The following are the sources the LAT team will monitor during the first year (and most likely throughout the mission). The resulting lightcurves will be posted. This list will most likely grow as the mission progresses. EGRET fluxes are above 100 MeV.
Source Type | Source Name | EGRET Name | Average or Min. Flux (10-8 γ cm-2s-1) |
Galactic Lattitude |
Redshift | TeV Source |
---|---|---|---|---|---|---|
Blazar | 0208-512 | 3EGJ0210-5055 | 85.5 ± 4.5 | -61.9 | 1.003 | |
0235+164 | 3EGJ0237+1635 | 65.1 ± 8.8 | -39.1 | 0.94 | ||
PKS 0528+134 | 3EGJ0530+1323 | 93.5 ± 3.6 | -11.1 | 2.060 | ||
S5 0716+71 | 3EGJ0721+7120 | 17.8 ± 2.0 | 28 | 0.3 | ||
0827+243 | 3EGJ0829+2413 | 24.9 ± 3.9 | 31.7 | 0.939 | ||
OJ 287 | 3EGJ0853+1941 | 10.6 ± 3.0 | 35.8 | 0.306 | ||
Mrk 421 | 3EGJ1104+3809 | 13.9 ± 1.8 | 65.0 | 0.031 | Yes | |
W Com 1219+285 |
3EGJ1222+2841 | 11.5 ± 1.8 | 83.5 | 0.102 | Yes | |
3C 273 | 3EGJ1229+0210 | 15.4 ± 1.8 | 64.5 | 0.158 | ||
3C 279 | 3EGJ1255-0549 | 74.2 ± 2.8 | 57.0 | 0.538 | Yes | |
1406-076 | 3EGJ1409-0745 | 27.4 ± 2.8 | 50.3 | 1.494 | ||
H 1426+428 | NA | 64.9 | 0.129 | Yes | 1510-089 | 3EGJ1512-0849 | 18.0 ± 3.8 | 40.1 | 0.36 |
PKS 1622-297 | 3EGJ1625-2955 | 47.4 ± 3.7 | 13.4 | 0.815 | ||
1633+383 | 3EGJ1635+3813 | 58.4 ± 5.2 | 42.3 | 1.814 | ||
Mrk 501 | NA | 38.9 | 0.033 | Yes | ||
1730-130 NRAO 530 |
3EGJ1733-1313 | 36.1 ± 3.4 | 10.6 | 0.902 | ||
1ES 1959+650 | NA | 17.7 | 0.048 | Yes | ||
PKS 2155-304 | 3EG2158-3023 | 13.2 ± 3.2 | -52.2 | 0.116 | Yes | |
BL_Lacertae (2200+420) |
3EGJ2202+4217 | 39.9 ± 11.6 | -10.4 | 0.069 | Yes | |
3C 454.3 | 3EGJ2254+1601 | 53.7 ± 4.0 | -38.3 | 0.859 | ||
1ES 2344+514 | NA | -9.9 | 0.044 | Yes | ||
HMXB | LSI+61 303 2CG135+01 |
3EGJ0241+6103 | 69.3 ± 6.1 | 1.0 | Yes | |
any source (except Crab, Vela, and Geminga pulsars) | monitor if flux exceeds 2x10-6 cm-2s-1 |
See the LAT team's first year data release plan for the expected latencies.
The lightcurves and spectra of transients sources will also be posted; see the data policy.