COLIBRE simulations find the galaxy gas-phase MZR already in place at z≈10 with little evolution until z≈5, then shallowens at low z, with high-mass turnover set by AGN feedback and low-mass end by core-collapse supernovae.
R., Mocz P., Federrath C., Klessen R
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
The thin-screen approximation for pulsar scintillation arcs has key limitations; 3D volume propagation produces variable curvature and features linked to branched flow from correlated weak scatterings.
citing papers explorer
-
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations
COLIBRE simulations find the galaxy gas-phase MZR already in place at z≈10 with little evolution until z≈5, then shallowens at low z, with high-mass turnover set by AGN feedback and low-mass end by core-collapse supernovae.
-
Pulsar scintillation arcs formed from branched flow
The thin-screen approximation for pulsar scintillation arcs has key limitations; 3D volume propagation produces variable curvature and features linked to branched flow from correlated weak scatterings.