tag:blogger.com,1999:blog-82051254221946815602024-03-08T11:21:46.340-08:00Fermi Gamma-Ray SkyJuliehttp://www.blogger.com/profile/11786203705833300495noreply@blogger.comBlogger381125tag:blogger.com,1999:blog-8205125422194681560.post-26889084862701376062018-01-01T08:46:00.000-08:002017-04-11T11:36:54.108-07:00NOTE<hr color="#800000" size="5">
<p align="center"><font color="#800000" size="3"><b>The weekly summary reports <br>
are now unevenly ingested (since feb. 2017)</b></font></p>
<hr color="#800000" size="5">
<p align="center"> </p>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-59406364262435979892017-07-05T09:21:00.001-07:002017-07-05T09:21:33.865-07:00Fermi LAT Weekly report N. 473<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 June 26 - July 2<br>
LAT Mission week: 473.57-474.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 1.0e-6 and 2.2e-6.</li>
<li><b>3C 279</b> detected all week in high state with daily fluxes between about 1.1e-6 and 1.8e-6.</li>
<li><b>NGC 1275</b> (Per A, <b> 3C 84</b>) detected all week in high state with daily fluxes between about 0.7e-6 and 1.3e-6 with peak
flare flux detected on June 26 and July 2.</li>
<li>Flare of <b> S4 0917+44 </b> detected in June 29 and July 1 with daily flux about 0.8e-6.</li>
<li>Further bright blazars detected, also sporadically, during the week with daily flux between about 0.5e-6 and 0.7e-6:
<b> PKS 1424-418, PKS 1502+106, PKS 0336-01</b>.</li>
<li>Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
<b> S4 1030+61, PKS 2255-282, PKS 2233-148, PMN J2250-2806, PMN J2345-1555, TXS 2016+386, PKS 2023-07, MH 2136-428, PKS 0346-27, GB6 J0742+5444, TXS 0506+056, PKS 2155-304, S5 0716+71, S4 1749+70, PG 1553+113, PKS 0426-380, 4C +01.02, BL Lac, 1ES 1959+650, 3C 454.3, RX J0940.3+6148, PMN
J0751-5134</b>.</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-48114323561767677972017-06-06T02:15:00.000-07:002017-06-06T02:20:37.914-07:00Fermi LAT Weekly report N. 469<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 May 29 - June 4<br>
LAT Mission week: 469.57-470.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li>Flare of <b> 3C 345</b> detected with daily flux 1.8e-6 on May 31. The 6h flux, on the same day, is 2.9e-6. The source is detected also on May 30 and June 1 and 2. More details in
<b><a href="https://gcn.gsfc.nasa.gov/gcn/other/1496330375_fermi.txt">GCN/FERMI NOTICE #1496330375</a>
</b> and <a href="http://www.astronomerstelegram.org/?read=10453"><b>ATel#10453</b></a>.</li>
<li><b>CTA 102 </b> detected all week with daily fluxes between about 1.0e-6 and 2.9e-6.</li>
<li><b>4C +28.07</b> (<b>B2 0234+28</b>) detected all week with daily fluxes between about 0.6e-6 and 1.0e-6.</li>
<li><b>3C 279</b> detected all week with daily fluxes between about 0.5e-6 and 0.9e-6.</li>
<li>Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
<b> TXS 2241+406, PKS 2023-07, PKS 2247-131, PKS 1424-41, PKS 1502+106, Mkn 421, S4 0917+44, PKS 2155-304, S4 1030+61, S5 1044+71, ON 246, PKS 0502+049, 3C 454.3
</b> (flux 0.8e-6 on May 30),<b> PKS 0426-380, S4 0917+44, AP Lib, PKS 0514-459, NGC 1275, GB6 J1542+6129, BL Lac
</b> (flux 0.8e-6 on June 3),<b> PG 1553+113, Ton 599, PKS 0346-27, PMN
J2345-1555</b>.</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]ssdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-40877834028187469912017-06-06T02:14:00.000-07:002017-06-06T02:14:18.959-07:00Fermi LAT Weekly report N. 468<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 May 22-28<br>
LAT Mission week: 468.57-469.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>3C 279</b> detected all week with daily fluxes between about 0.8e-6 and 1.6e-6.</li>
<li><b>CTA 102</b> detected all week with daily fluxes between about 0.9e-6 and 1.5e-6.</li>
<li>Further bright blazars detected, also sporadically, during the week with daily flux between about 0.6e-6 and 1.0e-6:
<b> 4C +01.02</b> (<b>PKS 0106+01</b>), <b> 3C 454.3</b>, <b> 4C +28.07</b>
(<b>B2 0234+28</b>).</li>
<li>Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
<b> PKS 1936-623, S5 0716+71, S4 1749+70, S5 1044+71, BL Lac, Ton 599, PKS 1424-41, Mkn 421, PKS 2155-304, NGC 1275, 3C 66A, PKS 1502+106, PG 1553+113, PMN J1544-0643
</b>(candidate)<b>, 1ES 1959+650, BL Lac, S4 1030+61, B3 1343+451, B2 2308+34, PKS 0426-380, ON 246, OG 50, PKS 1502+106, Ton
599</b>. <br>
</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]ssdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-24647851077899710352017-04-26T10:28:00.001-07:002017-04-26T10:32:18.941-07:00Fermi LAT Weekly report N. 463<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 April 17-23<br>
LAT Mission week: 463.57-464.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li>Rapid outburst of <b> CTA 102</b> detected on April 19 with a daily flux level of 13.2e-6 and corresponding photon spectral index of 1.9. The peak 6-hour integrated flux is 21.1e-6, about 130 times greater than the 3FGL flux, and two times the Vela flux. It decreased to a daily flux level of 5.9e-6 on April 20. More details in
<b><a href="http://www.astronomerstelegram.org/?read=10292">ATel#10292</a></b> and Flare
<a href="https://gcn.gsfc.nasa.gov/gcn/other/1492702671_fermi.txt"><b>CGCN/FERMI NOTICE
#1492702671</b></a>.</li>
<li>Flare of <b> S5 1044+71</b> with daily flux 1.4e-6 on April 23. Peak 6-hour interval flux of 1.9e-6 (28 times the 3FGL flux). See also the Flare
<a href="https://gcn.gsfc.nasa.gov/gcn/other/1493048036_fermi.txt"><b>GCN/FERMI NOTICE
#1493048036</b></a>. Detected all the other days of the week.</li>
<li>Flare of <b> 4C +28.07</b> (<b>B2 0234+28</b>) with daily flux 1.3e-6 on April 22. Detected all the other days of the week with daily fluxes above 0.7e-6.</li>
<li><b>3C 279</b> detected all week with daily fluxes between about 0.7e-6 and 1.0e-6.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.0e-6 and 1.5e-6.</li>
<li><b>4C +01.02</b> (<b>PKS 0106+01</b>) detected all week in high state with daily fluxes between about 0.6e-6 and 1.0e-6.</li>
