T 78: Gamma Astronomy II
Donnerstag, 3. April 2025, 16:15–18:15, VG 2.103
 |
16:15 |
T 78.1 |
Constraining the intergalactic Magnetic field with Fermi-LAT observations — •Yosef Abed, Dieter Horns, and Matías Sotomayor
|
|
|
 |
16:30 |
T 78.2 |
Adaptive Sampling in Simulations for the Cherenkov Telescope Array Observatory — •Tristan Gradetzke and Luca Di Bella
|
|
|
 |
16:45 |
T 78.3 |
Investigating the Effects of Symmetry Assumptions in the Instrument Response of the Cherenkov Telescope Array Observatory — •Luca Davide Di Bella and Tristan Franziskus Gradetzke
|
|
|
 |
17:00 |
T 78.4 |
FlashCam development and verification — •Anne Timmermans for the FlashCam collaboration
|
|
|
 |
17:15 |
T 78.5 |
SWGO Array Trigger Performance Evaluation — •Johannes Bennemann
|
|
|
 |
17:30 |
T 78.6 |
Modeling of dark matter prompt and secondary signatures in dwarf galaxies — •Athithya Aravinthan, Julia Becker Tjus, and Lukas Merten
|
|
|
 |
17:45 |
T 78.7 |
Analysis of the IC 443 Supernova Remnant with H.E.S.S. Data — •Lukas Großpietsch, Alison Mitchell, and Tina Wach for the H.E.S.S. collaboration
|
|
|
 |
18:00 |
T 78.8 |
Spatially coherent 3D distributions of HI and CO in the Milky Way — •Laurin Söding, Gordian Edenhofer, Torsten A. Enßlin, Philipp Frank, Ralf Kissmann, Vo Hong Minh Phan, Andrés Ramírez, Hanieh Zandinejad, and Philipp Mertsch
|
|
|