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View over the dome at night
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 News from astronomynow.com
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RSS  Latest preprints on astro-ph:
› Reconstruction of the dark matter density profile from cosmic positron anomaly data
› An Improved Machine Learning Approach for RFI Mitigation in FAST-SETI Survey Archival Data
› Milky Way disc & Bulge in situ populations: ESO white paper - Expanding horizons call
› Asteroseismology of white dwarfs in the 2040s
› Sailing to the next safe harbour in our trip to the early Universe: The massive star population of metal-poor galaxies
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› Accretion and Ejection Physics at High Time Resolution
› The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes
› What Builds and Quenches the Most Massive Galaxies in the Early Universe?
› Galaxies as stochastic systems: why the next breakthrough in galaxy evolution requires one hundred million spectra
› A JWST Transmission Spectrum of the Temperate Sub-Neptune TOI-732 c
› Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments
› Revealing Callisto's Near Subsurface Thermophysical Properties with ALMA Calibration Data
› From "The Cliff" to "Virgil": Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec
› The AIDA-TNG project: 3D halo shapes
› Hunting exomoons with a kilometric baseline interferometer
› A second planetesimal collision in the Fomalhaut system
› The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
› Dark Acoustic Oscillations as an Early-Universe Explanation of the DESI Anomaly
› In-plane Black-hole Spin Measurements Suggest Most Gravitational-wave Mergers Form in Triples
› Bright Long Secondary Period Stars for Follow-up Observations
› Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
› The AIDA-TNG project: abundance, radial distribution, and clustering properties of halos in alternative dark matter models
› Cored galaxies in cuspy dark matter halos
› Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
› The Next Generation Fornax Survey (NGFS).VIII. A Support Vector Machine Approach for Disentangling Globular Clusters from other Sources
› Dust evolution across cosmic times as seen through DUSTY-GAEA
› Binarity Beyond Gaia: The case for a dedicated spectroscopic survey of binary stars
› The Era of Binary Supermassive Black Holes: Coordination of Nanohertz-Frequency Gravitational-Wave Follow-up
› 2D or not 2D? Exploring 3D relativistic magnetic reconnection dynamics with highly accurate numerical simulations
› DESI-DR1 $3 \times 2$-pt analysis: consistent cosmology across weak lensing surveys
› Joint cosmological fits to DESI-DR1 full-shape clustering and weak gravitational lensing in configuration space
› Cosmological Constraints from Full-Scale Clustering and Galaxy-Galaxy Lensing with DESI DR1
› Clustering redshift distribution calibration of weak lensing surveys using the DESI-DR1 spectroscopic dataset
› The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000
› The Sesquinary Catastrophe on Deimos can reconcile its excited past with its dynamically cool present
› MAGellanic Outflow and chemistry Survey (MAGOS): Hot cores in the LMC
› ASKAP discovery of a 30 kpc bipolar outflow from the edge-on disk of the nearby spiral galaxy ESO 130-G012
› IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission
› HEGS : Revisiting a decade of H.E.S.S. extragalactic observations
› Exploring the Galactic Plane: A Comparative Study of Fermi-LAT Sources and HESS's Non-Detection at TeV Energies
› LSTM-MDNz: Estimating Quasar Photometric Redshifts with an LSTM-Augmented Mixture Density Network
› Direct calculation of steady-state hydrodynamic solar wind solutions with newtonian viscosity
› Astrometric and Spectroscopic Analysis of IC 2714: An Open Cluster Hosting a Lithium-Rich Giant
› Gas Accretion from a Neighbouring Galaxy Fuels the Low-luminosity AGN in NGC 4278
› Graph Neural Networks for Interferometer Simulations
› Axisymmetric Modeling of DSHARP Dusty Disks: Asymmetric Structures and Inner-Disk Dispersal
› Inferring the Intrinsic Energy Function of FRB 20220912A
› Pulsar Science with the SKA Observatory
› A Square Kilometre Array Pulsar Census
› Pulsars in Globular Clusters With the SKAO
› Galactic Centre Pulsars with the SKAO
› Understanding the Neutron Star Population with the SKAO telescopes
› Understanding pulsar magnetospheres with the SKAO
› Exploring Galactic plasma with pulsars in the SKA era
› Exploring the magnetic field structure of the Milky Way with pulsars in the SKA era
› Understanding Pulsar Wind Nebulae with the SKA
› Testing Gravity with Binary Pulsars in the SKA Era
› Probing neutron star interiors and the properties of cold ultra-dense matter with the SKAO
› The SKAO Pulsar Timing Array
› Bayesian Smooth-Fit Extrapolation of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Astrophysical $S$ Factor
› Physics-Informed Neural Networks for Modeling the Martian Induced Magnetosphere
› Fastest or Significant: A Systematic Framework for Validating Global Minimum Variability Timescale Measurements of Gamma-ray Bursts
› Unveiling the properties and origin of massive quenched galaxies at $z\ge2$ in the COLIBRE hydrodynamical simulations
