This page was adapted from the publicly available page LAT Monitored Sources
This page was last modified on Fri Feb 6 16:40:55 UTC 2009 (5.87361 hours later)
Source Type | Source Name | EGRET Name | BAT monitor Source Name | Average or Min. EGRET Flux above 100 MeV (10-8 γ cm-2s-1) |
Galactic Lattitude |
Redshift | TeV Source |
---|---|---|---|---|---|---|---|
Blazar | 0208-512 | 3EGJ0210-5055 | QSO B0208-5115 | 85.5 ± 4.5 | -61.9 | 1.003 | |
0235+164 | 3EGJ0237+1635 | AO 0235+16 | 65.1 ± 8.8 | -39.1 | 0.94 | ||
PKS 0528+134 | 3EGJ0530+1323 | PKS 0528+134 | 93.5 ± 3.6 | -11.1 | 2.060 | ||
S5 0716+71 | 3EGJ0721+7120 | QSO B0716+714 | 17.8 ± 2.0 | 28 | 0.3 | ||
0827+243 | 3EGJ0829+2413 | QSO J0830+2411 | 24.9 ± 3.9 | 31.7 | 0.939 | ||
OJ 287 | 3EGJ0853+1941 | 3EG J0853+1941 | 10.6 ± 3.0 | 35.8 | 0.306 | ||
Mrk 421 | 3EGJ1104+3809 | Mrk 421 | 13.9 ± 1.8 | 65.0 | 0.031 | Yes | |
W Com 1219+285 |
3EGJ1222+2841 | QSO B1219+285 | 11.5 ± 1.8 | 83.5 | 0.102 | Yes | |
3C 273 | 3EGJ1229+0210 | 3C 273 | 15.4 ± 1.8 | 64.5 | 0.158 | ||
3C 279 | 3EGJ1255-0549 | 3C 279 | 74.2 ± 2.8 | 57.0 | 0.538 | Yes | |
1406-076 | 3EGJ1409-0745 | QSO B1406-074 | 27.4 ± 2.8 | 50.3 | 1.494 | ||
H 1426+428 | NA | H 1426+428 | 64.9 | 0.129 | Yes | 1510-089 | 3EGJ1512-0849 | QSO J1512-0906 | 18.0 ± 3.8 | 40.1 | 0.36 |
PKS 1622-297 | 3EGJ1625-2955 | PKS 1622-297 | 47.4 ± 3.7 | 13.4 | 0.815 | ||
1633+383 | 3EGJ1635+3813 | 4C 38.41 | 58.4 ± 5.2 | 42.3 | 1.814 | ||
Mrk 501 | NA | Mrk 501 | 38.9 | 0.033 | Yes | ||
1730-130 NRAO 530 |
3EGJ1733-1313 | QSO B1730-130 | 36.1 ± 3.4 | 10.6 | 0.902 | ||
1ES 1959+650 | NA | 1ES 1959+650 | 17.7 | 0.048 | Yes | ||
PKS 2155-304 | 3EG2158-3023 | PKS 2155-304 | 13.2 ± 3.2 | -52.2 | 0.116 | Yes | |
BL_Lacertae (2200+420) |
3EGJ2202+4217 | QSO B2200+420 | 39.9 ± 11.6 | -10.4 | 0.069 | Yes | |
3C 454.3 | 3EGJ2254+1601 | 3C 454.3 | 53.7 ± 4.0 | -38.3 | 0.859 | ||
1ES 2344+514 | NA | 1ES 2344+514 | -9.9 | 0.044 | Yes | ||
HMXB | LSI+61 303 2CG135+01 |
3EGJ0241+6103 | 2CG 135+01 | 69.3 ± 6.1 | 1.0 | Yes | |
any source (except Crab, Vela, and Geminga pulsars) | monitor if flux exceeds 2x10-6 cm-2s-1 |
This page was last modified on Fri Feb 6 16:41:01 UTC 2009
The BAT Transient Monitor contact is:
Hans Krimm,
hans.krimm@nasa.gov,
301-286-6955