collaborators

15 papers

astro-ph.GA2026

Emulating the complex galactic-scale orbital dynamics of LISA massive black hole pairs with normalizing flows

Pedro R. Capelo, Carlos Moreno Martinez, Nodens Koren +6

The paper introduces a machine‑learning emulator based on conditional normalizing flows to rapidly predict the orbital decay of massive black hole pairs in galaxy merger remnants,…

astro-ph.GA2026

Gravitational Wave Astronomy With TianQin

En-Kun Li, Shuai Liu, Alejandro Torres-Orjuela +50

The paper outlines the scientific potential of the TianQin space‑based gravitational‑wave observatory, describing the types of compact‑object sources it can detect in the mHz band…

astro-ph.GA2026

Too shy to spin? Cosmic wallflowers as proto-globular clusters

Floor van Donkelaar, Lucio Mayer, Pedro R. Capelo

We investigate the rotational properties of star-forming clusters at in the high-resolution simulation MassiveBlackPS, focusing on two formation channels: clusters for…

astro-ph.HE2026

Multi-messenger and Multi-band Studies of Massive Black Holes: the Synergies Between LISA and SKAO

Pedro R. Capelo, Alberto Mangiagli, Lorenz Zwick +2

Depending on its mass, the same gas-embedded massive black hole (BH) binary can emit gravitational waves (GWs) in one or more bands (nHz and mHz) concurrently, along with electroma…

astro-ph.GA2026

The role of major mergers in triggering super-Eddington accretion

Riccardo Caleno, Tommaso Zana, Raffaella Schneider +6

JWST observations have opened a new era in the exploration of the high-redshift Universe, revealing black holes (BHs) with masses of several million solar masses already at ,…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…