Covered period: 2012.Nov.26 - 2012.Dec.02
LAT Mission week: 234.57 - 235.57
- TXS 1318+225 detected on 26, 27, 28 and 29 November with a daily flux between (0.4+/-0.2)e-6 and (0.9+/-0.2)e-6. On 26 November the source reached its maximum flux increasing of a factor around 35 with respect to the average 2FGL flux. An ATel on the enhanced gamma-ray activity of this source was posted (ATel#4609).
- MG1 J123931-0443 bright all the week but 29 and 30 November, with daily fluxes between (0.6+/-0.2)e-6 and (1.1+/-0.3)e-6.
- Mrk 421 detected on 27, 29, 30 November, 1 and 2 December with daily fluxes ranging between (0.3+/-0.1)e-6 and (0.5+/-0.2)e-6.
- 4C+38.41 detected on 26, 30 November and 1 December with a daily flux of (1.0+/-0.3)e-6, (0.7+/-0.3)e-6 and (0.9+/-0.2)e-6, respectively.
- The gravitationally lensed blazar S4 0218+35 was bright on 28 November, 1 and 2 December with daily fluxes between (0.6+/-0.2)e-6 and (1.4+/-0.2)e-6.
- PKS 1424-418 detected on 30 November, 1 and 2 December with a daily flux of (0.8+/-0.2)e-6, (0.6+/-0.2)e-6 and (0.5+/-0.2)e-6, respectively.
- PKS 1510-089 detected on 27 and 28 November with a daily flux of (0.9+/-0.3)e-6 and (1.1+/-0.2)e-6, respectively.
- PKS 0426-380 was bright on 30 November and 1 December with a daily flux of (0.5+/-0.2)e-6 and (0.6+/-0.3)e-6, respectively.
- PKS 1124-186 detected on 1 and 2 December with a daily flux of (0.7+/-0.2)e-6 and (0.3+/-0.1)e-6, respectively.
- Finally, S3 0827+24 detected on 26 November at a daily flux of (1.0+/-0.2)e-6, 4C+21.35 detected on 27 November at a daily flux of (1.0+/-0.3)e-6 and PKS 0454-234 bright on 2 December with a daily flux of (1.1+/-0.3)e-6.
- Sporadic daily detections of blazars (fluxes below 1e-6): B2 1846+32A (29 Nov.), BL Lac, 4C+55.17, PKS 2233-148 (30 Nov.), PKS 2155-304 (1 Dec.).
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:
- E. Torresi (torresi[at]iasfbo.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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