Covered period: 2017 April 10-16
LAT Mission week: 462.57-463.57
- CTA 102 detected all week in high state with daily fluxes between about 1.1e-6 and 2.5e-6. See also the Flare GCN/FERMI NOTICE #1492356303.
- 3C 454.3 detected all week with daily fluxes between about 1.4e-6 and 2.1e-6.
- PKS 2247-131 detected all week with daily fluxes between about 0.6e-6 and 1.2e-6.
- 3C 279 detected almost all week with daily fluxes between about 0.5e-6 and 1.2e-6.
- Flare of the VHE blazar 1ES 1215+303 (B2 1215+30, ON 325) with daily flux 0.8e-6 on April 13. More details in ATel#10270.
- Flare of PMN J2141-6411 with daily flux 0.4e-6 on April 10.
- Further bright blazars detected, also sporadically, during the week with daily flux between about 0.7e-6 and 0.8e-6: 3C 279, 3C 273, PKS 1510-08, 4C +01.02 (PKS 0106+01).
- Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
NGC 1275, S5 1044+71, S4 1030+61, BL Lac, PKS 1424-41, PKS 1441+25, 3C 66A, Mkn 421, PKS 1502+106, PKS 1510-08, S5 0716+71, PG 1553+113, PKS 2023-07, PKS 2155-304, 3C 66A, 4C +31.03 (OC 317), 4C +28.07, 4C +55.17, 4C +31.03, PKS 0447-439, PKS 0426-380, PKS 0438-43, B2 1436+37B, B3 1343+451, RX J0115.7+2519, PMN J1332-1256, S5
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are statistical only.
Note. All the flux reported above are by the ASP analysis and should be considered preliminary and should not be used for publication, however they are indicative of the flux range and the current status of a source. Source association is done on the basis of source location, considering spatial coincidence only, and it is not indicative of an identification.
- Please acknowledge the LAT team if you use information from this report.
For questions and comments please contact:
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to this week
- Contact persons on this page for individual sources cited above.