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Temperature
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 84%

Wind
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Pressure
1021.3 hPa

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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:
› Constraining Ultra-Light Dark Matter mass with Dwarf Galaxy Rotation Curves
› Diffusion models for polarimetric reconstruction of circumstellar environments
› Spatial Variations of Polarized Synchrotron Emission in the QUIJOTE MFI Data
› Simulation of Time-dependent Karhunen-Loeve Phase Screens: an Ergodic Approach
› Probabilistic Inference of Cosmological Density Parameters from Synthetic Hubble Expansion Data of Varying SNR Using Diverse Artificial Neural Network Architectures
› Unified kinetic theory of induced scattering: Compton, Brillouin, and Raman processes in magnetized electron and positron pair plasma
› Eccentric Disks With Self-Gravity
› Revealing evolution of Dark Energy density from observations
› ALMAGAL VIII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk
› Mean Motion Resonances in AGN Disks
› Towards High-Resolution Orbitrap Mass Spectrometry for Next- Generation In-Situ Space Dust Analysis
› InferA: A Smart Assistant for Cosmological Ensemble Data
› Strategy for identifying Vera C. Rubin Observatory kilonova candidates for targeted gravitational-wave searches
› Calibration of the ComPair Balloon Instrument
› J-PLUS: Turning Off the Bright Stars
› Only the Special Survive: Evolution of Long-Lived Star Clusters in Galaxy Simulations
› Simulation-Based Pretraining and Domain Adaptation for Astronomical Time Series with Minimal Labeled Data
› Cosmic Ray Transport and Gamma-Ray Signatures in the Interstellar Medium
› High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates I. X-ray Coronae
› Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
› Galactic X-ray Transients in the First eROSITA All Sky Survey
› When Tiny Halos Stir Spacetime: Gravitational Waves from Fifth-Force Mergers
› Probing the magneto-ionic medium of the Milky Way using pulsars
› Beyond OCCAM: Measuring Optical Neutron Capture Abundances of Open Cluster Stars
› Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A & EP250207b
› Improved Absolute Polarization Calibrator for BICEP CMB Polarimeters
› First Demonstration of Kernel Phase Interferometry on JWST/MIRI: Prospects for Future Planet Searches Around Post Main Sequence Stars
› Gravitational-Wave Signatures of Highly Eccentric Stellar-Mass Binary Black Holes in Galactic Nuclei
› Galactic chemical evolution with the short-lived isotopes Mn-53, Fe-60, Hf-182, and Pu-244
› Gravitational-Wave Signatures of Highly Eccentric Stellar Binary Black-Holes in Galactic Nuclei
› Strong Progenitor Age-bias in Supernova Cosmology. II. Alignment with DESI BAO and Signs of a Non-Accelerating Universe
› Numerical Cosmology
› Galaxy Protoclusters as Drivers of Cosmic Reionization: I. Bubble Overlap at Redshift z ~ 7 in LAGER-z7OD1
› The Dependency of Bar Formation Timescale on Disk Mass Fraction, Toomre $Q$, and Scale Height
› Dependency of the Bar Formation Timescale On The Halo Spin
› Some problems associated with the standardization of the light curve of type 1a supernovae
› Prospects for the Crossing of Comet 3I/ATLAS's Ion Tail
› Discovery of red galaxy candidates at z ~ 12: Early dust growth or significant nebular emission with high-temperature stars?
› The dependence of black hole formation in open clusters on the cluster formation process
› Monte Carlo simulation of the Compton scattering and disk reflection of a cylinder with hot electrons moving away from a black hole
› Old open clusters NGC 188 and M 67 in Gaia DR3
› Global linear analysis of the magneto-thermal instability in a stratified spherical model of the intracluster medium
› Relativistic reflection within an extended hot plasma geometry
› Abundance of heavy r-process elements in CEMP-rs stars: The role of the i-process
› ON the stability of triangular Lagrangian points in the spatial restricted three-body problem
› Evidence for Neutrino Emission from X-ray Bright Active Galactic Nuclei with IceCube
› Examining a new form of non-standard dark matter using DESI DR2 data
› Probing Primordial black holes with the distortion of Stochastic Gravitational Wave Background
› Chaotic Dynamics and Zero-Velocity Structures in the Pluto-Charon CR3BP
› Recent progress on interstellar radionuclides on Earth and the Moon
› A New Method for Aperture Masking Interferometric Imaging: Demonstration with the JWST
› Design of an Imaging Air Cherenkov Telescope array layout with differential programming
› Euclid: Exploring observational systematics in cluster cosmology -- a comprehensive analysis of cluster counts and clustering
› Investigating the Formation of Planets Interior to in situ Hot Jupiters
› The Formation Rate and Luminosity Function of Fast X-ray transients from Einstein probe
› The 2024 outburst of the neutron star LMXB EXO 0748-676: an investigation of bursts and eclipses with AstroSat
› Hyperons and $\Delta$'s in rotating protoneutron stars: Local properties
› Measuring the precise photometric period of the probable intermediate polar 1RXS J014549.6+514314 based on extensive photometry
› Solar Cycle Variation of Sustained Gamma-ray Emission Events from the Sun and Related Energetic Events
› The Supernova 1987A system and its recent evolution - a review
