Curriculum Vitae

Find a complete pdf version of my Academic CV or the summary below.

EDUCATION
2020 PhD Astrophysics MPIA Heidelberg, Germany
2017 MSc Astrophysics Lund University, Sweden
2015 BSc Physics Toulouse University, France
RESEARCH
Can the Milky Way tell how disk galaxies form and evolve?
How much dynamical memory is lost to radial migration?
Did the Milky Way disk grow from inside-out? How fast?
REFEERED PUBLICATIONS
Eilers, Hogg, Rix, Frankel et al. (2020), The Strength of the Dynamical Spiral Perturbation in the Galactic Disk ApJ
Frankel, Sanders, Ting, Rix (2020), Keeping it Cool: Much Migration, yet Little Heating in the Galactic Disk, ApJ
Maire, Desiderada, Trifonov, Molliere, D'Orazi, Frankel et al. (2020), Orbital and spectral characterization of the benchmark T-type brown dwarf HD 19467B
Frankel, Sanders, Rix, Ting, Ness (2019), The Inside-out Growth of the Galactic Disk, ApJ
Feuillet, Frankel, Lind, Frinchaboy, Garcia-Hernandez, Lane, Nitschelm, Roman-Lopez (2019), Spatial variations in the Milky Way disc metallicity-age relation, MNRAS
Frankel, Rix, Ting, Ness, Hogg (2018), Measuring Radial Orbit Migration in the Galactic Disk, The Astrophysical Journal, 865, 2, 96
TALKS
2021 EAS meeting Milky Way Analogs in TNG50: (what) can we learn from the bar?
2021 Strasbourg Observatory Fitting the Secular Evolution of the Milky Way's Disk
2021 INAF, Laura Bassi series What Sets the Structure of the MW Disk? Insight from Gaia and TNG50
2021 Heidelberg, MPIA GCTheory What Sets the Structure of Bars in TNG50’s MW Analogs?
2021 ECOGAL Meeting What Drives the Evolution of Simulated Milky Way-like Disks?
2020 ESO Seminar Inferring the Dynamical Structure of the Galactic Disk
2020 Barcelona, ICCUB Seminar Seeing the Galactic Disk Evolve
2020 Harvard, CfA seminar Seeing the Galactic Disk Evolve
2020 Heidelberg, Patzer Colloquium Keeping it Cool: Much Migration, yet Little Heating, in the MW Disk
2020 Harvard GC Group Meeting What Sets the Radial Structure of the Milky Way's Disk?
2020 EAS Meeting Measuring Radial Migration with APOGEE and Gaia
2020 Aarhus, Stars Group meeting Seeing the Milky Way Disk Evolve with Red Clump Stars
2020 Birmingham, Stars Group meeting What Sets the Radial Structure of the MW Disk?
2020 Cambridge UK, Galaxies Seminar Seeing the Milky Way Disk Evolve
2020 Cambridge UK, MW Group meeting Modelling the Disk: Dynamics, Chemistry and Supernovae
2020 Heidelberg MPIA, Seminar The Dynamical Evolution of the MW Disk is Cool
2019 Paris Observatory, GEPI Seminar Seeing the Milky Way Disk Evolve
2019 Stuttgart, AG meeting Building a Global Model for the Secular Evolution of the MW disk
2019 Lund, white board talk Evolution of Galaxy Disks: what the Milky Way can do for you
2019 Kloster Schoental, MPIA retreat How to Make a Galaxy Disk in Three Steps: Application to the Milky Way
2018 Shanghai, life and times of the MW Measuring Radial Orbit Migration in the Milky Way Disk
2018 Besancon, APOGEE-2 team meeting Obtained Diret Measure of Radial Migration with APOGEE
2018 Lund, Dynamics for All What Sets the Radial Structure of the Milky Way Disk?
2018 Heidelberg MPIA, Seminar What Sets the Radial Structure of the Milky Way Disk?
TEACHING / STUDENT SUPERVISION
2019 Teaching Assistant: Introduction to Astronomy and Astrophysics
2019 co-supervision: Audrey Destarac (BSc): Detectability of Black Hole - Main Sequence Binaries

This is it!