JS
Jason Sanders
University College London, University of Cambridge, University of Oxford
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena · Astrophysical Phenomena and Observations
0000-0003-4593-6788
Employment
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University College London Associate Professor in Near Universe Astrophysics2020 - Present
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University of Cambridge Postdoctoral Research Associate2014 - 2020
Education
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University of Oxford Doctor of Philosophy (DPhil)2011 - 2014
- 2007 - 2011
Projects & Funding
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Astronomy Observation and Theory Consolidated Grant 2016-2019 Science and Technology Facilities Council2016 - 2019
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Astronomy Observation and Theory Consolidated Grant 2012 Science and Technology Facilities Council2013 - 2017
Publications (106)
- Kinematic hints of a nuclear bar in the Milky Way Save
- Orbital migration and heating history of the Galactic disc: a transition between the bimodal discs Save
- The Milky Way–Large Magellanic Cloud interaction with simulation-based inference Save
- Enhanced rates of stellar radial migration in gas-rich discs at high redshift Save
- GSE versus LMC: reshaping of radially biased stellar haloes by satellites Save
- Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars Save
- Kinematic diagnostics for non-axisymmetry in the Milky Way’s nuclear stellar disc Save
- Correction to: Towards Galactic archaeology with inferred ages of giant stars from Gaia spectra Save
- Geometry of the Milky Way’s dark matter from dynamical models of the tilted stellar halo Save
- Towards Galactic archaeology with inferred ages of giant stars from Gaia spectra Save
- A simulation-based inference approach to the dynamics of the MW–LMC system - validation Save
- Chemical separation of stellar populations: analytic solutions for chemical evolution models with metallicity-dependent yields Save
- Thick-to-thin disc transition and gas disc shrinking induced by the Gaia-Sausage-Enceladus merger Save
- Carbon-enhanced dwarf stars are predominantly a halo population Save
- Bar-driven dispersal of Galactic substructure Save
- ChemZz I: comparing oxygen and iron abundance patterns in the Milky Way, the Local Group, and Cosmic Noon Save
- Dynamical streams in the local stellar halo Save
- Denoising Milky Way stellar survey data with normalizing flow models Save
- Observational Constraints of Radial Migration in the Galactic Disk Driven by the Slowing Bar Save
- Variable stars in the VVV globular clusters Save