Suomen ESO-keskus
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- SN 2021fxy: mid-ultraviolet flux suppression is a common feature of Type Ia supernovae (2023)
- SN 2021gno: a calcium-rich transient with double-peaked light curves (2023)
- SN 2021zny: an early flux excess combined with late-time oxygen emission suggests a double white dwarf merger event (2023)
- SN 2022ngb : A faint, slowly evolving Type IIb supernova with a low-mass envelope (2026)
- SN 2023gpw: Exploring the diversity and power sources of hydrogen-rich superluminous supernovae (2026)
- SN 2023ixf: Interaction signatures in the spectrum at 445 days (2025)
- SN 2023tsz: a helium-interaction-driven supernova in a very low-mass galaxy (2025)
- SN 2024abfo: A partially stripped type II supernova from a yellow supergiant (2025)
- Solar analogues and solar twins in the HARPS archive (2014)
- Solar-insolation-induced changes in the coma morphology of comet 67P/Churyumov-Gerasimenko Optical monitoring with the Nordic Optical Telescope (2017)
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