works on

From the 3 of 45 linked papers with an AI index.

activity
20242026
most citedThe SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts

2 citations · 3 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

13 papers · 1 filter

astro-ph.GA2026

The eROSITA X-ray luminosity function of active galactic nuclei

W. Roster, J. Buchner, M. Salvato +23

The paper measures the soft X‑ray luminosity function of active galactic nuclei using eROSITA data across a wide luminosity and redshift range, introduces a redshift‑dependent brok…

astro-ph.GA2026

The incidence of eROSITA X-ray AGN in the local Universe: from dwarf to massive galaxies

Z. Igo, A. Merloni, A. Georgakakis +22

Combining deep, wide-area X-ray surveys with multi-wavelength catalogues provides insights into rare, highly-accreting AGN and low-mass galaxies at low redshift, the latter potenti…

astro-ph.GA2026

Large-scale and local environmental drivers of quenching: tracing H concentration in X-ray and optical galaxy groups

Stefania Barsanti, Di Wang, Matthew Colless +11

To explore the environmental mechanisms causing quenching in nearby star-forming galaxies, we study the variation with local and large-scale environments of a star formation concen…

astro-ph.GA2025

Unveiling the Sources of X-ray Luminosity in DESI Galaxy Groups: Insights from the SRG/eROSITA All-Sky Survey

YunLiang Zheng, Xiaohu Yang, Teng Liu +10

We use the first eROSITA all-sky survey (eRASS1) to investigate the contributions of AGN and extended gas to the total X-ray luminosity () of galaxy groups with different halo…

astro-ph.GA2025

The hot circumgalactic medium in stacked X-rays: observations vs simulations

Skylar Grayson, Evan Scannapieco, Johan Comparat +5

Current cosmological simulations rely on active galactic nuclei (AGN) feedback to quench star formation and match observed stellar mass distributions, but models for AGN feedback a…

astro-ph.GA2025

The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters

V. Toptun, P. Popesso, I. Marini +15

Galaxy groups and clusters are among the best probes of structure formation and growth in a cosmological context. Most of their baryonic component is dominated by the intracluster…