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Astronomia w Krakowie
Photo: Międzynarodowa Stacja Kosmiczna i Księżyc z halo
Międzynarodowa Stacja Kosmiczna i Księżyc z halo
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 News from astronomynow.com
› 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
› Binoculars to boost your night-sky viewing
RSS  Latest preprints on astro-ph:
› AstroMMBench: A Benchmark for Evaluating Multimodal Large Language Models Capabilities in Astronomy
› Technosignatures of Self-Replicating Probes in the Solar System
› Architecturally Constrained Solutions to Ill-Conditioned Problems in QUBIC
› Geometry of the Milky Way's dark matter from dynamical models of the tilted stellar halo
› Updates to the WFC3/UVIS Saturation Map
› Dark forces suppress structure growth
› Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption
› A Cold and Super-Puffy Planet on a Polar Orbit
› The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
› The OATMEAL Survey. III. An Aligned Transiting Warm Brown Dwarf and Evidence for Quiescent Brown Dwarf Migration
› Constraints on the Thompson optical depth to the CMB from the Lyman-$\alpha$ forest
› JADES: An Abundance of Ultra-Distant T- and Y-Dwarfs in Deep Extragalactic Data
› JWST-discovered AGN: evidence for heavy obscuration in the type-2 sample from the first stacked X-ray detection
› Automated Modeling with AAP-Imfit: Astrometry and Photometry via CASA
› What's in Your Transit? Towards Reliably Getting $5\times$ More Science from Exoplanet Transit Data
› Accelerating SED Modeling of Astrophysical Objects Using Neural Networks
› SN 2025coe: A Triple-Peaked Calcium-Strong Transient from A White-Dwarf Progenitor
› Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint
› ADARI: Visualizing the quality of VLT data
› Bayesian Model Comparison and Significance: Widespread Errors and how to Correct Them
› Icy or Rocky? Convective or Stable? New interior models of Uranus and Neptune
› The Simons Observatory: Characterization of All DC/RF Routing Wafers for Detector Modules
› SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
› The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. II. Dependence on WIMP Properties
› Inconsistencies of Tsallis Cosmology within Horizon Thermodynamics and Holographic Scenarios
› JADES: The Star Formation and Dust Attenuation Properties of Galaxies at 3
› Effects of Primordial Black Holes on IGM History
› Late-afterglow Emission from a Quasi-spherical Outflow in a stratified environment
› Exotic PeVatrons as sources of ultra-high-energy gamma rays
› Searching for Ultra-light Dark Matter in Spatial Correlations of White Dwarf Structure
› The Colors of Ices: Measuring ice column density through photometry
› A planetary system with a sub-Neptune planet in the habitable zone of TOI-2093
› Solar limb faculae: intensity contrast from two vantage points
› oMEGACat. VII. Tracing Interstellar and Intracluster Medium of $\omega$ Centauri using Sodium Absorptions
› The Eclipsing $\gamma$ Doradus Star V421 Pegasi
› Progress towards stereo observation of ultra-high-energy cosmic rays with Fluorescence detector Array of Single-pixel Telescopes
› Uncertainties in high-$z$ galaxy properties inferred from SED fitting using JWST NIRCam photometry
› Kinetic Simulations of Particle Acceleration in Relativistic Perpendicular Electron-positron Shocks with Proton Admixture
› UV Spectral Slope and Nebular Dust Attenuation in Dwarf Galaxies at $1.4
› Faraday Depolarization Study of a Radio Galaxy Using LOFAR Two-metre Sky Survey: Data Release 2
› Serendipitous Discovery of an Optically-Dark Ultra-Luminous Infrared Galaxy at $z$ = 3.4
› Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode
› Evaluating solar wind forecast using magnetic maps that include helioseismic far-side information
› Multiband Optical Photometric and Spectroscopic Monitoring of the 2024 Flare Event in Transition Blazar OP313
› Dark-to-black super accretion as a mechanism for early supermassive black hole growth
› Diffuse neutrino flux from coronal magnetospheric current sheets of accreting black holes
› Addressing Selected Gamma-Ray Burst Science Topics with Future Space Instruments
