activity
20242026
most citedNonlinear quasinormal mode detectability with next-generation gravitational wave detectors

40 citations · 118 across the 20 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2026

Euclid Quick Data Release (Q1): Disc breaks highlight the structural evolution of galaxies through time

Euclid Collaboration, P. M. Sanchez-Alarcon, J. Román +302

Changes in the slope of the radial surface brightness profiles of disc galaxies, or disc breaks, encode valuable information about the processes driving disc formation and growth.…

astro-ph.GA2026

Investigating the formation channel of GW231123: Population III stars or hierarchical mergers?

Federico Angeloni, Konstantinos Kritos, Raffaella Schneider +5

The gravitational wave event GW231123, with component black hole masses lying within or above the pair-instability mass gap, poses a significant challenge to current stellar evolut…

astro-ph.GA2026

Predicting intermediate-mass black hole formation in star clusters with machine learning

Konstantinos Kritos, Digvijay Wadekar, Emanuele Berti

Whether intermediate-mass black holes reside in nearby star clusters has remained contested for decades. We address this question by training neural network and random forest regre…

astro-ph.GA2025★ 1 cited

Milky Way Globular Clusters: Nurseries for Dynamically-Formed Binary Black Holes

Federico Angeloni, Konstantinos Kritos, Raffaella Schneider +4

We present a novel self-consistent theoretical framework to characterize the formation, evolution, and merger sites of dynamically-formed black hole binaries, with a focus on expla…

astro-ph.GA2024

Supermassive black hole growth in hierarchically merging nuclear star clusters

Konstantinos Kritos, Ricarda S. Beckmann, Joseph Silk +5

Supermassive black holes are prevalent at the centers of massive galaxies, and their masses scale with galaxy properties, increasing evidence suggesting that these trends continue…