Wednesday, December 19, 2012

Fermi LAT Weekly Report N. 236



Covered period: 2012.December.10 - 2012.December.16
LAT Mission week: 236.57 - 237.57

  • PKS 0454-234 detected all week, with a daily flux between (0.7±0.2) X 10-6 and (1.1±0.2) X 10-6.
  • PKS 0426-380 detected on 11, 12, 13, 14, 15, and 16 December, with a daily flux between (0.6±0.2) X 10-6 and (0.8±0.2) X 10-6.
  • MG1 J123931+0443 detected on 10, 13, 14, 15, and 16 December, with a daily flux between (0.5±0.2) X 10-6 and (1.6±0.3) X 10-6.
  • PKS 1510-089 detected on 12, 13, 14, 15, and 16 December, with a daily flux between (0.8±0.3) X 10-6 and (2.0±0.5) X 10-6.
  • PKS B1424-418 detected on 10, 11, 13, and 15 December, with a daily flux between (0.9±0.3) X 10-6 and (1.4±0.3) X 10-6.
  • CTA 102 detected on 10, 11, 12, and 16 December, with a daily flux between (0.6±0.2) X 10-6 and (1.1±0.3) X 10-6.
  • S3 0218+35 detected on 10, 11, and 13 December, with a daily flux between (0.9±0.2) X 10-6 and (1.2±0.2) X 10-6.
  • PKS 1124-186 detected on 11, 12, and 14 December, with a daily flux between (0.3±0.1) X 10-6 and (0.6±0.2) X 10-6.
  • PKS 0521-36 detected in high activity on 12 December, with a daily flux of (1.8±0.2) X 10-6.
  • OJ 248 detected on 12, and 13 December, with a daily flux of (1.5±0.3) X 10-6 and (0.3±0.2) X 10-6, respectively.
  • Sporadic activity (fluxes below 1 X 10-6): B2 1324+22 (10 December), 4C +38.41 (10 and 11 December), Mkn 421 (11 and 14 December), PMN J2345-1555 (11 and 13 December), PKS 0250-225 (12 December), PKS 2233-148 (12 December), S5 0716+714 (16 December).
  • 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 (filippo.dammando[at]fisica.unipg.it) for generic information related to this week
    - Contact persons on this page for individual sources cited above.


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