› Condensation sequence of circumstellar cluster seeds (CSCCS)
› The Stellar Morphology & Size of X-ray-selected Active Galactic Nuclei Host Galaxies Revealed by JWST
› Planetary-mass companions to a retired B star BD+37 3172 and a retired F star BD+42 2315
› The collision and merger products of stars do not look alike: A magnetohydrodynamics comparison
› Comparing subgrid models for cosmic ray diffusion in a magnetized isolated galaxy simulation
› XRISM Resolves Relativistic Effects from the Innermost Accretion Disk in Serpens X-1
› Dynamics and Observational Signatures of Core-Collapse Supernovae with Central Engines: Hydrodynamics Simulations with Monte Carlo Post-Processing
› Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra
› Optimizing Supernova Classification with Interpretable Machine Learning Models
› Polarization dynamics of X-ray synchrotron emission from a multi-zone blazar jet
› Investigating double bump air showers with the SKA-Low
› Density reconstruction from biased tracers: Testing the equivalence principle through consistency relations
› $\texttt{SBi3PCF:}$ Simulation-based inference with the integrated 3PCF
› Impact of facility timing and coordination for next-generation gravitational-wave detectors
› On the maximum compactness of neutron stars
› New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO
› Dark Matter-Electron Interactions Alter the Luminosity and Spectral Index of M87
› Gravity and the Hierarchy Problem
› Statistical properties of compressible isothermal turbulence from sub- to supersonic conditions
› Orbital dynamics and precession in magnetized Kerr spacetime
› Mass and spin coevolution of black holes inspiralling through dark matter
› APRIL: Auxiliary Physically-Redundant Information in Loss - A physics-informed framework for parameter estimation with a gravitational-wave case study
› Unified Origin of Dirac Neutrino and Asymmetric Dark Matter Masses via a Dirac-Type Leptogenesis
› Primordial magnetogenesis in loop quantum cosmology
› The Third Workshop on Extremely Precise Radial Velocities: The New Instruments
› Catalog of outbursts of neutron star LMXBs
› Modified gravity constraints with Planck ISW-lensing bispectrum
› Origin of the two-armed vertical phase-spiral in the inner Galactic disk
› Matter Dipole and Hubble Tension due to Large Wavelength Perturbations
› The Cosmic Shoreline Revisited: A Metric for Atmospheric Retention Informed by Hydrodynamic Escape
› Constraining cosmic ray transport models using circumgalactic medium properties and observables
› Neutral gas phase distribution from HI morphology: phase separation with scattering spectra and variational autoencoders
› A joint analysis of 3D clustering and galaxy x CMB-lensing cross-correlations with DESI DR1 galaxies
› H3+ in irradiated protoplanetary disks: Linking far-ultraviolet radiation and water vapor
› The Online Data Filter for the KM3NeT Neutrino Telescopes
› Reconstruction of dark energy and late-time cosmic expansion using the Weighted Function Regression method
› Bayesian Quantification of Observability and Equation of State of Twin Stars
› Galactic echoes
› Gravitational Redshift for Rapidly Rotating Neutron Stars
› 20 GeV halo-like excess of the Galactic diffuse emission and implications for dark matter annihilation
› CO desorption from interstellar icy grains induced by IR excitation of superhydrogenated PAHs
› Is the Interstellar Object 3I/ATLAS Alien Technology?
› Low-frequency spectra of neutron star + OB supergiant binaries: Does wind density drive persistent and flaring modes of accretion?
› Evidence for Evolving Dark Energy from LRG1-2 and Low-$z$ SNe Ia Data
› Revisiting the Radial Metallicity Gradient-Age Relation in the Milky Way's Thin and Thick Disks
› The evolution of PUCHEROS from a basic to a competitive tool for stellar astrophysics
› Double-faced white dwarfs and the magnetic inhibition of convection
› The EBLM project XVI. Spin-orbit alignment of the low mass eclipsing binary EBLM J0021-16
› Advancing Interstellar Science: A Global Framework for Comprehensive Study of Interstellar Objects
› Mapping the Cloud-Driven Atmospheric Dynamics & Chemistry of an Isolated Exoplanet Analog with Harmonic Signatures
› Spectral Mixture Modeling with Laboratory Near-Infrared Data I: Insights into Compositional Analysis of Europa
› Introducing The SHell misAlignment Detection for straylight Estimation (SHADE) algorithm: the case of XMM-Newton
› Empirical Optimization of the Source-Surface Height in the PFSS extrapolation
› MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars
› GALACTICNUCLEUS: A high angular resolution JHKs imaging survey of the Galactic centre
› Limits of Standard Tidal Models at Quaoar: Matching Weywot's Orbit, Missing the Spin
› Polarization from Rapidly Rotating Massive Stars
› Mass dependence of halo baryon fractions from the kinetic Sunyaev-Zeldovich effect
› Gravitational-wave signatures of non-violent non-locality
› Spin oscillations of neutrinos scattered by the supermassive black hole in the galactic center
› Gravitational Wave Production and Baryogenesis in a Simple Left-Right model
› Extra-natural production of superheavy Kaluza-Klein particles
› Is the $\Lambda$CDM Model in Crisis?
› Quasinormal ringing and Unruh-Verlinde temperature of the Frolov Black Hole
› False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE

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