Michelle Cluver

Associate Professor

Swinburne University of Technology

Australia

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About

Michelle Cluver is an Associate Professor at Swinburne University of Technology in Australia. Her research focuses on various aspects of astrophysics, including star formation in the nearby universe, radio continuum observations of galaxies, and the environmental influences affecting galaxy dynamics. She has contributed to significant studies such as the MeerKAT view of Hickson Compact Groups and investigations into star-forming galaxies, enriching our understanding of galactic environments and evolution.

Articles (20)

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2022

Collaborators (18)

Matthew Colless

Distinguished Professor

Australian National University

AUSTRALIA

Michelle Cluver

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Articles (20)

WALLABY pilot survey

Real-time active learning for optimised spectroscopic follow-up: Enhancing early SN Ia classification with the Fink broker

The S4G-WISE View of Global Star Formation in the Nearby Universe

MeerKAT view of Hickson Compact Groups

MeerKAT view of Hickson Compact Groups

Low-frequency turnover star-forming galaxies I: Radio continuum observations and global properties

The central spectra of massive star-forming galaxies

Galaxy and Mass Assembly (GAMA): Stellar-to-dynamical Mass Relation. II. Peculiar Velocities

A comprehensive investigation of environmental influences on galaxies in group environments

Galaxy and Mass Assembly (GAMA)

A New Wide-field Infrared Survey Explorer Calibration of Stellar Mass

Galaxy and Mass Assembly (GAMA): Stellar-to-dynamical Mass Relation. I. Constraining the Precision of Stellar Mass Estimates

Multiphase Gas Interactions on Subarcsec Scales in the Shocked Intergalactic Medium of Stephan’s Quintet with JWST and ALMA

Measurement of the evolving galaxy luminosity and mass function using clustering-based redshift inference

Specific star formation rates in the Mbh-M*,sph diagram and the evolutionary pathways of galaxies across the sSFR-M* diagram

Dark matter halos and scaling relations of extremely massive spiral galaxies from extended H i rotation curves

Connecting MeerKAT Radio Continuum Properties to GAMA Optical Emission-line and WISE Mid-infrared Activity

The stellar populations of quiescent ultra-diffuse galaxies from optical to mid-infrared spectral energy distribution fitting

An empirical measurement of the halo mass function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data

Decoding the star forming properties of gas-rich galaxy pairs

Collaborators (18)

Matthew Colless

Aaron Romanowsky

Sabine Bellstedt

Agnieszka Pollo

Jon Loveday

William Reach

Lister Staveley-Smith

John-David Smith

Michael Brown

Dian P Triani

Nicholas Seymour

Karen Lee-Waddell

Maciej Bilicki

Michael Fall

Julien Peloton

Nobuhiro Okabe

Trystan Lambert

Jonghwan Rhee

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Specific star formation rates in the Mbh-M,sph diagram and the evolutionary pathways of galaxies across the sSFR-M diagram