activity
20072026
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 13.4k across the 233 of their papers we have counts for

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Showing 2017Show all

18 papers · 1 filter

astro-ph.GA2017★ 4 cited

Caught in the rhythm II: Competitive alignments of satellites with their inner halo and central galaxy

Charlotte Welker, Chris Power, Christophe Pichon +3

The anisotropic distribution of satellites around the central galaxy of their host halo is well-documented. However the relative impact of baryons and dark matter in shaping this d…

astro-ph.GA2017★ 82 cited

Escape of ionizing radiation from high redshift dwarf galaxies: role of AGN feedback

Maxime Trebitsch, Marta Volonteri, Yohan Dubois +1

While low mass, star forming galaxies are often considered as the primary driver of reionization, their actual contribution to the cosmic ultraviolet background is still uncertain,…

astro-ph.GA2017★ 89 cited

AGN Feedback Compared: Jets versus Radiation

S. Cielo, R. Bieri, M. Volonteri +2

Feedback by Active Galactic Nuclei is often divided into quasar and radio mode, powered by radiation or radio jets, respectively. Both are fundamental in galaxy evolution, especial…

astro-ph.GA2017★ 14 cited

Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation

G. Martin, S. Kaviraj, J. E. G. Devriendt +3

As endpoints of the hierarchical mass-assembly process, the stellar populations of local early-type galaxies encode the assembly history of galaxies over cosmic time. We use Horizo…

astro-ph.GA2017★ 33 cited

Group quenching and galactic conformity at low redshift

M. Treyer, K. Kraljic, S. Arnouts +13

We quantify the quenching impact of the group environment using the spectroscopic survey Galaxy and Mass Assembly (GAMA) to z=0.2. The fraction of red (quiescent) galaxies, whether…

astro-ph.GA2017★ 55 cited

Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies

Akos Bogdan, Lorenzo Lovisari, Marta Volonteri +1

Supermassive black holes (BHs) residing in the brightest cluster galaxies are over-massive relative to the stellar bulge mass or central stellar velocity dispersion of their host g…