Livia Vallini
Ruolo: Ricercatore
Contatti
- Stanza: B-3W6
- Telefono: +39 051 6357 371
- Email: livia.vallini@inaf.it
Informazioni personali
- Orcid: 0000-0002-3258-3672
Paper più recenti su ADS
(based on ORCID, see here how to claim missing papers)
- Direct detection of cool molecular gas in a star-forming galaxy at z=7.31, Monthly Notices of the Royal Astronomical Society, 2026
- The ALPINE─CRISTAL─JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z ∼ 5, The Astrophysical Journal, 2026
- The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main-sequence star-forming galaxies and their kinematics at 4 < z < 6, Astronomy and Astrophysics, 2026
- The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison between the ISM and CGM of Main-sequence Galaxies at z = 4─6, The Astrophysical Journal, 2026
- The ALPINE-CRISTAL-JWST Survey: Stellar and Nebular Dust Attenuation of Main-sequence Galaxies at z ∼ 4─6, The Astrophysical Journal, 2026
- JWST/MIRI-MRS View of the Metal-poor Galaxy CGCG 007-025: The Spatial Location of Polycyclic Aromatic Hydrocarbons and Very Highly Ionized Gas, The Astrophysical Journal Letters, 2026
- The early Universe with JWST and ALMA, Nature Astronomy, 2026
- The observed total star formation rate function up to z ∼ 6: Complementary UV and IR contributions and comparison with state-of-the-art galaxy formation models, Astronomy and Astrophysics, 2026
- The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-sequence Galaxies at z = 4─6, The Astrophysical Journal Supplement Series, 2026
- The ALPINE-CRISTAL-JWST survey: Spatially resolved star formation relations at z ∼ 5, Astronomy and Astrophysics, 2025