<li>Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
<b> 1ES 1215+303, Mkn 421, PKS 2155-304, 1ES 1959+650, NGC 1275, PKS 2247-131, B2 1732+38A, 4C +38.41</b>
(<b>B2 1633+38</b>), <b> PKS 1424-41, PG 1553+113, 4C +31.03</b> (<b>B2
0110+31</b>), <b> PMN J2250-2806, PKS 0426-380, 3C 66A, PKS 1954-388, 3C 66A, B2 0748+33, B2 1520+31, GB6 J1542+6129, PKS
0336-01</b>.</li>
<li>Preliminary there is not an evident detection in the days of the week of the potential source at the coordinates reported by AGILE in
<a href="http://www.astronomerstelegram.org/?read=10282"><b>ATel#10282</b></a>.</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]ssdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-11748276619018133102017-04-26T06:48:00.000-07:002017-04-26T06:48:00.948-07:00Fermi LAT Weekly report N. 462<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 April 10-16<br>
LAT Mission week: 462.57-463.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 1.1e-6 and 2.5e-6. See also the Flare
<a href="https://gcn.gsfc.nasa.gov/gcn/other/1492356303_fermi.txt"><b>GCN/FERMI NOTICE
#1492356303</b></a>.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.4e-6 and 2.1e-6.</li>
<li><b>PKS 2247-131 </b> detected all week with daily fluxes between about 0.6e-6 and 1.2e-6.</li>
<li><b>3C 279 </b> detected almost all week with daily fluxes between about 0.5e-6 and 1.2e-6.</li>
<li>Flare of the VHE blazar <b> 1ES 1215+303</b> (<b>B2 1215+30</b>, <b> ON
325</b>) with daily flux 0.8e-6 on April 13. More details in <b><a href="http://www.astronomerstelegram.org/?read=10270">ATel#10270</a></b>.</li>
<li>Flare of <b> PMN J2141-6411</b> with daily flux 0.4e-6 on April 10.</li>
<li>Further bright blazars detected, also sporadically, during the week with daily flux between about 0.7e-6 and 0.8e-6:
<b> 3C 279, 3C 273, PKS 1510-08, 4C +01.02</b> (<b>PKS 0106+01</b>).</li>
<li>Other blazars detected, also sporadically, during the week with daily flux around or below 0.5e-6:
<b> NGC 1275, S5 1044+71, S4 1030+61, BL Lac, PKS 1424-41, PKS 1441+25, 3C 66A, Mkn 421, PKS 1502+106, PKS 1510-08, S5 0716+71, PG 1553+113, PKS 2023-07, PKS 2155-304, 3C 66A, 4C +31.03 (OC 317), 4C +28.07, 4C +55.17, 4C +31.03, PKS 0447-439, PKS 0426-380, PKS 0438-43, B2 1436+37B, B3 1343+451, RX J0115.7+2519, PMN J1332-1256, S5
1803+78</b>.<br>
<br>
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</li>
</ul>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-13698976074240212272017-04-11T07:28:00.003-07:002017-04-12T11:05:05.508-07:00Fermi LAT weekly report N. 461<div dir="ltr" style="text-align: left;" trbidi="on">
<hr color="#800000" size="4" />
<span style="color: maroon;"><b>Covered period: 2017 Apr 3 - 9<br />LAT Mission week: 461.57-462.57</b></span><br />
<hr color="#800000" size="4" />
<div style="text-align: left;">
</div>
<ul>
<li><span style="font-family: inherit;">High-redshift, z=2.4, blazar <b>B2 1436+37B</b> with flux of 0.3 +/- 0.1 on April 6 and 9. That is 8x its 3FGL J1438.7+3710 flux.</span></li>
</ul>
<ul>
<li><span style="font-family: inherit;">VHE blazar, <b>1ES 1215+303</b>, with 1-day flux on April 9 of 0.2 +/- 0.1, that is 4x its 3FGL value. Its peak 6-hr flux is ~0.5 +/- 0.1 with photon index 1.8 +/- 0.2. Its peak LAT flux has reached ~1.0 in the past. See: http://adsabs.harvard.edu/abs/2017ApJ...836..205A</span></li>
</ul>
<ul>
<li><span style="font-family: inherit;">New LAT source on April 7 with 1-day flux 0.4 +/- 0.1 (peak 6-hr flux of 0.6 +/- 0.2) that is positionally consistent with z=0.381 blazar, <b>PKS 1200-051</b></span></li>
</ul>
<ul>
<li><span style="font-family: inherit;">Gamma-ray emission from <b>Cygnus X-3</b> detected by Fermi/LAT at the onset of a major radio flare on 2017 April 3. See: http://www.astronomerstelegram.org/?read=10243</span></li>
</ul>
<span style="font-family: inherit;">Fluxes are in the unit of </span><span style="background-color: white; color: #333333; font-family: Georgia, serif; font-size: 13px;">10</span><sup style="color: #333333; font-family: Georgia, serif;">-6</sup><span style="background-color: white; color: #333333; font-family: Georgia, serif; font-size: 13px;"> </span><span style="font-family: inherit;">photons/cm^2/s above 100 MeV. All uncertainties are statistical only.</span><br />
<span style="font-family: inherit;"><br />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.<br />- Please acknowledge the LAT team if you use information from this report.<br /> <br />For questions and comments please contact:<br />- C.C. Cheung (Teddy.Cheung [at] nrl.navy.mil) for generic information related to this week</span><br />
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.</div>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-67760636926947594072017-04-11T06:33:00.000-07:002017-04-11T07:43:18.101-07:00Fermi LAT Weekly report N. 459<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 March 20-26<br>
LAT Mission week: 459.57-460.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 2.2e-6 and 3.6e-6.</li>
<li><b>3C 279 </b> detected all week in high state with daily fluxes between about 1.2e-6 and 3.5e-6.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.0e-6 and 2.4e-6.</li>
<li><b>4C +01.02</b> (<b>PKS 0106+01</b>) detected all week with daily fluxes between about 0.7e-6 and 1.2e-6.</li>
<li>Flare of <b> PKS 2247-131</b> (source not in the 3FGL catalog) on March 26 with daily flux 1.8e-6 (see also:
<a href="https://gcn.gsfc.nasa.gov/gcn/other/1490628995_fermi.txt"><b>GCN/FERMI NOTICE
#1490628995</b></a>).</li>
<li>Flare of <b> PKS 1830-211</b> (gravitationally lensed) on March 21 with daily flux about 1.4e-6.</li>
<li>No significant excess gamma-ray emission on timescales below one week associated to the cosmic neutrino
<b> event IceCube 170321</b> (see <a href="https://gcn.gsfc.nasa.gov/gcn3/20929.gcn3"><b> IceCube GCN CIRCULAR#20929</b></a> and
<a href="https://gcn.gsfc.nasa.gov/gcn3/20971.gcn3"><b> LAT GCN
CIRCULAR#20971</b></a>).</li>
<li>The <b> Crab</b> is observed fluctuating with possible enhanced activity.
