collaborators

44 papers

astro-ph.CO2026

Learning Cosmology from Nearest Neighbour Statistics

Atrideb Chatterjee, Arka Banerjee, Francisco Villaescusa-Navarro +1

Extracting cosmological parameters from galaxy/halo catalogues with sub-percent level accuracy is an important aspect of modern cosmology, especially in view of ongoing and upcomin…

cs.AI2026

AI Scientists as Engines of Discovery: A Case for Development within Reformed Institutions

Raul Jimenez, Boris Bolliet, Francisco Villaescusa-Navarro +7

Agentic artificial intelligence (AI) systems are beginning to assist, accelerate, and partially automate scientific discovery, performing tasks that span literature synthesis, code…

astro-ph.CO2026

Learning the Universe with the 2nd Generation of CAMELS: Varying 35 parameters of the IllustrisTNG model in (50Mpc/h)^3 boxes

Shy Genel, Yongseok Jo, Boon Kiat Oh +10

We present a new set of 1,192 cosmological simulations as part of the CAMELS project, in which a space of 35 cosmological, astrophysical, and numerical parameters is explored aroun…

astro-ph.GA2026

Reconciling the Fundamental Plane of Early-Type Galaxies with hydrodynamical simulations: The case of IllustrisTNG100-1

Pedro de Araujo Ferreira, Nicola R. Napolitano, Crescenzo Tortora +2

The Fundamental Plane (FP) of Early-Type Galaxies (ETGs) encapsulates a tight correlation among their structural and dynamical properties and provides an important benchmark for ga…

astro-ph.CO2026

Cosmology with one galaxy: An analytic formula relating with galaxy properties

Kito Liao, Francisco Villaescusa-Navarro, Romain Teyssier +1

Standard cosmological analyses typically treat galaxy formation and cosmological parameter inference as decoupled problems, relying on population-level statistics such as clusterin…

astro-ph.CO2026

Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters

Christopher C. Lovell, Max E. Lee, William J. Roper +4

We present a new method for emulating the halo mass function (HMF) and other distribution functions in large effective volumes, down to low halo masses, whilst simultaneously modif…