Thursday, December 4, 2014

Fermi LAT Weekly Report N. 338


Covered period: 2014.November.24 - 2014.November.30
LAT Mission week: 338.57 - 339.57

  • B2 1504+37 detected in flaring activity on November 25, 26, 27, with a daily flux between (0.4+/-0.1)e-6 and (1.3+/-0.2)e-6 (ATel #6760).
  • NGC 1275 (3C 84) detected all week, with a daily flux between (0.7+/-0.1)e-6 and (1.0+/-0.3)e-6.
  • 3C 454.3 detected all week with a daily flux between (1.7+/-0.7)e-6 and (5.4+/-0.9)e-6.
  • 3C 279 detected all week, with a daily flux between (1.9+/-0.3)e-6 and (3.6+/-0.4)e-6.
  • Mrk 421 detected on November 24, 25, 26, 28, 29, and 30, with a daily flux between (0.2+/-0.1)e-6 and (0.5+/-0.2)e-6.
  • PKS 1510-089 detected on November 24, 25, 26, 29, and 30 with a daily flux between (0.4+/-0.1)e-6 and (0.7+/-0.1)e-6.
  • PKS 1424-418 detected on November 26, 28, 29, and 30, with a daily flux between (0.3+/-0.1)e-6 and (0.6+/-0.2)e-6.
  • B2 1520+31 detected on November 25, 28, and 29, with a daily flux between (0.2+/-0.1)e-6 and (0.3+/-0.1)e-6.
  • PKS 0736+01 detected on November 24, 25, and 27, with a daily flux between (0.6+/-0.1)e-6 and (1.4+/-0.3)e-6.
  • PKS B1222+216 (4C +21.35) detected on November 28, 29, and 230, with a daily flux between (0.5+/-0.2)e-6 and (1.6+/-0.5)e-6.
  • Sporadic activity: PKS 2255-282 (November 25 and 26), CTA 102 (November 26 and 27), PKS 1824-582 (November 24), S5 0716+714 (November 24), PKS 0454-234 (November 24), PKS 0402-362 (November 24), Mkn 501 (November 24), 4C +01.02 (November 26), 4C +21.35 (November 27), PKS 0537-441 (November 29), PG 1553+113 (November 30), VER 0521+211 (November 30), 3C 66A (November 30).
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:
- Yutaro Tachibana (tachibana[at]hp.phys.titech.ac.jp) and Yasuyuki Tanaka (ytanaka[at]hep01.hepl.hiroshima-u.ac.jp) for generic information related to this week -
- Contact persons on this page for individual sources cited above.

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