A daily flux of about 3.3e-6 and of about 4.4e-6 is observed
respectively on March 20 and March 25.</li>
<li>Further bright blazars detected all week with daily flux between about 0.7e-6 and 0.9e-6:
<b> NGC 1275, PKS 1510-08, S5 1044+71, BL Lac, PKS 1424-41</b>.</li>
<li>Other blazars of the week (daily flux around or below 0.5e-6): <b> Mkn 421, PKS
0426-380, 3C 66A, TXS 0322+222, PKS 1502+106, 4C +28.07, TXS 2241+406, 4C +28.07, PKS 1502+106, B2 1633+38, PKS 0458-02, 1ES 1215+303
</b>(<b>ON 325</b>)<b>, PKS 0507+17, PKS 2155-304, 1ES 1959+650, PMN J0634-2335, TXS 0628-240, OJ 287, B2 0748+33, PKS
0447-439, TXS 2358+209, 4C +31.03 </b>(<b>OC 317</b>,<b> B2 0110+31</b>),<b> B2 1520+31, PKS
0447-439</b>.</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
<p><br>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-34273143580499822722017-03-16T07:57:00.002-07:002017-03-16T07:57:14.554-07:00<hr color="#800000" size="4">
<strong><font color="#800000">Covered period: 2017.Feb.27 - 2017.Mar.5</font></strong><br>
<strong><font color="#800000">LAT Mission week: 456.57 - 457.57</font></strong><br>
<hr color="#800000" size="4">
<ul>
<li>New source <b>Fermi J0713+5739</b> was detected on Mar. 5 with daily averaged flux of (0.29 +/- 0.03). For more information see <a href="http://www.astronomerstelegram.org/?read=10149">ATel #10149</a>.</li>
<li><b>CTA 102</b> was detected all week with daily averaged fluxes between (1.1 +/- 0.2) and (3.2 +/- 0.4).</li>
<li><b>3C 454.3</b> was detected all week with daily averaged fluxes between (1.0 +/- 0.2) and (1.7 +/- 0.3).</li>
<li><b>S5 1044+71</b> was detected all week with daily averaged fluxes between (0.7 +/- 0.1) and (1.1 +/- 0.2).</li>
<li><b>3C 279</b> was detected Feb. 27 to Mar 2 with daily averaged fluxes between (0.7 +/- 0.2) and (1.4 +/- 0.2).</li>
<li><b>PKS 1510-08</b> was detected on Feb. 27 with daily averaged flux of (1.0 +/- 0.3).</li>
<li><b>PKS B1424-418</b> was detected all week with daily averaged fluxes between (0.8 +/- 0.2) and (1.6 +/- 0.3).</li>
<li><b>4C +01.02</b> was detected all week with daily averaged fluxes between (0.5 +/- 0.2) and (1.0 +/- 0.2).</li>
<li><b>PKS 2247-131</b> was detected on Mar. 4 with daily averaged flux of (1.1 +/- 0.3).</li>
<li>Sporadic daily detections of blazars (fluxes below 1)2 <b>Mkn 421</b>, <b>PKS 0426-380</b>, <b>4C +28.07</b>,
<b>PKS 0447-439</b>, <b>IC 310</b>, <b>B3 1343+451</b>, <b>PKS 1424+240</b>, <b>NGC 1275</b>, <b>1ES 1215+303</b>,
<b>GB6 J1542+6129</b>.</li>
</ul>
<p>Fluxes are in the unit of 10<sup>-6</sup> photons/cm<sup>2</sup>/s above 100 MeV. All errors are statistical only.</p>
<p>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. <br>- Please acknowledge the LAT team if you use information from this report.<br>
<br> For questions and comments please contact:<br>
- B.Carpenter (carpbr01[at]gmail.com) for generic information related to this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-60467829265609798242017-02-07T13:44:00.002-08:002017-02-07T16:15:04.122-08:00Fermi LAT Weekly report N. 452<div dir="ltr" style="text-align: left;" trbidi="on">
<h3 class="post-title entry-title" itemprop="name" style="color: #cc6600; font-family: Georgia, serif; font-size: 18.200000762939453px; font-weight: normal; line-height: 1.4em; margin: 0.25em 0px 0px; padding: 0px 0px 4px;">
</h3>
<div class="post-body entry-content" id="post-body-3355701064432055010" itemprop="description articleBody" style="color: #333333; font-family: georgia, serif; line-height: 1.6em; margin: 0px 0px 0.75em;">
<hr color="#800000" size="4" style="font-size: 13px;" />
<div style="font-size: 13px;">
<span style="color: maroon;"><b>Covered period: January 30 - February 5<br />LAT Mission week: 452.57-453.57</b></span></div>
<hr color="#800000" size="4" style="font-size: 13px;" />
<ul>
<li><b style="font-size: 13px;">CTA 102</b><span style="font-size: x-small;"> </span><span -36px="" courier="" style="color: #323333;" text-indent:="">detected all week in outburst state with daily fluxes between 4.8e-6 and 2.1e-6.</span></li>
<li><b style="font-size: 13px;">3C 454.3</b><span style="font-size: x-small;"> </span><span -36px="" courier="" style="color: #323333;" text-indent:="">detected all week with daily fluxes between 2.7e-6 and 1.8e-6.</span></li>
<li><b style="font-size: 13px;">PKS 1424–41</b><span style="font-size: x-small;"> </span><span -36px="" courier="" style="color: #323333;" text-indent:="">detected all week with daily fluxes between 1.5e-6 and 0.8e-6.</span></li>
<li><b style="font-size: 13px;">3C 279</b><span style="font-size: x-small;"> </span><span -36px="" courier="" style="color: #323333;" text-indent:="">detected in the first part of the week with daily fluxes between 1.2e-6 and 0.7e-6.</span></li>
<li><span style="color: #323333; font-family: "courier"; font-size: 13px;">Other blazars of the day (daily flux around or below 0.5e-6):</span></li>
<span style="font-size: 13px;"> </span><span -36px="" courier="" style="color: #323333;" text-indent:=""><b>S5 1044+71, NGC 1275, PKS 2155–304, 4C +01.02, PKS 1510–08, PKS 1502+106, B3 1343+451, Mkn 421, 1ES 1215+303, PKS 0048–09, PKS 0426–380, PKS 0447–439, S4 0954+65, PKS 2247-131</b></span></ul>
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are statistical only.<br />
<br />
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.<br />
- Please acknowledge the LAT team if you use information from this report.<br />
<br />
For questions and comments please contact:<br />
- M. Kreter (mkreter[at]astro.uni-wuerzburg.de) for generic information related to this week<br />
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources" style="color: #999999; text-decoration: none;"><b>this page</b></a> for individual sources cited above.
