activity
19932026
most citedThe cored distribution of dark matter in spiral galaxies

583 citations · 8.5k across the 126 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

29 papers · 1 filter

astro-ph.GA2026

Extended Universal Rotational Curve of Spiral Galaxies

Esha Bhatia, Paolo Salucci, Tiziano Schiavone +1

In this work, we aim to advance the Universal Rotation Curve (URC) paradigm by leveraging new data and extending its observational domain. Building on previous studies that establi…

astro-ph.GA2023

Euclid preparation. Spectroscopy of active galactic nuclei with NISP

Euclid Collaboration, E. Lusso, S. Fotopoulou +246

The statistical distribution and evolution of key properties (e.g. accretion rate, mass, or spin) of active galactic nuclei (AGN), remain an open debate in astrophysics. The ESA Eu…

astro-ph.GA2023★ 6 cited

Dark Matter Fraction in Disk-Like Galaxies Over the Past 10 Gyr

G. Sharma, G. van de Ven, P. Salucci +1

We present an observational study of the dark matter fraction in star-forming disk-like galaxies up to redshift , selected from publicly available integral field spectr…

astro-ph.GA2023★ 12 cited

Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales

Francesco Benetti, Andrea Lapi, Giovanni Gandolfi +2

[abridged] We explore the possibility that the dark matter (DM) component in galaxies may originate fractional gravity. In such a framework, the standard law of inertia continues t…

astro-ph.GA2021★ 22 cited

Observational Evidence of Evolving Dark Matter Profiles at

Gauri Sharma, Paolo Salucci, Glenn van de Ven

We investigate the dark matter halos of 256 star-forming disc-like galaxies at using the KMOS redshift one spectroscopic survey (KROSS). This sample covers the redshifts…

astro-ph.GA2021★ 12 cited

Dark Matter Fraction in z~1 Star-Forming Galaxies

Gauri Sharma, Paolo Salucci, Glenn van de Ven

We present a observational study of the dark matter fraction in 225 rotation supported star-forming galaxies at having stellar mass range: $ 9.0 \leq log(M_* \ \math…