Detectors are a key feature of the contemporary scientific approach to cultural heritage (CH),
both for diagnostics and conservation. INFN-CHNet is the network of the Italian National …

For millennia, mankind has been fascinated by the marvel of the starry night sky. Yet, a
proper scientific understanding of how stars form, shine, and die is a relatively recent …

The lockdowns held due to the COVID-19 pandemic conducted to changes in air quality.
This study aimed to understand the variability of PM 2.5 levels and composition in an urban …

The modelling of molecular excitation and dissociation processes relevant to astrochemistry
requires the validation of theories by comparison with data generated from laboratory …

The Ice Chamber for Astrophysics–Astrochemistry (ICA) is a new laboratory end station
located at the Institute for Nuclear Research (Atomki) in Debrecen, Hungary. The ICA has …

Direct measurements of reaction cross-sections at astrophysical energies often require the
use of solid targets able to withstand high ion beam currents for extended periods of time …

The worldwide restrictions due to the COVID-19 pandemic induced a radical change in
urban air quality. The objective of this work was to study and understand the variation of PM …

The ubiquity of sulfur ions within the Jovian magnetosphere has led to suggestions that the
implantation of these ions into the surface of Europa may lead to the formation of SO2 …

A sensitive in-air millibeam PIXE setup has recently been installed at the external beamline
of the ATOMKI 2 MV Tandetron accelerator (Debrecen, Hungary) for high-throughput …

Background: N 14 (p, γ) O 15 is one of the key reactions of nuclear astrophysics, playing a
role in various stellar processes and influencing energy generation of stars, stellar evolution …