</div>
</div>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-27075531885847271132017-01-31T06:31:00.000-08:002017-04-12T11:07:18.685-07:00Fermi LAT Weekly report N. 451<div dir="ltr" style="text-align: left;" trbidi="on">
<div dir="ltr" style="text-align: left;" trbidi="on">
<h3 class="post-title entry-title" itemprop="name" style="color: #cc6600; font-family: Georgia, serif; font-size: 18.200000762939453px; font-weight: normal; line-height: 1.4em; margin: 0.25em 0px 0px; padding: 0px 0px 4px;">
<br /></h3>
<div class="post-header" style="color: #333333; font-family: Georgia, serif; font-size: 13px;">
<div class="post-header-line-1">
</div>
</div>
<div class="post-body entry-content" id="post-body-3355701064432055010" itemprop="description articleBody" style="color: #333333; line-height: 1.6em; margin: 0px 0px 0.75em;">
<hr color="#800000" size="4" style="font-family: georgia, serif; font-size: 13px;" />
<div style="font-family: georgia, serif; font-size: 13px;">
<span style="color: maroon;"><b>Covered period: 2017 January 23-29<br />LAT Mission week: 451.57-452.57</b></span></div>
<hr color="#800000" size="4" style="font-family: georgia, serif; font-size: 13px;" />
<div style="text-align: left;">
</div>
<div style="text-align: left;">
</div>
<ul>
<li><span style="font-family: inherit;"><span style="font-size: 13px;">CTA 102</span><span style="font-size: xx-small;"> </span><span style="color: #323333; text-indent: -36px;">bright all week with daily flux range = (4.4 +/- 0.3) to (7.1 +/- 0.4) with peak flux observed on Jan 26</span></span></li>
</ul>
<ul>
<li><span style="font-family: inherit;"><span style="color: #323333; font-family: "courier"; font-size: 10.6px;">Other blazars regularly detected on daily basis throughout the week: </span><span style="color: #323333; font-family: "courier"; font-size: 10.6px;">4C +01.02, NGC 1275, PKS 0426–380, S5 1044+71, 3C 279, PKS B1424-418, PKS 2247-131, 3C 454.3</span></span></li>
</ul>
</div>
</div>
<div style="text-align: left;">
Fluxes are in the unit of <span style="background-color: white; color: #333333; font-family: "georgia" , serif;">10</span><sup style="color: #333333; font-family: Georgia, serif;">-6</sup><span style="background-color: white; color: #333333; font-family: "georgia" , serif;"> </span>photons/cm^2/s above 100 MeV. All uncertainties are statistical only.</div>
<br />
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.<br />
- Please acknowledge the LAT team if you use information from this report.<br />
<br />
For questions and comments please contact:<br />
- C.C. Cheung (Teddy.Cheung [at] nrl.navy.mil) for generic information related to this week<br />
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources" style="color: #999999; text-decoration: none;"><b>this page</b></a> for individual sources cited above.</div>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-33557010644320550102017-01-10T12:22:00.000-08:002017-01-10T12:23:08.840-08:00Fermi LAT Weekly report N. 448<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2017 January 2-8<br>
LAT Mission week: 448.57-449.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in outburst state with daily fluxes above 10.0e-6 from Jan. 4 to Jan 8. In particular on Jan. 6 and Jan. 7,
the source reached the daily flux level of (19.8 +/-0.7)e-6 (with photon index 1.9+/-0.1) and of (18.3 +/-0.7)e-6 (with photon index 2.1+/-0.1) respectively. The 6-hour averaged peak flux of
<b> CTA 102</b> on Jan. 6 was (24.3+/-1.7)e-6 corresponding to about 150 times the averaged 3FGL flux of the source, and about 2.4 times the averaged 3FGL flux of the Vela pulsar. </li>
<li><b>3C 454.3 </b> detected all week with daily fluxes between about 1.7e-6 and 2.8e-6.</li>
<li><b>NGC 1275</b> (<b>Per A</b>, <b> 3C 84</b>) detected all week with daily fluxes between about 0.6e-6 and 0.8e-6. In particular on Jan. 3, NGC 1275 showed a photon index around 1.8 and one possible photon of 241 GeV energy spatially consistent with the source.</li>
<li><b>PKS 1424-41</b> detected all week with daily fluxes between about 0.7e-6 and 0.9e-6.</li>
<li><b>PKS 0426-380</b> detected in high state on Jan. 2, Jan. 4 and Jan. 5, each day at a flux level of (1.2+/-0.2)e-6. </li>
<li><b>S5 1044+71</b> detected in high state all week with daily fluxes between about 0.6e-6 and 1.0e-6. </li>
<li><b>S4 0917+62</b> (<b>OK 630</b>) detected in flaring state on Jan. 4 with daily flux (0.8+/-0.1)e-6. </li>
<li><b>PKS 0438-43</b> detected in flaring state on Jan. 3 with daily flux (0.9+/-0.1)e-6. </li>
<li><b>PKS 0907-023</b> detected in flaring state on Jan. 4 with daily flux (0.7+/-0.2)e-6. </li>
<li><b>PMN J2153-1136 </b> detected in flaring state on Jan. 2 with daily flux (0.9+/-0.2)e-6. </li>
<li><b>PKS 1510-08</b> detected on Jan. 5 with daily flux about 1.0e-6. </li>
<li>3C 279 detected in the second paert of the week with daily fluxes between about 0.6e-6 and 0.8e-6. </li>
<li>Other blazars of the day (daily flux around or below 0.5e-6): <b>1ES 2344+514, 1ES 1959+650, Ton 599, PKS 0736+01, S5 2007+77, B2 2308+34, PKS
0131-522, PKS 0447-439, Mkn 421, Mkn 501, AO 0235+164, S5 1053+70, Mkn 421, BL Lac, PKS 1502+106, PKS 0537-441, TXS 0518+211
</b> (<b>Ver 0521+211</b>)<b>, PKS 0208-512, S3 0218+35 </b> (gravitationally lensed),
<b> PKS 0035-252, PG 1553+113, 4C +28.07 </b>(<b>B2 0234+28</b>)<b>, 4C +01.02
</b> (<b>PKS 0106+01</b>)<b>, 4C +31.03 </b>(<b>B2 0110+31</b>)<b>, 3C 273, PKS 2155-304, PKS 2320-035, PKS 2136-642, PKS 2247-131</b> .<br>
<br>
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</li>
</ul>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-60193970636811935932017-01-03T13:21:00.000-08:002017-01-03T13:21:25.452-08:00Fermi LAT Weekly Report N. 447<hr color="#800000" size="4">
<strong><font color="#800000">Covered period: 2016.Dec.26 - 2017.Jan.1</font></strong><br>
<strong><font color="#800000">LAT Mission week: 447.57 - 448.57</font></strong><br>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> was detected all week with daily averaged fluxes between (7.0 +/- 0.5) and (21.7 +/- 0.7). This is the highest daily averaged flux the LAT has ever observed from <b>CTA 102</b>. ToO observations were made for 430 ks starting on 2016 Dec. 29. For more information see <a href="http://www.astronomerstelegram.org/?read=9924"><b>ATel #9924</b></a>. </li>
