Search Publications
Measuring the stellar and planetary parameters of the 51 Eridani system
Mann, Andrew W.; von Braun, Kaspar; Schaefer, Gail +3 more
In order to study exoplanets, a comprehensive characterisation of the fundamental properties of the host stars – such as angular diameter, temperature, luminosity, and age, is essential, as the formation and evolution of exoplanets are directly influenced by the host stars at various points in time. In this paper, we present interferometric observ…
Galaxy spin direction asymmetry in JWST deep fields
Shamir, Lior
The unprecedented imaging power of James Webb Space Telescope (JWST) provides new abilities to observe the shapes of objects in the early Universe in a way that has not been possible before. Recently, JWST acquired a deep field image inside the same field imaged in the past as the Hubble Space Telescope (HST) Ultra Deep Field. Computer-based quant…
New radio continuum study of the large magellanic cloud supernova remnant N49
Sasaki, Manami; Haberl, Frank; Kavanagh, Patrick +12 more
We present new Australia Telescope Compact Array (ATCA) radio observations towards N 49, one of the brightest extragalactic supernova remnants (SNRs) located in the Large Magellanic Cloud (LMC). Our new and archival ATCA radio observations were analysed along with Chandra X-ray data. These observations show a prominent 'bullet' shaped feature beyo…
A jet-induced shock in a young, powerful radio galaxy at z = 3.00
Noirot, Gaël; Gupta, Anshu; Emonts, Bjorn +9 more
The bright radio source, GLEAM J091734 - 001243 (hereafter GLEAM J0917 - 0012), was previously selected as a candidate ultra-high redshift ( z > 5 ) radio galaxy due to its compact radio size and faint magnitude ( K(AB)=22.7 ). Its redshift was not conclusively determined from follow-up millimetre and near-infrared spectroscopy. Here we present…
MOSEL survey: Unwrapping the Epoch of Reionisation through mimic galaxies at Cosmic Noon
Harshan, Anishya; Gupta, Anshu; Trott, Cathryn M. +4 more
The nature of the first galaxies that reionised the universe during the Epoch of Reionisation (EoR) remains unclear. Attempts to directly determine spectral properties of these early galaxies are affected by both limited photometric constraints across the spectrum and by the opacity of the intergalactic medium to the Lyman Continuum (LyC) at high …