Carlotta Gruppioni
Ruolo: Primo ricercatore
Contatti
- Stanza: B-4W8
- Telefono: +39 051 6357 380
- Email: carlotta.gruppioni@inaf.it
Informazioni personali
- Orcid: 0000-0002-5836-4056
- Skype: carlotta_gruppioni
Paper più recenti su ADS
(based on ORCID, see here how to claim missing papers)
- A3COSMOS: Measuring the cosmic dust-attenuated star formation rate density at 4 < z < 5, Astronomy and Astrophysics, 2024
- The impact of stellar bars on star-formation quenching: Insights from a spatially resolved analysis in the local Universe, Astronomy and Astrophysics, 2024
- Dark progenitors and massive descendants: A first ALMA perspective of radio-selected near-IR-dark galaxies in the COSMOS field, Astronomy and Astrophysics, 2024
- Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances, and intracluster light from a semi-empirical perspective, Monthly Notices of the Royal Astronomical Society, 2024
- The ALPINE-ALMA [C II] survey: characterization of spatial offsets in main-sequence galaxies at z 4-6, Monthly Notices of the Royal Astronomical Society, 2024
- The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe, Astronomy and Astrophysics, 2024
- COSMOS2020: Investigating the AGN-obscured accretion phase at z ∼ 1 via [Ne V] selection, Astronomy and Astrophysics, 2024
- Protoclusters as drivers of stellar mass growth in the early Universe, a case study: Taralay - a massive protocluster at z 4.57, Monthly Notices of the Royal Astronomical Society, 2024
- MIRACLE: Mid-IR Activity of Circumnuclear Line Emission, JWST Proposal. Cycle 3, 2024
- A Deep Look into PAHs: Resolved PAH and Fine-Structure Emission in z=1 Main-Sequence Galaxies, JWST Proposal. Cycle 3, 2024