<li><b>S5 1044+71</b> was detected all week with daily averaged fluxes between (0.6 +/- 0.1) and (1.1 +/- 0.2). For more information see <a href="http://www.astronomerstelegram.org/?read=9928"><b>ATel #9928</b></a>.</li>
<li><b>NGC 1275</b> was detected all week with daily averaged fluxes between (0.4 +/- 0.1) and (2.2 +/- 0.3).</li>
<li><b>3C 454.3</b> was detected on Dec. 26 with a daily averaged flux of (2.1 +/- 0.3).</li>
<li><b>PKS 1510-08</b> was detected Dec. 26-29 with daily averaged fluxes between(0.5 +/- 0.1) and (1.0 +/- 0.2).</li>
<li>Sporadic daily detections of blazars (fluxes below 1): <b>Ton 599</b>, <b>PKS B1424-418</b>, <b>OK 630</b>,
<b>3C 279</b>, <b>Mkn 421</b>, <b>3C 66A</b>, <b>PKS 0426-380</b>, <b>PKS 0208-512</b>,
<b>4C +48.51</b>, <b>PKS 2155-304</b>, <b>B2 2113+29</b>, <b>3C 273</b>.</li>
</ul>
<p>Fluxes are in the unit of 10<sup>-6</sup> photons/cm<sup>2</sup>/s above 100 MeV. All errors are statistical only.</p>
<p>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. <br>- Please acknowledge the LAT team if you use information from this report.<br>
<br> For questions and comments please contact:<br>
- R. Ojha (Roopesh.Ojha[at]gmail.com) for generic information related to this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-36227683306887787372017-01-03T07:08:00.000-08:002017-01-03T07:08:02.211-08:00Fermi LAT Weekly Report N. 446<hr color="#800000" size="4">
<strong><font color="#800000">Covered period: 2016.Dec.19 - 2016.Dec.25</font></strong><br>
<strong><font color="#800000">LAT Mission week: 446.57 - 447.57</font></strong><br>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> was detected all week with daily averaged fluxes between (7.6 +/- 0.3) and (12.9 +/- 0.6).</li>
<li><b>3C 454.3</b> was detected all week with daily averaged fluxes between (3.9 +/- 0.2) and (5.3 +/- 0.2).</li>
<li><b>PKS 2247-131</b> was detected all week with daily averaged fluxes between (0.8 +/- 0.2) and (1.2 +/- 0.1).</li>
<li>Sporadic daily detections of blazars (fluxes below 1): <b>3C 279</b>, <b>OK 630</b>, <b>1ES 1215+303</b>,
<b>NGC 1275</b>, <b>S5 1044+71</b>, <b>PKS B1424-418</b>, <b>Mkn 421</b>, <b>PKS 0537-441</b>, <b>PKS 0426-380</b>,
<b>3C 345</b>, <b>PKS 1502+106</b>, <b>3C 273</b>.</li>
</ul>
<p>Fluxes are in the unit of 10<sup>-6</sup> photons/cm<sup>2</sup>/s above 100 MeV. All errors are statistical only.</p>
<p>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. <br>- Please acknowledge the LAT team if you use information from this report.<br>
<br> For questions and comments please contact:<br>
- B.Carpenter (carpbr01[at]gmail.com) for generic information related to this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-48949565920909187602016-12-22T03:59:00.000-08:002016-12-22T08:59:48.503-08:00Fermi LAT Weekly report N. 445<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2016 December 12-18<br>
LAT Mission week: 445.57-446.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in outburst state with daily fluxes above
5.0e-6. The source was above 10.0e-6 on at least three days, from Dec. 14 to
Dec. 16 ((see more details in Fermi LAT
<b><a href="http://www.astronomerstelegram.org/?read=9869">ATel#9869</a></b> and
<b><a href="https://gcn.gsfc.nasa.gov/gcn/other/1481817437_fermi.txt">GCN/FERMI NOTICE
#1481817437</a></b>). The peak daily flux was observed on Dec. 16:
(15.8+/-0.3)e-6 with corresponding photon index 1.9+/-0.1. One Fermi ToO
pointing to <b>CTA 102</b> was performed following this very high-flux state
and a second one is ongoing.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.0e-6
and 3.3e-6.</li>
<li><b>PKS 2247-131</b> detected all week with daily fluxes between about
0.7e-6 and 1.5e-6 (see <b><a href="https://gcn.gsfc.nasa.gov/gcn/other/1482077947_fermi.txt">GCN/FERMI NOTICE
#1482077947</a></b>).</li>
<li><b>4C +28.07</b> (<b>B2 0234+28</b>, <b>OD 258</b>) detected in flaring
state on Dec. 16 and 17 with daily flux about 1.0e-6.</li>
<li><b>MG2 J071354+1934</b> detected in flaring state on Dec. 15 with daily
flux about 0.9e-6 (see <b><a href="https://gcn.gsfc.nasa.gov/gcn/other/1481903722_fermi.txt">GCN/FERMI NOTICE
#1481903722</a></b>).</li>
<li><b>S5 1044+71</b> detected all week with daily fluxes between about 0.5e-6
and 0.8e-6.</li>
<li><b>S3 0218+35</b> (gravitationally lensed) detected in high state on Dec.
16 with daily flux about 0.8e-6.</li>
<li><b>S5 1053+70</b> detected in high state on Dec. 16 with daily flux about
0.8e-6.</li>
<li><b>PKS 1424-41</b> detected all week with daily fluxes between about
0.5e-6 and 0.8e-6.</li>
<li><b>PKS 1502+106</b> detected all week with daily fluxes between about
0.5e-6 and 0.7e-6.</li>
<li><b>NGC 1275</b> (<b>Per A</b>, <b>3C 84</b>) detected all week with daily
fluxes between about 0.5e-6 and 0.7e-6.</li>
<li>Other blazars of the day (daily flux around or below 0.5e-6):<br>
<b>BL Lac</b>,<b> Mkn 421</b>,<b> PKS 2155-304</b>,<b> 1ES 1959+650</b>,<b> B2
1846+32B</b>,<b> B2 2234+28A</b>,<b> PG 1553+113</b>,<b> PG 1246+586</b>,<b> PKS 0438-43, PKS 0426-380, PKS 0502+049, PKS 0736+01, PKS 0208-512, OK 630, S5 0716+71, 3C 66A, OX 169, PKS
2320-035</b>,<b> OJ 287</b>,<b> B2 0748+33</b>,<b> S5 2007+77</b>,<b> PKS
0736+01</b>,<b> Ton 599</b>.<br>
<br>
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</li>
</ul>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-44623097209000625452016-12-20T13:52:00.001-08:002016-12-20T13:52:42.344-08:00Fermi LAT weekly report N. 444<div dir="ltr" style="text-align: left;" trbidi="on">
<hr color="#800000" size="4" />
<span style="color: maroon;"><b>Covered period: 2016 December 5 - December 11<br />
LAT Mission week: 444.57-445.57</b></span><br />
<hr color="#800000" size="4" />
<div style="text-align: left;">
</div>
<ul>
