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 News from astronomynow.com

› JWST’s ‘impossible’ early galaxies may be even more massive than we thought
› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
› Dark matter may come in multiple forms, new model suggests
› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
RSS  Latest preprints on astro-ph:

› CosmoFit: A Graphical User Interface for Bayesian Cosmological Parameter Estimation with User-Defined H(z) Models
› Constraining the Inner Dark-Matter Slope of Sculptor: A Comparative Analysis of Dynamical Methods
› CHIANTE I: Obliquity Measurements of Four High-Priority Ariel Targets in Binaries
› Solar-Cycle Variation of Newly Emerging Coronal Holes during Solar Cycle 24
› BlueBird 6 is Fainter than Block 1 Satellites
› More Numerous and Bluer: Companions of the Brightest Little Red Dots Differ from Control Galaxies at $>3\sigma$, Hinting at Synchronized Black Hole Seed Formation
› Spin inference with the Black Hole Explorer. I. Fisher information matrix forecast
› A simulation-based quality-control framework for the broad-line region radius-luminosity relation
› Signatures of Compact Object Mergers Inside Stars in AGN Disks
› WASP-12b Exhibits Persistent In-Transit H$\alpha$ Absorption
› Quantitative Links between Formation and Atmospheric Composition for Giant Planets
› Exact Equivalence of the Observed Redshift and the Pulsar Timing Modulation in the Infinitesimal-Pulse Limit
› Cool CGM MgII Absorption Across the Star-Forming, Green Valley, and Quiescent Transition
› Agentic Active Learning Meets Visual Embeddings: Finding Anomalies among 370 000 Variable Stars from ASAS-SN
› A General Response Theory for Closure Phases through Visibility Nulls and Image Structure
› A giant magnetic eruption from the asymptotic giant branch star Mira A
› The Highly Unusual Behavior and Chemical Composition of Interstellar Comet 2I/Borisov
› Sub-Millisecond Pulsars: Missing or Impossible?
› Beyond $w_0-w_a$ and Phantom Crossing: Testing Models of Coupled Dark Sector
› Cows, Tasmanian Devils, and Other Mysteries: Diversity and Origins of Luminous Fast Blue Optical Transients
› GravDyn: A Python Framework for Gravitational Modeling of Irregular Celestial Bodies Using Polyhedral, mascon, and Series Expansion Methods
› Periodic activity on the (sub)mm surface of the AGB star Mira A
› An analysis of the Herbig star population and their protoplanetary disks within 1 kpc
› Chaotic cosmic ray acceleration in nonlinear Alfven waves
› A New Probe of Dark Matter Subhalos: Stellar Aberration with TESS
› The Evolution of Low-Ionization Electron Densities in Galaxies Across Cosmic Epochs
› The Local Origin of a Host Dispersion Measure-Stellar Mass Relation in Fast Radio Bursts
› An Evolving Cosmic Shoreline and Sandbar Bounding the Rocky Airless Valley
› Linear Continuum Modelling to Explain The Majority of Bulk Features of Kuiper Belt Object Spectra
› Linking high-mass X-ray binaries to binary compact object mergers in Milky Way-like galaxies
› Projected Constraints on Primordial Black Holes from Scalar-Induced Gravitational Waves with Taiji
› Occultation of microlensed images by circum-lens disks: Implications for surveys
› Validation and extension of the PAWS Zemax model as a first step in the development of a Compact Arrayed Waveguide Stacked Multi-Object Spectrograph (CAWSMOS)
› Spatially resolved spectral properties of M87* on event horizon scales
› Comparing the Nebular and Stellar Dust Attenuation Curves in Nearby Star-Forming Galaxies
› Interplay of Compaction, Quenching, and Black Hole Growth in the Most Massive Galaxies since $z\sim5$: Insights from JWST and Chandra Data
› Decoupling candidate dual AGN from chance superpositions in the GOTHIC survey via a deep-learning framework
› The impact of circumstellar wind-blown bubbles on the dynamics of pulsar wind nebulae and supernova remnants
› Observations of ionized carbon towards the $\gamma$-ray-bright supernova remnant RX J1713.7-3946
