MG
Marta Galbiati
Trieste Astronomical Observatory, University of Milano-Bicocca
Research areas: Medicine · Hematology · Acute Lymphoblastic Leukemia research · Acute Myeloid Leukemia Research · Galaxies: Formation, Evolution, Phenomena
Employment
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Osservatorio Astronomico di Trieste Postdoctoral Researcher2026 - Present
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University of Milano-Bicocca Assegnista2024 - 2026
Education
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University of Milano-Bicocca Ph.D. in Physics and Astrophysics2021 - 2024
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University of Milano-Bicocca M.Sc. (Astrophysics and Space Physics)2019 - 2021
Projects & Funding
Projects & funding information is unavailable.
Publications (17)
- The hydrodynamical response of cold circumgalactic clouds to quasar radiation Save
- A quiescent galaxy in a gas-rich cosmic web node at z ∼ 3 Save
- Metal enrichment of galaxies in a massive node of the cosmic web at z ∼ 3 Save
- Resolving circumgalactic gas flows around a z ≈ 3.6 quasar using MUSE and ALMA Save
- MUSE Analysis of Gas around Galaxies (MAGG) Save
- ALMA survey of a massive node of the Cosmic Web at z ∼ 3 Save
- Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3 Save
- The MUSE Ultra Deep Field (MUDF) Save
- A giant disk galaxy two billion years after the Big Bang Save
- X-ray view of a massive node of the Cosmic Web at z ∼ 3 Save
- The MUSE Ultra Deep Field (MUDF). VI. The Relationship between Galaxy Properties and Metals in the Circumgalactic Medium Save
- MUSE Analysis of Gas around Galaxies (MAGG) Save
- ALMA survey of a massive node of the Cosmic Web at z ∼ 3 Save
- Resolving the physics of quasar Ly α nebulae (RePhyNe): I. Constraining quasar host halo masses through circumgalactic medium kinematics Save
- MUSE Analysis of Gas around Galaxies (MAGG) – V. Linking ionized gas traced by C iv and Si iv absorbers to Ly α emitting galaxies at z ≈ 3.0–4.5 Save
- Towards an automatic approach to modelling the circumgalactic medium: new tools for mock making and fitting of metal profiles in large surveys Save
- MUSE Analysis of Gas around Galaxies (MAGG) - IV. the gaseous environment of z ∼3-4 Ly α emitting galaxies Save