Covered period: 2016 July 4-10
LAT Mission week: 422.57-423.57
LAT Mission week: 422.57-423.57
- 3C 454.3 was detected with average daily fluxes from 3.1 to 1.7 units (see its light curve).
CTA 102 showed some variability during the week with average daily fluxes from 1.8 to 0.7 units (see its light curve). 4C +01.02 (PKS 0106+01) detected during the week with average daily fluxes of 2.8 to 1.0 units (see its light curve).- The BL Lac object OT 081 (z=0.322) was detected on July 9 and 10 with average daily fluxes of 1 and 0.8 units, respectively. See ATel #9231 for details.
- The BL Lac object PKS 0426–380 (z=1.111) was detected on July 5, 9 and 10 with average daily fluxes of 0.6, 0.9 and 1 units, respectively.
- Other blazars of the week detected sporadically below 1 unit: Mrk 421, AO 0235+164, PKS 2155–
304, PKS B1424–418, PKS 1510–08, BL Lacerate, PKS 1256–220, TXS 2241+406, N GC 1275 and/or IC 310, 1ES 1959+650, S4 0954+65, S5 1044+71.
Fluxes are in the unit of 10^-6 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:
- J. Becerra (Josefa.Becerra[at]nasa.gov) for generic information related to this week
- Contact persons on this page for individual sources cited above.
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:
- J. Becerra (Josefa.Becerra[at]nasa.gov) for generic information related to this week
- Contact persons on this page for individual sources cited above.
No comments:
Post a Comment