› Infrared SED Modeling of Velocity-Excess Maser Sources: Identifying Incipient Water-Fountain Candidates
› ALMA and JWST Identification of Faint Dusty Star-Forming Galaxies up to z~8
› Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars
› Expanding Horizons - Transforming Astronomy in the 2040s Time-Domain Multi-Messenger Astronomy in the 2040s: EM Follow-up of LGWA Sources
› Radio frequency interference identification using eigenvalue decomposition for multi-beam observations
› Astrophysical Implications of Eccentricity in Gravitational Waves from Neutron Star-Black Hole Binaries
› The dominant role of dark matter halo in quenching central galaxies
› Multi-Energy Proton Events and Geomagnetic Storms in Solar Cycles 23 and 24
› Discovery of a rapidly evolving global magnetic field in the M-dwarf YZ Cet and constraints on the magnetic field of its planet YZ Cet b
› Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center
› New methods to improve the decontamination of slitless spectra
› Maximizing the sensitivity of ELT to habitable worlds with a space-based starshade
› Observational methods for solar origin diagnostics of energetic protons
› The AGN nature of strong CIII emitters in the Early Universe with JWST
› High mass accretion rates onto evolved stripped-envelope massive stars by jet-induced mass removal
› Transformational astrophysics and exoplanet science with Habitable Worlds Observatory's High Resolution Imager
› Understanding the chemistry of temperate exoplanets atmospheres through experimental and numerical simulations
› MUSE Analysis of Gas around Galaxies (MAGG) - VII. Emission line galaxies near strong blended Ly$\alpha$ absorption systems at $z\gtrsim3$
› A direction-dependent framework for visibility plane mosaicing and primary beam correction
› Classification of the equation of state of neutron stars via sparse dictionary learning
› Uniform Rolling: An LSST Observing Cadence Offering Sufficient Survey Uniformity for Comprehensive Cosmological Analysis
› How massive neutrinos reshape the cosmic web
› XMM-Newton multi-year campaign on NGC 55 ULX-1: Resolving the wind and its variability with RGS
› Pulsar B1237+25 at 111~MHz: average profile, mode switching, nullings, microstructure
› Galaxy evolution in compact groups - III. Structural analysis of galaxies and dynamical state of non-isolated compact groups
› N-emitters as possible sign-posts of GC formation
› Warm Jupiter Tidal Migration Can Spare Inner Planets; Hot Jupiter Tidal Migration May Not
› Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the alleviation of the $\sigma_8$ tension
› Double shell structure in supernova 2024ggi
› Prompt Searches for Very-High-Energy {\gamma}-Ray Counterparts to IceCube Astrophysical Neutrino Alerts
› A Tidal Disruption Event from an Intermediate-mass Black Hole Revealed by Comprehensive Multi-wavelength Observations
› Probing thermal gradients of habitable-zone rocky planets using direct imaging as an anti-indicator of a global surface ocean
› JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon
› An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4
› Closed Form Expressions for the Potentials and Accelerations of Generalized Ring Models
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› The high-redshift radio galaxy 3C 294 at low frequencies: radio detection of the X-ray Ghost
› Cygnus X-3: A variable petaelectronvolt gamma-ray source
› The Preliminary Mauve Science Programme: Science themes identified for the first year of operations
› Einstein Probe Discovery of an X-ray Flare from K-type Star PM J23221-0301
› Comparison of General Circulation Models of the Venus upper atmosphere
› Discovery of two new millisecond pulsars towards the Galactic bulge
› On the Origin of Kinematic Structure in the Young Association Serpens OB2
› Simulation-based inference with neural posterior estimation applied to X-ray spectral fitting - III Deriving exact posteriors with dimension reduction and importance sampling
› Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge
› Evidence of Possible Spectral Variability in the Patroclus-Menoetius Binary System
› A finite temperature framework for quark matter with color-superconducting phases
› A faint M$_{\rm UV} = -14.5$ Lyman continuum leaker in the reionization epoch: unprecedented Ly$\alpha$ properties at z=5.725
› Current observations favour phantom-enhanced nature of dark energy
› The WINTER Observatory: A One-Degree InGaAs Survey Camera to study the Transient Infrared Sky
› N-body interactions and collisions in circumstellar disks for planar and inclined binary star configurations
› Strategies for Accurate Effective Point Spread Function (ePSF) Modelling on Undersampled Images
› Dark energy and neutrinos along the cosmic expansion history
› SNR 1987A : Spitzer data from days 6000 to 8000 revisited
› Future Dark Energy Constraints from Atomic Clocks
› Connecting current and future dual AGN searches to LISA and PTA gravitational wave detections
› BeppoSAX-WFC catalog of fast X-ray transients
› A Radio Search for Star-Planet Interaction in TOI-540 and SPECULOOS-3
› Robust CMB B-mode analysis with Needlet-ILC and simulation-based inference
› Discovering gravitational waveform distortions from lensing: a deep dive into GW231123
› Density reconstruction from biased tracers: Testing the equivalence principle through consistency relations
