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Sunset from the kitchen window
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 News from astronomynow.com
› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
RSS  Latest preprints on astro-ph:
› Detecting Ca II Absorption Lines with a Fe II assisted Dual Neural Network
› Bell Instability and Cosmic-Ray Acceleration in AGN Ultrafast Outflow Shocks
› An Explicit M1 Radiation-hydrodynamics Scheme for Three-dimensional Protostellar Evolution
› Modelling the nebular emission of galaxies across cosmic time with COLT
› Radiation Magnetohydrodynamic Simulation of sub-Eddington Circumbinary Disk in a 10:1 Massive Black Hole Binary
› Strong Evidence for Cosmic Ray-Supported $\sim$L$^{\ast}$ Galaxy Halos via X-ray \& tSZ Constraints
› Simulation budgeting for hybrid effective field theories
› Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning
› Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey. IV. Lens Mass and Distance Measurements
› The ASTRID Simulation at z=0: from Massive Black Holes to Large-scale Structure
› The THESAN-ZOOM project: The Hidden Neighbours of OI Absorbers during Reionization
› The Nephele ecosystem: stars, globular clusters, and stellar streams associated with the progenitor galaxy of $\omega$ Centauri
› Dynamic SBI: Round-free Sequential Simulation-Based Inference with Adaptive Datasets
› Anatomy of the Class I protostar L1489 IRS with NOEMA - II. A disk replenished by a massive streamer
› Conversion and Damping of Non-axisymmetric Internal Gravity Waves in Magnetized Stellar Cores
› Investigating Nonlinear Landau Damping in Hybrid Simulations
› Exploring the impact of electromagnetic dissipation on ultra-relativistic plasma outflows
› Probing Helium Reionization Through the $^{3}\mathrm{He}^{+}$ Hyperfine Transition Line
› NGTS-11 c: a transiting Neptune-mass planet interior to the warm Saturn NGTS-11 b
› Towards field-level likelihood for projected fields: Evolved projected fields from initial projected fields
› Extracting latent representations from X-ray spectra. Classification, regression, and accretion signatures of Chandra sources
› Axisymmetric hydrodynamics in numerical relativity: treating coordinate singularity, artificial heating and modeling MHD instabilities
› A formation mechanism for narrow rings around minor bodies
› The 2025 Failed Outburst of IGR J17091-3624: Spectral Evolution and the Role of Ionized Absorbers
› Probing cosmic velocities with the pairwise kinematic Sunyaev-Zel'dovich signal in DESI Bright Galaxy Sample DR1 and ACT DR6
› Analysis of Planetary Nebulae in the Milky Way: Physical Properties, Chemical Abundances, and Galactic Distributions
› Connecting outflows with radio emission in AGN at Cosmic Noon
› Breaking gyrochronology through the collapse of coronal winds
› Radiation pressure and equation of state are important in the envelope unbinding process in common envelope evolution
› Polarisation Performance of Offset Phase Antennas: A Study for FARSIDE
› Quasi-periodic oscillations in optical color evolutions to support sub-pc binary black hole systems in broad line active galactic nuclei
› Molecular gas content of gravitational-lensed quasars at cosmic noon
› Hierarchical Simulation-Based Inference of Supernova Power Sources and their Physical Properties
› Design and Performance of the SPT-SLIM Receiver Cryostat
› An On-Sky Atmospheric Calibration of SPT-SLIM
› Demonstrating Exoplanet Transit Photometry from Space with a 15-mm Aperture Optical Navigation Camera on Hayabusa2
› Estimation of gravitational wave from solar emerging magnetic flux tube
› Water Snowline in Young Stellar Objects with Various Density Structures Using Radiative Transfer Models
› Combining spectral analysis and narrow band pass filtering to predict solar cycle parameters in the next solar grand minimum
› Is GW231123 a hierarchical merger?
