543 citations
- ARC Centre of Excellence for All-sky AstrophysicsAU518 papers
- Australian National UniversityAU211 papers
- International Centre for Radio Astronomy ResearchAU204 papers
- The University of Western AustraliaAU162 papers
- Swinburne University of TechnologyAU120 papers
- The University of SydneyAU106 papers
- Macquarie UniversityAU85 papers
- UNSW SydneyAU81 papers
- Centre National de la Recherche ScientifiqueFR78 papers
- Monash UniversityAU72 papers
- Max Planck Institute for AstronomyDE71 papers
- Space Telescope Science InstituteUS70 papers
48 papers · 2 filters
Supermassive black holes in a mass-limited galaxy sample
Zachary Byrne, Michael J. Drinkwater, Holger Baumgardt +8
The observed scaling relations between supermassive black hole masses and their host galaxy properties indicate that supermassive black holes influence the evolution of galaxies. H…
The Tully-Fisher relation from SDSS-MaNGA: Physical causes of scatter and variation at different radii
Andrei Ristea, Luca Cortese, Amelia Fraser-McKelvie +4
The stellar mass Tully-Fisher relation (STFR) and its scatter encode valuable information about the processes shaping galaxy evolution across cosmic time. However, we are still mis…
Lyman-alpha at Cosmic Noon I: Ly-alpha Spectral Type Selection of z ~ 2-3 Lyman Break Galaxies with Broadband Imaging
Garry Foran, Jeff Cooke, Naveen Reddy +2
High-redshift Lyman break galaxies (LBGs) are efficiently selected in deep images using as few as three broadband filters, and have been shown to have multiple intrinsic and small-…
Compact to extended Lyman- emitters in MAGPI: strong blue peak emission at
T. Mukherjee, T. Zafar, T. Nanayakkara +10
We report the discovery of three double-peaked Lyman- emitters (LAEs) exhibiting strong blue peak emission at 2.9 4.8, in the VLT/MUSE data obtained as par…
MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe
Anshu Gupta, Ravi Jaiswar, Vicente Rodriguez-Gomez +7
Extreme emission line galaxies (EELGs), where nebular emissions contribute 30-40% of the flux in certain photometric bands, are ubiquitous in the early universe (z>6). We utilise d…
A new method for spatially resolving the turbulence driving mixture in the ISM with application to the Small Magellanic Cloud
Isabella A. Gerrard, Christoph Federrath, Nickolas M. Pingel +12
Turbulence plays a crucial role in shaping the structure of the interstellar medium. The ratio of the three-dimensional density contrast () to the turbulent sonic Mach n…