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Research
Cosmology and Fundamental Physics
Galaxies and Active Galactic Nuclei
Instrumentation, Surveys and Projects
Milky Way and Local Group Stars
Star Formation and Exoplanets
Stars and Stellar Evolution
X-ray Astrophysics
Recent IoA Publications
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Recent IoA Publications
J0332-3557: A comprehensive metallicity analysis of a z~3.8 gravitationally lensed galaxy
Cataclysmic Variables from Sloan Digital Sky Survey V -- the search for period bouncers continues
A non-linear solution to the $S_8$ tension II: Analysis of DES Year 3 cosmic shear
The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
Optimizing the Evolution of Perturbations in the $\Lambda$CDM Universe
Mini-Quenching of High-Redshift Galaxies by Bursty Star Formation
NGTS clusters survey $-$ V: Rotation in the Orion Star-forming Complex
Formation of Gaps in Self-gravitating Debris Disks by Secular Resonance in a Single-planet System. II. Towards a Self-consistent Model
The Gaia-ESO Survey: Empirical estimates of stellar ages from lithium equivalent widths (EAGLES)
Photometric metallicity for 694233 Galactic giant stars from Gaia DR3 synthetic Stromgren photometry. Metallicity distribution functions of halo sub-structures
NGTS clusters survey IV. Search for Dipper stars in the Orion Nebular Cluster
The Gaia-ESO Survey: homogenisation of stellar parameters and elemental abundances
The effect of the LMC on the Milky Way system
Current and Future constraints on Very-Light Axion-Like Particles from X-ray observations of cluster-hosted Active Galaxies
Signatures of Cosmic Ray Heating in 21-cm Observables
The Kinematics, Metallicities, and Orbits of Six Recently Discovered Galactic Star Clusters with Magellan/M2FS Spectroscopy
A catalogue of cataclysmic variables from 20 years of the Sloan Digital Sky Survey with new classifications, periods, trends and oddities
Vertical wind structure in an X-ray binary revealed by a precessing accretion disk
Measuring the photo-ionization rate, neutral fraction and mean free path of HI ionizing photons at $4.9 \leq z \leq 6.0$ from a large sample of XShooter and ESI spectra
An optimal envelope ejection efficiency for merging neutron stars