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› Dr Allan Chapman (1946-2026)
RSS  Latest preprints on astro-ph:

› JWST Constraints on Primordial Magnetic Fields
› The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model
› The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
› spectroxide: A code package for computing cosmic microwave background spectral distortions
› ORCHARD: A General Planetary Evolution Code
› SN Ia Population Machine. I. A Unified Cosmological Simulation-Binary Synthesis Framework Establishing Non-universal Delay-time Distributions and Cosmic Progenitor-channel Dominance Crossover
› Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation
› Galactic tides and the outer density profile of the Sculptor and Ursa Minor dwarf spheroidals
› Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
› The Bulge Cluster Origin (BulCO) survey with CRIRES at the ESO-VLT: a chemical screening of the Globular Cluster NGC 6553
› A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks
› The effects of image augmentations when training machine learning models in astronomy
› Bound or blown: the fate of hot gas in galaxy groups
› Seismic background mitigation with the Lunar Gravitational-wave Antenna
› $N$-body modelling of the ED-2 stream progenitor shows Gaia BH3's formation involved dynamical interactions
› Joint Multiband Photometry with crowdsource
› Decoupling the AGN outflow and star-forming disk kinematics in the nuclear region of NGC 7582 with JWST NIRSpec and MIRI/MRS
› Ultra-thick warm absorbers: Enlarging the parameter space of AGN ionised outflows
› Can BLR line profile shape improve single-epoch black hole mass estimates?
› TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars
› Forward modeling solar spectra onto Doppler images of {\lambda} And
› A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State
› Pair-Rich Corona of an Accreting Kerr Black Hole
› Moving-Mesh Simulations of Mini-Common Envelope Ejection in Classical Novae
› Galaxy mergers and disk angular momentum evolution: stellar halos as a critical test
› Core Collapse Supernova Modeling: The Next Ten Years
› Variance-aware model discrimination with the Sunyaev-Zel'dovich effect of the 21 cm background (SZE-21cm)
› RSCL Earth Lookback Simulator: A Real-Time Multi-Physics Framework for Relativistic Signal Propagation from Confirmed Milky Way Exoplanets
› Hourly radio variability of PDS70c from time-differential photometry
› The Singular Behaviour of Ambipolar Diffusion Revealed by 1D Cartesian Solutions
› The Unstable Chromosphere: Effects of the Thermal Farley-Buneman Instability Across a Broad Range of Solar Chromospheric Conditions
› Exploring the Impact of Tilted Magnetic Dipoles on the Atmospheric Dynamics of Hot Jupiters: Towards an Improved Magnetohydrodynamic Framework
› Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity
› V446 Cephei: a $\beta$ Cep pulsator in a multiple system
› Non-Monotonic Rotation Imprint on Time-Integrated Neutrino Spectral Moments in a 15\,$M_\odot$ Core-Collapse Supernova Sequence
› Constraining the nature of active galactic nuclei through circumgalactic Lya emission at z=2-3
› The Impact of Elliptical Broad-Line Regions on Reverberation-Based Black Hole Mass Estimates
› Multi-tracers, multi-surveys: data-driven EFT prior calibration from the PFS--DESI overlap
› Spectral Evolution and Transient Broad-Line Features in the Isolated AGN UNAM-KIAS 613
› Revealing a Systematic High-latitude Current Sheet at Jupiter
› Oxygen Isotopic Compositions of Chondrules as Probes of Solar Protoplanetary Disk Formation
› Disc lifetime distribution as a function of the mass of host star
› The GMRT High-Resolution Southern Sky Survey for pulsars and transients -- VIII: Orbital Variability and the Evolution of a 1-Day He-WD Millisecond Pulsar J2101-4208
› Correlation Between Lunar Surface and Exospheric Sodium: Effects of Albedo-Driven Temperature on Multilayer Sodium Reservoirs Rather Than Surface Abundance Variations
› Recovering cosmological parameters from the mock gravitational wave data of the Einstein Telescope
› LAMOST J052016.79+345651.7: An EW-type Binary with Emission Line Spectra and Circumstellar Material
› Generalizing the CPL Parametrization through Dark Sector Interaction
› On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods
› Effects on vsini determinations of O-stars from 3D model atmospheres with large turbulent velocities
› Microlensing of fast and slow compact objects
› Rotation Measure Substructures Induced by the Ponderomotive Force of Inertial \alfven Waves
› Enabling real-time multi-messenger follow-up of transient events with Astro-COLIBRI
› Compton-thick AGN Characterisation in a Multi-wavelength Context: Insights from the 70-Month \textit{SWIFT}/BAT Catalogue
› Massive Black holes and their galaxies
› HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH
› Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system
› The PHANGS-H{\alpha} survey. Ground-based narrow-band imaging of nearby star-forming galaxies
› Environmental dependence of the Mass-Metallicity Star Formation Relations at z=4-10 with JWST
› Intergalactic Magnetic Field constraints from detected very high-energy Gamma-Ray Bursts using the Cherenkov Telescope Array Observatory
› Euclid: Asteroid rotation periods from the Euclid Ecliptic Survey
› Impact of segmented deformable mirrors on high-contrast testbeds for exoplanet imaging with future large space telescopes: contrast stability assessment on the HiCAT bench
› Suppression of Resonant Overstability at Sharp Migration Gradients
› Characterisation of the Clouds' young stellar Bridge using Gaia DR3
› A multifluid approach for polydisperse pebble accretion: From particles to fluids, establishing the multifluid framework
› Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters
› Substructure in redMaPPer clusters and its impact on X-ray morphology and scaling relations
› Homogeneous Stellar Parameters from Heterogeneous Spectra with Deep Learning
› Equifinality of Venus-like CO$_2$ Atmospheres
› Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension
› Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion
› Fast radio burst dispersion is an unbiased tracer of matter on large scales
› From short-lived to long-lived clouds: impact of star formation models on giant molecular cloud evolution in simulations of an NGC 300-like galaxy
› JOYS+ analyses of OCN$^-$, N$_2$O, NO, and complex cyanides in ices -- Thermal processing results in modest enhancement of OCN$^-$ ice
› 3D Kinetic Simulations of Driven Reconnection in Merging Flux Tubes
› Joint Estimation of Properties of the Lunar Subsurface and Galactic Foregrounds with LuSEE-Night
› Peculiar velocities in the $\Lambda$CDM universe
› Solar Energetic Particle Reflection by Precursor ICMEs: Multi-spacecraft Observations of Bi-Directional Electron Beams at 1 AU
› A magnetotelluric image of the Curnamona Province and the adjacent Delamerian Orogen margin: new insights into the crustal architecture
› Gauge Theoretic Signal Processing II: Zero-Latency Whitening for Early Warning Pipelines
› Towards Seamless Lunar Mosaics: Deep Radiometric Normalization for Cross-Sensor Orbital Imagery Using Chandrayaan-2 TMC Data
› Simple Analytical Solutions of the Wheeler-DeWitt Equation in the Classical Hamilton-Jacobi Limit
› Plausible but Wrong: A case study on Agentic Failures in Astrophysical Workflows
› Polarization-preserving wavefront rotator
› Collective neutrino-antineutrino pair oscillations
› $\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity
› The case for super-Eddington accretion in JWST broad-line AGN during the first billion years
› Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers
› The Emergence of Little Red Dots from Binary Massive Black Holes
› Dimensional reduction for sampled priors and application to photometric redshift distributions
› Schwinger effect in axion inflation on a lattice
› R-process heating implementation in hydrodynamic simulations with neural networks
› Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array
› Resolving the Planck-DESI tension by nonminimally coupled quintessence
› Reionization in Protocluster Environments at $z>7$ with JWST/NIRSpec
› Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts
› CAZ catalog and optical light curves of 7918 blazar-selected active galactic nuclei
› Association of the IceCube neutrinos with CAZ blazar light curves
› SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
› $H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
› Coupling of neutrino beam-driven MHD waves and resonant instabilities in rotating magnetoplasmas with neutrino two-flavor oscillations
› Diverse Emission Patterns from Precessing Super-Eddington Disks Formed in Tidal Disruption Events
› Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies
› Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays
› A Novel Parameterization for Rapid Cooling in Supernova Remnants, with applications to the Pa 30 nebula
› Identification of Candidate Halos Hosting Massive Black Hole Seeds in the $\textit{Renaissance}$ Simulations with Support Vector Machines
› Stochastic gravitational-wave background search using data from five pulsar timing arrays
› The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS
› Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing
› Unprecedented Multipoint Observation of Spatially Varying ICME Turbulence of Different Ages during October 2024 Extreme Solar Storm at 1 AU
› Chiral gravitational waves from multi-phase magnetogenesis
› Willman 1 Revisited: The Kinematics, Chemistry, and Orbital Properties of a Potentially-Disrupting Dwarf Galaxy
› Single-star optical turbulence profiling techniques for the SHIMM and other Shack-Hartmann instruments
› An updated model for the Perseus Spiral Arm from Trigonometric Parallax and 3-dimensional kinematic distances of distant massive stars
› Enhancing Gravitational Lens Study with Deep Learning: A Study on Effects of Dropout Regularization
› ZTF J021804.16+071152.93: a dead cataclysmic variable and potential solution to the missing period bouncers
› Asteroseismology of red giants in the globular cluster 47 Tuc using the HST
› CIV wind properties of the SDSS-V X-ray selected quasars: strong optical-to-UV emission is key regardless of X-ray strength
› Towards physically more comprehensive AGN modelling in cosmological simulations: A MACER-based modification of IllustrisTNG
› High efficiency superconducting filterbanks with impedance-defined resolution for millimeter-wave spectroscopy
› Do little red dots really form a distinct class of astronomical objects?
› Nonperturbative stochastic inflation in perturbative dynamical background
› Plate Sensitivity Is Invariant Across Geomagnetic Storm Intensity at Harvard and Palomar: A Protocol for Artifact Control in Historical Plate Archive Studies
› The trigger and localization system of SVOM-GRM
› Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds
› Asteroseismic rotation rates of hot subdwarf B stars hint at transient accretion from leftover common envelope matter
› First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST
› It\^o tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics
› Nonparametric Variational Inference Reconstruction of the Cosmic Expansion History from SNe Ia -- the charm2 code
› Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
› Thermodynamics of magnetized BPS baryonic layers and the effects of the Isospin chemical potential
› Probing Heavy Dark Matter in Red Giants
› Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess
› Multimodal axion emissions from Abelian-Higgs cosmic strings
› Impact of facility timing and coordination for next-generation gravitational-wave detectors
› Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment
› WIMP Meets ALP: Coherent Freeze-Out of Dark Matter
› Quantum dynamics of cosmological particle production: interacting quantum field theories with matrix product states
› A framework for LISA population inference
› Plotting correlated data
› Global structure of the time delay likelihood
› Local Origin of Hidden Symmetry in Rotating Spacetimes
› The read-out electronics for the FLASH experiment

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