Wednesday, December 31, 2014

Fermi LAT Weekly Report N. 341


Covered period: 2014 December 15 - 21
LAT Mission week: 341.57 - 342.57
  • 3C 454.3 detected all week long with daily averaged fluxes between 2.0e-6 and 7.1e-6.
  • 4C +01.02 (PKS 0106+01) detected in flaring activity in the second part of the week with daily averaged flux around 1.0e-6. See ATel#6844 for more details.
  • PKS 1510-08 detected in most days of the week with daily averaged flux between 0.6e-6 and 0.9e-6.
  • PKS 0402-362 detected in some days of the week peaking at 1.2e-6 on Dec. 19. See GCN/FERMI Notice 1419868271 reporting activity on Dec. 29.
  • B2 1144+40 detected in high state with daily flux 1.0e-6 on Dec. 20.
  • PKS 2142-75 detected on Dec. 15, 17 and 19 with daily averaged flux between 0.7e-6 and 1.0e-6.
  • PKS 0736+01 detected in high state with daily flux 0.9e-6 on Dec. 15.
  • PKS 0116-219 detected in high state with daily flux 0.8e-6 on Dec. 16.
  • PKS 2032+107 detected in high state with daily flux 0.7e-6 on Dec. 20.
  • PKS 0426-380, TXS 2241+406 and NGC 1275 (Per A, 3C 84) detected in some days of the week, all with daily flux around 0.6e-6.
  • 3C 279 detected with daily flux 0.9e-6 on Dec. 16.
  • Further daily-detected blazars (fluxes below 0.6e-6): S5 1217+71, S5 0716+71, 1ES 2322-409, B2 1520+31, GB6 J0742+5444 (RX J0742.6+5444), S4 0954+65, VER 0521+211 (MG2 J052147+2112), Ton 599, Mkn 421, PKS 2155-304.
  • Unidentified source Fermi J1057-6027 (2FGL J1056.2-6021) detected several times during the week with daily flux around 1.0e-6.

Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are statistical only.
  
Note. All the flux reported above are by 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:
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to this week
- Contact persons on this page for individual sources cited above.


Monday, December 29, 2014

Fermi LAT Weekly Report N. 340


Covered period: 2014.December.08 - 2014.December.14
LAT Mission week: 340.57 - 341.57

  • 3C 454.3 detected all week long with daily averaged fluxes between (2.0+/-0.3) and (4.4+/-0.4).
  • PKS 1510-089 detected on Dec. 11 and 12 with a daily averaged flux (1.2+/-0.2) and (0.7+/-0.2), respectively.
  • PG 1222+216 (4C +21.35) detected on Dec. 11 with a daily averaged flux of (1.0+/-0.2).
  • CTA 102 detected on Dec. 8, 11 and 12 with daily averaged fluxes between (0.9+/-0.3) and (1.1+/-0.3).
  • TXS 2241+406 detected on Dec. 13 and 14 with a daily averaged flux of (0.7+/-0.1) and (0.4+/-0.1), respectively. These fluxes correspond to 13 and 8 times the flux reported in the 2FGL catalog for this source.
  • PKS 0736+01 detected on Dec. 14 with a daily averaged flux of (1.6+/-0.3).
  • 1H 0323+342 detected on Dec. 9 with a daily averaged flux of (0.6+/-0.2).
  • Sporadic daily detections of other blazars (fluxes below 1): NGC 1275/IC 310Mkn 421PKS 1424-41PKS 2155–304PKS 2032+107PKS 2052–47S4 1144+403C 279.
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:
J. Becerra Gonzalez (josefa.becerra[at]nasa.gov) for generic information related to this week.
- Contact persons on this page for individual sources cited above.

Monday, December 8, 2014

Fermi LAT Weekly Report N. 339


Covered period: 2014.December.01 - 2014.December.7
LAT Mission week: 339.57 - 340.57

  • 3C 454.3 was detected all week, excluding December 1 and 2 with daily averaged fluxes between (1.1 ± 0.5) and (2.2 ± 0.4).
  • 3C 279 was detected several days in the week reaching a daily flux maximum of (2.8 ± 0.4) on December 1.
  • MKN 421 was detected several days in the week reaching a daily flux maximum of (0.4 ± 0.2) on December 3.
  • PKS 1510–08 was detected several days in the week reaching a daily flux maximum of (0.8 ± 0.1) on December 5.
  • PKS B1424–418 was detected several days in the week reaching a daily flux maximum of (1.1 ± 0.1) on December 2.
  • Sporadic daily detections of blazars: PKS 0736+01,PKS 2326–502, B2 1520+31, PG 1553+113, NGC 1275, B2 1504+37,1633+382,B2 1144+40, CTA 102

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:
- S. Cutini (Sara.Cutini[at]asdc.asi.it) for generic information related to this week
- Contact persons on this page for individual sources cited above.



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.