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Lorenzo Zanisi

University of Southampton

22

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218

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The size function of massive satellites from the R e -R h and M star -M h relations: constraining the role of environment

2021 Monthly Notices of the Royal Astronomical Society
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LeMMINGs. III. The e-MERLIN Legacy Survey of the Palomar sample. Exploring the origin of nuclear radio emission in active and inactive galaxies through the [O III] -- radio connection

2021 Monthly Notices of the Royal Astronomical Society
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A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations

2021 Monthly Notices of the Royal Astronomical Society
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The evolution of compact massive quiescent and starforming galaxies derived from the Re − Rh and Mstar − Mh relations

2021 Monthly Notices of the Royal Astronomical Society
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LeMMINGs. III. The e-MERLIN Legacy Survey of the Palomar sample. Exploring the origin of nuclear radio emission in active and inactive galaxies through the [O III] -- radio connection

2021 arXiv: Astrophysics of Galaxies
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Galaxy sizes and the galaxy–halo connection – I. The remarkable tightness of the size distributions

2020 Monthly Notices of the Royal Astronomical Society
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Monte Carlo simulation of uncertainty to identify barriers to optimizing blood pressure control.

2020 Journal of Hypertension
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The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view.

2020 arXiv: Astrophysics of Galaxies
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Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL steel.

2019 Monthly Notices of the Royal Astronomical Society
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Constraining black hole–galaxy scaling relations and radiative efficiency from galaxy clustering

2019 Nature Astronomy
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