Computational Astrophysics: Publications
Read the latest papers published by our research teams.
Visit CCA’s Astrophysics Data System (ADS) library.
Results
-
Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 4: Validation and Performance
-
Cosmology Likelihood for Observables in Euclid (CLOE). 1. Theoretical recipe
-
Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 5. Extensions beyond the standard modelling of theoretical probes and systematic effects
-
Resolving stellar populations, star formation, and ISM conditions with JWST in a large spiral galaxy at z \(\sim\) 2
-
Luminous Fast Blue Optical Transients as "Failed" Gravitational Wave Sources: Helium Core\(-\)Black Hole Mergers Following Delayed Dynamical Instability
-
The CEERS Photometric and Physical Parameter Catalog
-
The \(M_{\rm BH}-M_{*}\) Relationship at \(3
-
GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation
-
Euclid preparation: Towards a DR1 application of higher-order weak lensing statistics
-
The Milky Way - Large Magellanic Cloud Interaction with Simulation Based Inference
-
A Data-Driven Prism: Multi-View Source Separation with Diffusion Model Priors
-
Diffuse neutrino flux from coronal magnetospheric current sheets of accreting black holes
-
The First Radio-bright Off-nuclear Tidal Disruption Event AT 2024tvd Reveals the Fastest-evolving Double-peaked Radio Emission
-
The Landscape of Collapsar Outflows: Structure, Signatures, and Origins of Einstein Probe Relativistic Supernova Transients
-
Detecting Molecular Hydrogen (H\(_{2}\)) Emission at Cosmic Dawn
-
The HST Legacy Archival Uniform Reduction of Local Group Imaging (LAURELIN). I. Photometry and Star Formation Histories for 36 Ultra-faint Dwarf Galaxies
-
Spectral Evolution of Rotating Population III Stars
-
Betelgeuse's Buddy: X-Ray Constraints on the Nature of \(\alpha\) Ori B
-
Radio Variability in Recently Quenched Galaxies: The Impact of Tidal Disruption Event or Active Galactic Nucleus-Driven Outflows
-
Joint Analysis of H I Absorption Zeeman Measurements and the Morphology of Filamentary H I Emission
-
Stars Born in the Wind: M82's Outflow and Halo Star Formation
-
Magnetosonic Waves as a Potential Driver of Observed Temperature Fluctuation Patterns in AGN Accretion Disks
-
paired: A Statistical Framework for Detecting Stellar Binarity with Gaia RVs. I. Sensitivity to Unresolved Binaries
-
A Spectroscopic Hunt for Post–Red Supergiants in the Large Magellanic Cloud. II. Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants
-
Development of Turbulence in Postshock Regions
-
QPEs from EMRI Debris Streams Impacting Accretion Disks in Galactic Nuclei
-
Inside-out versus Upside-down: The Origin and Evolution of Metallicity Radial Gradients in FIRE Simulations of Milky Way-mass Galaxies and the Essential Role of Gas Mixing
-
The Rise of the Galactic Empire: Ultraviolet Luminosity Functions at z \(\sim\) 17 and z \(\sim\) 25 Estimated with the MIDIS+NGDEEP Ultra-deep JWST/NIRCam Data Set
-
Magnetic Fields in the Eos Cloud: Dynamically Important Fields in the Interface between Atomic and Molecular Gas
-
SN 2019tsf: Evidence for Extended Hydrogen-poor CSM in the Three-peaked Light Curve of Stripped Envelope of a Type Ib Supernova
-
Requirements for Joint Orbital Characterization of Cold Giants and Habitable Worlds with Habitable Worlds Observatory
-
Fast X-ray Transient Detection with AXIS: Application to Magnetar Giant Flares
-
Extended-path intensity correlation: Microarcsecond astrometry with an arcsecond field of view
-
Tests of general relativity with GWTC-3
-
Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies
-
Astrometry with extended-path intensity correlation
-
Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z > 10
-
Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
-
Testing the local supervoid solution to the Hubble tension with direct distance tracers
-
Mergers all the way down: stellar collisions and kinematics of a dense hierarchically forming massive star cluster in a dwarf starburst
-
Emulating dark matter halo merger trees with graph generative models
-
MISTRAL: a model for AGN winds from radiatively efficient accretion in cosmological simulations
-
Prevention is better than cure? Feedback from high specific energy winds in cosmological simulations with ARKENSTONE
-
How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations: magnetic field effects
-
Dynamics of tidal spiral arms: Machine learning-assisted identification of equations and application to the Milky Way
-
Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
-
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations: III. The physics behind the emergence of the golden mass scale
-
Euclid preparation: LXXV. Estimating galaxy physical properties using CatBoost chained regressors with attention