Anish M. Amarsi

Theoretical astrophysics
Department of Physics and Astronomy
Uppsala University
Box 516, 75120 Uppsala
Sweden
Email: anish.amarsi [at] physics.uu.se

Biography

I am a researcher at Uppsala University (since 2021; docent/habilitated since 2023). Before that, I was a postdoc here (2019 -- 2021), and before that I was a postdoc at MPIA in Germany (2016 -- 2019). Earlier, I was a PhD student at ANU in Australia supervised by Martin Asplund and Remo Collet (2013 -- 2016), and a BA/MSci student at the University of Cambridge in the UK (2009 -- 2013).

Research

The focus of my research is on improving the accuracy of models of the light that emerges from the atmospheres of stars like the Sun. By comparing these models against real observations of stars, we can infer their essential properties --- in particular, their chemical compositions. To a good approximation, the present-day chemical compositions of Sun-like stars reflect the compositions of the gas from which the stars formed at their respective times of birth. Thus, by studying stars of different ages and different orbits in this way, it we may learn about the history and evolution of our Galaxy and of the cosmos.

Keywords include:

Movies

Solar surface convection with STAGGER -- Cis Lagae, University of Warwick.
Log of gas temperature in a vertical slice of a solar model atmosphere (red line shows the Rosseland mean optical depth unity).
3D non-LTE formation of the silver 328nm line in the solar atmosphere with BALDER (Caliskan et al. 2026).

Funding

My funding comes from the Swedish Research Council (currently via an individual Project Grant, Optimised 3D non-equilibrium models for accurate abundance analyses of the Milky Way halo, VR 2025-05167; formerly via an individual Starting Grant, Accurate compositions of Sun-like stars, VR 2020-03940) and the Royal Swedish Academy of Sciences (individual Crafoord Grant, The nature of neutron-star mergers via high-accuracy stellar abundances, CR 2024-0015).

Teaching and supervision

I am currently responsible for the Master's courses Cosmology and The Physics of Galaxies; and earlier I was responsible for The Physics of Stars and the Bachelor's course Astrophysics I. I (co-)supervise(d) several PhD students: Irene Amateis (Uppsala), Sema Caliskan (Uppsala; lead supervisor), Cis Lagae (Stockholm) Jack Mallinson (Stockholm), and Xudong Gao (MPIA). I also try to supervise one or two Bachelor's or Master's projects each year; feel free to reach out if you are interested in developing astrophysical methods and codes, or in running and analysing computer simulations, or in using these models to analyse and interpret observed stellar spectra!

Publications

Listed in a PDF document

Listed on NASA ADS

Google scholar profile

ORCID profile

PhD theses

Sema Caliskan's thesis

Cis Lagae's thesis

Jack Mallinson's thesis

Xudong Gao's thesis

My thesis

Data

1D non-LTE departure coefficients (different "versions" for different elements and models)

3D non-LTE line profilesand abundance corrections for Na1 (Canocchi+ 2026)

3D non-LTE line profiles and abundance corrections for Ca2 in metal-poor stars (Lagae+ 2025)

1D non-LTE abundance corrections for Cu1 (Caliskan+ 2025)

3D non-LTE abundance corrections for Mg1 (Matsuno+ 2024)

3D non-LTE abundance corrections for Fe1 and Fe2 (Amarsi+ 2022)

3D non-LTE line profiles and abundance corrections for Li1 (Wang+ 2021)

3D non-LTE abundance corrections for C1, O1, Fe2 (Amarsi+ 2019)

1D non-LTE abundance corrections for K1 (Reggiani+ 2019)

3D non-LTE line profiles for H-alpha, H-beta, and H-gamma (Amarsi+ 2018)

1D non-LTE abundance corrections for Si1 (Amarsi & Asplund 2017)

1D/Mean-3D non-LTE abundance corrections for Fe1 and Fe2 (Amarsi+ 2016)

3D non-LTE equivalent widths and abundance corrections for O1 (Amarsi+ 2015,2016)

Other resources

Homepage of the Atomic Astrophysics group at UU

1D non-LTE abundance corrections via INSPECT

WebSME for online spectral synthesis (and 1D non-LTE abundance corrections -- work in progress)

PySME for spectral synthesis (can use pre-computed departure coefficients for 1D non-LTE analyses)

Atomic data and codes via Paul Barklem's github page

UU Astronomy/Space Physics seminars

Online talk for the IAU G5 seminar series in 2023

Online talk for the IReNA seminar series in 2024

Conference talk at STScI in 2017