SC
Sebastiano Cantalupo
University of Milano-Bicocca, ETH Zurich
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
Employment
-
Università degli Studi di Milano-Bicocca Professor2020 - Present
-
ETH Zurich Assistant Professor? - 2021
Education
Education history is unavailable.
Projects & Funding
Projects & funding information is unavailable.
Publications (130)
- Strong environmental active galactic nuclei enhancement among dusty star-forming galaxies in z > 2 protoclusters Save
- A Partial Lyman Limit Absorber in the Halo of a Galaxy Pair: A Possible Signature of Gas Inflow Save
- MUSEQuBES: Probing Anisotropies in Gas and Metal Distributions in the Circumgalactic Medium Save
- 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
- X-ray view of a massive node of the cosmic web 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
- MUSEQuBES: the column density, covering fraction, mass, and environmental dependence of cool H i gas around low-redshift galaxies Save
- Kinematic Analysis of an Ultrastrong Mg II Absorber at z ≈ 1.13 Linked to Circumgalactic Gas Structures Save
- H i Properties of Field Galaxies at z ≈ 0.2–0.6: Insights into Declining Cosmic Star Formation Save
- ALMA survey of a massive node of the Cosmic Web at z ∼ 3 Save
- Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg2 Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM H i Save
- MUSEQuBES: The Column Density, Covering Fraction, and Mass of O vi-bearing Gas in and Around Low-redshift Galaxies Save
- The Morphology and Kinematics of a Giant, Symmetric Nebula around a Radio-loud Quasar 3C 57: Extended Rotating Gas or Biconical Outflows? Save
- Formation and Environmental Context of Giant Bulgeless Disk Galaxies in the Early Universe: Insights from Cosmological Simulations Save
- A giant disk galaxy two billion years after the Big Bang Save
- MUSEQuBES: Connecting H i Absorption with Lyα Emitters at z ≈ 3.3 Save
- MUSEQuBES: The Kinematics of O vi-bearing Gas in and around Low-redshift Galaxies Save
- MUSEQuBES: Unveiling Cosmic Web Filaments at z ≈ 3.6 through Dual Absorption and Emission Line Analysis Save