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 News from astronomynow.com

› 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
› Diamond downpours in the outer Solar System
› The Moon’s February world tour
RSS  Latest preprints on astro-ph:

› PyCBC Live Search for Compact Binary Mergers in Advanced LIGO and Virgo's Fourth Observing Run
› The X-ray-to-UV relation does not evolve in homogeneous quasar samples
› The Effects of Cosmic Ray Protons on Galactic Nonthermal Filaments
› Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\alpha$ Surface Brightness Ratio
› CMBolic: Symbolic emulators for the Cosmic Microwave Background. I. Lensing
› Euclid Quick Data Release (Q1): The impact of AGN emission on SED-derived physical properties
› A Colour-colour Fingerprint Links the UV Upturn in Early-type Galaxies to Second-generation Stars from Dissolved Globular Clusters
› MORFEO wavefront error budget
› SynIM: a high-performance GPU-accelerated Python library for synthetic interaction and tomographic reconstruction matrices in next-generation adaptive optics
› Towards Instrument-Agnostic Exoplanet Candidate Prioritization
› Beyond Point Estimates: Benchmarking Uncertainty Quantification Methods on the AION-1 Astronomical Foundation Model
› Do Vision-Language Models See Dwarf Galaxies the Way We Do?
› Extending asteroseismic magnetometry across the diverse landscape of magnetic structures
› Dynamic Range Beyond Bit Depth of a CMOS Image Sensor Using Interleaved Row Readout
› Measurements of the Angular Homogeneity Scale from DESI DR1
› Faraday Complexity and Depolarisation in a High-Rotation-Measure Radio Galaxy from the Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) DR2
› Effective Bayesian ranking of low order monomial potentials in low temperature warm inflation
› Modern Time-Series and Spectral Methods for Analyzing Solar and Stellar Oscillatory Signals
› Sunrise III: Instrument, mission, data, and first results
› Isolated neutron star candidates from the fourth generation XMM-Newton catalogues
› Detector Development for HUBS I: Initial Testing of Small-Area TES Microcalorimeters
› XRISM Observations of Abell 1795: Evidence for Low Turbulence and Resonant Scattering
› Population synthesis of Galactic middle-aged pulsar wind nebulae II. Observational signatures of superefficiency
› Single-dish observations and non-LTE analysis of CH3OH, HCN, and CO line emission in the Oort cloud comet C/2017 K2 (PANSTARRS)
› Fast Astronomical Transients in Archival Photographic Plates: Using optical aberrations as a tool for discerning real images, from plate artifacts
› Old pulsar wind nebulae and the role of the thermal filaments
› Reconciling large-scale Lyman-$\alpha$ correlations with the SCRIPT Semi-numerical Model
› Dust to Dust: Prospects for Passive Technosignatures as Relics of ETI
› $\delta$-CDM: A Minimal Deformation of $\Lambda$CDM with Scalar Field Reconstruction
› Virial-based extraction of structures in numerical simulations: The vibes tool
› Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra
› Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints
› Bayesian Reconstruction of the Local Universe from 2MRS: Testing the Gravitational Flow with Cosmicflows-4
› Discovery of a Candidate 2 keV Cyclotron Resonance Scattering Feature in the HLX NGC 3583 X-1
› ALMA High-resolution Observation of the HH46/47 Outflow/disk/envelope System
› Thermal emission from dark matter-heated neutron stars in the Galactic Center
› Reconstructing Synthetic SDO/AIA 193 A EUV Images from He I 10830 A Observations with Diffusion Model Translator
› On The Nature of Einstein Probe Transient EP250916a: Insights from X-ray, Optical, and Radio Observations
› Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context
› From filaments to clumps: filament properties with synthetic Herschel observations
› JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe
› A Framework to Model Stellar Irradiated Disks with Frequency-dependent Absorption and Scattering Opacities in Athena++
› Disk reflection as the origin of the X-ray polarization of NGC 4151 with IXPE
› Mock Catalogs of Strongly Lensed Gravitational Waves via a Halo Model Approach with Space-borne Detectors
› Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes
› Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission
› Rapid intermediate-mass black hole formation via runaway mergers of black holes
› Precise scaling relations for self-interacting bosonic dark matter stars