<li><b><span style="font-family: monospace; font-weight: normal;">PKS 0438-43 (z=2.852) peak daily flux = (1.1 ± 0.2) on Dec 11 ; reported in ATel#9854</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">CTA 102 bright all week with daily flux range = (4.0 +/- 0.4) to (6.1 +/- 0.4); peak on Dec 8</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">S5 1044+71 peak = (0.9 +/- 0.2) on Dec 5. First and only LAT ATEL on this source was from April 2013 with the same peak flux of 0.9 (</span><a href="https://ssd2.ssd.nrl.navy.mil/owa/14.3.319.2/scripts/premium/redir.aspx?C=pHY6kf5ixhNux97gd0CA9Dj2ckevxxUpY02AstXl3UEVzPZXISnUCA..&URL=http%3a%2f%2fwww.astronomerstelegram.org%2f%3fread%3d4941" style="font-family: monospace; font-weight: normal;" target="_blank">http://www.astronomerstelegram.org/?read=4941</a><span style="font-family: monospace; font-weight: normal;">).</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">4C +01.02 peak flux = (0.7 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">NGC 1275 peak flux = (0.6 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">PKS 0426–380 peak flux = (0.5 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">B2 0748+33 peak flux = (0.5 ± 0.1)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">S5 1027+74 peak flux = (0.5 ± 0.1)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">3C 273 peak flux = (0.9 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">3C 279 peak flux = (0.3 ± 0.1)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">PKS B1424–418 peak flux = (0.9 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">PKS 1502+106 peak flux = (0.8 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">BL Lacertae peak flux = (0.6 ± 0.2)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">PKS 2247-131 peak flux = (0.7 ± 0.1)</span></b></li>
<li><b><span style="font-family: monospace; font-weight: normal;">3C 454.3 peak flux = (1.6 ± 0.3) on Dec 10</span></b></li>
</ul>
Fluxes are in the unit of 1e-6 photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br />
<br />
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.<br />
- Please acknowledge the LAT team if you use information from this report.<br />
<br />
For questions and comments please contact:<br />
- C.C. Cheung (Teddy.Cheung [at] nrl.navy.mil) for generic information related to
this week<br />
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br />
<br />
<hr color="#800000" size="8" />
</div>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-2243332215850189052016-12-06T11:33:00.002-08:002016-12-06T11:33:33.135-08:00Fermi LAT Weekly report N. 443<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2016 November 28 - December 4<br>
LAT Mission week: 443.57-444.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li> <b> CTA 102</b> detected all week in outburst state with daily fluxes between about 3.2e-6 and 5.7e-6 peaking at the end of the week. </li>
<li> <b>PKS 0903-57</b> detected in flaring state on Nov. 28 with daily flux 1.2e-6. </li>
<li> <b>4C +01.02 </b>(<b>PKS 0106+01</b>) detected all week in high state with daily fluxes between about 0.8e-6 and 1.6e-6. </li>
<li> <b>3C 454.3</b> detected all week with daily fluxes between about 1.3e-6 and 2.7e-6. </li>
<li> <b>PKS 1502+106</b> detected all week with daily fluxes between about 0.6e-6 and 1.0e-6. </li>
<li> <b>PKS 1424-41</b> detected all week with daily fluxes between about 0.5e-6 and 0.9e-6. </li>
<li> <b>NGC 1275</b> (<b>Per A</b>, <b> 3C 84</b>) detected all week with daily fluxes between about 0.4e-6 and 0.8e-6. </li>
<li> <b>PKS 2247-131</b> detected all week with daily fluxes between about 0.4e-6 and 0.7e-6. </li>
<li> <b>BL Lac</b> detected in active state on Dec. 1 with daily flux 0.9e-6. </li>
<li> <b>PKS 0521-36</b> detected in active state on Dec. 2 with daily flux 0.7e-6. </li>
<li> <b>B2 1520+31</b> detected in active state on Dec. 1 with daily flux 0.7e-6. </li>
<li> <b>3C 279</b> detected in active state on Nov. 29 with daily flux 0.7e-6. </li>
<li> <b>MG1 J120953+1809</b> (<b>GB6 J1209+1810</b>) detected in active state on Dec. 4 with daily flux 0.7e-6. </li>
<li> Other blazars of the day (daily flux around or below 0.5e-6): <b>PKS 2155-304</b>,<b> 1ES
1959+650</b>,<b> PG 1553+113</b>,<b> Mkn 421</b>,<b> Mkn 501</b>,<b> Ton 599</b>,<b> PKS
0426-380</b>,<b> PKS 0208-512</b>,<b> PKS 1016-311</b>,<b> 3C 279</b>,<b> 3C
66A</b>,<b> OJ 287</b>,<b> S5 1044+71</b>,<b> S4 1800+44</b>,<b> S5 1803+78</b>,<b> S5
2007+77</b>,<b> S3 0218+35 </b> (gravitationally lensed),<b> TXS 0529+483</b>,<b> TXS
1549+089</b>,<b> AO 0235+164</b>,<b> B3 1343+451</b>,<b> PMN J2234-2656</b>.<b> </b> </li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-3410663810317608732016-12-05T07:15:00.001-08:002016-12-06T11:38:24.843-08:00Fermi LAT Weekly report N. 442<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2016 November 21-27<br>
LAT Mission week: 442.57-443.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li> <b>CTA 102</b> detected all week in high state with daily fluxes between about
1.8e-6 and 6.2e-6 (peak flux on November 23).</li>
<li> <b>3C 454.3</b> detected all week with daily fluxes between about 0.7e-6 and
2.2e-6.</li>
<li> <b>4C +01.02</b> detected almost all week with daily fluxes between about 0.7e-6
and 1.2e-6. (see also <a href="http://gcn.gsfc.nasa.gov/gcn/other/1480175539_fermi.txt"><b>GCN/FERMI NOTICE
#1480175539</b></a>).</li>
<li> <b>PKS 2247-1371</b> detected all week with daily fluxes between about 0.7e-6 and
1.2e-6 </li>
<li> Sporadic daily detections of blazars (fluxes below 1): <b> PKS 1502+106</b>,<b> PKS
0447-439</b>,<b> PKS 0208-512</b>,<b> TXS 2358+209</b>,<b> PKS 0426-380</b>,<b> NGC
1275</b>,<b> PKS 1424-41</b>,<b> 3C 279</b>,<b> S5 1044+71</b>,<b> PKS 0903-57</b>.</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- N. Alvarez Crespo (nuriaalvarezcrespo[at]gmail.com) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-55693341557677348202016-12-01T14:22:00.000-08:002016-12-01T14:22:36.648-08:00Fermi LAT Weekly report N. 441<hr color="#800000" size="4">
<p><b><font color="#800000">Covered period: 2016 November 14 - 20<br>
LAT Mission week: 441.57-442.57</font></b></p>
<hr color="#800000" size="4">
<ul>
<li><b>PKS 0507+17</b> was detected on Nov 20, 2016 with a daily flux of about 1.9e-6 and a daily averaged photon index of about 1.8. See more details in ATel #<a href="http://www.astronomerstelegram.org/?read=9779"><b>9779</b></a>.</li>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 4.1e-6 and 1.1e-6.</li>
