Samir Salim
Physics and Astronomy · Indiana University
Publications
197
Citations
7,203
Est. group size
—
Recurring co-author estimate
Active years
29
Publishing since 1998
Samir Salim studies how galaxies form and evolve, with a particular focus on interstellar dust—how it builds up, how it dims and reddens the light we observe from galaxies, and how to correct for these effects. The research combines large sky surveys, computer simulations of galaxies, and methods for reconstructing galaxy properties (such as star formation and stellar mass) from their light, and also examines how galaxy mergers trigger actively feeding supermassive black holes.
Publication activity grew markedly through the late 2010s and peaked around 2021-2024, remaining consistently high in recent years (about 10 papers per year over the last five years).
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- GalSyn I: A Forward-Modeling Framework for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG
arXiv (Cornell University) · 2026
- GalSyn I: A Forward-Modeling Framework for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG
arXiv (Cornell University) · 2026
- A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection
arXiv (Cornell University) · 2026
- Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference"
arXiv (Cornell University) · 2026
- A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection
arXiv (Cornell University) · 2026
- Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference"
arXiv (Cornell University) · 2026
- Ashes of FIRE: modelling dust grain size evolution in the Local Group with <scp>fire</scp>
Monthly Notices of the Royal Astronomical Society · 2026
- Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
Open MIND · 2026
- Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
arXiv (Cornell University) · 2026
- Galaxy evolution in the post-merger regime. III – The triggering of active galactic nuclei peaks immediately after coalescence
The Open Journal of Astrophysics · 2025
- FORECASTOR – II. Simulating galaxy surveys with the Cosmological Advanced Survey Telescope for Optical and UV Research
Monthly Notices of the Royal Astronomical Society · 2025
- The CASTOR mission
Journal of Astronomical Telescopes Instruments and Systems · 2025
- Introducing Smart Asset Criticality (SAC) and How it Differs from Conventional Asset Criticality
2025
- A dusty dawn: galactic dust buildup at <i>z</i> ≳ 5
Monthly Notices of the Royal Astronomical Society · 2025
- Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ∼ 1 and z ∼ 2 in the Absence of Infrared Data
The Astrophysical Journal · 2024
- arXiv (Cornell University)×27
- The Astrophysical Journal×13
- Monthly Notices of the Royal Astronomical Society×11
- Astronomy and Astrophysics×8
- The Astrophysical Journal Supplement Series×3
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
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