Poster Presentations
Room:
Poster presentations have to be provided in printed form. The format should not exceed DIN A0 portrait (841 mm width x 1189 mm height). Poster space will be available for display during the whole week of the conference.
In addition we encourage you to upload an electronic version (PDF) of your poster to the conference site if you wish to make your poster available online.
EScience FutureRadio GalaxyEvol JungeAG LowMet MassiveStars Multimessenger SNR General
E-Science / E-Infrastructures / Virtual Observatory / Machine Learning
Presenter | Title | Type |
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Johanna Riedel | Probabilistic Reconstruction of Spectra from Photometry | Poster |
Future perspectives for radio astronomy in Germany
Presenter | Title | Type |
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Jompoj wongphecauxsorn | Improved Coverage for Southern-Hemisphere VLBI through the SKAMPI telescope | Poster |
Milky Way and Nearby Galaxies: Templates for Galaxy Evolution Studies
Presenter | Title | Type |
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Oerd Xhemollari | Decoding Dense Gas with 3D MHD Simulations: Molecular Signatures in Galactic Star Formation | Poster |
junge AG / young AG
Presenter | Title | Type |
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Polina Smirnova | Machine learning analysis of supernova remnant simulations | Poster |
Star formation, feedback and chemistry of the low-metallicity ISM
Presenter | Title | Type |
---|---|---|
Sanjit Pal | The impact of variable far-UV radiation field and cosmic-ray ionisation rate on the formation of molecular clouds in low-metallicity environments | Poster |
The lives of massive stars and their influence on star formation
The Physics behind the Multimessenger Emissions of Active Galactic Nuclei
Presenter | Title | Type |
---|---|---|
Crystal Mele | Multimessenger Emissions of Active Galactic Nuclei: From a Radio Perspective | Poster |
Daniela Dorner | FACT - Highlights from Ten Years of Blazar Monitoring | Poster |
Florian Rösch | TANAMI VLBI Observations of Southern-Hemisphere AGN Associated with High-Energy Emission | Poster |
Multiwavelength studies of supernova remnants and their impact on the interstellar medium
Presenter | Title | Type |
---|---|---|
Ekaterina Makarenko | How do supernova remnants cool in the optical emission lines? | Poster |
Ekaterina Makarenko | Modeling thermal X-ray emission from supernova remnant interacting with the CSM | Poster |
Leonard Romano | Cloud Formation by Supernova Implosion | Poster |
Mattia Pacicco | The turbulent magnetic field produced by clustered supernova explosions | Poster |
General Poster
Presenter | Title | Type |
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Anna Gebhardt | Spectrophotometric investigations of hot subdwarf stars in the Plato field with Gaia DR3 | Poster |
Lennart Buhlmann | A subgrid model for the turbulent circumgalactic medium in massive, high redshift star-forming galaxies: Understanding the [CII] line emission | Poster |
Maryam Raouph | Photometric Calibration of Astronomical Photp Plates by Gaia SED Fluxes | Poster |
Michael Weis | Properties of Molecular Clumps and Cores in Colliding Magnetized Flows | Poster |
R.-J. Dettmar | The ASPERA SmallSat | Poster |
Steven Hämmerich | BlazEr1: The eROSITA Blazar Catalog | Poster |
Sven Thorwirth | High-resolution spectroscopic study of vinyl cyanide isotopologues for radio astronomy: (13)CH2CHCN AND CH2CH(13)CN | Poster |
Tom Richtler | In-situ dust formation in M87 and the jet | Poster |
Wajdee Chayeb | The Interplay Between Stellar Feedback and Gas Turbulence in Giant Molecular Clouds | Poster |