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 News from astronomynow.com

› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
› Binoculars to boost your night-sky viewing
› Lyra’s stunning smoke ring – M57
› Is the Hubble Tension Resolved?
› Universe’s end – sooner rather than later
› Caught in the current of the wonderful Whirlpool
› A faint star will reveal itself as it throws a hissy-fit
› Saturn’s Rings to “Disappear”
RSS  Latest preprints on astro-ph:

› Additive Manufacturing of PEEK/Lunar Regolith Composites for Sustainable Lunar Manufacturing
› Predictive calibration for digital sun sensors using sparse submanifold convolutional neural networks
› A Census of Variable Radio Sources at $3\,$GHz
› Mapping the Distant and Metal-Poor Milky Way with SDSS-V
› Cosmological Zoom-In Simulation of Odd Radio Circles as Merger-Driven Shocks in Galaxy Groups
› Star formation histories and gas content limits of three ultra-faint dwarfs on the periphery of M31
› Metal-Poor Star-Forming Clumps in Cosmic Noon Galaxies: Evidence for Gas Inflow and Chemical Dilution Using JWST NIRISS
› Challenges to the Two-Infall Scenario by Large Stellar Age Catalogs
› HST Observations of the CV Propeller LAMOST J024048.51+195226.9
› Disks no more: the morphology of low-mass simulated galaxies in FIREbox
› Viability of generalized $\alpha$-inflation from Planck, ACT, and DESI Data
› Transient LoBALs at high velocities: A Case of Extreme Broad Absorption Line Variability in J115636.82+085628.9
› Preliminary census of galaxies in the LISA localisation volume: I. Searching for LISA candidate massive black hole binary merger hosts using Sloan Digital Sky Survey photometry
› Estimate of Current Mass of the Large Magellanic Cloud from the Orphan-Chenab Tidal Stream
› XRISM Observations of Cassiopeia A: Overview, Atomic Data, and Spectral Models
› The 2025 Release of Cloudy
› Revisiting the Proper Motions of M31 and M33 Using Massive Supergiant Stars with Gaia DR3
› Equation vs. AI: Predict Density and Measure Width of molecular clouds by Multiscale Decomposition
› GW231123 Formation from Population III Stars: Isolated Binary Evolution
› A Catalog of Forty-two Heartbeat Stars Discovered in TESS Data
› Energy-dependent anisotropy of cosmic-ray muons: A twelve-year study with IceCube Neutrino Observatory
› Detailed radial scale height profile of dust grains as probed by dust self-scattering in HL Tau
› Corotating Interaction Regions (CIRs): impacts with exoplanets
› Unveiling the Atmosphere of HR 7672 B from the Near-Infrared High-Resolution Spectrum Using REACH/Subaru
› Revisiting symbiotic binaries with interferometry: II. New PIONIER data
› Numerical simulations of the line-force-driven winds from active galactic nuclei: The special relativistic effects
› Can cosmic rays explain the high ionisation rates in the Galactic centre?
› Testing Gamma/Hadron Separation for Ultra-High-Energy Cherenkov Astronomy
› A Nitrogen-rich AGN Powering a Large Ionizing Bubble at z=8.63
› Daily fluctuations propagate damply through a black hole accretion disk
› Measurement of the Primary Beam of the Tianlai Cylindrical Antenna Using an Unmanned Aerial Vehicle
› HI asymmetries of galaxies in the Ursa Major and Perseus-Pisces environments
› SN 2024gy: Multi-epoch Spectroscopic Evidence for Delayed Detonation in a Type Ia Supernova
› Asymmetries in the LMC velocity maps
› Deciphering The Launching of Multi-phase AGN-driven Outflows and Their (Spatially Resolved) Multi-scale Impact
› Theoretical Diagnostics for the Physical Conditions in Active Galactic Nuclei under the View of JWST
› Error dependencies in the space-based CNEOS fireball database
› Identifying Radio Active Galactic Nuclei with Machine Learning and Large-Area Surveys
› A fast radio burst from the first 3 billion years of the Universe
› Cosmological Constraints on $f(T,B)$ Gravity from Observations of Early and Late Universe
› The role of the pre-exponential factor on temperature programmed desorption spectra: A computational study of frozen species on interstellar icy grain mantles
› Binary stellar evolution yields in galactic chemical evolution calculations
› Rotational evolution of deformed magnetized neutron stars: implications for obliquity distribution and braking indices statistics
› Revealing a ribbon-like jet in OJ 287 with RadioAstron
