 | 1AGLR J0240+6115 | 3FGL J0240.5+6113 | 2.29 |
| 19 | TeVJ0319+415 | FRI | 1.80 ± 0.14 | 1AGLR J0321+4137 | 3FGL J0319.8+4130 | 2.08 |
| 26 | TeVJ0534+220 | PWN | 2.27 ± 0.03 | 1AGL J0535+2205 | 3FGL J0534.5+2201 | 2.23 |
| 30 | TeVJ0616+225 | SNR | 1.95 ± 0.07 | 1AGL J0617+2236 | 3FGL J0617.2+2234e | 1.98 |
| 32 | TeVJ0632+173 | PWN | 1.88 ± 0.02 | 1AGL J0634+1748 | 3FGL J0633.9+1746 | 1.87 |
| 36 | TeVJ0721+713 | LBL | 1.87 ± 0.07 | 1AGLR J0723+7121 | 3FGL J0721.9+7120 | 2.04 |
| 45 | TeVJ1018-589 | BIN | 2.07 ± 0.11 | 1AGLR J1018-5852 |
|
|
| 66 | TeVJ1418-609 | PWN | 2.00 ± 0.07 | 1AGLR J1417-6108 | 3FGL J1418.6-6058 | 2.27 |
| 75 | TeVJ1459-608 | PWN | 2.16 ± 0.12 | – |
|
|
| 87 | TeVJ1632-478 | UNID | 2.05 ± 0.14 | – | 3FGL J1633.0-4746e | 2.11 ± 0.02 |
| 88 | TeVJ1634-472 | UNID | 2.58 ± 0.08 | 1AGL J1639-4702 | – | – |
| 95 | TeVJ1708-443 | PWN | 2.02 ± 0.02 | 1AGL J1709-4428 | 3FGL J1709.7-4429 | 2.02 |
| 109 | TeVJ1747-248 | GC | 1.99 ± 0.17 | – | 3FGL J1748.0-2447 | 2.26 |
| 112 | TeVJ1801-233 | SNR/MC | 2.07 ± 0.07 | 1AGL J1801-2317 | 3FGL J1801.3-2326e | 2.15 |
| 113 | TeVJ1804-216 | UNID | 2.13 ± 0.12 | 1AGLR J1805-2149 | 3FGL J1805.6-2136e | 2.07 |
| 125 | TeVJ1841-055 | UNID | 2.41 ± 0.08 | 1AGLR J1839-0550 | 3FGL J1840.9-0532e | 1.81 ± 0.04 |
| 132 | TeVJ1907+062 | UNID | 2.36 ± 0.07 | 1AGL J1908+0614 | 3FGL J1907.9+0602 | 2.24 |
| 133 | TeVJ1911+090 | SNR/MC | 2.21 ± 0.12 | – | – | – |
| 135 | TeVJ1923+141 | SNR/MC | 2.23 ± 0.12 | 1AGL J1923+1404 | 3FGL J1923.2+1408e | 2.15 |
| 142 | TeVJ2019+368 | PWN | 1.98 ± 0.04 | 1AGLR J2021+3653 | 3FGL J2021.1+3651 | 2.17 |
| 144 | TeVJ2032+415 | UNID | 2.05 ± 0.10 | 1AGLR J2031+4130 | 3FGL J2032.2+4126 | 2.08 |
| 147 | TeVJ2227+608 | SNR | 2.30 ± 0.06 | 1AGL J2231+6109 | 3FGL J2225.8+6045 | 1.95 ± 0.20 |
Notes. The spectral indexes for all sources that were detected with a significance 
(see upper part of Table A.3) and Galactic latitude | b | < 30° are reported. The last column shows the Fermi power–law index as given in the indicated reference; when the Fermi sources spectrum has been fitted with a power–law function (i.e. the spectral form is PowerLaw), the corresponding error is also available and reported.
(Acero et al. 2015). The errors on the Fermi power-law spectral indices in the 3FGL catalog are available only for three sources: 3FGL J1633.0-4746e, 3FGL J1840.9-0532e, 3FGL J2225.8+6045. See also footnote(5).
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