Fermi LAT Weekly Report N. 337

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Covered period: 2014.November.17 - 2014.November.23
LAT Mission week: 337.57 - 338.57

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• PKS 0736+01 detected in flaring activity on November 18, 20, 22, 23, with a daily flux between (0.5+/-0.2)e-6 and (1.1+/-0.3)e-6 (ATel #6731). The high activity of the source was confirmed by Swift observations in optical, UV and X-rays (ATel #6742).
• 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 (1.2+/-0.4)e-6 and (2.4+/-0.6)e-6.
• PKS 1424-418 detected on November 17, 18, 19, 21, 22, and 23, with a daily flux between (0.2+/-0.1)e-6 and (0.8+/-0.2)e-6.
• PKS 1824-582 detected on November 17, 18, 19, 20, and 23, with a daily flux between (0.9+/-0.1)e-6 and (2.5+/-0.4)e-6.
• B2 1520+31 detected on November 19, 20, 21, 22, and 23, with a daily flux between (0.4+/-0.1)e-6 and (0.7+/-0.2)e-6.
• S5 0716+714 detected on November 17, 19, 20, 22, and 23, with a daily flux between (0.3+/-0.1)e-6 and (0.6+/-0.2)e-6.
• Mrk 421 detected on November 17, 20, 21, 22, and 23, with a daily flux between (0.2+/-0.1)e-6 and (0.5+/-0.2)e-6.
• 4C +21.35 (PKS 1222+21) detected on November 17, 20, 21, and 22, with a daily flux between (1.3+/-0.3)e-6 and (2.9+/-0.5)e-6.
• 3C 279 detected on November 19, 21, 22, and 23 with a daily flux between (0.8+/-0.3)e-6 and (2.2+/-0.4)e-6.
• PKS 1510-089 detected on November 18, 21, 22, and 23 with a daily flux between (0.5+/-0.1)e-6 and (0.9+/-0.2)e-6.
• PKS 0454-234 detected on November 17, 18, 20, and 22, with a daily flux between (0.3+/-0.1)e-6 and (0.7+/-0.2)e-6.
• S4 0954+65 detected on November 17, 18, and 19, with a daily flux between (0.6+/-0.2)e-6 and (0.9+/-0.2)e-6.
• Sporadic activity (fluxes below 1e-6): B2 1144+40 (November 17 and 21), PKS 2326-502 (November 17), PKS 0426-380 (November 17), 4C +01.02 (November 19), CTA 102 (November 19), B2 0200+30 (November 20), B2 0716+33 (November 20).

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:
- Filippo D'Ammando (dammando[at]ira.inaf.it) and Monica Orienti (orienti[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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