BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Kugel R, Schaye J, Schaller M, et al. (2023) FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning. Monthly Notices of the Royal Astronomical Society. 526: 6103-6127
Thomas GF, Martin NF, Fattahi A, et al. (2021) Observing the Stellar Halo of Andromeda in Cosmological Simulations: The AURIGA2PANDAS Pipeline The Astrophysical Journal. 910: 92
Gonzalez-Perez V, Comparat J, Norberg P, et al. (2021) Erratum: The host dark matter haloes of [O ii]  emitters at 0.5 < z < 1.5 Monthly Notices of the Royal Astronomical Society. 503: 28-30
Gonzalez-Perez V, Cui W, Contreras S, et al. (2020) Do model emission line galaxies live in filaments at z∼1? Monthly Notices of the Royal Astronomical Society
Simpson CM, Gargiulo I, Gómez FA, et al. (2019) Simulating cosmological substructure in the solar neighbourhood. Monthly Notices of the Royal Astronomical Society. 490
Baugh CM, Gonzalez-Perez V, Lagos CdP, et al. (2019) Galaxy formation in the Planck Millennium : the atomic hydrogen content of dark matter haloes. Monthly Notices of the Royal Astronomical Society. 483: 4922-4937
Grand RJJ, Helly J, Fattahi A, et al. (2018) Aurigaia : mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations. Monthly Notices of the Royal Astronomical Society. 481: 1726-1743
Knebe A, Pearce FR, Gonzalez-Perez V, et al. (2018) Cosmic CARNage I: on the calibration of galaxy formation models Monthly Notices of the Royal Astronomical Society. 475: 2936-2954
Gonzalez-Perez V, Comparat J, Norberg P, et al. (2018) The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5 Monthly Notices of the Royal Astronomical Society. 474: 4024-4038
Han J, Cole S, Frenk CS, et al. (2018) HBT+: an improved code for finding subhaloes and building merger trees in cosmological simulations. Monthly Notices of the Royal Astronomical Society. 474: 604-617
See more...