ANTONIO PENSABENE

Employment

• Universita' di Milano Bicocca Assegnisti
  2021 - 2025

Education

• University of Bologna Ph.D. in Astrophysics
  2018 - 2021
• University of Florence M.Sc. in Physical and Astrophysical Sciences, curriculum: Astrophysics
  2014 - 2017
• University of Florence B.Sc. in Physics and Astrophysics
  2010 - 2014

Projects & Funding

Projects & funding information is unavailable.

Publications (34)

• A quiescent galaxy in a gas-rich cosmic web node at z ∼ 3
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202659351
  +Save
• Morphology, sizes, and scatter in a large sample of distant quiescent galaxies
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202659598
  +Save
• CO(7–6) and [C I](2–1) survey in z > 6 quasars
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202557762
  +Save
• Dynamical properties and star formation history of a low-mass quenched galaxy at cosmic noon
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202558795
  +Save
• Metal enrichment of galaxies in a massive node of the cosmic web at z ∼ 3
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202558229
  +Save
• Resolving circumgalactic gas flows around a z ≈ 3.6 quasar using MUSE and ALMA
  M. Galbiati, Antonio Pensabene, Sebastiano Cantalupo +10 more
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202558310
  +Save
• Infrared emission from z ∼ 6.5 quasar host galaxies: a direct estimate of dust physical properties
  Astronomy & Astrophysics 2026 DOI: 10.1051/0004-6361/202556812
  +Save
• ALMA survey of a massive node of the Cosmic Web at z ∼ 3
  Astronomy & Astrophysics 2025 DOI: 10.1051/0004-6361/202554769
  +Save
• The properties of X-ray-selected active galactic nuclei in protoclusters pinpointed by enormous Lyman alpha nebulae
  Astronomy & Astrophysics 2025 DOI: 10.1051/0004-6361/202555443
  +Save
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3
  Astronomy & Astrophysics 2025 DOI: 10.1051/0004-6361/202452493
  +Save
• The MUSE Ultra Deep Field (MUDF)
  Antonio Pensabene, M. Galbiati, Michele Fumagalli

  +12 more

  • Matteo Fossati
  • Ian R. Smail
  • Marc A. Rafelski
  • Mitchell Revalski
  • Fabrizio Arrigoni Battaia
  • +7 more
  Astronomy & Astrophysics 2025 DOI: 10.1051/0004-6361/202452462
  +Save
• A giant disk galaxy two billion years after the Big Bang
  Nature Astronomy 2025 DOI: 10.1038/s41550-025-02500-2
  +Save
• X-ray view of a massive node of the Cosmic Web at z ∼ 3 I. An exceptional overdensity of rapidly accreting supermassive black holes
  2025 DOI: 10.1051/0004-6361/202452179
  +Save
• Constraining the Excitation of Molecular Gas in Two Quasar-starburst Systems at z ∼ 6
  The Astrophysical Journal 2024 DOI: 10.3847/1538-4357/ad8de2
  +Save
• A quasar-galaxy merger at z ∼ 6.2: Rapid host growth via the accretion of two massive satellite galaxies
  Astronomy & Astrophysics 2024 DOI: 10.1051/0004-6361/202449239
  +Save
• MUSE view of PDS 456: Kiloparsec-scale wind, extended ionized gas, and close environment
  Astronomy and Astrophysics 2024 DOI: 10.1051/0004-6361/202449201
  +Save
• ALMA survey of a massive node of the Cosmic Web at z ∼ 3
  Astronomy & Astrophysics 2024 DOI: 10.1051/0004-6361/202348659
  +Save
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: The hidden circumgalactic medium
  arXiv e-prints 2024 DOI: 10.48550/arXiv.2403.00924
  +Save
• A benchmark for extreme conditions of the multiphase interstellar medium in the most luminous hot dust-obscured galaxy at z = 4.6
  2024 DOI: 10.1051/0004-6361/202347869
  +Save
• A quasar-galaxy merger at z ~ 6.2: Black hole mass and quasar properties from the NIRSpec spectrum
  2024 DOI: 10.1051/0004-6361/202348535
  +Save