T 10: Gamma astronomy 1
Monday, March 4, 2024, 16:00–18:00, Geb. 30.22: kl. HS A
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16:00 |
T 10.1 |
Background estimation for IACTs combining a run matching approach with a background template — •Tina Wach, Alison Mitchell, and Lars Mohrmann
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16:15 |
T 10.2 |
Towards a multiwavelength analysis of Pulsar Wind Nebulae at gamma-ray and X-ray energies with Gammapy — •Katharina Egg and Alison Mitchell
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16:30 |
T 10.3 |
High-energy variability of the gravitationally lensed blazar PKS 1830-211 — •Sarah M. Wagner, Jeffrey D. Scargle, Greg Madejski, Andrea Gokus, and Krzysztof Nalewajko
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16:45 |
T 10.4 |
Investigation of the influence of an updated model for the extragalactic background light on the multi-messenger signatures of Blazar 3C279 with CRPropa — •Yannick Schmidt, Lukas Merten, and Julia Becker Tjus
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17:00 |
T 10.5 |
Multi-Messenger Picture of J1048+7143 Consistent with a Supermassive Black Hole Binary Origin* — •Ilja Jaroschewski, Emma Kun, and Julia Becker Tjus
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17:15 |
T 10.6 |
Expanding the Multi-Messenger Picture of J1048+7143 with the Optical Light Curve* — •Johannes Just, Ilja Jaroschewski, Emma Kun, and Julia Becker Tjus
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17:30 |
T 10.7 |
On the possible jet contribution to the γ-ray luminosity in NGC 1068 — •Silvia Salvatore, Björn Eichmann, Xavier Rodrigues, Ralf-Jürgen Dettmar, and Julia Becker Tjus
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17:45 |
T 10.8 |
Spatially Coherent 3D Distributions of HI and CO in the Milky Way — •Laurin Söding, Philipp Mertsch, and Vo Hong Minh Phan
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