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 News from astronomynow.com
› 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
› XRISM solves gamma-Cas’s 50-year X-ray mystery
› Molten lava world points to new class of planet
RSS  Latest preprints on astro-ph:
› Something new under the Sun: A magnetically driven CH/CN anti-correlation
› The Research Impact of the Jodrell Bank Observatory and Other Facilities affected by the UK Science Funding Cuts in 2025
› AT 2022csn: A Photometrically Peculiar Optical/UV Tidal Disruption Event in a Type II AGN
› The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc
› Galaxy-LRD Strong Lenses: A Missing Population?
› A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory
› Enhancing the sensitivity of next-generation X-ray imaging detectors with artificial intelligence and advanced event reconstruction algorithms
› Cloud Scale Star Formation and Gas Scaling Relations in the Milky Way
› Molecular absorption lines toward the Galactic ISM detected at 89 GHz with VLBI
› Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation
› Rings in the Sky: Orbital Data Centres and Potential Impacts to Astronomy and the Sky
› Gamma-ray and radio populations of millisecond pulsars in globular clusters
› The Indian Pulsar Timing Array Data Release 2: III. Search for a Stochastic Gravitational Wave Background
› The Bimodal Mass Ratio Distribution of the Hyades
› Structural quasi-universality in highly magnetized differentially rotating neutron stars
› Single-Photon Counting CMOS Detectors for the Habitable Worlds Observatory
› New Spatially Resolved Observations of Betelgeuse from the VLA and ALMA: Evidence for Atmospheric Perturbations from a Close Companion
› A new NASA Pioneer: the Globe Orbiting Soft X-ray Polarimeter (GOSoX)
› Tracing luminous infrared galaxy populations through cluster evolution in a cosmological mock redshift survey
› Fast, low noise, megapixel detector and readout systems for future X-ray astronomy missions
› Kick Velocities and Mass Function of Free-Floating Planets from Dynamical Ejection in Hierarchical Three-Body Systems
› Visual Orbits of Spectroscopic Binaries with the CHARA Array. V. HD 210763 and HD 221950
› The Space Coronagraph Optical Bench (SCoOB): X. Dark zone maintenance
› The Space Coronagraph Optical Bench (SCoOB): 11. Modeling and correction of chromatic aberrations
› EP241113a: dissipative photospheric emission from a dirty fireball
› HIP 61637 b: a TESS Brown Dwarf in a Near-circular Orbit around a Massive A-type Star
› Lithium as a Signpost for Compact Object Binary Candidates in the LAMOST Medium Resolution Survey
› PDRs4All XXII. Near-Infrared continuum in the Orion Bar
› The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies
› Investigating Possible Stellar Coronal Mass Ejections in M-type Dwarfs Using the CARMENES DR1 Spectra
› One year of broadband radio monitoring of the enigmatic transient GRB 250702B reveals the evolution of the relativistic jet
› A Possible Stellar CME Event Associated with a Long-duration Optical Flare on the RS CVn-type Star UX Arietis
› The One-Loop Power Spectrum of Fast Radio Burst Dispersion Measures
› Binary Constraints on the Origin of Nitrogen-rich Field Stars
› Electron transport in a radiation-dominated plasma Application to solar corona brightenings
› The double white dwarf merger model for the progenitors of SN 2021yfj-like events
› Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies
› Long-lived thermal dynamo generation on differentiated, impact-disrupted planetesimals
› Unravelling Mass Transfer in Algols from Surface Abundances. I. Z Vulpeculae
› Pixel-Level Calibration for Space-Based High Precision Astrometry Using Young's Fringes
› The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
› Bridging perturbation theory and simulations: initial conditions and fast integrators for cosmological simulations
› Phase-curve approach to study atmospheric flows in hot Jupiters
› Tomographer: End-to-end Redshift Distribution Estimation for Source Catalogs and Intensity Maps
› A study on the contribution of the interplanetary medium in radio occultation experiments
› SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations
› Modified Cosmological Expansion and the JWST CMB Optical Depth Tension in Self Interaction Gravity
› Wave excitation by a collapsing granule: insights from IFU observations and high-resolution RMHD simulations
› V557 Mon: Hot water vapour observed on an eruptive young star
› Cosmic Velocity Flows: from Theory to Observations
› MIGHTEE-HI / LADUMA: Investigating the link between baryons and dynamics with 130 resolved HI-selected galaxies
› A JWST redshift for the host galaxy of EP250207b of z=3.2: a collapsar origin is viable
› General-relativistic structure of two-component quantum dark fermion stars
› Revisiting the XMM-Newton Observations of the Galactic Microquasar SS 433: Implications for the Origin of the Ultrahigh-Energy Emission Detected by LHAASO
› Circumgalactic medium depletion drives satellite quenching in IllustrisTNG
› How Dilatation Invariance Suppresses Loop Corrections to Curvature Perturbations on CMB Scales
› Statistical Study of Solar Prominence Plumes Based on NVST H$\alpha$ Observations
› Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts
› Integrated cosmological memory: A dark-siren method to probe dark energy
› Horizontal Magnetic Fields Dominate the Quiet Sun Internetwork in Sunrise III Observations. Evidence from Traditional and Transformer-Based Inversions
› SuMAC: On-sky demonstration of multi-pixel on-chip millimeter-wave spectroscopy at the Large Millimeter Telescope
› Data reduction pipeline for the SuMAC millimeter-wave spectrometer at the LMT