› Dust extinction map of the Galactic plane based on the UKIDSS survey data
› Evidence for the dynamical dark energy with evolving Hubble constant
› Accounting for the absence of anomalous microwave emission in the M 31 halo
› Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
› High-Precision Photometry with a scientific CMOS Camera: I Lab Testing of the Marana camera
› SETI Post-Detection Protocols: Progress Towards a New Version
› New Level Resolved Ground and Excited State Pb III, IV, V & VI Photoionization Cross Sections for Heavy Metal Subdwarf Modeling
› Influence of kinetic effects in large-scale magnetic reconnection with multi-hierarchy simulation code KAMMUY
› The bimodal distribution of donor stars in X-ray binaries
› The variability of active galaxies: I. Broad-band noise X-ray power spectra from XMM-Newton and Swift
› Revisiting electron-capture decay for Galactic cosmic-ray data
› Eclipsing Stellar Flare on the Demon Star Algol Binary System Observed during the MAXI-NICER Follow-up Campaign in 2018
› The multimessenger view of Pulsar Timing Array black holes with the Horizon-AGN simulation
› Performance of the Prototype Station of the IceCube Surface Array Enhancement
› Local Particle Acceleration in an ICME-in-Sheath Structure Observed by Solar Orbiter
› Active galactic nucleus outflows accelerate when they escape the bulge
› Diffusion-Free Dynamics in Rotating Spherical Shell Convection Driven By Internal Heating and Cooling
› Detection of spin-modulated circular polarisation and radial velocity variations in the long period Intermediate Polar 1RXS J080114.6-462324
› Search for exocomets transits in Kepler light curves: Ten new transits identified
› Numerical Studies on the Radio Afterglows in TDE (I): Forward Shock
› Expansion kinematics of young clusters. II. NGC 2264 N & S and Collinder 95 with HectoSpec
› Mergers lighting the early Universe: enhanced star formation, AGN triggering, and Ly$\alpha$ emission in close pairs at $z=3-9$
› QFP Waves Driven by the Tuning-Fork Effect during Magnetic Reconnecion
› The Hidden Story of Chemical Evolution in Local Star-Forming Nuclear Rings
› Predicting the Subhalo Mass Functions in Simulations from Galaxy Images
› CHILLING: Continuum Halos in LVHIS Local Irregular Nearby Galaxies - Radio continuum spectral behavior of dwarf galaxies
› Evaluating Habitability and Biosignature Detection on TOI-700 d: The Role of UV Environment and Atmospheric Pressure
› The dark side of early galaxies: $\texttt{geko}$ uncovers dark-matter fractions at $z\sim4-6$
› Stellar population astrophysics (SPA) with the TNG. The Phosphorus abundance on the young side of MilkyWay
› A new photometric ephemeris for the 2M1510 AB double brown dwarf eclipsing binary system
› The Nearby Evolved Stars Survey III: First data release of JCMT CO-line observations
› Exploring a cosmic ray inverse-Compton origin to the SZ-to-X-ray pressure deficit in the cool core cluster ZwCl 3146
› The Launching of Galactic Winds from a Multiphase ISM
› Antarctic Infrared Binocular Telescope. I. System Overview, Laboratory Testing, and On-Sky Performance Evaluation
› General-relativistic radiation magnetohydrodynamics simulations of binary neutron star mergers: The influence of spin on the multi-messenger picture
› Deuterated water ice on the satellites of Saturn
› AREPO-RSG: Aspherical Circumstellar Material and Winds from Pulsating Dusty Red Supergiants in Global 3D Radiation Hydrodynamic Simulations
› Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study
› Multi-wavelength analysis of the progenitor of GRB 230307A via Bayesian model comparison
› Modeling nonlinear scales for dynamical dark energy cosmologies with COLA
› Fermi Bubbles Without AGN: Gamma-Ray Bubbles in MHD Galaxy Formation Simulations with Full Cosmic Ray Spectra
› StarStream on Gaia: Stream discovery and mass loss rate of globular clusters
› NIRPS and TESS reveal a peculiar system around the M dwarf TOI-756: A transiting sub-Neptune and a cold eccentric giant
› StarStream: Automatic detection algorithm for stellar streams
› X-ray panorama of the SS433/W50 complex by SRG/eROSITA
› Non-Minimally Coupled Quintessence in Light of DESI
› Dark Matter Subhalos and Higher Order Catastrophes in Gravitational Wave Lensing
› Phantom Mirage from Axion Dark Energy
› Cross-correlation of Luminous Red Galaxies with ML-selected AGN in HSC-SSP III: HOD Parameters for Type I and Type II Quasars
› Probing Quadratically Coupled Ultralight Dark Matter with Pulsar Timing Arrays
› Large Neutrino "Collider"
› The quasinormal mode content of binary black hole ringdown
› No cosmological constraints on dark photon dark matter from resonant conversion: Impact of nonlinear plasma dynamics
› Resonant Loop Interferometers for High-Frequency Gravitational Waves
› MHDuet : a high-order General Relativistic Radiation MHD code for CPU and GPU architectures
› Quantum Damping of Cosmological Shear: A New Prediction from Loop Quantum Cosmologies
› Glitch noise classification in KAGRA O3GK observing data using unsupervised machine learning
› Recursive Target Body Approach for Low-Thrust Multiple Gravity-Assist Sequence Optimization
› A unified model of dark energy and inflation from the Markov-Mukhanov action
› The Stochastic Schwinger Effect
› ALP couplings to muons and electrons: a comprehensive analysis of supernova bounds
› Linear damping of magneto-acoustic waves in two-fluid partially ionized plasmas
› Toward a unified view of agnostic parametrizations for deformed black holes
› The predictive power of the calculated line lists of carbon monoxide
› Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies
› Learned harmonic mean estimation of the Bayesian evidence with normalizing flows
› Profiling stellar environments of gravitational wave sources
› Asking Fast Radio Bursts for More than Reionization History
› Exomoons of Circumbinary Planets
› Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
› Effects of Galaxy Cluster Structure on Lensed Gravitational Waves
› Do tides play a role in the determination of the pre-stellar core mass function?
