Lamiya A. Mowla

Assistant Professor

Wellesley College

United States

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About

Dr. Lamiya A. Mowla is an Assistant Professor at Wellesley College, USA. Her research focuses on the study of galaxy formation and evolution, particularly in relation to star formation during the Epoch of Reionization. She has published extensively on topics such as the properties of dwarf star-forming galaxies and the impact of dust on galaxy morphology.

Articles (12)

Year:

2025

Year:

2024

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2024

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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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2022

Year:

2022

Collaborators (8)

Carolin Villforth

University of Bath

UNITED KINGDOM

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Patricia Schady

University of Bath

UNITED KINGDOM

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Kartheik Iyer

Columbia University

UNITED STATES

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Masayuki Akiyama

Associate Professor

Tohoku University

JAPAN

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Stijn Wuyts

University of Bath

UNITED KINGDOM

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Greg Bryan

Professor

Columbia University

UNITED STATES

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Gabriel Brammer

Københavns Universitet

DENMARK

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Johannes Zabl

CANADA

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Lamiya A. Mowla

Research Interests

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About

Articles (12)

In Search of the First Stars: An Ultra-compact and Very-low-metallicity Lyα Emitter Deep within the Epoch of Reionization

CANUCS: UV and ionizing properties of dwarf star-forming galaxies at z ~ 5–7

Katachi (形): Decoding the Imprints of Past Star Formation on Present-day Morphology in Galaxies with Interpretable CNNs*

Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry

Star Formation at the Epoch of Reionization with CANUCS: The Ages of Stellar Populations in MACS1149-JD1

Formation of a low-mass galaxy from star clusters in a 600-million-year-old Universe

Dust attenuation, dust content, and geometry of star-forming galaxies

An Extremely Compact, Low-mass Galaxy on its Way to Quiescence at z = 5.2

A First Look at Spatially Resolved Balmer Decrements at 1.0 < z < 2.4 from JWST NIRISS Slitless Spectroscopy

Color Gradients and Half-mass Radii of Galaxies Out to z = 2 in the CANDELS/3D-HST Fields: Further Evidence for Important Differences in the Evolution of Mass-weighted and Light-weighted Sizes

The Sparkler: Evolved High-redshift Globular Cluster Candidates Captured by JWST

3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey

Collaborators (8)

Carolin Villforth

Patricia Schady

Kartheik Iyer

Masayuki Akiyama

Stijn Wuyts

Greg Bryan

Gabriel Brammer

Johannes Zabl

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