Thursday, January 23, 2014

Fermi LAT Weekly report N. 293



Covered period: 2014.January.13 - 2014.January.19
LAT Mission week: 293.57 - 294.57

  • S5 1044+71 detected in flaring activity on January 17 with a daily flux (1.3±0.4) X 10-6. See ATel#5784. The source was also detected on January 16 and 18, with a daily flux (0.9±0.4) X 10-6 and (0.6±0.3) X 10-6, respectively.
  • 3C 279 detected from January 13 to 18, with a daily flux between (0.6±0.2) X 10-6 and (2.5±0.4) X 10-6.
  • 4C +38.41 detected on January 13, 14, 15, 17, and 19, with a daily flux between (0.5±0.1) X 10-6 and (0.7±0.1) X 10-6.
  • NGC 1275 detected on January 14, 15, 17, 18, and 19, with a daily flux between (0.7±0.2) X 10-6 and (1.1±0.3) X 10-6.
  • B3 1343+451 detected on January 14, 15, 16, 18, and 19, with a daily flux between (0.3±0.1) X 10-6 and (0.6±0.2) X 10-6.
  • PKS 2326-502 detected on January 13, 15, 17, and 18, with a daily flux between (0.6±0.2) X 10-6 and (1.0±0.3) X 10-6.
  • PKS 1510-08 detected on January 13, 18, and 19, with a daily flux between (0.4±0.1) X 10-6 and (0.9±0.2) X 10-6.
  • 4C +21.35 detected from January 15 to 17, with a daily flux between (0.5±0.2) X 10-6 and (0.6±0.2) X 10-6.
  • CTA 102 detected on January 16 with a daily flux of (1.8±0.9) X 10-6.
  • Sporadic activity (daily fluxes below 10-6): PKS 0135-247 (January 13), PKS 1424-418 (January 14 and 16), PKS 0735+17 (January 15), S4 1144+40 (January 15), GB6 J1542+6129 (January 15), 4C +28.07 (January 16), PKS 0426-380 (January 17), PKS 2322-482 (January 17), Mrk 501 (January 18), B2 1520+31 (January 19), and 1ES 1959+650 (January 19).
  • Fluxes are in the unit of photons/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.
    - Please acknowledge the LAT team if you use information from this report.

    For questions and comments please contact:
    - M. Orienti (orienti[at]ira.inaf.it) and F. D'Ammando (dammando[at]ira.inaf.it) for generic information related to this week
    - Contact persons on this page for individual sources cited above.


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