Webb's First Deep Field, galaxy cluster SMACS 0723 Engraving of Galileo with a telescope

§ 03 · TALKS & ROLES

Talks & Roles

Roles in surveys and collaborations, and invited and contributed talks

NASA, ESA, CSA, STScI, Webb's First Deep Field (2022)

Andreas Cellarius, Scenographia Compagis Mundanae Brahea, Harmonia Macrocosmica (1661)

§ 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

2026

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

2025

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

2024

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

2023

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

2022

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

2021

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