<li><b>PKS 1502+106</b> detected almost all week with daily fluxes between about 0.7e-6 and 0.5e-6.</li>
<li><b>BL Lacertae</b> detected almost all week with daily fluxes between about 1.1e-6 and 0.5e-6.</li>
<li><b>PKS B1424–418</b> detected almost all week with daily fluxes between about 0.9e-6 and 0.4e-6.</li>
<li><b>3C 454.3</b> detected almost all week with daily fluxes between about 1.7e-6 and 0.8e-6.</li>
<li><b>PKS 2247-131</b> detected almost all week with daily fluxes between about 2.4e-6 and 0.7e-6.</li>
<li>Other blazars of the week detected, also sporadically, around or below 0.5e-6:
<b>PKS 0447–439</b>, <b>4C +01.02</b>, <b>PKS 0338–214</b>, <b>PKS 0426–380</b>, <b>PKS 0346–27</b>, <b>NGC 1275</b>, <b>OK 290</b>, <b>Mkn 421</b>, <b>PKS 0426–380</b>, <b>PG 1553+113</b>, <b>PKS 0208–512</b>, <b>PKS B1310–041</b>,
<b>RBS 1888</b>.<br>
</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- M. Kreter (mkreter[at]astro.uni-wuerzburg.de) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-67682698138685837102016-11-16T02:49:00.000-08:002016-11-16T02:59:23.324-08:00Fermi LAT Weekly report N. 440<hr color="#800000" size="4">
<p><b><font color="#800000">Covered period: 2016 November 7 - 13<br>
LAT Mission week: 440.57-441.57</font></b></p>
<hr color="#800000" size="4">
<ul>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 1.8e-6 and 2.9e-6. A large optical activity is reported recently
in some ATels.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.3e-6 and
2.6e-6.</li>
<li><b>PKS 2247-131</b> detected all week with daily fluxes between about 1.0e-6
and 1.3e-6.</li>
<li><b>4C +01.02 </b>(<b>PKS 0106+01</b>) detected all week with daily fluxes between
about 0.5e-6 and 1.1e-6.</li>
<li><b>NGC 1275</b> (<b>Perseus A</b>, <b> 3C 84</b>) detected all week with daily fluxes
between about 0.5e-6 and 1.0e-6.</li>
<li><b>PKS 1424-41</b> detected all week with daily fluxes between about 0.3e-6
and 1.0e-6.</li>
<li><b>PKS 1502+106</b> (<b>OR 103</b>) detected all week with daily fluxes between
about 0.3e-6 and 0.7e-6.</li>
<li><b>PKS 1824-582</b> detected almost all week with daily fluxes above 0.3e-6. The peak daily flux of 0.7e-6 was recorded on Nov. 12.</li>
<li><b>B2 0748+33 </b> detected almost all week with daily fluxes between about 0.7e-6 and 0.8e-6. See more details about a dedicated
Swift follow-up in <a href="http://www.astronomerstelegram.org/?read=9752"><b>ATel#9752</b></a>.</li>
<li><b>MRC 1659-621</b> (<b>PMN J1703-6212</b>) detected in high state on Nov. 7 with
daily flux 0.7e-6.</li>
<li>Other blazars of the week detected, also sporadically, around or below 0.5e-6:
<b> S5 1044+71</b>,<b> S4 1030+61</b>,<b> 1ES 1959+650</b>,<b> PKS 2155-304</b>,<b> PG
1553+113</b>,<b> Mkn 421</b>,<b> TXS 0518+211 </b>(<b>Ver 0521+211</b>),<b> 1ES
1215+303</b>,<b> S3 0218+35</b> (gravitational lens<b> B0218+357</b>),<b> PKS
0208-512</b>,<b> PKS 0426-380</b>,<b> PKS 0447-439</b>,<b> PKS
0454-234</b>,<b> PKS 0507+17</b>,<b> PKS 0524-485</b>,<b> PKS 0521-36</b>,<b> S5
0716+71</b>,<b> MG1 J050533+0415</b>,<b> 3C 66A</b>,<b> 4C +38.41 </b>(<b>B2
1633+38</b>), <b> PKS 0727-11</b>,<b> PKS 2247-131</b>,<b> S5 1803+78</b>,<b> PKS
1510-08</b>.<br>
</li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-43321450541298586872016-11-14T06:50:00.000-08:002016-11-14T06:50:11.771-08:00Fermi LAT Weekly Report N. 439<hr color="#800000" size="4">
<strong><font color="#800000">Covered period: 2016.Oct.31 - 2016.Nov.6</font></strong><br>
<strong><font color="#800000">LAT Mission week: 439.57 - 440.57</font></strong><br>
<hr color="#800000" size="4">
<ul>
<li><b>3C 454.3</b> was detected all week with daily averaged fluxes between (2.1 +/- 0.3) and (4.5 +/- 0.5).</li>
<li><b>CTA 102</b> was detected Oct. 31 and Nov 4 with a daily averaged flux of (1.1 +/- 0.2) and (1.9 +/- 0.3), respectively.</li>
<li>Sporadic daily detections of blazars (fluxes below 1): <b>PKS 1502+106</b>, <b>NGC 1275</b>, <b>PKS 0502+049</b>,
<b>4C +01.02</b>, <b>1ES 1215+303</b>, <b>OX 169</b>, <b>OK 630</b>, <b>PKS B1424-418</b>, <b>PKS 0426-380</b>,
<b>PKS 0447-439</b>, <b>TXS 0213+619 </b>.</li>
</ul>
<p>Fluxes are in the unit of 10<sup>-6</sup> photons/cm<sup>2</sup>/s above 100 MeV. All errors are statistical only.</p>
<p>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. <br>- Please acknowledge the LAT team if you use information from this report.<br>
<br> For questions and comments please contact:<br>
- B.Carpenter (carpbr01[at]gmail.com) for generic information related to this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-2116160605501179792016-11-14T06:49:00.000-08:002016-11-14T06:49:04.679-08:00Fermi LAT Weekly Report N. 438<hr color="#800000" size="4">
<strong><font color="#800000">Covered period: 2016.Oct.24 - 2016.Oct.30</font></strong><br>
<strong><font color="#800000">LAT Mission week: 438.57 - 439.57</font></strong><br>
<hr color="#800000" size="4">
<ul>
<li><b>3C 454.3</b> was detected all week with daily averaged fluxes between (1.9 +/- 0.3) and (3.0 +/- 0.4).</li>
<li><b>CTA 102</b> was detected all week with daily averaged fluxes between (0.8 +/- 0.2) and (2.7 +/- 0.3).</li>
<li><b>S5 1044+71</b> was detected Oct. 26 with a daily averaged flux of (1.0 +/- 0.4).</li>
<li>Fermi LAT observed no significant gamma-ray excess associated with IceCube event 161103. </li>
<li>TOO observations of <b>V5853 SGR</b> were in progress after Oct. 25.</li>
<li>Sporadic daily detections of blazars (fluxes below 1): <b>PKS 0507+17</b>, <b>PKS 1510-08</b>, <b>NGC 1275</b>,
<b>MG2 J201534+3710</b>, <b>PKS 0524-485</b>, <b>PKS 0426-380</b>, <b>PKS 1502+106</b>, <b>4C +01.02</b>,
<b>BL Lacertae</b>, <b>S5 1053+70</b>, <b>B2 0716+33</b>.</li>
</ul>
<p>Fluxes are in the unit of 10<sup>-6</sup> photons/cm<sup>2</sup>/s above 100 MeV. All errors are statistical only.</p>
<p>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. <br>- Please acknowledge the LAT team if you use information from this report.<br>
<br> For questions and comments please contact:<br>
- R. Ojha (Roopesh.Ojha[at]gmail.com) for generic information related to this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this page</b></a> for individual sources cited above.