› The complex kinematics of the young stars orbiting the supermassive black hole in the Galactic center can be explained by the presence of an intermediate mass companion of Sgr A$^\star$
› The origin of WHAM Point Source~46
› Parameter Effects in Circumplanetary Disk Spectra and Prospects for Spectral Fitting
› Statistical Estimation and Correction of Model-Measurement Bias in Time-Dependent Correction Factors of KAGRA
› CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision
› On the Nonlinear Dependence of Underground Muon Rate on Atmospheric Temperature Observed at Daya Bay
› Ages and ZAMS spin distribution of stars in detached eclipsing binaries
› Optimising ultra-light dark matter searches with ground-based interferometers
› Predictability of a solar flare in May 2024 using observational data-driven MHD simulations
› GRB 250706B/C: Insight-HXMT Discovery of a High-Luminosity Burst as a Candidate for Fallback-Regulated Accretion in the Prompt Emission
› Bayesian analysis of the shear modulus in the neutron-star crust
› A consistency check for the calibration of 5303{\AA} solar coronal emission line observations with Aditya-L1/VELC
› Disentangling chemical evolution histories with phylogenetic trees
› A Unified Ionization Framework for the Spectroscopic Diversity of Tidal Disruption Events
› TYC 170-1218-1: A new r-process-enhanced extremely metal-poor star, rich in Th
› Towards a consistent framework of determining active galactic nucleus contribution fraction and host galaxy properties
› Fast Radio Bursts produced during collapse of macroscopic X-mode in magnetized pair plasma
› Class I CH3OH Maser Emission from Bar-Driven Inflow Colliding with the Central Molecular Zone
› Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values
› Eccentricity as a probe of mass-transfer physics. Eccentric mass transfer as a solution to the wide eccentric binary problem
› MRI-triggered instability at the inner dead zone edge: disc evolution and burst modes tied to magnetic field strengths
› Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars
› Spectral distortion anisotropies from photon to dark photon conversions
› Control problem in millimeter-wave adaptive optics
› Apparent Transverse Motion of Light Bridges Coupled to Coronal Loop Dynamics
› Characterizing Stellar Streams with Error-Aware Machine Learning
› A thousand looks at X Persei: X-ray spectroscopy at high time resolution
› Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays
› Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as reveled by their stellar populations
› Measuring the radii of merging neutron stars with asteroseismology
› Peristaltic Flow in Compressible, Ideal Magnetohydrodynamics: A Mechanism For Solar Spicules
› Balmer decrements as a new diagnostic for period-bounce Cataclysmic Variable stars
› A differentiable forward model for weakly perturbed stellar streams: substructure forecasts from density and kinematics spectra
› Pantheon+ supernovae corrected for progenitor age indicate the universe is decelerating
› Star Formation Drives Production of Low Energy Cosmic Rays
› A Meta-Learning Framework for Multitask Reverberation Mapping in Active Galactic Nuclei
› Stochastic constant-roll inflation beyond the hilltop with the spectral method
› NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample
› A Scaling Relation of LRDs between Broad H$\alpha$ and Bolometric Luminosities: Enhanced Broad H$\alpha$ Emission Relative to Low-$z$ Type 1 AGN
› Mapping Interstellar Ice Inventory toward Class 0 Protostars in Star-forming Region Orion A with JWST Data
› Universal Suppression of Gravitational Waves from Black Hole Evaporation Dynamics
› Inflationary interpretation of the gravitational-wave signal in the European Pulsar Timing Array DR2 with constraints
› ALMA measurements of mass loss and wind clumping in the massive stars of the Arches cluster
› Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation
› Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au
› On an Airborne Proton Accelerator for Enhancing Cloud Formation or Inducing their Precipitation
› A Landscape of Cosmological Decoherence
› NICER Constraints on Low density Interpolation and High density Continuation in Neutron Star Equations of State
› Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling
› Hybrid simulations of the proton beam instabilities in the young solar wind. The formation of hammerhead-like distributions
› Does Eternal Inflation Violate the Smeared Null Energy Condition?
