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Measuring the stellar and planetary parameters of the 51 Eridani system
DOI: 10.1017/pasa.2024.40 Bibcode: 2024PASA...41...43E

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…

2024 Publications of the Astronomical Society of Australia
eHST 3
Galaxy spin direction asymmetry in JWST deep fields
DOI: 10.1017/pasa.2024.20 Bibcode: 2024PASA...41...38S

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…

2024 Publications of the Astronomical Society of Australia
eHST JWST 3
New radio continuum study of the large magellanic cloud supernova remnant N49
DOI: 10.1017/pasa.2024.73 Bibcode: 2024PASA...41...89G

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…

2024 Publications of the Astronomical Society of Australia
eHST 1
A jet-induced shock in a young, powerful radio galaxy at z = 3.00
DOI: 10.1017/pasa.2024.101 Bibcode: 2024PASA...41..114S

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…

2024 Publications of the Astronomical Society of Australia
Gaia eHST 0
MOSEL survey: Unwrapping the Epoch of Reionisation through mimic galaxies at Cosmic Noon
DOI: 10.1017/pasa.2024.37 Bibcode: 2024PASA...41...40J

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 …

2024 Publications of the Astronomical Society of Australia
eHST JWST 0
HST WFC3/Grism observations of the candidate ultra-high-redshift radio galaxy GLEAM J0917-0012
DOI: 10.1017/pasa.2022.4 Bibcode: 2022PASA...39...16S

Seymour, N.; Drouart, G.; Vernet, J. D. R. +11 more

We present Hubble Space Telescope Wide Field Camera 3 photometric and grism observations of the candidate ultra-high-redshift ( $z>7$ ) radio galaxy, GLEAM J0917-0012. This radio source was selected due to the curvature in its 70-230 MHz, low-frequency Murchison Widefield Array radio spectrum and its faintness in K-band. Follow-up spectroscopic…

2022 Publications of the Astronomical Society of Australia
Gaia eHST 4
Large-scale asymmetry in galaxy spin directions: evidence from the Southern hemisphere
DOI: 10.1017/pasa.2021.27 Bibcode: 2021PASA...38...37S

Shamir, Lior

Recent observations using several different telescopes and sky surveys showed patterns of asymmetry in the distribution of galaxies by their spin directions as observed from Earth. These studies were done with data imaged from the Northern hemisphere, showing excellent agreement between different telescopes and different analysis methods. Here, da…

2021 Publications of the Astronomical Society of Australia
eHST 19
Absolute V-band magnitudes and mass-to-light ratios of Galactic globular clusters
DOI: 10.1017/pasa.2020.38 Bibcode: 2020PASA...37...46B

Hilker, M.; Baumgardt, H.; Sollima, A.

We have used Hubble Space Telescope and ground-based photometry to determine total V-band magnitudes and mass-to-light ratios of more than 150 Galactic globular clusters. We do this by summing up the magnitudes of their individual member stars, using colour-magnitude information, Gaia DR2 proper motions, and radial velocities to distinguish cluste…

2020 Publications of the Astronomical Society of Australia
Gaia eHST 54
Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry
DOI: 10.1017/pasa.2020.46 Bibcode: 2020PASA...37...53S

Shamir, Lior

Several recent observations using large data sets of galaxies showed non-random distribution of the spin directions of spiral galaxies, even when the galaxies are too far from each other to have gravitational interaction. Here, a data set of$\sim8.7\cdot10^3$spiral galaxies imaged byHubble Space Telescope(HST) is used to test and profile a possibl…

2020 Publications of the Astronomical Society of Australia
eHST 18
ASKAP reveals giant radio halos in two merging SPT galaxy clusters
DOI: 10.1017/pasa.2020.34 Bibcode: 2020PASA...37...40W

Johnston-Hollitt, Melanie; Akamatsu, Hiroki; Hodgson, Torrance +4 more

Early science observations from the Australian Square Kilometre Array Pathfinder (ASKAP) have revealed clear signals of diffuse radio emission associated with two clusters detected by the South Pole Telescope via their Sunyaev Zel'dovich signal: SPT CLJ0553-3342 (MACS J0553.4-3342) and SPT CLJ0638-5358 (Abell S0592) are both high-mass lensing clus…

2020 Publications of the Astronomical Society of Australia
eHST 14