› X-ray Polarization of Inverse Compton Scattering by Thermal and Nonthermal Electrons
› Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103
› Flare waiting time as a novel proxy of stellar magnetic activity
› SDSS-IV MaNGA: Star Formation Cessation in Low-redshift Galaxies. III. Dependence on Quenching Criteria
› An HI study of a large sample of ultra-diffuse galaxies
› Nitrogen- and nitrogen-oxygen-bearing organic molecules in comet 67P/Churyumov-Gerasimenko: An untargeted investigation
› The Effect of Slitless Spectroscopic Redshift Uncertainty and Interlopers on BAO Measurements from CSST-like Samples
› Demonstration of simultaneous PIAA- coronagraphy and wavefront sensing using a single metasurface-based focal-plane optic
› The First X-Ray Polarimetry of the Typical Accretion Disk Corona Source 4U 1822-37
› The Photonic Lantern Nuller: from concept to laboratory and on-sky demonstrations
› A "MeerKAT-meets-LOFAR" Study of 2A 0335+096: Discovery of a Complex 500 kpc Radio Halo in a Disturbed Cool-Core Cluster
› The Hot Neptune Initiative (HONEI) III. An ultra-hot super Neptune orbiting the metal-rich subgiant star TOI-5646: the largest host for a desert dweller
› Quantum-optimal instruments for high-contrast imaging with multi-plane light converters
› Synchrotron filaments in radio galaxies: rarity, stability, and environmental influences from LOFAR and ROSAT observations
› The final design of GMagAO-X: the wavefront sensing and control (WFS&C) architecture of GMagAO-X
› Sub-diffraction-limited coronagraphic imaging with nano-printed PIAACMC phase masks
› On-sky demonstration of self-learning predictive control with MagAO-X
› Digging dark holes on-sky with the Self-Coherent Camera: Preliminary results
› Interstellar Aromatic Infrared Bands: IR absorption spectroscopy of the lowest triplet state of naphthalene
› Fingerprints of thermal Comptonization in accreting neutron stars. Plasma-vacuum interplay in cyclotron lines and polarisation
› Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion
› The Primordial power spectrum from the largest to smallest CMB scales
› Dark-to-black super-accretion as a spin-imprinting mechanism for supermassive Kerr black holes
› Gaussian process reconstruction of scalar field dynamics from recent cosmological data
› No need to modulate: On-sky results of a Neural Network enhanced pyramid wavefront sensor and prospects for the ELTs
› NEXT: The Netherlands EXoplanet Testbed I. Goals and opto-mechanical design
› Forward modelling coronagraphic images with a fully physical, differentiable digital twin of MagAO-X: first laboratory results
› CMB Birefringence from Axion String Networks Calibrated to an AMR Simulation
› A high-isolation wideband channelizer for MKID readouts: a custom HLS implementation on RFSoC
› Narrow Population Inference Enhanced by Analytical Likelihood Models
› Fourier Morphology Diagnostics of Delta Cephei MESA-RSP Light Curves
› Evolutionary Period-Change Modeling of Delta Cephei with MESA Tracks
› Probing the Three-Dimensional Structure of a Jet with Faraday Tomography
› Constraining the Tilted Dipole Cosmology with Primordial Nucleosynthesis and Baryogenesis
› Testing the QGP Star Hypothesis: The oMEGACat BH-2 System as a Candidate Color-Superconducting Quark-Gluon Plasma Star
› Verifying Gamma-Ray Burst Duration Analysis Using the Compton Gamma-Ray Observatory T50 Data
› A quadratic balance relation for radial nonadiabatic pulsations
› Assessing the Credibility of Gamma-Ray QPO Candidates in 41 TeV-Selected Blazars
› Cassiopee: Defining the next-generation deformable mirror and high-speed SWIR camera for adaptive optics applications
› A Broadband X-ray Analysis and Optical Counterpart Search of IC5052 ULX
› Estimator forensics for the wide-binary gravity test: the eccentricity-triple coupling manufactures a pseudo-signal, and a pre-registered protocol for Gaia DR4
