Tommaso Ronconi
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  • Contacts
  • Software
    • GalaPy
    • SCAMPy
    • T-RECS
    • CosmoBolognaLib
  • Research
    • The galaxy–halo connection
    • Galaxy formation and evolution
    • Cosmic voids
  • Page under construction
  • Publications
    • Cosmology from Synergies Between SKAO Surveys and Gravitational Wave Observations
    • HI Simulations for Cosmology with the SKA Observatory
    • Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory
    • GalaPy—Implementation strategies of the spectral modelling tool for galaxies in Python
    • Ultrahigh-redshift or closer-by, dust-obscured galaxies?: Deciphering the nature of faint, previously missed F200W dropouts in CEERS
    • Painting a full radio sky -- Empirical mock catalogues with multiple source populations for future radio surveys
    • Spatially resolved spectrophotometric SED modeling of NGC 253's central molecular zone: I. Star formation in extragalactic giant molecular clouds
    • GalaPy: A highly optimised C$_++$/Python spectral modelling tool for galaxies. I. Library presentation and photometric fitting
    • Little Ado about Everything: ensuremathηCDM, a Cosmological Model with Fluctuation-driven Acceleration at Late Times
    • The tiered radio extragalactic continuum (T-RECS) simulation II: H I emission and continuum-H I cross-correlation
    • The Way of Water: ALMA Resolves H$_2$O Emission Lines in a Strongly Lensed Dusty Star-forming Galaxy at z ensuremath∼ 3.1
    • ALMA Resolves the First Strongly Lensed Optical/Near-IR-dark Galaxy
    • A Stochastic Theory of the Hierarchical Clustering. III. The Nonuniversality and Nonstationarity of the Halo Mass Function
    • Astroparticle Constraints from the Cosmic Star Formation Rate Density at High Redshift: Current Status and Forecasts for JWST
    • Euclid: Cosmological forecasts from the void size function
    • Astroparticle Constraints from Cosmic Reionization and Primordial Galaxy Formation
    • Cosmology with the submillimetre galaxies magnification bias. Tomographic analysis
    • An ALMA view of 11 dusty star-forming galaxies at the peak of cosmic star formation history
    • Intensity and anisotropies of the stochastic gravitational wave background from merging compact binaries in galaxies
    • VizieR Online Data Catalog: Tomography with Magnification Bias (Bonavera+, 2021)
    • Unveiling the nature of 11 dusty star-forming galaxies at the peak of cosmic star formation history
    • From cosmic voids to collapsed structures: HPC methods for Astrophysics and Cosmology
    • SCAMPY - A sub-halo clustering and abundance matching based PYTHON interface for painting galaxies on the dark matter halo/sub-halo hierarchy
    • Cosmology with the submillimetre galaxies magnification bias: Proof of concept
    • Cosmology with the submillimetre galaxies magnification bias: Proof of concept
    • ScamPy: Sub-halo Clustering and Abundance Matching Python interface
    • Cosmic voids uncovered - first-order statistics of depressions in the biased density field
    • Cosmological exploitation of the size function of cosmic voids identified in the distribution of biased tracers
    • Cosmological exploitation of cosmic void statistics. New numerical tools in the CosmoBolognaLib to extract cosmological constraints from the void size function
  • Experience
  • Recent & Upcoming Talks

ScamPy: Sub-halo Clustering and Abundance Matching Python interface

Feb 1, 2020·
Tommaso Ronconi
,
Andrea Lapi
,
Matteo Viel
,
Alberto Sartori
· 0 min read
Type
Manuscript
publications
Last updated on Feb 1, 2020
← Cosmology with the submillimetre galaxies magnification bias: Proof of concept Jul 1, 2020
Cosmic voids uncovered - first-order statistics of depressions in the biased density field Oct 1, 2019 →

© 2026 Tommaso Ronconi. This work is licensed under CC BY NC ND 4.0

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