› Disturbed cold gas in galaxy and structure formation
› Where are the Population III star relics in the simulated Milky Way analogues?
› Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations
› A Neural Symbolic Model for Space Physics
› Multi-copy Axion Transfer Function and Observational Implications of Effective de Broglie Scales
› X-ray Polarimetry in the Low Statistics Regime using the Bayesian Approach Reveals Polarization Angle Variations
› Cosmology Constraints from Type Ia Supernova Simulations of the Nancy Grace Roman Space Telescope Strategy Recommended by the High Latitude Time Domain Survey Definition Committee
› Detecting wide binaries using machine learning algorithms
› Stellar-gas kinematic misalignments in EAGLE: enhanced SMBH growth in misaligned galaxies
› Many-Body Simulations of the Fast Flavor Instability
› A Systematic Search for Spectral Hardening in Blazar Flares with the Fermi-Large Area Telescope
› Insights for Early Massive Black Hole Growth from JWST Detection of the [Ne v] {\lambda}3427 Emission Line
› Does DESI DR2 challenge $\Lambda$CDM paradigm ?
› The X-ray$-$UV Luminosity Relation of eROSITA Quasars
› LAP1-B is the First Observed System Consistent with Theoretical Predictions for Population III Stars
› NGC 2392 and NGC 4361: Spectroscopic Diagnostics of Planetary Nebula Evolution
› A Panchromatic View of Late-time Shock Power in the Type II Supernova 2023ixf
› Role of symmetry energy at subnuclear densities in protoneutron star crusts
› Galaxy-halo internal alignments across cosmic time
› Attributing the supernova remnant RCW 89 to the jittering jets explosion mechanism
› Quantifying the Effects of Parameters in Widespread SEP Events with EPREM
› Excursion Set Approach to Primordial Black Holes: Cloud-in-Cloud and Mass Function Revisited
› Inferring Stellar Densities with Flexible Models I: The Distribution of RR Lyrae in the Milky Way with $\textit{Gaia}$ DR3
› CHILES X: Molecular and atomic gas at intermediate redshift
› A revision of the lifetime of submoons: tidal dynamics with the Euler-Lagrange equation
› On The Orbital Evolution of Multiple Wide Super-Jupiters: How Disk Migration and Dispersal Shape the Stability of The PDS 70 System
› Using gravitational lensing to probe for bright quintessential galaxies in the Epoch of Reionization
› Tycho supernova exploded inside a planetary nebula (SNIP)
› Diffusion models for polarimetric reconstruction of circumstellar environments
› Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A & EP250207b
› The Dependency of Bar Formation Timescale on Disk Mass Fraction, Toomre $Q$, and Scale Height
› Dynamics and Observational Signatures of Core-Collapse Supernovae with Central Engines: Hydrodynamics Simulations with Monte Carlo Post-Processing
› Flavor solitons in dense neutrino gases
› From kinetic gases to an exponentially expanding universe - The Finsler-Friedmann equation
› Prospects of detecting cosmic ray up-scattered dark matter with DUNE
› Cosmological scalar perturbations for a metric reconstructed from group field theory
› Impact of $\Xi$-Hypernuclear Constraints on Relativistic Equation of State and Properties of Hyperon Stars
› Running scalar spectral index in warm natural inflation
› Higher-order gravity models: corrections up to cubic curvature invariants and inflation
› Quantum Computing Tools for Fast Detection of Gravitational Waves in the Context of LISA Space Mission
› Asymptotic Schwarzschild solutions in $f(R)$ gravity and their observable effects on the photon sphere of black holes

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