67 citations · 200 across the 5 of their papers we have counts for
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astro-ph.GA2014★ 33 cited
Atomic carbon as a powerful tracer of molecular gas in the high-redshift Universe: perspectives for ALMA
Matteo Tomassetti, Cristiano Porciani, Emilio Romano-Diaz +2
We use a high-resolution hydrodynamic simulation that tracks the non-equilibrium abundance of molecular hydrogen within a massive high-redshift galaxy to produce mock Atacama Large…
astro-ph.GA2014★ 30 cited
Simulating the H2 content of high-redshift galaxies
Matteo Tomassetti, Cristiano Porciani, Emilio Romano-Diaz +1
We introduce a sub-grid model for the non-equilibrium abundance of molecular hydrogen in cosmological simulations of galaxy formation. We improve upon previous work by accounting f…