High- <i>z</i> [OI] emission lines: COLDSIM simulations and ALMA observations
Neutral-oxygen [OI] far-infrared emission lines at 63 μm and 145 μm are powerful probes of the physical conditions in the interstellar medium, although they have not been fully exploited in high-redshift studies.
Authors
- L. Tornatore (ORCID: https://orcid.org/0000-0003-1751-0130)
- Umberto Maio (ORCID: https://orcid.org/0000-0002-0039-3102)
- C. Feruglio (ORCID: https://orcid.org/0000-0002-4227-6035)
- Carl Ferkinhoff (ORCID: https://orcid.org/0000-0001-6266-0213)
- M. Bischetti
- G. L. Granato (ORCID: https://orcid.org/0000-0002-4480-6909)
- M. Parente (ORCID: https://orcid.org/0000-0002-3552-2672)
- Cinthia Ragone-Figueroa (ORCID: https://orcid.org/0000-0003-2826-4799)
- Francesco Salvestrini (ORCID: https://orcid.org/0000-0003-4751-7421)
- C. De Breuck
- R. Tripodi
Institutions
- University of Ljubljana (SI)
- Astronomical Observatory of Rome (IT)
- Trieste Astronomical Observatory (IT)
- Instituto de Astronomía Teórica y Experimental (AR)
- Computing Center (RU)
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (IT)
- Institute for Fundamental Physics of the Universe (IT)
- Centre for High Performance Computing (ZA)
- Winona State University (US)
- National Institute for Astrophysics (IT)
Publication Details
- Journal
- Astronomy and Astrophysics
- Published
- 2025-11-24
- DOI
- https://doi.org/10.1051/0004-6361/202557033
- Primary Topic
- Astrophysics and Star Formation Studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00