AJ
Alexander P Ji
University of Chicago, Observatories of the Carnegie Institution of Washington, Massachusetts Institute of Technology, Stanford University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
0000-0002-4863-8842
Employment
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University of Chicago Assistant Professor2021 - Present
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Observatories of the Carnegie Institution of Washington2017 - 2021
Education
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Massachusetts Institute of Technology PhD Physics2012 - 2017
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Stanford University MS Statistics2011 - 2012
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Stanford University BS Physics2007 - 2011
Projects & Funding
Projects & funding information is unavailable.
Publications (142)
- Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits Save
- Scylla at APOGEE: The Impact of Starbursts on the Chemical Evolution of the Magellanic Clouds Save
- Relics of the first stars spotted in a distant, ultra-faint galaxy Save
- Not-so-heavy Metal(s): Chemical Abundances in the Ultrafaint Dwarf Galaxies Eridanus IV and Centaurus I Save
- Aeos Is Mixing It Up: The (In)homogeneity of Metal Mixing Following Population III Star Formation Save
- Sifting for a Stream: The Morphology of the 300 S Stellar Stream Save
- A nearly pristine star from the Large Magellanic Cloud Save
- Discovery of the First Five Carbon-enhanced Metal-poor Stars in the LMC Save
- Evaluating Classifications of Extremely Metal-poor Candidates Selected from Gaia XP Spectra Save
- Mapping the Distant and Metal-poor Milky Way with SDSS-V Save
- Epicyclic density variations in the Indus stellar stream Save
- Enrichment by the first stars in a relic dwarf galaxy Save
- No Observational Evidence for Dark Matter Nor a Large Metallicity Spread in the Extreme Milky Way Satellite Ursa Major III/UNIONS 1 Save
- DELVE Milky Way Satellite Galaxy Census. I. Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS Save
- EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy Save
- Ultra-faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3 Save
- Chemodynamics of Boötes I with S 5: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints Save
- Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams* Save
- A Chemodynamical Census of the Milky Way's Ultra-Faint Compact Satellites. I. A First Population-Level Look at the Internal Kinematics and Metallicities of 19 Extremely-Low-Mass Halo Stellar Systems Save
- Chemical Abundances in the Metal-Poor Globular Cluster ESO 280-SC06: A Formerly Massive, Tidally Disrupted Globular Cluster Save