Marla Geha

Professor

Yale University

United States

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About

Marla Geha is a Professor at Yale University in the United States. Her research focuses on stellar mass calibrations, star formation history of dwarf galaxies, and the characteristics of galaxies hosting active galactic nuclei. Recent works include studies on low-mass Milky Way satellite galaxies and multiwavelength constraints on black hole occupation fractions.

Articles (24)

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2025

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2021

Collaborators (20)

Ariyeh Maller

Professor

New York City College of Technology

UNITED STATES

Marla Geha

Research Interests

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About

Articles (24)

Stellar Mass Calibrations for Local Low-mass Galaxies

The JWST Resolved Stellar Populations Early Release Science Program. VIII. The Spatially Resolved Star Formation History of WLM

The Morphology of Dwarf Galaxies Hosting Variable Active Galactic Nuclei

A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Ultra-faint Dwarf Galaxy with DELVE Early Data Release 3

Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy

Multiwavelength Constraints on the Local Black Hole Occupation Fraction

Signatures of Tidal Disruption of the Hercules Ultrafaint Dwarf Galaxy*

The Discovery of the Faintest Known Milky Way Satellite Using UNIONS

SAGAbg. I. A Near-unity Mass-loading Factor in Low-mass Galaxies via Their Low-redshift Evolution in Stellar Mass, Oxygen Abundance, and Star Formation Rate

SAGAbg. II. The Low-mass Star-forming Sequence Evolves Significantly between 0.05 < z < 0.21

The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way–mass Galaxies

The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way–mass Galaxies

The SAGA Survey. V. Modeling Satellite Systems around Milky Way–Mass Galaxies with Updated UniverseMachine

The JWST Resolved Stellar Populations Early Release Science Program. II. Survey Overview

Target Selection and Sample Characterization for the DESI LOW-Z Secondary Target Program

X-Ray Properties of Optically Variable Low-mass AGN Candidates

Forecasts on the Dark Matter Density Profiles of Dwarf Spheroidal Galaxies with Current and Future Kinematic Observations

A Comparison between the Morphologies and Structures of Dwarf Galaxies with and without Active Massive Black Holes

A Standardized Framework for Collecting Graduate Student Input in Faculty Searches

The JWST Resolved Stellar Populations Early Release Science Program. I. NIRCam Flux Calibration

Extending the SAGA Survey (xSAGA). I. Satellite Radial Profiles as a Function of Host-galaxy Properties

Illuminating the darkest galaxies

IQ Collaboratory. II. The Quiescent Fraction of Isolated, Low-mass Galaxies across Simulations and Observations

The Diverse Morphologies and Structures of Dwarf Galaxies Hosting Optically Selected Active Massive Black Holes

Collaborators (20)

Ariyeh Maller

John Moustakas

Nora Shipp

Evan Skillman

Yao-Yuan Mao

Anirudh Chiti

Kartheik Iyer

Julio Navarro

Tom Abel

Alessandro Savino

Risa Wechsler

Daniel Weisz

Peter Behroozi

Mithi Alexa de los Reyes

Simon Smith

Joshua Peek

Anna Frebel

Lina Necib

Konstantin Gerbig

Louis Strigari

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