AD
Alis Deason
Durham University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astrophysical Phenomena and Observations
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Publications (103)
- Slow stellar halo rotation as a signature of disc flips and GES-like mergers Save
- Stirring things up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue Save
- The Milky Way Stellar Halo Is Twisted and Doubly Broken: Insights from DESI DR2 Milky Way Survey Observation Save
- Stellar streams around dwarf galaxies in the local Universe Save
- A galactic tug-of-war: how (not) to simultaneously fit the Milky Way satellite luminosity function and the mass–metallicity relation Save
- From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor Save
- Auriga Streams III: the mass–metallicity relation does not rule out tidal mass-loss in Local Group satellites Save
- The accreted stellar haloes of Milky Way-mass galaxies as a probe of the nature of the dark matter Save
- No certainty of a Milky Way–Andromeda collision Save
- Galactic Archaeology with Gaia Save
- Detection of Accretion Shelves Out to the Virial Radius of a Low-mass Galaxy with JWST Save
- The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation Save
- The proto-galaxy of Milky Way-mass haloes in the FIRE simulations Save
- Can we really pick and choose? Benchmarking various selections of Gaia Enceladus/Sausage stars in observations with simulations Save
- The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies Save
- HALO7D. III. Chemical Abundances of Milky Way Halo Stars from Medium-resolution Spectra Save
- The 3D kinematics of stellar substructures in the periphery of the Large Magellanic Cloud Save
- The progenitor galaxies of stellar haloes as ‘failed’ Milky Ways Save
- Overview of the DESI Milky Way Survey Save
- Constraining the shape of dark matter haloes with globular clusters and diffuse stellar light in the E-MOSAICS simulations Save