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 News from astronomynow.com

› 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
› How to see the 3 March total lunar eclipse
RSS  Latest preprints on astro-ph:

› Understanding constraints on primordial mass black holes made of dark matter using fast radio bursts
› Single Frequency CMB Foreground Removal with Inter-scale Machine Learning
› Searching for Population III stars with line intensity mapping cross-correlations
› Peering through the dip: IXPE unveils the extended scattering environment of GX 13+1
› Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry
› Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
› A New Sirius-like System at Only 21 Parsecs: An Elusive White Dwarf Companion to the Nearby K-dwarf HD 38230
› Deep Learning-Based Classification and Analysis of Pulsar Candidates in Fermi-LAT Unassociated Sources
› A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations
› End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer
› The s-process at Subsolar Metallicity: Insights from High-Resolution Infrared Spectroscopy of Magellanic Cloud Planetary Nebulae
› Quiescent Host Galaxies of Extended Quasars Revealed by Spectrophotometric Decomposition
› Changing-Look AGNs from DESI. VI. Host Galaxies
› Cataclysmic variables from Gaia XP spectra: The Gaia emission-line magnitude (GEM) diagram
› Fishing for Jellyfish Galaxies: Exploring ram-pressure stripping with crowd science
› Averaging Effects on the Solar Wind Alfven Mach Number: Implications for Switchbacks and Alfven Transition
› Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization
› Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation
› SDSS-V Local Volume Mapper (LVM): The Integrated Light and Internal Rotation of Omega Centauri
› Multi-sensor fusion for fine-guidance and milliarcsecond-level attitude estimation of balloon-borne telescope
› LUVCam: A high-performance, low-cost, UV/optical camera for the future of astronomy in space
› EWOCS-VIII: Internal kinematics and expansion of Westerlund 1 from VVVX proper motions
› Optical and acoustic ground effects simulations from terminal defense asteroid disruption via the PI method
› Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613
› Quasi-Keplerian Be-Star Disks with Mimicking Viscosity
› Determining Total Infrared Luminosities from Submm Measurements of High Redshift Galaxies
› On-sky results from REDWOODS, a platform at Lick/ShaneAO for testing second stage AO technologies
› A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal
› Strongly Magnetized Super-Eddington Accretion: How Spin and Accretion Rate Regulate Energy Output and Mass Loss
› A New Approach to Modeling Line Shapes with Quasi-H$_2^+$ Satellites in Stellar Atmospheres
› Asymmetric, variable H$\alpha$ line profile in planetary mass object SR 12 c
› Gravitational waves from oscillons in a generalized exponential plateau potential
› The Open Cluster Chemical Abundances and Mapping Survey XI. First Gradients from SDSS/MWM BOSS Determined Clusters
› A Physically Driven Parameterisation of Multidimensional Atmospheres: Application to the JWST Phase Curve of WASP-121b
› Reincarnations of massive stars in active galactic nucleus discs
› Direct shear $\times$ kSZ correlation: controlling baryons without modeling galaxies
› HARMONI at ELT: Developing a Modular Review Process using TRIZ
› Optical Images of the Braneworld Black Hole Surrounded by an Optically Thin Accretion Disk
› Polar cap plasma loading and the morphology of pulsar $\gamma$-ray light curves
› Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks
› Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations
› Joint X-ray and gamma-ray analysis at the photon level: Application to MSH 15-52
› A Quantitative Framework for Testing the Hubble Tension in a Bianchi Type I Cosmological Background
› Pulsations along the Asymptotic Giant Branch (AGB): a global view
› The CUSP CubeSat mission for space weather multi-physics analysis, design, and testing
› Spectral densification and macroscopic phase delay of gravitational echoes from exotic compact objects
› Turbulent Convection: Modal Equations and Energy Pathways
› Liquid nitrogen pre-cooling system for ELT instruments utilizing additively manufactured heat exchangers, integrated temperature and liquid level control
› The Radial Acceleration Relation in Galaxies and Clusters from a Two-Component, Virial-Motivated Framework
› Spectroscopic investigation of the southern late-K/early-M dwarf binary CC Eri
› Spectroscopy of flares on AU Mic
› Maximising the mid-infrared high-contrast performance of ELT/METIS despite water vapour seeing
› Information limits of photonic lantern wavefront sensing: a Fisher- and quantum-Fisher-information framework and its relation to Fourier-filtering sensitivity limits
› Gas Phase Ion Species Released During Grain Collisions: Implications For Protoplanetary Disks
› Recovering pattern speeds of simulated face-on barred galaxies via Schwarzschild modelling
› Planck Constraints on Turbulence in the Coma Cluster
› Visual analytics for cosmological simulation results
› Persistence characteristics of H4RG-15 detectors for ESO instruments
› CatBoost versus Spectral Energy Distribution-Fitting: Estimating Galaxy Properties under Controlled Photometric Incompleteness
› Charge migration characterization in the METIS H2RG detectors
› Rates of tidal disruption events from constrained cosmological simulations of the local Universe: population properties and implications for transient surveys
› The Fe I 4377 {\AA} Line as a Solar Faculae Indicator: Insights from Spectral Ratio Analysis
› Twin Impact Lunar Telescope network: Lunar Impact Flash observations of the 2025 Geminids
› Gamma-ray emission from particle illumination and shock-cloud interaction in the W51 Complex
› Spectroscopic Analysis of the 2025 Eclipse of the Symbiotic Binary V1413 Aquilae
› ROLLIN': Rotating globular cluster simulations II. The complex morphology of globular clusters driven by multi-scale dynamics