› Resolving the Planck-DESI tension by non-minimally coupled quintessence
› Families of Transfers from circular low Earth orbit to Distant Prograde Orbit around the Moon
› Silicate Sundogs: Probing the Effects of Grain Directionality in Exoplanet Observations
› $\texttt{GENGARS}$: Accurate non-Gaussian initial conditions with arbitrary bispectrum for N-body simulations
› The multi-faceted variability of HD 192639: Stochastic behaviour, regularities, and an exceptional mass-ejection event
› Thermoelastic Contraction as a Suppressor of Atmospheric Escape in Close-in Exoplanets
› Clustering of Primordial Black Holes in Excursion Set Theory
› SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
› Using Faded Changing-Look Quasars to Unveil the Spectral Energy Distribution Evolution of Low-Luminosity Active Galactic Nuclei
› HAWC, VERITAS, Fermi-LAT and XMM-Newton follow-up observations of the unidentified ultra-high-energy gamma-ray source LHAASO J2108+5157
› The Second Stellar Spectrum: Rotating hot massive star linear spectropolarimetry with the Ohman Effect
› On the origin of a possible hard VHE spectrum from M87 discovered by LHAASO
› $\nu p$-process in Core-Collapse Supernovae: Imprints of General Relativistic Effects
› Mission Analysis for the HENON CubeSat Mission to a Large Sun-Earth Distant Retrograde Orbit
› STRRINGS: STReams in Residual Images of Nearby GalaxieS
› Wiener filtering and multi-tracer techniques for dark matter cross-correlations between gamma-ray emission and galaxy catalogs
› Discovery and dynamics of a Sedna-like object with a perihelion of 66 au
› Binary Systems Search with TESS
› Effect of magnetic field inclination on black hole jet power and particle acceleration
› New Radio Data on Sources of the Big Trio Program for Searching for Distant Radio Galaxies
› Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?
› The ALMA REBELS survey: [OIII]$_{88\mu \text{m}}$ line scans of UV-bright $z \gtrsim 7.6$ galaxies
› PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
› On the formation of multiple dust-trapping rings in the inner Solar system
› Placing the Near-Earth Object Impact Probability in Context
› Higher order methods for Radiative Transfer in Astrophysical simulations: $\rm P_n$ vs $\rm M_1$
› Pre-discovery TESS Observations of Interstellar Object 3I/ATLAS
› A Comprehensive Analysis of X-ray Sources in Terzan 5 Using Chandra Observations
› Energy flow and radiation efficiency in radiative GRMHD simulations of neutron star ultraluminous X-ray sources
› MINDS. Young binary systems with JWST/MIRI: Variable water-rich primaries and extended emission
› EDGES-3: Instrument Design and Commissioning
› The multi-physics analysis, design and testing of CUSP, a CubeSat mission for space weather and solar flares x-ray polarimetry
› Spectroscopic Confirmation: Fast rotators in the young clusters NGC 1856 and NGC 1953
› PSR J0614-3329: A NICER case for Strange Quark Stars
› Optical and near-infrared nebular-phase spectroscopy of SN 2024ggi: constraints on the structure of the inner ejecta, progenitor mass, and dust
› Testing Dark Matter with Generative Models for Extragalactic Stellar Streams
› Improved Limits on Exotic Interactions Mediated by Axion-Like Particles Between Muons
› Revealing the Origins of Galactic Globular Clusters via Their Mg-Al Abundances
› (Non-)Perturbative Dynamics of a Light QCD Axion: Dark Matter and the Strong CP Problem
› Complementary Planetary Spectroscopy Probes of Dark Matter
› A General Model for Dark Energy Crossing the Phantom Divide
› Geometric multipartite entanglement from gravitational particle production
› Attitude Determination and Control of GPS Satellites: Stabilization, Orbital Insertion, and Operational Control Mechanisms
› Revisiting Polynomial Hybrid Inflation: Planck and ACT Compatibility via Radiative Corrections
› Low-Energy Calibration of SuperCDMS HVeV Cryogenic Silicon Calorimeters Using Compton Steps
› Trustworthy scientific inference for inverse problems with generative models
› Lepton parity dark matter and naturally unstable domain walls
› Indication for a compact object next to a LIGO-Virgo binary black hole merger
› Redshift Evolution of the HII Galaxy $L$-$\sigma$ Relation: Gaussian Process Analysis and Cosmological Implications
› Interpreting Multi-band Galaxy Observations with Large Language Model-Based Agents
› How Early Could the Milky Way's Disk Form?
