activity
20192026
most citedIntroducing the AIDA-TNG project: galaxy formation in alternative dark matter models

20 citations · 26 across the 6 of their papers we have counts for

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6 papers · 1 filter

astro-ph.CO2026

Observation-driven simulations of strong lensing galaxy clusters

L. Leuzzi, M. Meneghetti, A. Adam +9

Galaxy clusters are the most powerful strong lenses: they greatly magnify the flux of distant and faint sources. Strong lensing also allows for the reconstruction of their mass dis…

astro-ph.CO2026★ 2 cited

The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models

Giulia Despali, Carlo Giocoli, Lauro Moscardini +3

In the standard Cold Dark Matter (CDM) scenario, the density profiles of dark matter haloes are well described by analytical models linking their concentration to halo mass. Altern…

astro-ph.CO2026★ 2 cited

The AIDA-TNG project: 3D halo shapes

C. Giocoli, G. Despali, L. Moscardini +4

Context. The shapes of dark matter halos can be used to constrain the fundamental properties of dark matter. In standard Cold Dark Matter (CDM) cosmologies, halos are typically tri…

astro-ph.CO2025★ 1 cited

The AIDA-TNG project. Abundance, radial distribution, and clustering properties of halos in alternative dark matter models

Massimiliano Romanello, Giulia Despali, Federico Marulli +3

Warm and self-interactive dark matter cosmologies have been proposed as nonbaryonic solutions to the tensions between the cold dark matter model and observations at the kilopar…

astro-ph.CO2025★ 20 cited

Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models

Giulia Despali, Lauro Moscardini, Dylan Nelson +3

We introduce the AIDA-TNG project, a suite of cosmological magnetohydrodynamic simulations that simultaneously model galaxy formation and different variations of the underlying dar…

astro-ph.CO2019★ 1 cited

Polarisation as a tracer of CMB anomalies: Planck results and future forecasts

M. Billi, A. Gruppuso, N. Mandolesi +2

The lack of power anomaly is an intriguing feature at the largest angular scales of the CMB anisotropy temperature pattern, whose statistical significance is not strong enough to c…