› A New Route to the Annihilation of Multi-Wall String Topological Configurations
› Stimulated Emission from Boson Clouds
› On the effect of higher order symmetry energy corrections in Skyrme models for neutron star matter
› Fire at the Tip of the Throat: Hagedorn Phase after brane-antibrane inflation?
› Classifying galaxies in the Galaxy10 DECals dataset using Inception and Residual CNNs
› Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity
› A Polarization-Decomposed Method for Simulating Inhomogeneous Birefringence in Laser-Interferometric Gravitational-Wave Detectors
› Semi-supervised Source Detection in Astronomical Images: New Benchmark and Strong Baseline
› Detectability to extreme mass ratio inspirals with alternative space-based detector networks
› Satellite gravity constraints on inner core viscosity and LLVPs density anomalies
› High-Efficiency Broadband Mid-Infrared Absorption in Asymmetrically Matched Metallic Meanders: Development of Ti40V60 Alloy based LEKIDs for Mid-Far IR
› Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach
› PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference
› A Numerical Experiment on Oscillatory Magnetic Reconnection in a Laboratory Plasma System Driven by Alternating Currents
› The integral and correlation scales of solar wind turbulence
› Neutron stars in Poincar\'e gauge gravity with quadratic torsion
› Linear Ricci-Trace Deformations and Operational Equivalence in Rastall-Type Gravity
› A stellar dynamical mass measurement of an inactive black hole at redshift 2
› To CPL, or not to CPL? What we have not learned about the dark energy equation of state
› Probing gravity with non-linear clustering in redshift space
› Gravitational Lenses in UNIONS and Euclid (GLUE) I: A Search for Strong Gravitational Lenses in UNIONS with Subaru, CFHT, and Pan-STARRS Data
› Robustness of pairwise kinematic Sunyaev-Zel'dovich effect to optical-cluster-selection bias
› The 2MIG isolated AGNs -- 2. X-ray general properties and peculiarities
› Non-Gaussian Expansion of Minkowski Tensors in Redshift Space
› X-ray polarization of reflected thermal emission
› Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS
› Dark Matter and the Early Formation of Supermassive Black Holes
› Les Houches on Dark Universe 2025: Elements of cosmology beyond FLRW
› Probing initial isocurvature perturbation with 21cm one-point statistics
› Aligned hierarchical black hole mergers in active-galactic-nuclei disks revealed by GWTC-4
› The Colors of Ices: Measuring ice column density through photometry
› Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback
› The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
› The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- II. Were Splash stars heated or already born hot?
› Positive AGN Feedback Enhances Star Formation in Starburst Dwarf Galaxies
› CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
› Searching for Electromagnetic Counterpart Candidates to GW231123
› Detection of Multiband Lensed Gravitational Waves from Dark Matter Halos with Deep Learning
› Ultra-extreme high-frequency-peaked BL Lacs: A potential population of MeV synchrotron blazars
› Where Galaxies Point: First Measurement of the Large-Scale Axial Intrinsic Alignment
› Impact of Cosmic Ray Distribution on the Growth and Saturation of Bell Instability
› Wavelet-Scattering Signatures of Fuzzy Dark Matter in Simulated 21 cm Brightness-Temperature Maps
› NICER Perspective on TeV Blazar Mrk~421: X-ray Variability and Particle Acceleration
› National Mapping and Testing of Astronomical Sites in Ethiopia (NMTASE)
› Bayesian Smooth-Fit Extrapolation of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Astrophysical $S$ Factor
› The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
› Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample
› Assessing systematic uncertainties from spectral re-analysis of Cyg X-1 with different coronal geometries
› Widespread Extended [CII] Emission in High-Redshift Galaxies: Insights from the FIRE-2 Cosmological Zoom-in Simulations
› Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
› MeV absorption in gamma-ray bursts as a probe of their progenitor environments
› Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
› Dynamical Systematics for Time Delay Lenses and the Impact on the Hubble Constant
› A simple mechanism for the enhancement of the inflationary power spectrum
› Cosmo3DFlow: Wavelet Flow Matching for Spatial-to-Spectral Compression in Reconstructing the Early Universe
› Cosmological Simulation with Population III Stellar Feedback and Metal Enrichment I: Model Description And Convergence Test
› The spectral state transition of Mkn 590, a potential link between AGNs and X-ray binaries?
