§ 01 · Roles
Roles
- 2026 – now
- Euclid Consortium: Lead of the Key Project on the joint 2PCF+3PCF full-shape analysis of Euclid DR1.
- 2024 – now
- Wide-Field Spectroscopic Telescope: Lead of the Quasar and Galaxy Clustering + IGM/Lyman-α forest Work Package of the Cosmology Working Group.
- 2023 – 2026
- Euclid Consortium: Lead of the Key Project on full-shape modelling of two-point and three-point correlation functions in configuration space on the Flagship simulations (Euclid Collaboration: Guidi et al. 2026, A&A 707, A228).
- 2020 – now
- Euclid Consortium: Associate active member (SWG-GC and OU-PF).
- 2024 – now
- INAF (National Institute of Astrophysics): Bologna Unit Associate.
- 2024 – now
- CosmoVerse (COST Action CA21136): Associate Member.
- Feb 2026 – now
- Cosmology Journal Club: organiser, Bologna Physics and Astronomy Department.
- July 2025
- Scientific Organizing Committee: Optimizing the Extraction of Cosmological Information from the Latest Spectroscopic Redshift Surveys, Sexten, Italy.
§ 02 · Talks
Talks
Constraining cosmology combining lower- and higher-order statistics of Large Scale Structure
Institute of Cosmos Sciences (ICCUB), University of Barcelona, Barcelona, Spain
First full-shape joint analysis of the 2PCF and 3PCF in redshift space on real data
European Astronomical Society Annual Meeting, Lausanne, Switzerland
Towards cosmological constraints from the first full-shape joint 2PCF + 3PCF analysis on real data
Rencontres de Moriond, La Thuile, Italy
Full-shape joint two-point and three-point clustering statistics in configuration space
Euclid Galaxy Clustering Science Working Group Meeting, Marseille, France Lightning talk
Modeling higher-order peculiar velocity density correlations
DESC workshop on cosmology with peculiar velocities, Marseille, France
Cosmology from Large Scale full-shape analyses combining 2PCF and 3PCF
Optimizing the Extraction of Cosmological Information from the Latest Spectroscopic Redshift Surveys, Sexten, Italy
Cosmology with full-shape galaxy clustering statistics beyond 2-point
Cosmology on Safari, Hluhluwe, South Africa
Cosmology with higher-order statistics with the Wide Field Spectroscopic Telescope
WST Italian Workshop, Napoli, Italy
Toward the first, joint full-shape 2PCF + 3PCF analysis on real data
Euclid Galaxy Clustering Science Working Group Meeting, Garching, Germany
Accelerating Likelihood Exploration to Constrain Cosmological Parameters Using 2- and 3-Point Correlation Functions Emulators
Aurum, Gabriele D'Annunzio University and Icranet, Pescara, Italy
Constraining Cosmological Parameters Combining 2- and 3-Point Correlation Functions: First Step Towards the Future Euclid Dataset
Aurum, Gabriele D'Annunzio University and Icranet, Pescara, Italy
Accelerating Maximum Likelihood Estimation to Constrain Cosmological Parameters Using 2- and 3- Point Correlation Functions
Sapienza University, Rome, Italy
A joint 2PCF + 3PCF analysis in real space in view of Euclid
Laboratoire d'Astrophysique de Marseille, Marseille, France
Modelling the large-scale structure with three-point correlation function (3PCF)
Post-Industrial Bispectrum Meeting, University of Milan, Milan, Italy
Modelling the three-point correlation function (3PCF) of the large-scale structure in the small-scale regime
University of Milan, Milan, Italy
Constraining the large-scale structure with new modelling approaches of the three-point correlation function
Laboratoire d'Astrophysique de Marseille, Marseille, France
The 2PCF + 3PCF analysis in real space
Euclid GC Modelling Challenge Meeting, IFPU, Trieste, Italy Invited talk
Going nonlinear: modelling the real-space next-to-leading order three-point correlation function of Large Scale Structure of the universe
European Astronomical Society Annual Meeting, Valencia, Spain
Modelling the next-to-leading order 3-point correlation function
Euclid Early Career Workshop, online
Going nonlinear: toward a 1-loop model for the 3-point matter correlation function
PRIN meeting: discovering the Dark Universe, from Darklight to Dark Matter, Barolo, Italy
Modelling higher order statistics of the cosmic density field
Astrophysics Journal Club, Sapienza University of Rome, Rome, Italy