Monday, June 10, 2013

Fermi LAT weekly report N. 260

Covered period: 2013 May 26 - Jun 2
LAT Mission week: 259.57 - 260.57
  • CTA 102 is active during the week peaking at 1.9E-6 on May 28th and 1.5E-6 on May 31st.
  • PKS 1424-41 is bright and active with daily flux of 1.6E-6 on June 1st.
  • PKS 0426-380 is active during the week and peaking at 1.3E-6 on May 31st.
  • Other blazars detected, also sporadically, during the week, with daily flux below 1E-6 level are: Mkn 421, PKS 0454–234, S5 0716+71, PMN J2345-1555, PMN J0017–0512, S5 1044+71, NRAO 190, 3C 454.3 and 4C +38.41 (B2 1633+382).
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:
- D. Bastieri (denis.bastieri[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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Wednesday, May 29, 2013

Fermi LAT weekly report N. 259

Covered period : 2013.May 20 - 2013.May 26
LAT Mission week: 259.57 - 260.57
  • The source PKS 1424-41 was seen all week in a bright state with flux values greater than 1 X 10-6, while the blazar PKS 0426-380 was detected in a high state only on May 20.
  • The FSRQ PMN J0017–0512 was detected on May 24, with daily flux of 1.1 X 10-6; the day after the flux increased its value up to 2.0 X 10-6, 52 times the mean flux value recorded in 2FGL. This detection was eligible for an ATel that was published on May 27.See ATel#5089.
  • PKS 1124-186 was detected three times with daily flux of about 0.5-0.6 X 10-6 and PKS 0454–234 was seen after May 22 with fluxes always lower than 1 X 10-6.
  • The sources significantly detected sporadically were PKS 0507+17, S5 1044+71, PKS 2326–502, PMN J2345-1555, 4C 38.41 and S5 0716+71.
  • LS I+61 303 was detected on May 26 with flux value greater than 2 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:
- E. Antolini (elisa.antolini@fisica.unipg.it) or D. Bastieri (denis.bastieri@pd.infn.it) for generic information related to this week.
- Contact persons on this page for individual sources cited above.

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Monday, May 27, 2013

Fermi LAT weekly report N. 258

Covered period: 2013 May 13 - May 19
LAT Mission week: 258.57 - 259.57
  • The LAT detected a huge solar activity in coincidence with the X3.2 Solar Flare of May 13th and with the X1.2 flare of May 15th
  • The LAT detected also an activity toward the location of GRB130518, see GCN 14675
  • PKS 1424-41 is bright and active with daily flux of 1.8E-6 on May 13th and 2.1E-6 on May 16th.
  • PKS 0507+17 is active during the week and peaking at 2E-6 on May 19.
  • Blazars 4C +38.41 (B2 1633+382) detected in some days of the week in bright state (daily flux level above or around 1e-6).
  • Galactic plane TeV source VER J0521+211 flaring on May 15th at 1.8E-6.
  • Some activity detected by a source positionally coincident with TXS 0500+640 (GB6 J0505+6406), detected on May 16th and 17th between 0.3 and 0.5E-6
  • Detected also NGC 1275 on May 17th.
  • Other blazars detected, also sporadically, during the week, with daily flux below 1E-6 level are: Mkn 421, PKS 0426-380, S5 0716+71, CRATES J1435+2021, OX 169, PMN J2345-1555, B3 1343+451, 3C 454.3 and TXS 1700+685 (RX J1700.1+6830).

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:
- D. Bastieri (denis.bastieri[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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Thursday, May 23, 2013

Fermi LAT weekly report N. 257

Covered period: 2013.May.6 - 2013.May.12
LAT Mission week: 257.57 - 258.57
  • PKS 1424-41 is quite bright and active with daily flux about 2 X 10-6 during the week.
  • PKS 0507+17 continues to be in high state with daily flux about 1 X 10-6 during the week and peaking at 1.6 X 10-6 on May 8th.
  • PKS 1510-089 continues to be detected with daily fluxes around or above 1 X 10-6 .
  • MRK 421, PKS 0426-380, 3C66A, PMN J2345-1555, 4C +38.41 and NGC 1275 detected in one or two days of the week (flux below 1 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:
- 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.

