Lucarelli, FabrizioFabrizioLucarelliPittori, CarlottaCarlottaPittoriVerrecchia, FrancescoFrancescoVerrecchiaPicozza, P.P.PicozzaAntonelli, A.A.AntonelliGiommi, PaoloPaoloGiommi2020-09-172020-09-172016-08-01https://hdl.handle.net/20.500.13025/4712The Astronomer's Telegram, No. 9295Following the GCN notice posted by the ICECUBE Collaboration on July 31, 2016, reporting the detection at T0=16/07/31 01 55 04 UT of a very high energy neutrino with reconstructed arrival direction pointing at RA, DEC (J2000)=(214.5440, -0.3347 [deg]) with a 90% containement radius of 45.00 arcmin (stat+sys), we searched for transient gamma-ray emission in the AGILE data above 100 MeV. Integrating over the 48 hours from 2016-07-29 02 00 UT to 2016-07-31 02 00 UT a maximum likelihood analysis yields a possible detection at a significance level of about 3 sigma with a flux F(E > 100 MeV)=(1.5 +/- 0.7)x 10^-06 ph/cm^2/s within the GCN/AMON_ICECUBE_HESE notice error region.Transienthttp://adsabs.harvard.edu/abs/2016ATel.9295....1L2016ATel.9295....1L