Computational Astrophysics: Publications
Read the latest papers published by our research teams.
Visit CCA’s Astrophysics Data System (ADS) library.
Results
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Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?
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Revisiting the classics: on the evolutionary origin of the 'Fe II' and 'He/N' spectral classes of novae
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Inferring warm dark matter masses with deep learning
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ARKENSTONE - I. A novel method for robustly capturing high specific energy outflows in cosmological simulations
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Spatially resolved Kennicutt-Schmidt relation at z~7 and its connection with the interstellar medium properties
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Seeding the CGM: how satellites populate the cold phase of milky way haloes
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Cold Dust and Low [OIII]/[CII] Ratios: an Evolved Star-forming Population at Redshift 7
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TOI-5126: a hot super-Neptune and warm Neptune pair discovered by TESS and CHEOPS
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Dissecting the Gaia HR diagram - II. The vertical structure of the star formation history across the solar cylinder
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Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4
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The persistent shadow of the supermassive black hole of M 87. I. Observations, calibration, imaging, and analysis
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ACT-DR5 Sunyaev-Zel'dovich clusters: Weak lensing mass calibration with KiDS
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Ionized gas extends over 40 kpc in an odd radio circle host galaxy
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Fast-forward {FARGO}: Accelerating Protoplanetary Disk Simulations with Limited Data
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A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics
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Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-wave Progenitors
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Code Comparison in Galaxy-scale Simulations with Resolved Supernova Feedback: Lagrangian versus Eulerian Methods
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An unusual pulse shape change event in PSR J1713+0747 observed with the Green Bank Telescope and CHIME
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Active galactic nucleus jet feedback in hydrostatic haloes
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A 3D View of Orion. I. Barnard's Loop
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Applying the Metallicity-dependent Binary Fraction to Double White Dwarf Formation: Implications for LISA
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Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
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Astrophysics with the Laser Interferometer Space Antenna
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(An)isotropy measurement with gravitational wave observations
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An empirical model of the Gaia DR3 selection function
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Sensitivity analysis of simulation-based inference for galaxy clustering
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Characterizing Observed Extra Mixing Trends in Red Giants using the Reduced Density Ratio from Thermohaline Models
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"Super-Kilonovae" from Massive Collapsars as Signatures of Black-Hole Birth in the Pair-instability Mass Gap
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The case for a minute-long merger-driven gamma-ray burst from fast-cooling synchrotron emission
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A Kilonova Following a Long-Duration Gamma-Ray Burst at 350 Mpc
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A measurement of the distance to the Galactic centre using the kinematics of bar stars
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data
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A closer look at supernovae as seeds for galactic magnetization
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pmwd: A Differentiable Cosmological Particle-Mesh N-body Library
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Differentiable Cosmological Simulation with Adjoint Method
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Charting Galactic Accelerations with Stellar Streams and Machine Learning
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AGN quenching in simulated dwarf galaxies
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A short gamma-ray burst from a proto-magnetar remnant
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Angular Momentum Transport in Proto-Neutron Stars and the Fate of Neutron Star Merger Remnants
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A Sun-like star orbiting a black hole
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Circumbinary discs for stellar population models
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A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 b
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A Mildly Relativistic Outflow Launched Two Years after Disruption in the Tidal Disruption Event AT2018hyz
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A Generative Model for Quasar Spectra
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Can we detect deep axisymmetric toroidal magnetic fields in stars?
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An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev–Zel’dovich effects
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A hidden population of massive black holes in simulated dwarf galaxies
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A follow-up on intermediate-mass black hole candidates in the second LIGO–Virgo observing run with the Bayes Coherence Ratio