Covered period: 2016.Mar.21 - 2016.Mar.27
LAT Mission week: 407.57 - 408.57
- S4 1800+44 detected all week with a daily flux between (0.3±0.2) and (2.5±0.2).
- CTA 102 detected all week with a daily flux between (1.5±0.2) and (2.8±0.3).
- PKS 2023-07 detected all week with a daily flux between (0.6±0.1) and (1.6±0.2). AGILE detected an increased activity from this source from 25 Mar to 27 Mar. SeeATel#8879.
- 3C 454.3 detected all week with a daily flux between (0.5±0.2) and (1.4±0.3).
- TXS 2241+406 detected from 22 Mar to 25 Mar with daily flux between (0.9±0.2) and (1.3±0.2).
- Preliminary no activity was detected for AGL J1835-6040 during 23 and 24 Mar. See ATel#8866.
- Sporadic daily detections of blazars (fluxes below 1): BL Lacertae, OG 050, AO 0235+164, PKS 1502+106, NGC 1275, S4 1738+49, 4C +40.25, S4 1030+61, Mkn 421, 4C +01.02, OJ 287, S5 1044+71, 3C 279, S5 0716+71, S5 0836+71, Mrk 501, PKS 1424-41, PKS 2032+107, PKS 1830-211, B2 1846+32B, TXS 2358+209, PKS 2155-304.
Fluxes are in the unit of 10-6photons/cm2/s above 100 MeV. All errors are statistical only.
Note. All the fluxes reported above are from 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.
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