Conveners
Splinter: Large infrastructure and instrumentation
- Jan Geralt bij de Vaate (SRON)
-
Marc Botz (Max-Planck-Institut für Kernphysik)12/05/2026, 11:00Large infrastructure and instrumentationContributed Talk
Most of the visible matter in the universe exists as highly ionized plasmas, consisting of highly charged ions (HCIs). Due to their high effective nuclear charge, HCIs strongly emit radiation in the X-ray regime and can be observed with X-ray satellites, such as XRISM.
Go to contribution page
To study these ions in a laboratory setting and establish spectral benchmarks that meet the accuracy requirements of XRISM... -
Vadym Voitsekhovskyi (Anton Pannekoek Institute for Astronomy / GRAPPA, University of Amsterdam)12/05/2026, 11:15Large infrastructure and instrumentationContributed Talk
The Cherenkov Telescope Array Observatory (CTAO) will be the next-generation ground-based facility for very-high-energy gamma-ray astronomy. In contrast to space-based instruments, ground-based gamma-ray observatories detect the brief flashes of Cherenkov light produced when high-energy gamma rays interact with the Earth’s atmosphere, generating particle cascades. This technique enables the...
Go to contribution page -
Paul Groot (Radboud Universiteit)12/05/2026, 11:30Large infrastructure and instrumentationContributed Talk
This will be a talk in two parts.
In the first part I will given an overview of the European Southern Observatory, its capabilities (VLT, ALMA, VLTI, La Sila) and current developments, including the construction of the Extremely Large Telescope where The Netherlands plays an important role, among others through the METIS, Micado and MOSAIC instruments.
In the second part I will give an...
Go to contribution page -
Elena Tonucci (Leiden University)12/05/2026, 11:45Large infrastructure and instrumentationContributed Talk
Current high-contrast imaging instruments are limited by wavefront errors originating from non-common path aberrations due, for example, to manufacturing errors in the optics and temperature drifts in the system. These create quasi-static speckles in the final science image that are difficult to distinguish from companions. The Self-Coherent Camera (SCC) exploits the light incoherence between...
Go to contribution page -
Dr Thomas Wijnen (NOVA)12/05/2026, 12:00Large infrastructure and instrumentationContributed Talk
NOVA’s instrumentation program is driven by scientific ambition: the need for access to specific data shapes our participation in major international projects. With a strong focus on ESO facilities, NOVA aims both to contribute to future instruments and to sustain and develop key technical expertise within its instrumentation groups.
As ESO prepares for the post-2030 landscape through the...
Go to contribution page -
Joseph Callingham (ASTRON / University of Amsterdam)12/05/2026, 12:15Large infrastructure and instrumentationContributed Talk
After more than 30 years of talking, the construction of the Square Kilometre Array (SKA) is now well underway. In this talk, I will give a update on construction, science verification, and what this stage of project development means for the Dutch astronomy community. In particular, I will focus on the establishment of our own regional centre, and its expected role in the community. NAC is...
Go to contribution page