</p>
<hr color="#800000" size="8">Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-28258687964433128032016-11-12T12:20:00.003-08:002016-11-12T12:22:16.561-08:00Fermi LAT Weekly report N. 437<hr color="#800000" size="4">
<p><font color="#800000"><b>Covered period: 2016 October 17-23<br>
LAT Mission week: 437.57-438.57</b></font></p>
<hr color="#800000" size="4">
<ul>
<li> The <b>Crab</b> is still in active state during the week, peaking with
daily flux 5.4e-6 on Oct. 21.</li>
<li> <b>PKS 2247-131</b> (recent <a href="http://www.astronomerstelegram.org/?read=9620"><b>ATel#9620</b></a>)
detected all week in high state with daily fluxes above 1e-6 and peaking on
Oct. 17, Oct.18, Oct. 22 and Oct. 23 respectively with fluxes 2.1e-6,
2.2e-6, 2.6e-6 and 2.8e-6.</li>
<li> <b>4C +01.02</b> (<b>PKS 0106+01</b>) detected all week in high state
with daily fluxes between 1e-6 and 1.9e-6.</li>
<li> <b>3C 454.3</b> detected all week with daily fluxes between about 0.9e-6
and 2.4e-6.</li>
<li> <b>CTA 102</b> detected all week with daily fluxes between about 1.1e-6
and 1.6e-6.</li>
<li> Gravitationally lensed blazar <b>S3 0218+35</b> (<b>lens B0218+357</b>)
detected almost all week with daily fluxes around 0.3e-6.</li>
<li> Other blazars of the week detected, also sporadically, around or below
0.5e-6: <b>B2 0748+33, AO 0235+164, PKS 1502+106, PKS 0502+049, NGC 1275
(Per A), S5 1044+71, PKS 0426-380, TXS 1452+516, PKS 0524-485, PG 1553+113,
PKS 0507+17, BL Lac, PKS 0336-01, 1ES 1959+650, S5 1053+70, PMN J0422-0643,
PKS 1510-08, VER 0521+211, Mkn 421, PKS 2155-304, TXS 0628-240, 3C 66A, S4
1849+67</b>. <b> </b> </li>
</ul>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-11919790863524313122016-10-12T13:39:00.000-07:002016-10-13T05:04:29.091-07:00Fermi LAT weekly report N. 434<div dir="ltr" style="text-align: left;" trbidi="on">
<hr color="#800000" size="4" />
<b><span style="color: maroon;">Covered period: 2016 September 26 - Ocotber 2<br />
LAT Mission week: 434.57-435.57</span></b>
<br />
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<ul>
<li><b>Crab nebula</b> flare with peak daily flux (4.8 ± 0.5) on Sep 30 ; reported in
<a href="http://www.astronomerstelegram.org/?read=9588"><b>ATel#9588</b></a></li>
<li><b> B2 0748+33</b> peak daily flux = (0.8 ± 0.2) on Oct 2 ; reported in
<a href="http://www.astronomerstelegram.org/?read=9590"><b>ATel#9590</b></a></li>
<li><b> Nova Lupi 2016</b> (ASASSN-16kt) sky-survey and ToO observations ; reported in
<a href="http://www.astronomerstelegram.org/?read=9594"><b>ATel#9594</b></a></li>
<li><b> 4C +01.02</b> peak daily flux = (1.0 ± 0.2) </li>
<li>Gravitational lens <b>B0218+357</b> peak daily flux = (0.7 ± 0.2) </li>
<li><b> PMN J0422–0643</b> peak daily flux = (0.4 ± 0.1) </li>
<li><b> PKS 0426–380</b> peak daily flux = (1.0 ± 0.1) </li>
<li><b> PKS 0447–439</b> peak daily flux = (0.5 ± 0.1) </li>
<li><b> PKS 0524–485</b> peak daily flux = (0.4 ± 0.1) </li>
<li><b> S5 0716+71</b> peak daily flux = (0.3 ± 0.1)</li>
<li><b> S5 1044+71</b> peak daily flux = (0.5 ± 0.1)</li>
<li><b>PKS 1424–41</b> peak daily flux = (0.6 ± 0.1)</li>
<li><b> PKS 1502+106 </b> peak daily flux = (0.6 ± 0.1) </li>
<li><b> PKS 1510–08</b> peak daily flux = (1.1 ± 0.2)</li>
<li><b> 4C +38.41</b> peak daily flux = (0.6 ± 0.1) </li>
<li><b> PKS 2155–304 </b> peak daily flux = (0.3 ± 0.1)</li>
<li><b> TXS 2241+406</b> peak daily flux = (0.4 ± 0.1)</li>
<li><b> PKS 2247-131</b> peak daily flux = (1.1 ± 0.3) ; see July 2016 flare:
<a href="http://www.astronomerstelegram.org/?read=9285"><b>ATel#9285</b></a></li>
<li><b> BL Lacertae </b> peak daily flux = (0.5 ± 0.1)</li>
<li><b> CTA 102</b> peak daily flux = (2.6 ± 0.4)</li>
<li><b> 3C 454.3 </b> peak daily flux = (1.5 ± 0.3)</li>
</ul>
Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br />
<br />
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.<br />
- Please acknowledge the LAT team if you use information from this report.<br />
<br />
For questions and comments please contact:<br />
- C.C. Cheung (Teddy.Cheung [at] nrl.navy.mil) for generic information related to
this week<br />
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br />
<br />
<hr color="#800000" size="8" />
</div>
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0tag:blogger.com,1999:blog-8205125422194681560.post-31578134506797417622016-10-11T07:11:00.001-07:002016-10-11T07:13:27.973-07:00Fermi LAT Weekly report N. 430<hr color="#800000" size="4">
<b><font color="#800000">Covered period: 2016 August 29 - September 4<br>
LAT Mission week: 430.57-431.57</font></b>
<hr color="#800000" size="4">
<ul>
<li>Flare of the GeV-TeV BL Lac object <b> AP Librae</b> with daily flux 1.1e-6 and peak 6h flux 2.5e-6 on Aug.30. More details in
<b><a href="http://www.astronomerstelegram.org/?read=9442">ATel#9442</a></b>.</li>
<li>Outburst of <b> PKS 1510-08</b> with daily flux peaking at 5.3e-6 on Sept.3.</li>
<li>Flare of blazar <b> MG2 J201534+3710</b> with daily flux 1.6e-6 on Aug.30.</li>
<li><b>PKS 1824-582</b> detected almost all week with daily fluxes above 0.7e-6 and peaking on Sept. 3 with daily flux 1.3e-6.</li>
<li><b>CTA 102</b> detected all week in high state with daily fluxes between about 2.4e-6 and 3.2e-6.</li>
<li><b>3C 454.3</b> detected all week with daily fluxes between about 1.8e-6 and 3.5e-6.</li>
<li>Increased activity of <b> Cen A</b> detected on Sep.1 with daily flux 0.8e-6.</li>
<li><b>4C +01.02</b> (<b>PKS 0106+01</b>) detected all week with daily fluxes between about 0.7e-6 and 1.3e-6.</li>
<li><b>S5 1044+71</b> detected all week with daily fluxes between about 0.6e-6 and 0.8e-6.</li>
<li><b>PKS 0502+049</b> detected all week with daily fluxes between about 0.6e-6 and 0.8e-6.</li>
<li>BL Lac object <b> 3C 371</b> detected at 0.2e-6 on Aug.30.</li>
<li>Possible hard state of the BL Lac object <b> TXS 1055+567</b> (7C 1055+5644, GB6 J1058+5628, z=0.1433) detected on Sept. 1 with daily flux 0.06e-6 and ph.index 1.5.</li>
<li>Other blazars of the week detected, also sporadically, around or below 0.5e-6:<br>
<b>PG 1553+113</b> and <b>3C 66A</b> (both in possible hard state with flux about 0.1e-6 and photon index about 1.5), <b>MG1 J021114+1051, PKS
2155-304, PKS 1424-41, PKS 1502+106, PKS 2052-47, 1ES 1215+303 </b> (or<b> PG
1218+304</b>)<b>, NGC 1275, </b> gravitationally lensed blazar<b> S3 0218+35 (lens B0218+357), 4C +55.17, 1ES 1959+650, PKS 0002-478, S4 1849+67, BL Lac, PKS 0426-380, PKS 0402-362, TXS 2241+406, S4
0110+49</b>.</li>
<li>Enhanced activity of the microquasar <b> Cyg X-3</b> being detected during some days of the week.</li>
<li>Quiet Sun and the Moon detected in a few 6h intervals of the week.</li>
</ul>
<p> </p>
<p>Fluxes are in the unit of photons/cm^2/s above 100 MeV. All uncertainties are
statistical only.<br>
<br>
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.<br>
- Please acknowledge the LAT team if you use information from this report.<br>
<br>
For questions and comments please contact:<br>
- S. Ciprini (stefano.ciprini[at]asdc.asi.it) for generic information related to
this week<br>
- Contact persons on <a href="https://confluence.slac.stanford.edu/display/GLAMCOG/Contact+Information+for+Individual+Sources"><b>this
page</b></a> for individual sources cited above.<br>
</p>
<hr color="#800000" size="8">
Flare Advocatehttp://www.blogger.com/profile/16037859223942934450noreply@blogger.com0