› ATLAS100 -- I. A volume-limited sample of supernovae and related transients within 100 Mpc
› Neutrino mass limits and decaying dark matter: background evolution versus perturbations
› Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation
› The In Situ Growth of Stellar-mass "Light" Seed Black Holes in Nuclear Star Clusters
› Sensitivity to Axion-like Particle dark matter with very-high-energy gamma-ray observations of Active Galactic Nuclei located behind Galaxy Clusters
› Bayesian analysis of $\alpha$-Starobinsky model with Planck, ACT and DESI data
› Data-driven discovery of dynamo cycle equations
› Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics
› A Salpeter-like filament linear density function across nearby molecular clouds
› Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway
› Stellar nucleosynthesis in the era of large surveys: s-process polluted binaries in GALAH DR4
› Forecasts of CMB $E$-mode anomalies for AliCPT-1
› Diversity in Evolutionary Status and Magnetic Activity among Solar-Type Twin Detached Eclipsing Binaries
› Strong Gravitational Lensing with the James Webb Space Telescope
› From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
› Solar Vortices: Catalysts of Magnetoacoustic Wave Dissipation and Atmospheric Heating
› The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars
› Cosmological constraints from neighbor-density-weighted marked correlation functions
› Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
› The Persistent Missing Mass Problem in Planet Formation
› From Images to Orbits: A Hubble 2030s Astrometric Legacy for the M31-M33 Star Cluster Systems
› Choosing the right MCMC sampler: a systematic benchmark of gradient-free methods
› Eigenvalue formulation of Stochastic Inflation and application to large perturbation generating inflationary features
› Some Thoughts on the Future of Technosignature Searches: Constraining the Fermi Paradox
› One Transit Is All You Need: Detecting Exoplanets Through Learned Stellar Behaviour with EXOVEIL
› Possible explanation of primordial $^7$Li deficit
› A Model Selection Criterion for Multidimensional Gaussian Processes: Application to Radial Velocities
› Joint Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 Using Profile Likelihood with Gaussian Copula Correlation
› Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer
› EPISODE II: Variability in the CO and H$_2$O rovibrational absorption lines in a periodically variable protostar EC 53
› Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing
› The Universe Observed with Particle Detectors: Astrophysical Legacy of Guido Barbiellini Amidei
› Phenomenology of bubble size distributions in a first-order phase transition
› Bayesian Deep Gaussian Processes for Correlated Functional Data: A Case Study in Cosmological Matter Power Spectra
› Influence of Rotation on Fingering Convection in Planetary Cores
› Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers
› Revisited apparent horizon entropy and GSL in modified gravity
› Dark Dimension Right-handed Neutrinos Confronted with Long-Baseline Oscillation Experiments
› Sterile Neutrino Dark Matter as a Probe of Inflationary Reheating
› DC response of an interferometer topology with an L-shaped cavity: a tabletop study
› High-bandwidth frequency domain multiplexed readout of transition-edge sensors for neutrinoless double beta decay searches
› UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
› Big Bang revisited
› X-ray Response of the Fully-Depleted, p-Channel SiSeRO-CCD
› Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity
› Irreducible Gravitational Wave Background as a Particle Detector
› Rotation-Induced Effective Anisotropy in White Dwarfs as a Newtonian Benchmark with Relativistic Scale Assessment

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