› The Interplay of Magnetic Fields, Turbulence and Vorticity in Core-Collapse Supernovae
› First application of weak lensing peak steepness statistics to HSC Y1 data: effectively probing halo density profiles
› Arcminute Microkelvin Imager observations at 15.5 GHz of the tidal disruption event Swift J164449.3+573451 from 2011 Mar to 2014 Mar
› Broad Paschen lines as black hole mass tracers: A reverberation mapping calibration
› NIRC2-Pol: First Light of Near-Infrared Polarimetry on Keck II
› Spatially resolved molecular gas conditions in the circumnuclear disc of 3C 84
› Chebyshev interpolation in Einstein-Boltzmann codes
› Improving the Physical Interpretability of Gaussian Processes in Stellar Activity Modeling: A Study Case on Photometric Variability Among Stellar Clusters
› Potential survivable niches for microbial life on the lunar south pole
› Photospheric index of geomagnetic activity
› Calculation of Field Line Slippage Rates in Coronal Simulations
› The impact of the IGM thermal state on the Ly$\alpha$ flux 3D power spectrum from linear to highly non-linear scales
› Quantum-Gravity-Inspired Effects in Neutron Stars: A Critical Map from Microscopic Assumptions to Observables
› Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion
› Atmospheric Retrieval of Combined JWST, HST, and Ground-Based Observations Reveals a Featureless Transmission Spectrum for GJ 1132 b
› Measurement of spin-orbit misalignment in binary black holes via the total spin
› The Mass Dependence of the Fundamental Metallicity Relation in Observations and Simulations
› Thermal Stability of Radiation-Pressure-Dominated Accretion Disks Threaded by Net Vertical Magnetic Flux
› The GPSP Atlas: High-resolution Galactic Photon Survival Probability Atlas for Very-High- and Ultra-High-Energy Gamma-Ray Astronomy
› Magnesium silicate condensation in sub-Neptune envelopes: the fundamental link between chemistry, structure, and observables
› Flyby-induced high-eccentricity migration and the prevalence of hot Jupiters in M67
› Impact of Scale-dependent Primordial Non-Gaussianity on Scalar-induced Gravitational Waves
› Across the Universe: GW231123 as a magnified and diffracted black hole merger
› Determination of $H_{0}$ with a Photometric AGN Golden Sample derived from a joint SN Ia-QSO cosmological reconstruction
› A survey detection channel overrides the pixels in an astronomical foundation model, and biases tomographic mean redshifts
› Wilsonian Cosmology: de Sitter (in)Stability
› When the HL-LHC is blind, LISA is deaf (but not vice versa): 2HDM collider-cosmology synergies
› Color-Kinematics Duality and the Double Copy in Curved Spacetimes
› Topics in the phenomenology of axions: the cases of cosmic strings and superradiance
› Nonequilibrium pulse dynamics and metastable latching in nonlinear kinetic inductance detectors
› Searching for Solar-Basin Axionlike-Particle Decay with XMM-Newton Blank-Sky Observations
› Self-Consistent Determination of the Transition Temperature Between the $^{14}\mathrm{C}(n,\gamma)^{15}\mathrm{C}$ and $^{14}\mathrm{C}(p,\gamma)^{15}\mathrm{N}$ Reactions
› Anomalous Electric Fields in Earth's Turbulent Magnetosheath: Insights From 3D Hybrid Simulations
› Comprehensive solar eruption analyses enabled by the tools of the SOLER project
› Cluster emission and its impact on the r-process nucleosynthesis
› The Bondi Dipole in Full Numerical Relativity: a Self-Accelerating Positive-Negative Mass Binary
› Global uniqueness of Kerr black hole spin and inclination from a segment of the critical curve
› Unsupervised Deep Learning Method for Clustering KAGRA O3GK Transient Noise Data
› Cosmic muon arrival directions as a source of entropy
› Dynamical Friction as Environmental Gravitational Self-Force
› Generative AI for Validating Physics Laws
› Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence
› Triggering and quenching in the shadow of AGN: How does AGN proximity affect star formation in the EAGLE simulation?
