Covered period: 2015.Nov.16 - 2015.Nov.22
LAT Mission week: 389.57 - 390.57
- 4C +40.25 (B2 1020+40) was detected Nov. 20 through Nov. 22 with daily averaged fluxes between (0.4 +/- 0.1) and (0.8 +/- 0.2). See ATel #8339 for more information.
- B2 1846+32B was detected Nov. 19 and Nov. 20 with daily averaged fluxes of (1.0 +/- 0.1). See ATel #8315 for more information.
- TXS 2241+406 was detected all week with daily averaged fluxes between (0.2 +/- 0.1) and (1.2 +/- 0.2). See ATel #8319 for more information.
- Ton 599 was detected all week with daily averaged fluxes between (0.4 +/- 0.1) and (1.0 +/- 0.2). See ATel #8319 for more information.
- 4C +01.02 (PKS 0106+01) was detected all week with daily averaged fluxes between (0.4 +/- 0.1) and (2.8 +/- 0.3). See ATel #8319 for more information.
- 3C 454.3 was detected all week with daily averaged fluxes between (1.6 +/- 0.3) and (3.2 +/- 0.3).
- PKS 0336-01 was detected all week with daily averaged fluxes between (0.4 +/- 0.1) and (1.4 +/- 0.2).
- S5 0836+71 (4C +71.07) was detected Nov. 19 and Nov. 20 with daily averaged fluxes of (0.8 +/- 0.1) and (0.9 +/- 0.2), respectively.
- 3C 279 was detected all week with daily averaged fluxes between (0.9 +/- 0.3) and (1.5 +/- 0.3).
- PKS 1424-41 was detected all week with daily averaged fluxes between (0.7 +/- 0.3) and (1.1 +/- 0.3).
- Sporadic daily detections of blazars (fluxes below 1): S5 0716+71, NGC 1275, PKS 0426-380, S4 0917+44, PKS 1550-242, PKS 0454-234, Mkn 421, AO 0235+164, 3C 273, PKS 0736+01, PKS 1502+106, PKS 2032+107, S5 0716+71, B2 1504+37, PMN J2345-1555, PKS 2320-035, S5 1803+784, PKS 2155-304, PKS 2023-07, 1ES 1959+650.
Fluxes are in the unit of 10-6 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:
- R. Ojha (roopesh.ojha[at]gmail.com) for generic information related to this week
- Contact persons on this page for individual sources cited above.
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