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F. Pace

4 papers hereh-index 114 citations5 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO4
same name
  • F. Pace — 25 papers, h 24
  • F. Pace — 12 papers, h 5
  • F. Pace — 9 papers, h 5
  • F. Pace — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
collaborators

4 papers

astro-ph.CO2026

Redshift dependence and dipolar velocity corrections in cosmographic reconstructions through Type Ia supernova samples

Anna Chiara Alfano, Youri Carloni, Orlando Luongo +1

We perform a cosmographic analysis of Type Ia supernovae using the Pantheon+\&SH0ES, DES-SNY5 and Union3 compilations. We consider different redshift intervals, analyzed through a…

astro-ph.CO2024

Effects of dynamical friction on perturbations for evolving dark energy

Francesco Pace, Orlando Luongo, Antonino Del Popolo

We explore the impact of dynamical friction on scales where the linear growth factor and the spherical collapse model can be applied and show its influence on the evolution of pert…

astro-ph.CO2023

Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition

Orlando Luongo, Francesco Pace, Sebastiano Tomasi

We analyze time-dependent dark energy equations of state through linear and nonlinear structure formation and their quintessence potentials, characterized by fast, recent transitio…

astro-ph.CO2023

Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-ΛCDM models

Euclid Collaboration, B. Bose, P. Carrilho +229

We investigate the approximations needed to efficiently predict the large-scale clustering of matter and dark matter halos in beyond-ΛCDM scenarios. We examine the normal branch…

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