Fermi LAT weekly report N. 285

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Covered period : 2013 November 18-24
LAT Mission week : 285.57 - 286.57

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• PKS 2326-502 was detected all week with a daily averaged flux between 0.7 x 10^-6 and 1.2 x 10^-6.
• PKS 2032+107 was seen three times during the second part of the week with flux values around 0.8 x 10^-6.
• 4C +21.35 was detected during the first two days of the week with daily flux values respectively of 0.9x 10^-6 and 0.8 x 10^-6.
• 4C +38.41 was detected during the second part of the week at about 0.8 x 10^-6 on November 20 and at 0.5 x 10^-6 on November 22.
• BL Lacertae was detected twice with flux of 0.8 x 10^-6 (November 21 and 22).
• Other blazars detected in some days of the week with a daily flux lower than about 0.7 x 10^-6: NGC 1275, PKS 0426–380, PKS 1244–255, PKS 1454–354, PKS 1510–08, B2 1520+31. The only exception was 3C 454.3 detected on November 18 with daily flux of 0.9 x 10^-6.

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:
- Elisa Antolini (elisa.antolini@fisica.unipg.it) for generic information related to this week
- Contact persons on this page for individual sources cited above.

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Fermi LAT Weekly report N. 284

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Covered period: 2013 November 11-17
LAT Mission week: 284.57 - 285.57

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• PKS 1510-08 in high state during the first part of the week and peaking on November 14 with daily flux 2.5E-6.
• PKS 2326-502 in high state during the week and peaking on November 14 with daily flux 2E-6.
• 3C 454.3 detected during the week with daily flux oscillating around a value of 1.2E-6.
• CTA 102 is increasing during the last part of the week (daily flux about 1.3 on November 16 and 17).
• 4C +21.35 (PG 1222+216) flaring at 1.2E-6. on November 15.
• Other blazars detected in some days of the week with a daily flux lower than about 0.7E-6: Mkn 421,  Mkn 501, 3C 66A, NGC 1275, PKS 0454-234, PKS 0426-380, 4C +01.02 (PKS 0106+01, OC 012), 4C +47.44 (S4 1636+47), 4C +38.41 (B2 1633+38), B2 2319+31, BL Lacertae, S5 1044+71, PMN J2345-1555, PKS 0208-512 , PKS 1424-41.
• High mass gamma-ray binary 1FGL J1018.6-5856> detected in high state with daily flux 2.4E-6 on November 11.

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.

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Fermi LAT Weekly Report N. 283

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Covered period: 2013.November.04 - 2013.November.10
LAT Mission week: 283.57 - 284.57

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• PKS 2326-502 was detected all week with a daily averaged flux between (0.7±0.2) X 10^-6 and (1.4±0.2) X 10^-6.
• 3C 454.3 was detected on November 4 and November 8, with a daily averaged flux between (1.1±0.3) X 10^-6 and (1.6±0.4) X 10^-6.
• 4C +21.35 was detected all week with a daily averaged flux between (0.5±0.2) X 10^-6 and (1.5±0.3) X 10^-6.
• PKS 1510-08 was detected on November 6 with a daily averaged flux of (1.1±0.4) X 10^-6
• GRB 131108A was detected on November 8 with a daily averaged flux of (12.2±1.2) X 10^-6. See GCN #15464
• Sporadic activity (daily fluxes below 10^-6): Mrk 421, NGC 1274, PKS 0454-234, PKS 0426-380, PKS 2325-408, PMN J2345-1555, S5 1044+71, VER J0521+211.

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:
- Roopesh 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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Fermi LAT Weekly Report N. 282

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Covered period: 2013.October.28 - 2013.November.3
LAT Mission week: 282.57 - 283.57

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• Fermi ended its dedicated pointing observation of the Sun on October 29.
• PKS 1510-089 detected on October 28, 29, 30, 31, and November 1 and 3, with a daily flux between (2.9±0.3) X 10^-6 and (0.9±0.3) X 10^-6.
• 4C +21.35 detected on October 28, and November 1, and 3, with a daily flux between (1.0±0.3) X 10^-6 and (0.3±0.1) X 10^-6.
• PKS 2326-502 detected on October 30 and November 1, 2, and 3, with a daily flux between (2.1±0.3) X 10^-6 and (0.8±0.2) X 10^-6, respectively.
• 3C 454.3 detected on October 30 and November 1, 2, and 3, with a daily flux between (1.3±0.4) X 10^-6 and (0.8±0.3) X 10^-6, respectively.
• Sporadic activity (daily fluxes below 10^-6): PKS 1329-049 (October 29, 30), MG1 J123931+0443 (October 29), Mkn 421 (October 30, November 2, 3), CTA 102 (October 30, November 3), PKS 0454-234 (November 1, 3), BL Lacertae (November 1), S4 1144+40 (November 2, 3), PMN J2345-1555 (November 2, 3), NGC 1275 (November 3).