› Towards First Detection of the Solar MSW Transition With JUNO
› Multiple mountains on a pulsar: implications for gravitational waves and the spin-down rate
› GRHayL: a modern, infrastructure-agnostic, extensible library for GRMHD simulations
› Cosmological Neutron Stars Produce Diffuse Axion X-Ray Signatures
› Particle Production by Time-Varying Dark Energy and the End of Cosmic Expansion
› Kination and the Inert Doublet Model
› Modeling the frequency-domain ringdown amplitude of comparable-mass mergers with greybody factors
› Fifty shades of grayness: parameterizations of spectral distortions and applications in cosmology
› Introduction to Symbolic Regression in the Physical Sciences
› Unraveling the anomaly in the production of $^{60}$Fe nucleus in massive stars
› Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model
› Modified light-cylinder and centrifugal acceleration in Schwarzschild geometry
› GWTC-4.0: Searches for Gravitational-Wave Lensing Signatures
› Implementing F (T ) Gravity in Boltzmann Codes: A Framework for Power Spectrum Computation
› Constraining the nuclear equation of state from terrestrial experiments and neutron star observations using relativistic mean-field models
› Cosmology with non-linear barotropic Israel-Stewart fluid with causal relaxation time
› Chiral magnetic effect amplified baryogenesis at first-order phase transitions
› Photon Accelerator in Magnetized Plasma
› On Non-Minimal Couplings to Gravity and Axion Isocurvature Bounds
› Impact of Supercooling on Direct Searches for Dark Matter and Gravitational Wave Backgrounds
› Exponential plateaus and inflation in metric-affine gravity
› Delayed Scaling of Multi-Type Cosmic F- and D-strings in VOS Models
› Multiple Axions in Laboratory Experiments
› Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025)
› Binary Black Hole Mergers: Spin and mass ratio effects on gravitational waveforms
› Radiation-driven dusty outflows from early galaxies
› Benchmarking field-level cosmological inference from galaxy redshift surveys
› LITMUS: Bayesian Lag Recovery in Reverberation Mapping with Fast Differentiable Models
› Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation
› Spatial and velocity anisotropies of stellar halos across cosmic web environments: Insights from IllustrisTNG simulation
› Inferring and Interpreting the Visual Geometric Albedo and Phase Function of Earth
› Spiral Structure Properties, Dynamics, and Evolution in MW-mass Galaxy Simulations
› Design and Commissioning of an LWA Swarm Station: The Long Wavelength Array -- North Arm
› The Hidden Role of Anisotropies in Shaping Structure Formation in Cosmological N-Body Simulations
› Linear map-making with LuSEE-Night
› J-VAR: Analysis of RR Lyrae light curves in seven optical bands
› Segmentation and Tracking of Eruptive Solar Phenomena with Convolutional Neural Networks
› A Spatial Gap in the Sky Distribution of Fast Radio Burst Detections Coinciding with Galactic Plasma Overdensities
› SN 2024aecx: a fast-evolving Type IIb supernova with a prominent shock-cooling peak
› Backtracking Bipolar Magnetic Regions to their emergence: Two groups and their implication in the tilt measurements
› JWST occultation reveals unforeseen complexity in Chariklo's ring system
› What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the interstellar medium
› Eclipsing Stellar Flare on the Demon Star Algol Binary System Observed during the MAXI-NICER Follow-up Campaign in 2018
› Variance of dust temperature and spectral index in Planck polarization data using spin-moment expansion
› An accurate measure of the size of dark matter halos using the size of galaxies
› A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene
› Rapid Brightening of 3I/ATLAS Ahead of Perihelion
› Oscillations of dark matter halos in galaxies and their effects on motion of stars
› Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes
› First Resolution of a Main Sequence G-Star Astrosphere Using Chandra
› Stellar properties and chemical features of the Gaia Catalogue of Nearby Stars observed by GALAH DR4
› Super-resolving Herschel - a deep learning based deconvolution and denoising technique
› From ASTRID to BRAHMA -- The role of overmassive black holes in little red dots in cosmological simulations
› Characterisation of the Bedretto Underground Site for Fundamental Physics Experiments
› Stellar Morphology of Optically Dark or Faint Galaxies at $z>3$ with JWST
› Dual-coding contrastive learning based on ConvNeXt and ViT models for morphological classification of galaxies in COSMOS-Web
› An updated efficient galaxy morphology classification model based on ConvNeXt encoding with UMAP dimensionality reduction
› Robustness Analysis of USmorph: I. Generalization Efficiency of Unsupervised Strategies and Supervised Learning in Galaxy Morphological Classification
› Ultralight Dark Matter Constraints from NanoHertz Gravitational Waves
› JWST NIRSpec finds no clear signs of an atmosphere on TOI-1685 b
› Searching potential astronomical sites in Ethiopia
› Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition
› No Dark Matter Axion During Minimal Higgs Inflation
› Lensing by black holes within astrophysical environments
› Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector

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