New research indicates that early galaxies contain large amounts of gas and dust, essential for star formation, more than theoretical models would indicate. In a recently published paper, a team of scientists from the NCBJ Astrophysics Division used observations from the ALPINE-ALMA program to investigate the presence of gas and dust in galaxies that formed within the first billion years after the Big Bang.

With 40 world-class collaborating institutions from 14 countries, ACME brings together the astroparticle and astronomy communities in a joint effort to forge a basis for strengthened long-term collaboration between these research infrastructures irrespective of location and level up access opportunities across Europe and beyond. The National Centre for Nuclear Research node is one of the most active partners of the ACME consortium.

On Monday, June 24, 2024, a Special Colloquium of the Fundamental Research Department of the National Centre for Nuclear Research was held, during which awards for achievements in 2023 were presented. The jury distinguished research on low brightness galaxies and for attempts to explain phenomena occurring during collisions of relativistic ions. Popular science stories and essays in which the author managed to hide his fascination with discovering the universe were also honored.

When we look at the night sky, we cannot free ourselves from questions. We wonder if it is possible to count the stars. We imagine how great a distance separates us from them. When we realize what a light year actually is, we are surprised to discover that we are actually looking into the further or closer past. Scientists from the National Center for Nuclear Research experience a similar fascination, looking for answers to these and other questions about how the Universe looks and works. In the coming years, this search will be able to be more effective thanks to the project „ Barely visible: low surface brightness galaxies in the LSST era” under the supervision of Prof. dr hab. Agnieszka Pollo financed by the National Science Center under the MAESTRO program.

Dr William James Pearson will investigate how we can more reliably identify galaxy mergers using their morphologies and how mergers influence their dust content, dust attenuation, and metallicity. This will be done by combining artificial intelligence (AI) with more traditional methods to detect galaxy mergers as well as use state of the art. observations and techniques to study the galaxies’ dust and metal. Exploration of this fascinating topic will be possible thanks to a grant from the National Science Center under the SONATA programme.

On 14 May, nominations for members of the Committee on Astronomy of the Polish Academy of Sciences for the term 2024-2027 were announced. Among the members were scientists from the NCBJ's Astrophysics Division. Prof Katarzyna Małek was also elected to the Presidium of the Committee.