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- Searching for lensed gravitational waves with unlensed templates
- The Solar System through dust maps. Encounter statistics with interstellar gas
- Kinematic structure and age of a Scorpius--Centaurus subcomponent: implications for PDS 70 planetary system
- A high-Galactic-altitude scattering screen: scintillation from Globular Cluster pulsar M53A
- Velocity-resolved Ionization Mapping of the Broad-line Region. II. Signatures of Eccentric Broad-line Regions from a Quantitative Photoionization-Based Model
- Towards breaking the degeneracy between stellar ages and unresolved multiplicity
- The impact of recombination during tidal disruption events
- The stability of radially anisotropic rotating stellar systems with a central density cusp
- When X-ray Features Fail to Identify Intrinsic Emitters: Label Noise and Luminosity Overlap in Machine Learning Classification of AGN and Star-forming Galaxies
- A comprehensive Gaia DR3 study of the open cluster NGC 6134: Bayesian distances, present-day mass function, mass segregation, and structural decomposition
- Something green beneath the surface: The dynamical nature of Fossil Structures in IllustrisTNG-100
- The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at redshift ≈6
- Disentangling the dark and stellar mass through precise lens modelling of the JWST observation of lensed quasar WFI2033–4723
- A MIGHTEE robust measurement of the star formation rate – radio correlation
- Comparing infrared and X-ray-selected active galactic nuclei host galaxy star formation rates to the galaxy main sequence
- Galaxy bias of radio AGN and star-forming galaxies from MIGHTEE and CMB lensing
- The connection between massive galaxies and their dark matter haloes from z = 0.25 to z ∼ 4 from the combined COSMOS, XMM-LSS and ECDF-S fields
- A Machine Learning Quasar Candidate Catalog with Photometric Redshifts from KiDS DR5 and AllWISE
- Fast Radio Burst Scattering Statistics through the Circumgalactic Medium Are Sensitive to Morphology and Intermittency
- VENUS: A Strongly Lensed Clumpy Galaxy at z ∼ 11–12 Behind the Galaxy Cluster MACS J0257.1-2325
- An Exploratory Analysis of New Large Gaia-informed Quasar Samples in SDSS-V
- Inferring the shapes of low-mass galaxies at z>6 from FIREboxHR. Where are the disks?
- Upper bounds on the number of images produced by point-mass lenses at different distances
- Reading Between the Lines: How Much Information Remains After Fitting a Stellar Spectrum?
- The Next Generation Virgo Cluster Survey (NGVS). XXIX. Demography of Nuclear Star Clusters