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Secondary halo bias through cosmic time I: Scaling relations and the connection with the cosmic web
Andrés Balaguera-Antolínez, Antonio D. Montero-Dorta, Ginevra Favole
We measure the signal of secondary halo bias as a function of a variety of intrinsic and environmental halo properties, and characterize its statistical significance as a function…
The dependence of assembly bias on the cosmic web
Antonio D. Montero-Dorta, Facundo Rodriguez
For low-mass haloes, the physical origins of halo assembly bias have been linked to the slowdown of accretion due to tidal forces, which are expected to be more dominant in some co…
Characterizing the ELG luminosity functions in the nearby Universe
G. Favole, V. Gonzalez-Perez, Y. Ascasibar +12
Nebular emission lines are powerful diagnostics for the physical processes at play in galaxy formation and evolution. Moreover, emission-line galaxies (ELGs) are one of the main ta…
High-fidelity reproduction of central galaxy joint distributions with Neural Networks
Natália V. N. Rodrigues, Natalí S. M. de Santi, Antonio D. Montero-Dorta +1
The relationship between galaxies and haloes is central to the description of galaxy formation, and a fundamental step towards extracting precise cosmological information from gala…