› Iron K$\alpha$ signatures from accretion disks around fermionic dark matter cores
› Expanding magnetic canopy structure and parasitic polarities in a quiet-Sun network element observed by Sunrise III/SCIP
› Formation of nitriles and isonitriles by the heavy-ion irradiation of propionitrile in N2-rich astrophysical ices
› A broad exploration of climate and observability of close-in rocky exoplanets: applications to Ross 128 b
› Probing Axion Like Particle-Proton Interactions through the Interplay of Dark Matter and Cosmic Rays in Large-Scale Structure
› Fisher Forecasting for the DESC with $\texttt{Augur}$
› First fast radio burst search campaign at the Argentine Institute of Radio Astronomy
› Profile Analysis of the Multiwavelength 2.1-year Oscillations of PG 1553+113
› Helium-poor winds do not require helium-poor planets
› Cosmology in the Einstein Telescope era: comparing traditional and simulation-based methods for population inference
› A multi-axion model of inflation and dark matter
› Abundant production of scalars and axions from phase transition bubble expansion
› Determination of the Angular Momentum of Radiated Gravitons, Scalars, and Dark Photons from Binary Orbits
› On Modeling Anisotropic Quark Stars: The Role of Anisotropy in Radial Oscillation Spectra
› The orientation of historic churches in Las Palmas de Gran Canaria and its surroundings: preliminary results
› Neutrino flavor-wave transport: Numerical tests and theoretical challenges
› Minimal Scale-Invariant Dark Matter
› Radiation reaction in the classical relativistic St{\o}rmer problem
› From St{\o}rmer to Schwarzschild: Analytical Dynamics of Charged Particles in a Dipole Magnetosphere
› Gravitational Enstrophy: Local Geometric Origin and Inverse-Cascade Constraints
› Simultaneous Mars-orbit observations reveal Kelvin-Helmholtz instability-driven bulk atmospheric ion escape
› A Tale of Two Couplings: Bayesian Selection in the Interacting Dark Sector
› Frequentist Cosmological Constraints from Full-Shape Clustering Measurements in DESI DR1
› Spin Constraints on 4U 1630-47 via combined Continuum Fitting and Reflection methods: a comparative study using Frequentist and Bayesian statistics
› Scheduling follow-up observations of energetic transients with the neutrino target scheduler (NuTS)
› Is Dark Energy Increasing or Decreasing in the Late Universe?
› CMB Hemispherical Power Asymmetry from Early Phase of Inflation
› Stellar Spectroscopy Using Diffraction Grating, CMOS Monochrome Sensor and Reflecting Telescopes
› Cosmological Implication of Cross-correlation between Galaxy Clustering and 21-cm Line Intensity Mapping
› Empirical Relationship Between Dark Matter and Baryon Profiles for Solving the Core-Cusp and Diversity Problems of Galaxies
› Physical origin of very-high-energy gamma rays from the low-luminosity active galactic nucleus NGC 4278 and implications for neutrino observations
› Relativistic Magnetohydrodynamic Simulations of Giant Magnetar Bursts
› Systematic and Statistical Uncertainties in the Non-Gravitational Acceleration of 3I/ATLAS
› Accurate and efficient simulation-based inference for massive black-hole binaries with LISA
› Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
› Enhancing event reconstruction for $\gamma$-ray particle detector arrays using transformers
› Beyond the mass-radius plane: Integrated radiative-convective and interior structure simulations of the exoplanet continuum
› Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks
› A Comprehensive Study of Morphology and Kinematics in Extended Nebulae Around UV Luminous Quasars at $z\approx1$
› Suppression of boosted relic neutrinos by photon backgrounds during ultra-high-energy cosmic ray propagation
› Nebular_AGN: A CIGALE module for fitting active galactic nucleus emission lines
› Modelling the delayed shock-breakout emission following jet-launching binary neutron star mergers via relativistic magnetohydrodynamic simulations simulations
› Archival Diagnostics for Potential Background Contaminantsof Project Hephaistos Dyson Sphere Candidates
› Finite-Field QED Corrections to Vacuum Birefringence and Magnetar Polarization Transport
› Tilted thin accretion disks in the full Kerr spacetime and their implications
› Core-Halo Mass Relation in Cosmological Vector Dark Matter
› When Galaxies Refuel: Evolution of the Perturbed Spiral Galaxy NGC1385
› ZTF SN Ia DR2 follow-up: early excess in Type Ia supernova light curves
› Predicted Ejecta Dynamics and Observability of the 2026 Falcon 9 Upper Stage Lunar Impact
› Validation of the DESI DR2 Ly$\alpha$ forest full-shape analysis
› Same explosion, many faces: numerical modeling reveals viewing angle as a driver of diversity for core-collapse SNe in binary systems
› Progenitor age-bias-corrected Type Ia supernovae favor a logarithmic luminosity-distance relation
› Accretion-induced spin-up: Implications for mass constraints of AMXPs
› A refined method for measuring cosmological distances using variability and proper motions in AGN with VLBI-detected counter-jets
› Spatial Mapping and Capacitor Trimming Developments to Improve Usable Pixel Yield in PRIMA FIRESS Kilo-Pixel Arrays
› Dark Baryon Black Holes
› Relativistic formulation for dual one-way Doppler Cancellation Scheme observables for gravitational redshift tests
› Extending Weinberg's EFT: effective scalar-tensor theories up to sixth order
› Traversable Wormholes induced by polytropic $n=1$ energy density
› Beyond Plane Waves: Coherent Network Response to Collimated Gravitational-Wave Wavepackets
› Primordial Black Holes: A Review of Formation and Evolution

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