510 citations · 3.9k across the 72 of their papers we have counts for
72 papers
The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
Daniel J. Cornwell, Alfonso Aragón-Salamanca, Ulrike Kuchner +3
Upcoming wide-field spectroscopic surveys will observe galaxies in a range of cosmic web environments in and around galaxy clusters. In this paper, we test and quantify how success…
Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
Ana Contreras-Santos, Alexander Knebe, Weiguang Cui +5
Using the data set of The Three Hundred project, i.e. 324 hydrodynamical resimulations of cluster-sized haloes and the regions of radius 15 Mpc around them, we study galaxy…
Supervised machine learning on Galactic filaments Revealing the filamentary structure of the Galactic interstellar medium
A. Zavagno, F. -X. Dupé, S. Bensaid +11
Context. Filaments are ubiquitous in the Galaxy, and they host star formation. Detecting them in a reliable way is therefore key towards our understanding of the star formation pro…
The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
Tomás Hough, Sofía A. Cora, Roan Haggar +6
In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the relaxed simulated galaxy clusters from The Three Hundred project, and we study…
The Three Hundred project: Galaxy groups do not survive cluster infall
Roan Haggar, Ulrike Kuchner, Meghan E. Gray +4
Galaxy clusters grow by accreting galaxies as individual objects, or as members of a galaxy group. These groups can strongly impact galaxy evolution, stripping the gas from galaxie…
Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
Daniel J. Cornwell, Ulrike Kuchner, Alfonso Aragón-Salamanca +7
Next-generation wide-field spectroscopic surveys will observe the infall regions around large numbers of galaxy clusters with high sampling rates for the first time. Here we assess…