THANK YOU ALL FOR YOUR PARTICIPATION !
In conjuction with the SKAO Council meeting in Zurich, SKACH probably invites you to participate in the March 17th Science meeting. This meeting will showcase Swiss science activities including the development of Swiss science tools. The purpose of this meeting is to find collaboration and synergy with other countries and to let the SKAO community know what activities are taking place in Switzerland.
The Swiss astrophysics community looks forward to contributing to all key science areas of the SKA and, in doing so, exploiting many of the different observing modes SKA LOW and MID will offer. In this presentation we will highlight some of the science topics which are of an esp. high priority to Swiss researchers, and where Swiss involvement in other projects generates synergies that are particularly beneficial for science with the SKA.
We will present an overview of SPH-EXA, the first Exascale-capable astrophysical simulation code for hydrodynamics and gravity with a native GPU implementation. We will show the
current and upcoming capabilities of SPH-EXA in simulating
star formation, tidal disruption events and other transient phenomena, protoplanetary disks and cosmological volumes
for galaxy formation. We will focus on applications that are most relevant for the SKAO scientific themes and its precursors, hinting at the transformative ability of SPH-EXA to model much
larger systems or samples of astrophysical objects at much higher resolution, which will allow to harness the upcoming datasets of SKA
Infrastructure for the Swiss SRC Node
Innovative approaches to extracting the 21-cm Hydrogen Signal
We will present initial results from the Phoebos simulation, emphasizing its connection to SKA's HI science. Using the ChaNGa code, Phoebos models a large volume of the Universe and accurately reproduces key galaxy statistics. This talk will focus on galaxy sizes at z > 8, providing new insights into the formation and evolution of early galaxies.
HPC, Data science, and astrophysics @ EPFL
Karabo is a powerful, accessible simulation tool designed to support researchers in radio astronomy, particularly in the context of the Square Kilometre Array (SKA). Karabo aims at facilitating learning, algorithm validation, and benchmarking within interferometry. This demonstration introduces Karabo’s capabilities with a very simple pipeline. Through a hands-on walkthrough, attendees will explore key features, including sky simulations, telescope configurations, observation setup, and image processing. Karabo’s integration with Renkulab enables users to run pipelines effortlessly, leveraging predefined telescope models and sky catalogs or creating custom setups. The session highlights practical applications, from generating synthetic sky data to processing interferometric observations using OSKAR, RASCIL, and WSClean. The demonstration is available at: https://bit.ly/karabo-demo.
Learn to set and run your Radiative Transfer Simulation for the Cosmic Epoch of Reionization with the pyC2Ray code
I will present a radio interferometric imager made using UnityHub and the C# language that has been used at multiple events across Switzerland for scientific outreach.
Following the successful development of an elegant breadboard/Proof of Conept for the 15-25GHz direct sampling receiver, a roadmap is presented towards an engineering model, witz discussion about way to extend the upper frequency limit up to 40 or 50GHz. The talk also presets ideas to retrofit the Mid-band 6 in the dish's foreseen infrastructure, integrating with the other bands' infrastructure.
I will provide a brief synopsis of current initiatives to establish astronomy research infrastructure and human capital across the African continent, and highlight specific opportunities for cooperation.