Desika Narayanan

Assistant Professor

University of Florida

United States

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About

Desika Narayanan is an Assistant Professor at the University of Florida, specializing in the fields of galaxy formation and star formation processes. His recent research includes studies on molecular gas dynamics in post-starburst galaxies, the resolved CO emission of star-forming galaxies at redshifts of 1 to 3, and the impact of star formation and dust on early universe galaxies. Professor Narayanan's work contributes to advancing our understanding of cosmic evolution and galactic properties in the context of both current observations and simulations.

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Collaborators (16)

David J Rosario

Newcastle University

UNITED KINGDOM

Desika Narayanan

Research Interests

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About

Articles (22)

The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission

Quenching through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ∼ 0.7 Post-starburst Galaxies

Predicting the resolved CO emission of z = 1−3 star-forming galaxies

SQuIGG L → E: Observational Evidence of Low Ongoing Star Formation Rates in Gas-rich Post-starburst Galaxies

Theoretical Strong-line Metallicity Diagnostics for the JWST Era

Cosmic Sands. II. Challenges in Predicting and Measuring High-z Dust Temperatures

[C ii] 158 μm emission as an indicator of galaxy star formation rate

Outshining by Recent Star Formation Prevents the Accurate Measurement of High-z Galaxy Stellar Masses

simba-EoR: early galaxy formation in the simba simulation including a new sub-grid interstellar medium model

Tracing the History of Obscured Star Formation with the SIMBA Cosmological Galaxy Evolution Simulation

slick: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations

A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations

The State of the Molecular Gas in Post-starburst Galaxies

Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization

Merger Signatures are Common, but not Universal, in Massive, Recently Quenched Galaxies at z ∼ 0.7

The connection between mergers and AGN activity in simulated and observed massive galaxies

Investigating the [C ii]-to-H i Conversion Factor and the H i Gas Budget of Galaxies at z ≈ 6 with Hydrodynamic Simulations

Star Formation Suppression by Tidal Removal of Cold Molecular Gas from an Intermediate-redshift Massive Post-starburst Galaxy

An orientation bias in observations of submillimetre galaxies

Inferring Halo Masses with Graph Neural Networks

Recovering the Star Formation Histories of Recently Quenched Galaxies: The Impact of Model and Prior Choices

How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-dust Geometry Model in Spectral Energy Distribution Fitting

Collaborators (16)

David J Rosario

Brandon S Hensley

Alice Shapley

Maximilien FRANCO

Fergus Cullen

John-David Smith

K. Decker French

Romeel Davé

Mark Vogelsberger

Daniel Stark

Britton Smith

Federico Marinacci

Laura V. Sales

Katherine Suess

Paul Torrey

Robert Feldmann

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