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Monday, May 6, 2013

Fermi LAT weekly report N. 256

Covered period: 2013 April 29 - May 5
LAT Mission week: 256.57 - 257.57
  • PKS 1424-41 is bright and active with daily flux above 2E-6 during the week and peaking at  3.1E-6 on April 30.
  • PKS 0507+17 is in high state with daily flux above 1.5E-6 during the week and peaking at 2E-6 on April 29 and May 2.
  • Blazars PMN J2345-1555, 4C +38.41 (B2 1633+382),  PKS 1510-08, and PKS 2345-16 are detected in some days of the week in bright state (daily flux level above or around 1e-6).
  • Other blazars detected, also sporadically, during the week, with daily flux below 1E-6 level are: Mkn 421, PKS 0426-380, PKS 0454-234, S5 0716+71, OJ 287, PKS 2326-502, PKS 2320-035, GB6 J1700+6830, S5 1044+71, 3C 454.3, Ton 599 and CTA 102.

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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Tuesday, April 30, 2013

Fermi LAT Weekly Report N. 255

Covered period: 2013.Apr.22 - 2013.Apr.28
LAT Mission week: 255.57 - 256.57
  • PKS 2320-035 was detected on Apr. 25 and 28 with peak daily averaged flux of (1.1 +/- 0.3) which is 18 times its daily average flux from the 2FGL catalog (see ATel #5022).
  • PMN J2345-1555 was detected all week with daily averaged flux between (0.9 +/- 0.2) and (2.4 +/- 0.4).
  • PKS B1424-418 was detected all week with daily averaged flux between (1.8 +/- 0.3) and (2.5 +/- 0.4).
  • PKS 0507+17 was detected all week with a daily averaged flux between (1.4 +/- 0.3) and (4.7 +/- 0.5). The peak on Apr. 25 triggered a GCN Notice (see GCN#1366987519)
  • PKS 0426-380 was detected on Apr. 24 with daily averaged flux of (1.1 +/- 0.3).
  • S5 0716+71 was detected Apr. 22, 23 and 28 with a daily averaged flux between (0.6 +/- 0.2) and (1.0 +/- 0.2).
  • 4C +38.41 was detected all week with a daily averaged flux between (0.7 +/- 0.2) and (1.4 +/- 0.5).
  • PKS 1510-08 was detected on Apr. 24 with daily averaged flux of (1.2 +/- 0.3).
  • On Apr. 27 The LAT detected a strong high-energy GRB with a flux of (10 +/- 1.0) (see GCN Circular #14471 and GCN Circular #14508).
  • Sporadic daily detections of blazars (fluxes below 1): Mkn 421, CTA 102, OX 169, B2 2319+31, S5 1044+71.

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:
- B. Carpenter (carpbr01[at]gmail.com) for generic information related to this week
- Contact persons on this page for individual sources cited above.

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Tuesday, April 23, 2013

Fermi LAT Weekly Report N. 254


Covered period: 2013.April.15 - 2013.April.21
LAT Mission week: 254.57 - 255.57
  • PKS 0507+17 detected in flaring activity on April 21 with a daily flux (1.8±0.3) X 10-6. See ATel#5001.
  • Mrk 421 detected all week, with a daily flux between (0.2±0.1) X 10-6 and (0.8±0.1) X 10-6.
  • PKS 1424-418 detected from April 16 to 21, with a daily flux between (2.0±0.3) X 10-6 and (2.9±0.4) X 10-6.
  • S5 0716+71 detected on April 15, 17, 18, 19, 20, and 21, with a daily flux between (0.3±0.1) X 10-6 and (0.7±0.2) X 10-6.
  • PKS 0426-380 detected on April 16, 17, 19, 20, and 21, with a daily flux between (0.6±0.2) X 10-6 and (1.1±0.2) X 10-6.
  • 4C +38.41 detected on April 15, 16, 19, and 21, with a daily flux between (0.6±0.1) X 10-6 and (1.1±0.3) X 10-6.
  • PMN J2345-1555 detected on April 17, 19, 20, and 21, with a daily flux between (0.4±0.1) X 10-6 and (0.6±0.2) X 10-6.
  • NGC 1275 detected on April 15, 19, and 20, with a daily flux between (0.3±0.1) X 10-6 and (0.6±0.2) X 10-6.
  • CTA 102 detected on April 19, and 20 with a daily flux of (1.0±0.3) X 10-6 and (0.6±0.2) X 10-6, respectively.
  • PKS 1510-089 detected on April 17 with a daily flux of (1.0±0.4) X 10-6.
  • Sporadic activity (daily fluxes below 10-6): PKS 2320-035 (April 16), PKS 0405-385 (April 18), OX 169 (April 19).

    • 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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