Vivienne Wild

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University of St. Andrews

United Kingdom

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Recent Grants

Grant: Close

Astronomy at St Andrews 2015-2018

Open Date: 2015-03-31

Close Date: 2019-03-31

Grant: Close

The origins of galaxy bimodality: Linking mergers, starbursts and feedback in observations and simulations

Open Date: 2012-09-01

Close Date: 2018-01-31

Grant: Close

The growth of galaxies

Open Date: 2012-01-01

Close Date: 2014-12-31

Articles (24)

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2020

Collaborators (15)

Michail Papathomas

University of St. Andrews

UNITED KINGDOM

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Paul Hewett

Professor of Observational Cosmology and Astrophysics

University of Cambridge

UNITED KINGDOM

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Jean-Charles Cuillandre

Université Paris-Saclay

FRANCE

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Scott Wilkinson

University of Victoria

CANADA

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Francisco Rodríguez Montero

University of Oxford

UNITED KINGDOM

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Michele Ginolfi

Research Assistant Professor

Università degli Studi di Napoli Federico II

ITALY

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K. Decker French

Assistant Professor

University of Illinois at Urbana-Champaign

UNITED STATES

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Omar Almaini

Professor of Astrophysics

University of Nottingham

UNITED KINGDOM

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Michael Merrifield

Professor of Astronomy

University of Nottingham

UNITED KINGDOM

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Peter Johansson

University of Helsinki

FINLAND

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Freeke van de Voort

Royal Society University Research Fellow & lecturer (proleptic)

Cardiff University

UNITED KINGDOM

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Gail Zasowski

Associate Professor

University of Utah

UNITED STATES

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Antje Kohnle

University of St. Andrews

UNITED KINGDOM

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Kate Rowlands

Johns Hopkins University

UNITED STATES

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Ken Mavor

University of St. Andrews

UNITED KINGDOM

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Vivienne Wild

Research Interests

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Recent Grants

Articles (24)

No evidence for excess AGN activity in recently quenched massive galaxies at cosmic noon

Stellar populations of quasar host galaxies with MFICA decomposition

Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs

The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA

The competing effects of recent and long-term star formation histories on oxygen, nitrogen, and stellar metallicities

An Intervention Addressing Impostor Phenomenon in Undergraduate Physics and Astronomy

The infrared luminosity of retired and post-starburst galaxies

A tight N/O–potential relation in star-forming galaxies

Correction to: Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation

Chemical evolution of local post-starburst galaxies: implications for the mass–metallicity relation

High-velocity outflows persist up to 1 Gyr after a starburst in recently quenched galaxies at z &gt; 1

The JWST EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 &lt; z &lt; 5

Galaxy evolution in the post-merger regime. II - post-merger quenching peaks within 500 Myr of coalescence

The role of mass and environment in the build-up of the quenched galaxy population since cosmic noon

A massive quiescent galaxy at redshift 4.658

Gas metallicity distributions in SDSS-IV MaNGA galaxies: what drives gradients and local trends?

SDSS-IV MaNGA: how do star formation histories affect gas-phase abundances?

Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past

Galaxy mergers can rapidly shut down star formation

The merger fraction of post-starburst galaxies in UNIONS

Rapidly quenched galaxies in the Simba cosmological simulation and observations

From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time

Introducing a Real-time Interactive GUI Tool for Visualization of Galaxy Spectra

Comparison of stellar populations in simulated and real post-starburst galaxies in MaNGA

Collaborators (15)

Michail Papathomas

Paul Hewett

Jean-Charles Cuillandre

Scott Wilkinson

Francisco Rodríguez Montero

Michele Ginolfi

K. Decker French

Omar Almaini

Michael Merrifield

Peter Johansson

Freeke van de Voort

Gail Zasowski

Antje Kohnle

Kate Rowlands

Ken Mavor

Make your next move.

High-velocity outflows persist up to 1 Gyr after a starburst in recently quenched galaxies at z > 1

The JWST EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5