Francesco Calura
Position: Researcher
Contact info
- Room: B-3W2
- Phone: +39 051 6357 333
- Email: francesco.calura@inaf.it
Personal info
- Orcid: 0000-0002-6175-0871
- Skype: fcalura
Curriculum vitae
2011-date: Researcher, INAF-OAS, Italy
2010-2011: Research Fellow, University of Central Lancashire, UK
2009-2010: Post-doc, Trieste Observatory, Italy
2008-2009: Post-doc, Trieste University, Italy
2006-2008: Post-Doc, Trieste Observatory, Italy
2004-2006: Post-Doc, Trieste University, Italy
2004: PhD in Physics, Trieste University, Italy
1999: Laurea in Physics, Ferrara University, Italy.
Latest papers on ADS
(based on ORCID, see here how to claim missing papers)
- Early Results from GLASS-JWST. VII. Evidence for Lensed, Gravitationally Bound Protoglobular Clusters at z = 4 in the Hubble Frontier Field A2744, The Astrophysical Journal, 2022
- Ionizing feedback effects on star formation in globular clusters with multiple stellar populations, Monthly Notices of the Royal Astronomical Society, 2022
- The probability of galaxy-galaxy strong lensing events in hydrodynamical simulations of galaxy clusters, Astronomy and Astrophysics, 2022
- The resolved scaling relations in DustPedia: Zooming in on the local Universe, Astronomy and Astrophysics, 2022
- Sub-parsec resolution cosmological simulations of star-forming clumps at high redshift with feedback of individual stars, Monthly Notices of the Royal Astronomical Society, 2022
- Exploring the physical properties of lensed star-forming clumps at 2 ≲ z ≲ 6, Monthly Notices of the Royal Astronomical Society, 2022
- The role of rotation on the formation of second generation stars in globular clusters, Monthly Notices of the Royal Astronomical Society, 2022
- SPRITZ is sparkling: Simulated CO and [C II] luminosities, Astronomy and Astrophysics, 2022
- Supermassive black holes at high redshift are expected to be obscured by their massive host galaxies' interstellar medium, Astronomy and Astrophysics, 2022
- Mapping the morphology of the ionizing radiation from a LyC emitting galaxy at z=4.00, HST Proposal, 2022
Contributions to this website