› From UV-bright Galaxies to Early Disks: the Importance of Turbulent Star Formation in the Early Universe
› The Impact of Local Stellar Radiation on Dwarf Galaxy Formation Around Milky Way Analogues Across Cosmic Reionization
› Correlation between Outlying Halo Abundance and Host Halo Properties
› Measurements of the Temperature and E-mode Polarization of the Cosmic Microwave Background from the Full 500-square-degree SPTpol Dataset
› Study of the IC 443 region with the HAWC observatory
› X-ray Spectra from General Relativistic RMHD Simulations of Thin Disks
› The Warm-Hot Disk-Halo Interface Below the Perseus Spiral Arm
› Galactic magnetic fields II. Applying the model to nearby galaxies
› Investigating the metallicity dependence of the mass-loss rate relation of red supergiants
› Neutrino Flavor Transformation in Neutron Star Mergers
› Constraining Axially Symmetric Bianchi Type I Model with Self-Consistent Recombination History and Observables
› Dynamical Dark Energy Implies a Coupled Dark Sector: Insights from DESI DR2 via a Data-Driven Approach
› The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
› The threshold for PBH formation in the type-II region and its analytical estimation
› Constraining the [CII] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
› Damping Wing-Like Features in the Spectra of High Redshift Quasars: a Challenge for Fully-Coupled Simulations
› Magnetic fields in the Eos Cloud: dynamically important fields in the interface between atomic and molecular gas
› Quasar lifetime measurements from extended Ly$\alpha$ nebulae at $z\sim 6$
› An interferometric study of B star multiplicity
› Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
› Rapid stellar and binary population synthesis with COMPAS: methods paper II
› Rotating Supermassive Pop III Stars On The Main Sequence
› HeII emitters in the cosmic noon and beyond. Characterising the HeII {\lambda}1640 emission with MUSE and JWST/NIRSpec
› Spot-Crossing Variations Confirm a Misaligned Orbit for a Planet Transiting an M Dwarf
› Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars
› Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf
› Spectroscopic Analysis of Pictor II: a very low metallicity ultra-faint dwarf galaxy bound to the Large Magellanic Cloud
› Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
› Deep Potential: Recovering the gravitational potential and local pattern speed in the solar neighborhood with GDR3 using normalizing flows
› First Robust Detection of Linear Polarization from Metric Solar Emissions: Challenging Established Paradigms
› From a Different Star: 3I/ATLAS in the context of the \={O}tautahi-Oxford interstellar object population model
› Noema formIng Cluster survEy (NICE): A Census of Star Formation and Cold Gas Properties in Massive protoclusters at 1.5
› All-sky search for short gravitational-wave bursts in the first part of the fourth LIGO-Virgo-KAGRA observing run
› Phase II of the LAMOST-Kepler/K2 Survey. II. Time Domain of Medium-resolution Spectroscopic Observations from 2018 to 2023
› Intercepting 3I/ATLAS at Closest Approach to Jupiter with the Juno spacecraft
› A Comprehensive Study of the Energy and Redshift Distributions of the Fast Radio Burst Population Based on the First CHIME/FRB Catalog
› Prompt identification of solar wind stream interaction regions from Survey Burst 1 Mode observations of the Radio and Plasma Wave experiment on Solar Orbiter
› Composite asymmetric dark matter with a dark photon portal: Multimessenger tests
› Pre-trained Audio Transformer as a Foundational AI Tool for Gravitational Waves
› The Massive Flat Space Limit of Cosmological Correlators
› Gravity as emergent phenomena for spherically symmetric black hole accretion of multi-component flow with relativistic equation of state
› Hunting for heavy $Z^\prime$ with IceCube neutrinos and gravitational waves
› Evolution of precessing binary black holes on eccentric orbits using orbit-averaged evolution equations
› Static horizons in cosmology
› Model-Independent Machine Learning Approach for Nanometric Axial Localization and Tracking
› Inflation Model Based on Virasoro Squeezing
› Connecting the Quenched $g_A$ in Nuclear Matter To Dense Compact-Star Matter
› Generation of Axions and Axion-Like Particles through Mass Parametric Resonance induced by Scalar Perturbations in the Early Universe
› Correlation and Redundancy of Time-Delay Interferometry Configurations

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