[vsnet-grb-info 26437] Fermi-LAT Gamma-ray Observations of IceCube-200929A
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Thu Oct 1 06:39:17 JST 2020
TITLE: GCN CIRCULAR
NUMBER: 28537
SUBJECT: Fermi-LAT Gamma-ray Observations of IceCube-200929A
DATE: 20/09/30 21:38:22 GMT
FROM: Simone Garrappa at DESY <simone.garrappa at desy.de>
S. Garrappa (DESY-Zeuthen) and S. Buson (Univ. of Wuerzburg) on behalf
of the Fermi-LAT collaboration:
We report an analysis of observations of the vicinity of the high-energy
IC200929A neutrino event (GCN 28532) with all-sky survey data from the
Large Area Telescope (LAT), on board the Fermi Gamma-ray Space
Telescope. The IceCube event was detected on 2020-09-29 at
17:48:36.84 UT (T0) with J2000 position RA = 29.53 (+0.53, -0.53) deg,
Decl. = 3.47 (+0.71, -0.35) deg 90% PSF containment. No cataloged >100
MeV gamma-ray sources (The Fourth Fermi-LAT catalog; The Fermi-LAT
collaboration 2020, ApJS, 247, 33) are located within the 90% IC200929A
localization error.
We searched for intermediate (days to years) timescale emission from a
new gamma-ray transient source. Preliminary analysis indicates no
significant (> 5 sigma) new excess emission (> 100 MeV) at the
IC200929A best-fit position. Assuming a power-law spectrum (photon index
= 2.0 fixed) for a point source at the IC200929A best-fit position, the
>100 MeV flux upper limit (95% confidence) is < 2.4e-10 ph cm^-2 s^-1
for ~12-years (2008-08-04 / 2020-09-29 UTC), < 1.2e-8 (< 8e-7) ph cm^-2
s^-1 for a 1-month (1-day) integration time before T0.
Since Fermi normally operates in an all-sky scanning mode, regular
monitoring of this source will continue. For these observations the
Fermi-LAT contact persons are S. Garrappa (simone.garrappa at desy.de
<http://desy.de/>) and S. Buson (sara.buson at uni-wuerzburg.de
<http://uni-wuerzburg.de/>). The Fermi-LAT is a pair conversion
telescope designed to cover the energy band from 20 MeV to greater than
300 GeV. It is the product of an international collaboration between
NASA and DOE in the U.S. and many scientific institutions across France,
Italy, Japan and Sweden.
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