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Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7*
(2017)arXivWorking Paper -
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The MUSE Hubble Ultra Deep Field Survey X. Lyα Equivalent Widths at 2.9 < z < 6.6
(2017)arXivWorking Paper -
Evolution of Density Profiles in High-z Galaxies: Compaction and Quenching Inside-Out
(2015)arXivWorking Paper -
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A physical model for the 0 < z < 8 redshift evolution of the galaxy UV luminosity and stellar mass functions
(2012)We present a model to understand the redshift evolution of the UV luminosity and stellar mass functions of Lyman Break Galaxies. Our approach is based on the assumption that the luminosity and stellar mass of a galaxy is related to its dark matter halo assembly and gas infall rate. Specifically, galaxies experience a burst of star formation at the halo assembly time, followed by a constant star formation rate, representing a secular star ...Working Paper