Most of the research will be based on the ALMA telescope in Chile, which uses SRON / NOVA-developed technology. Rybak’s research will especially benefit from the new Band 2, which was partially built at the Groningen lab and which will become operational this autumn. Credit: ALMA

Did stars in the early Universe form like they do today? Early galaxies formed stars much faster than those we see now. To understand this, Rybak studies the dense, cold gas that will collapse into stars, tracing it using complex molecules – especially cyanides. Using large radio telescopes and gravitational lensing – Nature’s magnifying glass – he will detect cyanides in the dense gas in over a hundred early galaxies. These observations will provide new insights into how stars formed in the young Universe, helping us uncover the physical conditions that fueled such rapid star formation.

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