› Propagation and Energy Dissipation of Shock Waves in the Solar Chromosphere
› Kinematic analysis of an Ultra-Strong MgII absorber at z~1.13 linking to Circumgalactic Gas Structures
› Exoplanets beyond the Conservative Habitable Zone: I. Habitability
› Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
› Dissecting the radiation mechanism of short GRB~160821B through multi-wavelength modelling
› Exoplanets beyond the Conservative Habitable Zone: II. Occurrence
› Gravitational lensing of 21 cm HI signal: detection prospects at z ~ 1 with uGMRT in galaxy cluster lenses
› Alleviating Cosmological Tensions with the Hadrosymmetric Twin Higgs
› Understanding the evolution of black hole spin in X-ray binary systems: Case study of XTE~J1550-564
› Deep XMM-Newton observation reveals hot gaseous outflow in NGC 5746
› Gravitational Waves sourced by Gauge Fields during Inflation
› High energy emission powered by accreting companions of Be/gamma Cas stars
› The gas streamer G1-2-3 in the Galactic Center
› Forecasting the Observable Rates of Gravitationally Lensed Supernovae for the PASSAGES Dusty Starbursts
› Fuzzy dark matter dynamical friction: Defying galactic cannibalism of globular clusters
› Euclid: Discovery of bright $z\simeq7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
› From atoms to stars: Modelling $\mathrm{H}_2$ formation and its impact on galactic evolution
› Machine Learning Approaches for Classifying Star-Forming Galaxies and Active Galactic Nuclei from MIGHTEE-Detected Radio Sources in the COSMOS Field
› Powerful lightning on Venus constrained by atmospheric NO
› The trigger design for AdvCam
› Molecular Mobility of Extraterrestrial Ices: Surface Diffusion in Astrochemistry and Planetary Science
› The Clustering of Active Galactic Nuclei and Star Forming Galaxies in the LoTSS DeepFields
› JADES Data Release 4 Paper I: Sample Selection, Observing Strategy and Redshifts of the complete spectroscopic sample
› JADES Data Release 4 -- Paper II: Data reduction, analysis and emission-line fluxes of the complete spectroscopic sample
› Carbon and nitrogen as indicators of stellar evolution and age. A homogeneous sample of 44 open clusters from the Gaia-ESO Survey
› Testing Gravitation from Light-second to Cosmological Scales with Radio Pulsars
› Revisiting the formation of molecules and dust in core collapse supernovae
› The Silicon Strip Detector Subsystem for the Trans-Iron Galactic Element Recorder for the International Space Station (TIGERISS)
› Quasar Main Sequence unfolded by 2.5D FRADO (Natural expression of Eddington ratio, black hole mass, and inclination)
› The causal structure of galactic astrophysics
› CosmoUiT: A Vision Transformer-UNet Hybrid for Fast and Accurate Emulation of 21-cm Maps from the Epoch of Reionization
› KiDS-1000 cosmic shear reanalysis using MetaCalibration
› Pan-STARRS follow-up of the gravitational-wave event S250818k and the lightcurve of SN 2025ulz
› iPTF16geu through the lens of thermonuclear explosion models
› Vanishing Acts: Quantifying Black Hole Formation with the DSNB Signal
› Chiral effects and Joule heating in hot and dense matter
› Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates
› Lectures on Open Effective Field Theories
› ELENA: a software for fast and precise computation of first order phase transitions and gravitational waves production in particle physics models
› Modified cosmology through generalized mass-to-horizon entropy: implications for structure growth and primordial gravitational waves
› Asymptotic Schwarzschild solutions in $f(R)$ gravity and their observable effects on the photon sphere of black holes
› Shadow of black holes with consistent thermodynamics
› Gluon Condensation as a Unifying Mechanism for Special Spectra of Cosmic Gamma Rays and Low-Momentum Pion Enhancement at the Large Hadron Collider
› Reducci\'on de ruido por medio de autoencoders: caso de estudio con la se\~nal GW150914
› Novel very-high-frequency quasi-periodic oscillations of compact, non-singular objects
› Properties of Neutron Stars with Hyperons within a Relativistic Metamodel
› GW250114 reveals black hole horizon signatures
› Do plasmoids induce fast magnetic reconnection in well-resolved current sheets in 2D MHD simulations?