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:
- W. McConville (wmcconvi[at]umd.edu) for generic information related to this week
- Contact persons on this page for individual sources cited above.

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Fermi LAT Weekly report N. 281

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Covered period: 2013.October.21 - 2013.October.27
LAT Mission week: 281.57 - 282.57

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• PKS 0454-234 detected on October 21, 23, 24, 25, and 27, with a daily flux between (1.4±0.2) X 10^-6 and (0.5±0.2) X 10^-6.
• PKS 1510-089 detected on October 23, 24, 25, 26, and 27, with a daily flux between (3.3±0.4) X 10^-6 and (1.7±0.4) X 10^-6.
• 4C +21.35 detected on October 25, 26, and 27, with a daily flux between (1.2±0.3) X 10^-6 and (0.9±0.2) X 10^-6.
• VER J0521+21 detected on October 21 and 25, with a daily flux of (2.5±0.3) X 10^-6 and (1.4±0.4) X 10^-6, respectively.
• PKS 2326-502 detected on October 23 and 24, with a daily flux of (1.0±0.3) X 10^-6 and (0.9±0.2) X 10^-6, respectively.
• 3C 454.3 detected on October 24 and 25, with a daily flux of (1.3±0.3) X 10^-6 and (1.6±0.3) X 10^-6, respectively.
• Sporadic activity (daily fluxes below 10^-6): NGC 1275 (October 21), B3 2308+34 (October 23), B3 1343+451 (October 24), S5 0716+71 (October 25), PKS 1424-418 (October 26).
• Fermi has interrupted all-sky scanning mode on 2013-10-28 16:23:34 for a dedicated pointing observation of the Sun.

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:
- F. D'Ammando (dammando[at]ira.inaf.it) and M. 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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Fermi LAT Weekly report N. 280

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Covered period: 2013 October 14-20
LAT Mission week: 280.57 - 281.57

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• The TeV blazar VER J0521+211 has been significantly detected since the beginning of the week on daily timescales and it exhibited an active state reaching the highest daily flux of 1.0 +/- 0.3 on 2013 October 14 (ATel #5472).
• B2 2308+34 in active state. On 2013 October 15 and 16 it reached the daily flux of 1.0+/- 0.2 (ATel #5477). This was the first Fermi LAT detection of the object on daily timescales since mid-2011.
• On 2013 October 17 the Crab Nebula has been observed in flaring state showing a daily flux of 9.7+/-0.7 (ATel #5485). Consequently, Fermi interrupted all-sky scanning mode to maximize the exposure toward the Crab Nebula. The pointing mode lasted until 2013 October 21. 
• PKS 1510–08 present most days of the week. The highest daily flux of 3.2 +/- 0.4 was recorded on 2013 October 14.
• Other blazars detected at daily fluxes between 0.6 - 0.9 : PKS 1424–418, 4C +38.41, NGC 1275, PKS 0426-380, 3C 454.3
• Sporadic daily detections of blazars (fluxes below 1): Mrk 421, CTA 102, PKS 0454-234, PKS 2142-75, B3 1343+451, BL Lac, PKS 1222+216, PKS 0716+714, 4C +01.02, Mkn 501.

Fluxes are in the unit of 10-6 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. Buson (sara.buson[at]pd.infn.it) for generic information related to this week
- Contact persons on this page for individual sources cited above.

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Fermi LAT Weekly report N. 279

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Covered period: 2013 October 7-13
LAT Mission week: 279.57 - 279.57

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• The BL Lac object 1ES 2322-409 (z=0.17359, 2FGL J2324.7-4042) detected in flaring state in the days from October 7 to October 10 (see ATel#5457).  The source reached its historical maximum on October 8 with daily flux of 1.5E-6. Another AGN (candidate FSRQ) PKS 2325-408 ( 2FGL J2327.9-4037) can be also a possible association for the LAT flaring source. It is located at about a half degree from 1ES 2322-409.
• PKS 1510-08 in high active state during the week and peaking on October 13 with daily flux 3.7E-6.
• 4C +21.35 (PG 1222+21) and 4C +38.41 (B2 1633+38) both in high state during the week with daily flux between about 1.2E-6 and 2E-6.
• PKS 2326-502 flaring during the week peaking on October 10 with daily flux 1.6E-6.   
• 3C 454.3 detected during the week with daily flux oscillating around a value of 1.2E-6.
• NGC 1275 (Perseus A) detected some days of the week peaking on October 9 with daily flux 1.2E-6. 
• 4C +01.02 (PKS 0106+01) detected on October 9 and 12 with a daily flux level of about 1E-6.
• BL Lacertae detected on October 12 with a daily flux level of 1E-6.  
• Other blazars of the week: PKS 0426-380, CTA 102, PKS 0454-234, 3C 279, PKS 1424-41, S4 1849+67, Mkn 421, PKS 2142-75, PMN J2145-3357, PMN J2345-1555, PKS 1622-253, 4C +55.17 (OK 591, S4 0954+55), B2 2308+34.

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.

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