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From the 2 of 13 linked papers with an AI index.

most citedGravitational Wave Astronomy With TianQin

53 citations · 53 across the 2 of their papers we have counts for

collaborators

13 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.GA202653 cited

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.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

Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D

Francesco Sinigaglia, Miroslava Dessauges-Zavadsky, Lucio Mayer +2

Bridging theory and observations is a key task to understand galaxy formation and evolution. With the advent of state-of-the-art observational facilities, an accurate modelling of…

astro-ph.GA2026

Super-Eddington accretion in protogalactic cores

Tommaso Zana, Pedro R. Capelo, Mairo Boresta +6

The presence of massive black holes (BHs) exceeding already at redshift challenges standard models of BH growth. Super-Eddington (SE) accretion has…