Samir Salim

assistant professor

Indiana State University

United States

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About

Samir Salim is an assistant professor at Indiana University in the United States. His research focuses on galaxy evolution, including studies on galactic dust buildup and spectral energy distribution fitting parameters. He has contributed to significant publications exploring various aspects of galaxy surveys, star formation rates, and the properties of active galactic nuclei.

Articles (16)

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2025

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2025

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2024

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2024

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2024

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2023

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2023

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2023

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2023

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2023

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2022

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2022

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2021

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2021

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2021

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2020

Collaborators (7)

Brian Siana

University of California Riverside

UNITED STATES

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Andreas Zezas

Associate Professor

University of Crete

GREECE

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Jiri Svoboda

Astronomical Institute of the Czech Academy of Sciences

CZECH REPUBLIC

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Ivana Damjanov

Associate Professor / Canada Research Chair

Saint Mary's University

CANADA

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Sandra Faber

Professor

University of California, Santa Cruz

UNITED STATES

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David Koo

Astronomer/Professor

UNITED STATES

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Janice Lee

Chief Scientist

UNITED STATES

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Samir Salim

Research Interests

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About

Articles (16)

A dusty dawn: galactic dust buildup at z ≳ 5

FORECASTOR – II. Simulating galaxy surveys with the Cosmological Advanced Survey Telescope for Optical and UV Research

Assessment of SDSS-derived Galaxy Morphologies Using HST Imaging

The Near-infrared Extinction Law at High and Low Galactic Latitudes

Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ∼ 1 and z ∼ 2 in the Absence of Infrared Data

Improved GALEX UV Photometry for 700,000 SDSS Galaxies

Star formation rate and stellar mass calibrations based on infrared photometry and their dependence on stellar population age and extinction

A New Physical Picture for Active Galactic Nuclei Lacking Optical Emission Lines

SIT 45: An interacting, compact, and star-forming isolated galaxy triplet

ΣSFR–M ∗ Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR–M ∗ Diagrams

Systematics in the Spectral Energy Distribution Fitting Parameter Estimation of Composite Galaxies

The MOSFIRE Deep Evolution Field Survey: Implications of the Lack of Evolution in the Dust Attenuation–Mass Relation to z ∼ 2*

Physical Drivers of Emission-line Diversity of SDSS Seyfert 2s and LINERs after Removal of Contributions from Star Formation

New-generation dust emission templates for star-forming galaxies

UV Extinction as a More Fundamental Measure of Dust than E(B − V) or A V

CANDELS Meets GSWLC: Evolution of the Relationship between Morphology and Star Formation Since z = 2

Collaborators (7)

Brian Siana

Andreas Zezas

Jiri Svoboda

Ivana Damjanov

Sandra Faber

David Koo

Janice Lee

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