Computational Astrophysics: Publications
Read the latest papers published by our research teams.
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Results
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An Earth-Sized Planet in a 5.4h Orbit Around a Nearby K dwarf
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Impact of Pretraining Word Co-occurrence on Compositional Generalization in Multimodal Models
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Open Source Planning & Control System with Language Agents for Autonomous Scientific Discovery
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Evaluating Retrieval-Augmented Generation Agents for Autonomous Scientific Discovery in Astrophysics
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Causal Foundation Models: Disentangling Physics from Instrument Properties
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CosmoBench: A Multiscale, Multiview, Multitask Cosmology Benchmark for Geometric Deep Learning
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Lost in Latent Space: An Empirical Study of Latent Diffusion Models for Physics Emulation
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Sloan Digital Sky Survey. V. Pioneering Panoptic Spectroscopy
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Simulation-Efficient Cosmological Inference with Multi-Fidelity SBI
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On the Universality of the Split Monopole Black Hole Magnetosphere
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CAPERS Observations of Two UV-Bright Galaxies at z>10. More Evidence for Bursting Star Formation in the Early Universe
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Radiation and Magnetic Pressure Support in Accretion Disks Around Supermassive Black Holes and the Physical Origin of the Extreme-ultraviolet to Soft X-Ray Spectrum
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Inferring the Density and Membership of Stellar Streams with Flexible Models: The GD-1 Stream in Gaia Data Release 3
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Accretion of Active Galactic Nucleus Stars Under the Influence of Disk Geometry
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On the effects of parameters on galaxy properties in CAMELS and the predictability of \(\Omega_{\rm m}\)
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Can We Discover Physical Models Using Machine Learning? A Case Study of Galaxy Sizes
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Time-resolved p-mode Oscillations for Subgiant HD 142091 with NEID at WIYN
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Circumplanetary Disks are Rare Around Planets at Large Orbital Radii: A Parameter Survey of Flow Morphology Around Giant Planets
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Relationships between PAHs, Small Dust Grains, H\(_2\), and HI in Local Group Dwarf Galaxies NGC 6822 and WLM Using JWST, ALMA, and the VLA
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ASURA-FDPS-ML: Star-by-star Galaxy Simulations Accelerated by Surrogate Modeling for Supernova Feedback
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Iron Snails: Nonequilibrium Dynamics and Spiral Abundance Patterns
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Bursts of Star Formation and Radiation-driven Outflows Produce Efficient LyC Leakage from Dense Compact Star Clusters
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Discovery of a Weak CN Spectral Absorption Feature in Red Supergiant Stars in the Andromeda (M31) and Triangulum (M33) Galaxies
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High-energy Neutrino Signatures from Pulsar Remnants of Binary Neutron-star Mergers: Coincident Detection Prospects with Gravitational Waves
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Detection of [OIII]88\(\mu\)m in JADES-GS-z14-0 at z=14.1793
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Searching for GEMS: Confirmation of TOI-5573 b, a Cool, Saturn-like Planet Orbiting an M Dwarf
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Five New Sirius-like White Dwarf–Main-sequence Star Systems with MagAO-X
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Stellar Obliquity of the Ultra-short-period Planet System HD 93963
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Lens Modeling of STRIDES Strongly Lensed Quasars Using Neural Posterior Estimation
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The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
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Far-infrared enhanced survey spectrometer for PRIMA: science drivers
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PRIMA mission concept
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Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
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Optical spectroscopic signatures of the red giant evolutionary state
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Stellar populations in STARFORGE II: comparison with observations
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JWST MIRI/MRS observations of hot molecular gas in an AGN host galaxy at Cosmic Noon
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A Hot Jupiter with a Retrograde Orbit Around A Sun-like Star and a Toy Model of Hot Jupiters in Wide Binary Star Systems
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Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
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CEERS: Possibly forging the first dust grains in the universe: A population of galaxies with spectroscopically derived extremely low dust attenuation (GELDA) at 4.0 \(< z \lesssim\) 11.4
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The MUSE view of ram pressure stripped galaxies in clusters: The GASP sample
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The completeness of the open cluster census towards the Galactic anticentre
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Simulation-based inference benchmark for weak lensing cosmology
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The mass-metallicity relation as a ruler for galaxy evolution: Insights from the James Webb Space Telescope
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A planetary-mass candidate imaged in the Young Suns Exoplanet Survey
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Euclid preparation. Full-shape modelling of 2-point and 3-point correlation functions in real space
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REBELS-MOSFIRE: Weak CIII] Emission is Typical Among Extremely UV-bright, Massive Galaxies at \(z\sim7\)
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Inferring Neutron Star Nuclear Properties from Gravitational-Wave and Gamma-Ray Burst Observations
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Synthesizer: Synthetic Observables For Modern Astronomy