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.

4MOST    CloseBinaries    Education    EScience    Galaxies    GalaxyClusters    LargeScale    MassiveStars    MeVSky    Relativistic    SMBHs    StellarEndpoints    General   

4MOST: facility performance and planned spectroscopic survey science

PresenterTitleType
Léa MarquesDynamics at the bar-spiral interfacePoster

Close Binaries and Stellar Mergers

PresenterTitleType
Lars ChrischillesPopulation study of Accreting White Dwarfs in M33 based on X-ray emissionPoster
Peter Cheung Siu HeiPlanetary Nebula from 3D MHD Common Envelope SimulationPoster
Todt, H.PoWR stellar atmosphere grids of OB-type starsPoster

Meeting Bildungsausschuss AG

PresenterTitleType
Ralf-Juergen DettmarThe European Space Education Regional Office (ESERO) in GermanyPoster

E-Science / E-Infrastructures / Virtual Observatory / Machine Learning

PresenterTitleType
Iliana CortésModelling AGN Optical Lightcurves via Inference of AD-BLR delay (MAGNOLIA)Poster

Star-forming Galaxies in the Early Universe

PresenterTitleType
Ke-Jung ChenHow Population III Supernovae Determined the Properties of the First GalaxiesPoster
Seok-Jun ChangStudy of the formation of Hα and Hβ Emission in Little Red Dots with Radiative Transfer in Multiphase GasPoster

From protoclusters to galaxy clusters: probing structure formation and cosmology with current and next-generation surveys

PresenterTitleType
Yinghua HuangExploring the Temperature Dependence of Intrinsic Scatter in the Galaxy Cluster X-ray Luminosity–Temperature RelationPoster

Beyond 2-Point Large Scale Structure Cosmology

PresenterTitleType
Phu Huy NguyenSimulation-based inference of Cosmological parameters from the Higher-order statistics of galaxy distributionPoster

The role of magnetic fields in the evolution of massive stars

PresenterTitleType
Pei-Cheng TungGalactic Environments as Architects of Supernova Remnant FormationPoster

Reopening the MeV Sky with COSI and Beyond

PresenterTitleType
Dimitris TsatsisExtension of the Source catalogue for INTEGRAL/SPI with 22 Years of DataPoster
Laura EisenbergerObservations of the dark matter halo of the Andromeda Galaxy with INTEGRAL/SPI Poster
Manja ZimmererContributions of massive stars and classical novae to Galactic 26AlPoster
Manuel SkalkaElectron-Positron Annihilation in Globular Clusters and the 511 keV – 2.223 MeV CorrelationPoster
Rudi ReinhardtImaging and Model FittingPoster
Saurabh MittalSearch for Axion-like Particles from Massive StarsPoster
Saurabh MittalStellar flares cannot explain the Galactic 511 keV emission Poster
Tomohiko OkaAll-sky models of cosmic-ray-induced nuclear gamma-ray line emissionPoster

Relativistic astrophysics

PresenterTitleType
Gh.SalehBeyond the Standard Atomic Model: Photon as the Primary Building BlockPoster

Deciphering AGN from new survey data: eROSITA, 5XMM, Euclid and JWST

PresenterTitleType
Li MaImproved analytic model for the abundance of Direct Collapse Black HolesPoster

Interfacing observations and theories at stellar endpoints

PresenterTitleType
Po-Sheng OuThe Critical Metallicity of Red Supergiant FormationPoster

General Poster

PresenterTitleType
Apostolos MenisThe fraction of AGNs detected in clusters from deep and wide-field X-Ray surveysPoster
Chris KarwinResolving the Origin of Positrons from the Inner Galaxy with GALEPoster
Jan-Hendrik GleißbergSearching for undetected exoplanet signals in the CARMENES DR1 with KimaPoster
Jatin ChopraStar Formation Quenching in Post-Merger GalaxiesPoster
Yerassyl TelmanWater transport in late stage accretion with N-body and SPH simulationsPoster