Covered period: 2016 March 28 - April 3
LAT Mission week: 408.57-409.57
- CTA 102 is the brightest extragalactic source of the week with daily fluxes between 1.3e-6 and 2.9e-6.
- 3C 454.3 detected all week with daily fluxes between 0.7e-6 and 1.2e-6.
- TXS 2241+406 detected all week with daily fluxes between 0.5e-6 and 1.0e-6, peaking in the first part of the week.
- TXS 2358+209 detected in high state with daily flux 1.0e-6 on April 2.
- S4 1800+44 detected in high state with daily flux 0.8e-6 on March 31.
- 4C +01.02 (PKS 0106+01) detected all week with daily fluxes between 0.7e-6 and 0.9e-6.
- Detection, on March 30, in the vicinity of both 1RXS J053629.4-334302 (2FHL J0536.4-3342) and PKS 0534-340 (no LAT catalogs) with daily flux 0.4e-6.
- MH 2136-428 detected with daily hard photon spectral index of 1.4+/-0.2 on April 1st.
- Further blazars detected in bright state in some days of the week, with daily fluxes between 0.5e-6 and 0.7e-6: PKS 2023-07, PKS 1502+106, 3C 279, PKS 1424-41, NGC 1275, S5 1044+71, NRAO 676 (TXS 2159+505).
- Other blazars of the week detected, also sporadically, around or below the daily flux level of 0.5e-6: S5 0716+71, S5 1039+81, 1ES 1215+303, BL Lac, OJ 287, Mkn 421, Ton 599, S4 1030+61, PKS 1510-08, AO 0235+164, TXS 2358+209, 4C +01.28 (PKS 1055+01), PKS 0454-234, PKS 2155-304, PKS 2136-642, B2 2113+29.
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.
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