MR
Marina Rejkuba
European Southern Observatory, Pontificia Universidad Católica de Chile
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
0000-0002-6577-2787
Employment
-
European Southern Observatory Associate Astronomer, User Support Astronomers Department Head
Education
- 1998 - 2002
Projects & Funding
Projects & funding information is unavailable.
Publications (443)
- Large Magellanic Cloud Globular Clusters in the Near-infrared. I. RR Lyrae in Reticulum Save
- The ESO science archive: a powerful resource for the worldwide science community (Erratum) Save
- 25 years science return of the Very Large Telescope Save
- ESO science operations: from the VLT to the ELT Save
- ESOFinder: an LLM-powered tool to help users navigate ESO documentation Save
- Evolving time allocation and scheduling for the ESO VLT and VLTI Save
- The ESO science archive: a powerful resource for the worldwide science community Save
- ESO User Support and Observation Preparation for VLTI Science Operations Save
- Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster: VI. A star-forming UDG in Hydra I: A rare UDG or a transition phase Save
- ESOFinder: an LLM-powered tool to help users navigate ESO documentation Save
- Intracluster globular clusters as tracers of the mass assembly of the Hydra I galaxy cluster Save
- The KMOS Spectroscopic Public Surveys Save
- Distance measurements from the internal dynamics of globular clusters: Application to the Sombrero galaxy (M 104) Save
- Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster Save
- Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra I cluster. V. Integrated stellar population properties Save
- Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUs Save
- Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Resolved Stellar Populations Studies in M31 and its Satellites Save
- Euclid preparation: LXXIII. Spatially resolved stellar populations of local galaxies with Euclid: A proof of concept using synthetic images with the TNG50 simulation Save
- Globular clusters in M 104: Tracing kinematics and metallicities from the centre to the halo Save
- New kinematic map of the Milky Way bulge Save