Göttingen 2025 –
wissenschaftliches Programm
T 53: Neutrino Astronomy III
Mittwoch, 2. April 2025, 16:15–18:15, VG 1.105
 |
16:15 |
T 53.1 |
A bayesian approach to study the multimessenger emission from AGN-starburst galaxies* — •Silvia Salvatore, Bjoern Eichmann, and Julia Becker-Tjus
|
|
|
|
16:30 |
T 53.2 |
Constraining the contribution of Seyfert galaxies to the astrophysical neutrino flux using NGC 1068 as a benchmark — •Lena Saurenhaus, Francesca Capel, and Foteini Oikonomou
|
|
|
|
16:45 |
T 53.3 |
IFT on ice: Utilizing numerical information field theory to reconstruct glacial ice parameters — •Matthias Hübl, Laurin Söding, and Philipp Mertsch
|
|
|
|
17:00 |
T 53.4 |
Search for Ultra-High Energy Neutrinos from Gamma-Ray Bursts with the Pierre Auger Observatory — •Therese Paulsen for the Pierre-Auger collaboration
|
|
|
|
17:15 |
T 53.5 |
Ultra-high-energy neutrino detection with radio antennas in the ground based observatory — •Baobiao Yue
|
|
|
|
17:30 |
T 53.6 |
Enhancing Sensitivity for Ultra-High Energy Down-Going Neutrino Detection with the Pierre Auger Observatory* — •Srijan Sehgal for the Pierre-Auger collaboration
|
|
|
|
17:45 |
T 53.7 |
ML discrimination of atmospheric neutrinos for DSNB detection in JUNO — •David Maksimovic, Daniel Tobias Schmid, Dhaval J. Ajana, Michael Wurm, Marcel Büchner, Arshak Jafar, George Parker, Oliver Pilarczyk, and Tim Charisse
|
|
|
|
18:00 |
T 53.8 |
Detecting Distant Supernovae Using Log-Likelihood Ratios — •Kashish Gupta, Thilo Birkenfeld, and Achim Stahl
|
|
|