› The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Molecular gas properties
› Towards Autodifferentiable Point Spread Function Modelling for the VLT/ERIS Vortex Coronagraph
› Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned
› Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension
› The Tartu Observatory Fiber-fed Echelle Spectrograph (TOFES) Data Reduction Pipeline
› Asteroseismic models of the magnetic binary HD 156424
› A Massive Galaxy at the Edge of Feedback-Free Efficiency
› On the use of field RR Lyrae as Galactic probes:. IX. Radial velocities
› Critical Sizes of Satellite Constellations
› The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants
› An optimal quadratic estimator for window-free cosmic shear power spectra
› Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction
› Signatures of kinetic gravity braiding in cosmological probes of the gravitational field
› Natural Phantom Crossing from Axion-WIMP Interactions
› Molecular clouds constraints on sub-GeV DM and asteroid-mass PBHs
› Dark Photon Dark Matter from Quantum Fluctuations during Starobinsky Inflation
› Rare processes in ultrahigh-energy tau-lepton transport
› Deviation of trajectories in nonrelativistic and relativistic cases and Shirokov effect
› Halbach Magnetic Weber Bars
› The price for monopole dark matter
› Inflation and Reheating by Dynamical Torsion
› Dark Photons from Perturbative Decay of a Misaligned Higgs Field
› Lensing in the McVittie metric
› Evolution of Stars and Gas in Galaxies
› Evaluating Short-Warning Mitigation via Intentional Robust Disruption of a Hypothetical Impact of Asteroid 2023 NT1
› Planet Formation at Cosmic Dawn: Planetesimals in H$_2$O-Rich Disks Around Low-Mass Stars
› A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
› High-redshift transverse BAO measurements with the SDSS quasar catalog
› Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA
› On the bin sensitivity of the transverse BAO
› Across the Universe: GW231123 as a magnified and diffracted black hole merger
› Long-term monitoring of repeating FRB 20220912A with the uGMRT at low radio frequencies
› Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
› A New Constraint on the Optical Depth from the Reionization History Independent of CMB Large-Scale E-Mode Polarization
› Euclid: Early Release Observations -- The extended stellar component of the IC10 dwarf galaxy
› PyISH: Python Integral Field Spectroscopy Simulation for HWO
› Small scale turbulence alongside with large scale turbulence in a z=1.87 star Forming Galaxy with outflowing wind, revealed by Multi-point structure functions
› Replicating weak-lensing summary-statistic covariances with normalizing flows
› Contrastive learning of extragalactic stellar streams. Sculpting a latent space of representations with DES DR2 photometry
› Fuzzy Dark Matter and the Impact of Core--Halo Diversity on Its Particle Mass Constraints
› A quasi-star is born: formation and evolution of accreting quasi-stars as a pathway to Little Red Dots at non-zero metallicity
› Radiative Feedback in Population III Protostellar Growth: HI Shielding \& HII Region Trapping
› Multiquark clustering in neutron-star matter from color-spin molecular dynamics
› XRF 241001A/SN 2024aiiq: A faint soft X-ray transient detected by SVOM with a broad-line type Ic supernova revealed by JWST
› Joint State-and-Dynamics Inference for Galaxy Population Evolution on an Effective Manifold
› Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
› Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems
› The Amplitude-Growth Degeneracy and Implied $A_s$ Diagnostic for Background-Inert Modified Gravity
› From reflection to scattering: Polarimetric signatures of funnel-type outflows. Modeling obscured ultraluminous X-ray sources
› A new Chandra look at the globular cluster NGC 6540 and its peculiar X-ray flaring source
› Faraday Complexity and Depolarisation in a High-Rotation-Measure Radio Galaxy from the Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) DR2
› Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints
› Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations
› PSRDISP: A novel approach to modeling dispersive processes in single-pulsar noise analysis using epoch-wise dispersion measures
› Investigating anomalous microwave emission near G107.2+5.20 in Ku-band with the Green Bank Telescope
› Features in the visible spectra of the Enceladus particle plume and E ring: Potential evidence of organic materials and/or missing sub-micron particles
› Impact of eccentricity and higher-modes on neutron star-black hole parameter estimation
› Volcanic Satellites and Ion Escape in the Magnetospheres of Ultra-Cool and Brown Dwarf Stars
› DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints
› Comparative Periodogram Analysis of 22 Years of Super-Kamiokande Solar $^{8}\mathrm{B}$ Neutrino Data: Classical, Phase-Based, and Information Theoretic Methods
› A no-go theorem in bumblebee vector-tensor cosmology
› Light Dark Matter Search with 7.8 Tonne-Year of Ionization-Only Data in XENONnT
› Dark Photon mediated Inelastic Dark Matter in Cosmology, Astrophysics and Colliders
› Inside the Black Box of Big Bang Nucleosynthesis: A Comprehensive Sensitivity Atlas for the Precision Era
› UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
› Phase Transitions and Gravitational Waves
› Observational signatures of negative mass wormholes through their shadows
› Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries
› Cooling of Hybrid Stars with a 2SC+$$ Phase
› Overcoming the low signal-to-noise problem for hybrid mode-selective photonic lantern-based wavefront correction using machine learning
› Leptogenesis with sub-electroweak-scale reheating temperature
› A High-Precision Numerical Framework for Time-Varying Solar Neutrino Flux with Full Earth Matter Oscillation Corrections for Global Underground Laboratories

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