EPSC Abstracts
Vol. 18, EPSC-DPS2025-1391, 2025, updated on 09 Jul 2025
https://doi.org/10.5194/epsc-dps2025-1391
EPSC-DPS Joint Meeting 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Hot Jupiters in crowded environements
Laura Magrini
Laura Magrini
  • Italy (laura.magrini@inaf.it)


 The Very High-Resolution Multi-Object Spectrograph (HRMOS) will be proposed as a new instrument for the ESO Very Large Telescope (VLT) as part of the VLT2030 roadmap. HRMOS will play a crucial role in bridging the gap in observational capabilities among the next generation of astronomical instruments planned for the coming decades.

By offering a unique combination of high-resolution and multi-object spectroscopy, HRMOS will enable groundbreaking scientific investigations that would otherwise remain inaccessible. These include the study of extrasolar planets in crowded stellar environments, like open and globular clusters, but also the Galactic bulge and the nearest dwarf galaxies.

How to cite: Magrini, L.: Hot Jupiters in crowded environements, EPSC-DPS Joint Meeting 2025, Helsinki, Finland, 7–12 Sep 2025, EPSC-DPS2025-1391, https://doi.org/10.5194/epsc-dps2025-1391, 2025.