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 News from astronomynow.com

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› Dr Allan Chapman (1946-2026)
RSS  Latest preprints on astro-ph:

› Uniform Reinterpretation of Rocky Exoplanet Secondary Eclipse Observations and the Impact of Stellar and Orbital Uncertainties
› The CARMENES search for exoplanets around M dwarfs. A homogeneous catalogue of projected rotational velocities accounting for limb-darkening
› GRMHD accretion beyond the black hole paradigm: Light from within the shadow
› PySCo-EFT and ECOSMOG-EFT: a tandem of N-body simulation codes for the Effective Field Theory of Dark Energy
› Surveying the Whirlpool at Arcseconds with NOEMA (SWAN). IV. Extent of active galactic nucleus feedback on the interstellar medium
› Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys
› Detectability of Gravitationally Lensed Kilonovae in the Rubin LSST
› Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP
› Refined Constraints on the Hard X-ray Polarization of the Crab Pulsar and Nebula Derived from an Extended XL-Calibur Dataset
› The Effect of External Photoevaporation on the Disk Fraction in M17
› Sequential and non-sequential Zemax Dynamic Link Libraries for generating image slicer integral field units
› On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons
› ExoNet: Multimodal Deep Learning for TESS Exoplanet Candidate Identification via Phase-Folded Light Curves, Stellar Parameters, and Multi-Head Attention Fusion
› The ubiquity of turbulence in the expanding kinematics of the ionized shells of Galactic planetary nebulae
› The Impact of the Bar on Dense Gas and Star Formation in M83
› Distances to molecular clouds in the Galactic longitude l=10-20 deg from the MWISP 12CO 1-0 survey
› Circular polarization images of Sgr A* for different magnetic field geometries
› Radiation-driven stellar winds at the fast-slow transition: new hydrodynamic solutions
› A New Cloud-Cloud Collision Source N68 toward the G35 Molecular Cloud Complex
› A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems
› Inverting Fisher biases for fast systematics exploration
› Induced Scattering of Strong Waves in Pair Plasmas
› Asteroid modelling by starlight diffraction: The shape of Dimorphos, the satellite of (65803) Didymos
› A gem system with a lava world and a habitable zone sub-Neptune orbiting TOI-1752
› Benchmarking Two Chemical Networks used in General Circulation Models of Hot Jupiters
› PISP: Projected-Space Inference of Stellar Parameters
› Beyond the mass-radius plane: Integrated radiative-convective and interior structure simulations of the exoplanet continuum
› The Reaction between Atomic Carbon and Molecular Nitrogen as a Source of Cyanamide and Carbodiimide on Interstellar Ices
› Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs
› Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries
› Missing pairs in open cluster catalogs
› Relativistic time scales in the Solar system
› Binary and neutron star evolution in low-mass X-ray binaries on the evolutionary tracks of accreting millisecond X-ray pulsars
› Kinematically cold and warm planetary nebulae samples, HII regions and supernovae remnants in the disc of the face-on spiral galaxy NGC 628 (M74) -- The Planetary Nebulae Spectrograph with the H$\alpha$ arm
› Machine learning isotope shifts in molecular energy levels
› JWST and Keck observations of the off-nuclear tidal disruption event TDE 2025abcr: An evolving reprocessing layer
› Towards a Robust Estimate of the Solar Photospheric Poynting Flux and Helicity Flux
› The 0.9 Megasecond XRISM/Resolve Spectrum of the Seyfert-1 AGN NGC 4151
› Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO
› A ready-to-fit inhomogeneous cosmological model: the axially symmetric Szekeres spacetime
› Magnetic switchback formation: a review of proposed mechanisms
› Extending Galactic foreground emission with neural networks
› On the relationship between the ellipticity of Galactic globular clusters and their X-ray luminosity
› Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>4
› Solar Cycle Prediction: Challenges, Progress, and Future Perspectives
› Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
› High-Frequency Gravitational Waves from the Galactic Pulsar Population
› FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis
› A XRISM Study of Highly Ionized Iron Emission Lines from the Low-Eddington-ratio AGN in NGC 7213
› Degradation mechanisms and efficiency of heavily cratered regions on Ceres
› Relative frequencies of core-collapse supernovae as a function of metallicity: observations vs theoretical predictions
› Prebiotic Chemistry Insights for Dragonfly II: Thermodynamic Favorability of Nucleobases, Ribose, and Fatty Acids in Selk Crater on Titan
› Challenge in Arrokoth's single merger to achieve the shape's principal axis configuration
› The DESIRED strong-line calibrations: I. New empirical metallicity relations for the local and high-redshift universe
› The hydrodynamical response of cold circumgalactic clouds to quasar radiation
› TTV-Not-So-Fast: Uniqueness and Degeneracy in Perturbing Planet Parameters
› The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
› Electro-Weak Phase Transitions and Collider Signals in the Aligned 2-Higgs Doublet Model
› OverCite: Add citations in LaTeX without leaving the editor
› Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms
› Geometrically Regular Black Holes with Hedgehog Scalar Hair
› Mechanical Long Baseline Differential Gradiometers as Low Frequency Gravitational Wave Detectors
› Gravitational-wave astronomy requires population-informed parameter estimation
› Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
› Measuring the rate of glitches in interferometric gravitational wave detectors with a hierarchical Bayesian model
› Thermal effects on Dark Matter production during cosmic reheating
› Experimental evidence for coronal mass ejection suppression in strong stellar magnetic fields
› Post-Newtonian Constraints on Scalar-Tensor Gravity
› Recent progress on inflation and dark energy from string theory
› Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$
› A Homogeneous Catalog of Oscillating Solar-Type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity
› Influence of penetration depth on jets on giant planets: equatorial jet direction, jet numbers, and jet energy fraction
› Tomographic Alcock-Paczynski Test with Marked Correlation Functions
› Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges
› Unraveling the Secrets of the lower Solar Atmosphere: One year of Operation of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1
› Sensitivity of spectral lines to granulation: The Sun
› Bulk viscosity from neutron decays to dark baryons in neutron star matter
› Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys
› Sub-Snowline Formation of Gas-Giant Planets in Binary Systems
› Study of Neutron Star Properties under the Two-Flavor Quark NJL Model
› Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes
› Forecasting synchrotron spectral parameters with QUIJOTE-MFI2 in combination with Planck and WMAP
› Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach
› Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars
› The contribution from small scales on two-point shear analysis: comparison between power spectrum and correlation function
› Improved lanthanide constraints for the kilonova AT 2017gfo
› Operational Non-identifiability of Single-epoch Low-rank RFI Mitigation: Controlled Failure-mode Analysis and HERA Evidence
› How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity
› A Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime
› The long-term evolution of Ultra Faint Dwarf Galaxies and observational implications
› Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure
› Bayesian Cosmic Void Finding with Graph Flows
› Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins
› A unified harmonic framework for dark siren cosmology
› Measurements on the kinetic physics in streamer dynamics
› Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces
› A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
› Magnetic-Field-Induced Inspiral of Binaries with Circumbinary Disk: Black Hole and Protostellar Systems
› Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide
› Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System
› The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations
› The physics of gravitational waves
› Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift
› TLS and Quasiparticle Loss in Thin-Film Aluminum CPW Resonators: A Modified Model and Design Implications
› Conformal form-invariant parametrization of scalar-tensor gravity theories: A critical analysis
› Classical constant electric fields and the Schwinger effect in de Sitter
› Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework
› Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
› Analytic Approximations for Fermionic Preheating
› Novel ringdown tests of general relativity with black hole greybody factors

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