Omar Almaini

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Professor of Astrophysics

University of Nottingham

United Kingdom

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About

Omar Almaini is a Professor of Astrophysics at the University of Nottingham, United Kingdom. His research focuses on the environmental quenching of low-mass galaxies, AGN activity in massive galaxies, and the evolution of star-forming systems. He has contributed significantly to our understanding of galaxy formation and evolution through recent publications involving the James Webb Space Telescope and ALMA.

Recent Grants

Grant: Close

Astrophysics at the University of Nottingham 2016-2020

Open Date: 2017-03-31

Close Date: 2020-03-30

Grant: Close

Nottingham PATT-Linked Travel Grant 2016 - 2018

Open Date: 2016-03-31

Close Date: 2018-03-30

Grant: Close

Nottingham PATT-Linked Travel Grant 2014 - 2016

Open Date: 2014-06-16

Close Date: 2016-06-15

Grant: Close

Nottingham PATT-Linked Travel Grant 2014 - 2016

Open Date: 2014-06-16

Close Date: 2016-06-15

Grant: Close

Astronomy & Astrophysics at Nottingham

Open Date: 2014-03-31

Close Date: 2017-03-30

Articles (17)

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2025

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2021

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2021

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2021

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2020

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2020

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2020

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2020

Collaborators (5)

Julie Wardlow

University of Lancaster

UNITED KINGDOM

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Robert Yates

University of Hertfordshire

UNITED KINGDOM

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Vivienne Wild

University of St. Andrews

UNITED KINGDOM

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Michael Merrifield

Professor of Astronomy

University of Nottingham

UNITED KINGDOM

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Kate Rowlands

Johns Hopkins University

UNITED STATES

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Omar Almaini

Research Interests

Explore related searches

Contact this professor

About

Recent Grants

Articles (17)

JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to z≃ 2

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

Correcting for the overabundance of low-mass quiescent galaxies in semi-analytic models

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

The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies

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

Increasing AGN sample completeness using long-term near-infrared variability

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

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

Cosmic Evolution of the H2 Mass Density and the Epoch of Molecular Gas

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies

Infrared lags in the light curves of AGNs measured using a deep survey

An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies

An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies

An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies

The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass

The star formation histories of z ∼ 1 post-starburst galaxies

Collaborators (5)

Julie Wardlow

Robert Yates

Vivienne Wild

Michael Merrifield

Kate Rowlands

Make your next move.

Omar Almaini

Research Interests

Explore related searches

Contact this professor

About

Recent Grants

Articles (17)

JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to z≃ 2

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

Correcting for the overabundance of low-mass quiescent galaxies in semi-analytic models

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

The structure of massive star-forming galaxies from JWST and ALMA: Dusty, high-redshift disc galaxies

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

Increasing AGN sample completeness using long-term near-infrared variability

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

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

Cosmic Evolution of the H2 Mass Density and the Epoch of Molecular Gas

An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies

Infrared lags in the light curves of AGNs measured using a deep survey

An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies

An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies

An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies

The clustering of X-ray AGN at 0.5 &lt; z &lt; 4.5: host galaxies dictate dark matter halo mass

The star formation histories of z ∼ 1 post-starburst galaxies

Collaborators (5)

Julie Wardlow

Robert Yates

Vivienne Wild

Michael Merrifield

Kate Rowlands

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

The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass