GCN Circular 36089
Subject
Fermi-LAT gamma-ray observations of IceCube-240412A
Date
2024-04-14T13:02:15Z (7 months ago)
From
chiara.bartolini-1@unitn.it
Via
Web form
C. Bartolini (INFN Bari), S. Garrappa (Weizmann Institute of Science), S. Buson (DESY; Univ. of Wuerzburg), L. Pfeiffer (Univ. of Wuerzburg) and J. Sinapius (DESY) on behalf of the Fermi-LAT collaboration:
We report an analysis of observations of the vicinity of the high-energy IC240412A neutrino event (GCN 36070) 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 2024-04-12 at 05:33:46.89 UT (T0) with J2000 position RA = 102.44 (+1.09, -0.67) deg, Decl. = +6.35 (+0.60, -0.46) deg (90% PSF containment). There are no cataloged gamma-ray (>100 MeV; The Fermi-LAT collaboration 2022, ApJS, 260, 53) sources located within the 90% IC240412A localization region.
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 IC240412A best-fit position. Assuming a power-law spectrum (photon index = 2.0 fixed) for a point source at the IC240412A best-fit position, the >100 MeV flux upper limit (95% confidence) is < 7.99e-10 ph cm^-2 s^-1 for ~15-years (2008-08-04 to 2024-04-12 UTC), and < 6.05e-9 (< 1.67e-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 region will continue. For this observation the Fermi-LAT contact person is C. Bartolini (chiara.bartolini at ba.infn.it).
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.