› Imaging Venus' surface at night in the near-IR from above its clouds: New analytical models for the effective spatial resolution, illustrated with new Parker Solar Probe data
› Slaying Axion-Like Particles via Gravitational Waves and Primordial Black Holes from Supercooled Phase Transition
› Fundamental modes of rotating neutron stars with various degrees of differential rotation in dynamical spacetimes
› Badminton Birdie-Like Aerodynamic Alignment of Drifting Dust Grains by Subsonic Gaseous Flows in Protoplanetary Disks
› Curvature Mapping Method: Mapping Lorentz Force in Orion A
› The spectra of a radiative reprocessing outflow model for fast blue optical transients
› Fermion-Boson Stars as Attractors in Fuzzy Dark Matter and Ideal Gas Dynamics
› Line-of-sight effects on double source plane lenses
› Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
› Learning the Universe: Learning to Optimize Cosmic Initial Conditions with Non-Differentiable Structure Formation Models
› Toward a Robust R2D2 Paradigm for Radio-interferometric Imaging: Revisiting Deep Neural Network Training and Architecture
› Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
› MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
› Seeding Cores: A Pathway for Nuclear Star Clusters from Bound Star Clusters in the First Billion Years
› Atacama Cosmology Telescope: Observations of supermassive black hole binary candidates. Strong sinusoidal variations at 95, 147 and 225 GHz in PKS 2131$-$021 and PKS J0805$-$0111
› Increase of $n_s$ in regularized pole inflation & Einstein-Cartan gravity
› A Multispacecraft Analysis and Modeling of Type III Radio Burst Exciter Deceleration in Inhomogeneous Heliospheric Plasma
› Tidal effects on primordial black hole capture in neutron stars
› Toward mapping turbulence in the intracluster medium IV. Using NewAthena/X-IFU and simulation based inference to constrain turbulence
› Modelling multiwavelength afterglows of the VHE-GRB population
› Updated predictions for gravitational wave emission from TDEs for next generation observatories
› Cosmography with DESI DR2 and SN data
› Polarization-shape alignment of IllustrisTNG star-forming galaxies
› FLORAH-Tree: Emulating Dark Matter Halo Merger Trees with Graph Generative Models
› Estimate of Current Mass of the Large Magellanic Cloud from the Orphan-Chenab Tidal Stream
› Equation vs. AI: Predict Density and Measure Width of molecular clouds by Multiscale Decomposition
› X-ray Polarimetry of Accreting White Dwarfs: A Case Study of EX Hydrae
› Wide binaries in an ultra-faint dwarf galaxy: discovery, population modeling, and a nail in the coffin of primordial black hole dark matter
› Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
› The Thousand-Pulsar-Array programme on MeerKAT -- XVIII. Complex sub-pulse modulation patterns, bi-drifting and mode changing of nine radio pulsars
› DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
› Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
› Ultra-long Gamma-ray Bursts from Micro-Tidal Disruption Events: The Case of GRB 250702B
› Comprehensive X-ray Observations of the Exceptional Ultra-long X-ray and Gamma-ray Transient GRB 250702B with Swift, NuSTAR, and Chandra: Insights from the X-ray Afterglow Properties
› The inner rotation curve of the Milky Way
› Testing the nature of GW200105 by probing the frequency evolution of eccentricity
› Tests of Evolving Dark Energy with Geometric Probes of the Late-Time Universe
› A nonperturbative test of nucleation calculations for strong phase transitions
› Costs of Bayesian Parameter Estimation in Third-Generation Gravitational Wave Detectors: an Assessment of Current Acceleration Methods
› Neutron star evolution by combining discontinuous Galerkin and finite volume methods
› A quantitative analysis of Galilei's observations of Jupiter satellites from the Sidereus Nuncius
› Supercooled Confinement
› Impact of Detector Calibration Accuracy on Black Hole Spectroscopy
› Multi-directional investigations on quiet time suprathermal ions measured by ASPEX-STEPS on-board Aditya L1
› Imprints of screened dark energy on nonlocal quantum correlations
› Gravitational wave experiments: achievements and plans

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