Covered period: 2016 August 29 - September 4
LAT Mission week: 430.57-431.57
- Flare of the GeV-TeV BL Lac object AP Librae with daily flux 1.1e-6 and peak 6h flux 2.5e-6 on Aug.30. More details in ATel#9442.
- Outburst of PKS 1510-08 with daily flux peaking at 5.3e-6 on Sept.3.
- Flare of blazar MG2 J201534+3710 with daily flux 1.6e-6 on Aug.30.
- PKS 1824-582 detected almost all week with daily fluxes above 0.7e-6 and peaking on Sept. 3 with daily flux 1.3e-6.
- CTA 102 detected all week in high state with daily fluxes between about 2.4e-6 and 3.2e-6.
- 3C 454.3 detected all week with daily fluxes between about 1.8e-6 and 3.5e-6.
- Increased activity of Cen A detected on Sep.1 with daily flux 0.8e-6.
- 4C +01.02 (PKS 0106+01) detected all week with daily fluxes between about 0.7e-6 and 1.3e-6.
- S5 1044+71 detected all week with daily fluxes between about 0.6e-6 and 0.8e-6.
- PKS 0502+049 detected all week with daily fluxes between about 0.6e-6 and 0.8e-6.
- BL Lac object 3C 371 detected at 0.2e-6 on Aug.30.
- Possible hard state of the BL Lac object TXS 1055+567 (7C 1055+5644, GB6 J1058+5628, z=0.1433) detected on Sept. 1 with daily flux 0.06e-6 and ph.index 1.5.
- Other blazars of the week detected, also sporadically, around or below 0.5e-6:
PG 1553+113 and 3C 66A (both in possible hard state with flux about 0.1e-6 and photon index about 1.5), MG1 J021114+1051, PKS 2155-304, PKS 1424-41, PKS 1502+106, PKS 2052-47, 1ES 1215+303 (or PG 1218+304), NGC 1275, gravitationally lensed blazar S3 0218+35 (lens B0218+357), 4C +55.17, 1ES 1959+650, PKS 0002-478, S4 1849+67, BL Lac, PKS 0426-380, PKS 0402-362, TXS 2241+406, S4 0110+49.
- Enhanced activity of the microquasar Cyg X-3 being detected during some days of the week.
- Quiet Sun and the Moon detected in a few 6h intervals of the week.
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
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.