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Table 4
γ-ray pulsars used to evaluate the instrument stability for E100 MeV.
| AGL source name | (l, b) positioning | γ-ray flux |
|
Counterpart name | |||
|
|
|||||||
| (degrees) | (10-8 ph. cm-2 s-1) | ||||||
| AGL J0247+6027 | (136.71, 0.70) ± 0.37 ± 0.1 | 11 ± 3 | 4.4 | PSR J0248+6021 | |||
| AGL J0303+7438 | (131.46, 13.98) ± 0.43 ± 0.1 | 7 ± 2 | 4.0 | PSR J0308+7442 | |||
| AGL J1136-6053 | (293.90, 0.67) ± 0.35 ± 0.1 | 12 ± 3 | 4.5 | LAT PSR J1135-6055 | |||
| AGL J1435-5932 | (315.68, 0.75) ± 0.70 ± 0.1 | 13 ± 4 | 4.0 | LAT PSR J1429-5911 | |||
| AGL J1953+3254 | (68.76, 2.86) ± 0.18 ± 0.1 | 17 ± 2 | 8.3 | PSR J1952+3252 | |||
| AGL J2224+6113 | (106.20, 3.20) ± 0.43 ± 0.1 | 11 ± 2 | 5.7 | PSR J2229+6114 | |||
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