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most citedGravitational Wave Astronomy With TianQin

56 citations · 68 across the 14 of their papers we have counts for

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astro-ph.HE2025

The LISA Astrophysics "Disc-IMRI" Code Comparison Project: Intermediate-Mass-Ratio Binaries in AGN-Like Discs

Andrea Derdzinski, Alexander J. Dittmann, Alessia Franchini +16

Upcoming space-based gravitational wave detectors such as LISA, the Laser Interferometer Space Antenna, will be sensitive to extreme- and intermediate-mass-ratio inspirals (EMRIs a…

astro-ph.GA2025★ 3 cited

The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier

Hyeonyong Kim, Ji-hoon Kim, Minyong Jung +22

Recent observations from JWST have revealed unexpectedly luminous galaxies, exhibiting stellar masses and luminosities significantly higher than predicted by theoretical models at…

astro-ph.GA2025★ 2 cited

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…

astro-ph.GA2025

Introducing the Phoebos simulation: galaxy properties at the dawn of galaxy formation

Floor van Donkelaar, Pedro R. Capelo, Lucio Mayer +2

The James Webb Space Telescope (JWST) now allows us to observe galaxies at the end of cosmic dawn () with unprecedented detail, revealing their morphologies, sizes, a…

astro-ph.GA2025★ 4 cited

The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at

Minyong Jung, Ji-hoon Kim, Thinh H. Nguyen +24

We investigate how differences in the stellar feedback produce disks with different morphologies in Milky Way-like progenitors over 1 , using eight state-of-the-art…

astro-ph.GA2025

A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations

Wei-Bo Kao, Pedro R. Capelo, Elia Cenci +3

Super-Eddington accretion has been proposed to explain the existence of black holes (BHs) with masses exceeding a billion solar masses within the first billion years after the Big…