› Exploring Ultra-Slow-Roll Inflation in Composite Pseudo-Nambu-Goldstone Boson Models: Implications for Primordial Black Holes and Gravitational Waves
› Exploring the Origin of Rejuvenating Gas from MaNGA Nearby Galaxies
› Extended Components of Little Red Dots in the Rest-Frame Optical
› Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI
› Discovery of Weak O VI Absorption in Underdense Regions of the Low-Redshift Intergalactic Medium
› Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
› A whole-planet model of the Earth without life for terrestrial exoplanet studies
› Microquasar Remnants as Pevatrons Illuminating the Galactic Cosmic Ray Knee
› Weighing gas-rich starless halos: Dark matter parameter inference based on gas distributions
› Long-Integration Magnetar Burst Observatory (LIMBO): Instrument Summary and Early FRB Rate Constraints
› Interaction between vegetation and Snowball phases in the late Proterozoic Earth
› Exoplanet Orbital Distribution around FGK Sun-like Host Stars I: planet occurrence rate derived from the Kepler Mission and theoretical interpretations from planet formation
› Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
› Deriving volume density profiles of filaments from observed surface densities
› The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
› Probing past mergers of supermassive black holes with pulsar timing arrays: The role of pulsar terms
› ORCHARD: A General Planetary Evolution Code
› Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters
› Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions
› The GALAH Survey: Neutron-Capture Elemental Abundances for 350,000 Gaia-RVS spectra and the Chemodynamics of Accreted Structures
› Bayesian analysis of the shear modulus in the neutron-star crust
› ATLAS. I. A Scaling Relation of LRDs between Broad H$\alpha$ and Bolometric Luminosities: Enhanced Broad H$\alpha$ Emission Relative to Low-$z$ Type 1 AGN
› Black Hole Polarimetry: Universal Polarization of Synchrotron Radiation at the Horizon
› Multi-band Structural Analysis of KiDS-selected Low Surface Brightness Galaxies with Hyper Suprime-Cam Imaging
› Dynamical Tides during High-Eccentricity Migration produces the Hot Jupiter Pile-up, Neptune Ridge, and Neptune Desert
› The local ultraviolet signature of Type Ia supernova environments from HST and MUSE
› Wind Acceleration as a Driver of Detached Blueshifted Absorption in Quasar Disk Winds
› Cosmological Constraints on the DGP Model in light of DESI DR2 2025 Data
› Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations
› Effect of Neutron Star Jets on Common Envelope Evolution
› Constraining primordial black holes and primordial curvature power spectrum with extragalactic muon neutrino
› Inferring 3D Coronal Magnetic Fields through Seismology-assisted Inversions of $IQU$-only Spectropolarimetric Observations
› Late-infall-induced formation of giant planets, multigenerational planetesimals, and disk substructures
› High-mass binary black hole mergers from detailed binary evolution models
› An extreme case of X-ray reflection in the symbiotic V648 Car
› Binary evolution at the extremes of mass-transfer efficiency: Contact, mergers, and population signatures
› NestyNet. I. Physics Functions Are Hard to Fit with Neural Networks: A Framework for Accurate Surrogates and Analytic Derivatives
› NestyNet. II. Coherent Function-Space Posteriors from Scientific Neural Surrogates (or How to Avoid Expensive MCMC)
› Decoding Exoplanetary Degeneracies Through Geometry: Applications for resonant systems
› Reconstruction of ASO-S/HXI Solar Flare Hard X-ray Source Images with Physics-Constrained Deep Network
› PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
› TomoSphero: Fast Differentiable Projector for Planetary and Solar Tomography on Spherical Grids
› The Kick Velocities of Neutron Stars in Binary Systems
› NestyNet. III. Symbolic Regression from Analytic Neural Surrogates
› NestyNet. IV. Laws Chosen by Nothing in Advance
› Where Do Periodic Density Structures Acquire Coherence? A Low-Coronal Resonator Candidate and a 12-Event STEREO/SECCHI Transfer Test
› Nonminimally Coupled Quintessence with Double Exponential Potential: Observational Evidence Against Big Crunch Singularity
› Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
› NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration
› Expanding Our Horizons: Rethinking Gravity's Role in the Quantum-to-Classical Transition
› Charged current neutrino processes in hot nuclear matter with a recent Skyrme parametrization constrained by microscopic calculations
› Comment on "Non-linear interactions in cosmologies with energy exchange"
› Probing Memory-Burdened Primordial Black Holes with High-Energy Neutrinos
› Heavy neutral leptons beyond the BBN bound: probing the lepton asymmetry of the Universe

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