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Astronomia w Krakowie
Photo: The Mt. Suhora 60cm telescope
The Mt. Suhora 60cm telescope
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Pressure
1020.1 hPa

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 News from astronomynow.com
› Moon dust preserves record of life’s building blocks
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› 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
› Dr Allan Chapman (1946-2026)
RSS  Latest preprints on astro-ph:
› Substructures Induced by Dust Drag in Protoplanetary Disks
› The Effects of Accretion Feedback on Stellar Evolution in AGN Disks
› IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament
› Diffusion-based Galaxy Simulations for the Roman High Latitude Survey
› The abundance and radial distribution of faint and ultra-faint dwarfs in galaxy clusters
› Cluster-green galaxy correlations: where do these galaxies live?
› Discovery of ultra-fast outflows with v$_{\rm out}>0.3 \rm c$ in local bright active galactic nuclei
› Supermassive stars with embedded stellar black hole cores: dense assembling star clusters as faint multiple Little Red Dot systems
› Quantitative modelling of type Ia supernovae spectral time series II: Exploring the diversity of thermonuclear explosion scenarios
› Quantitative modelling of type Ia supernovae spectral time series III: Implications for type Ia supernovae standardisation in cosmology
› Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
› Emerging Diversity Among the Main-Belt Comets: Insights from JWST and Ground-Based Observations of 457P/Lemmon-PANSTARRS
› Characterization of the Volatile Properties of 133P/Elst-Pizarro and Other Main-Belt Comets with JWST and Ground-Based Observations
› The Oort Cloud as a Gravitational Detector for Primordial Black Holes
› Cosmological evolution of interacting dark energy with a CPL equation of state
› Probable Detection of a Cooler Gas Component in the Perseus Cluster with XRISM
› The POKEMON Speckle Survey of Nearby M dwarfs. IV. Distance-Limited Catalog (POKEMON-DLC)
› A Machine Learning Approach to Meteor Classification
› KilonovaSCORER: Prior-Predictive Scoring of Kilonovae for Real-Time Multimessenger Follow-Up
› Current Unsolved Problems in Planetary Nebulae Research
› It\^o tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics
› Multi-Viewpoint Observation of a Failed Prominence Eruption on the Sun
› Analysis of a Septuple Open Cluster System and Its Extended Family in Gaia DR3
› UHECR doublets and their conditional association with nearby radio galaxies
› Hessian-based photometric substructure as an evolutionary tracer of OB cluster candidates in M31
› The Dependence of the Mean Spectral Energy Distributions on the Accretion Rate for Quasars with $z < 0.75$ from the Sloan Digital Sky Survey
› PEEPSS: Photonic-Enabled ExoPlanet Spectroscopic Sensor for the Habitable Worlds Observatory
› A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution
› The line modulations of H-like Fe, Ca, Ar, and S observed with $XRISM$/Resolve in Cyg X-3
› Successful irradiation campaign on PRIMA/PRIMAger KIDs detectors with DRACuLA
› Parametric Resonance in $\phi^4$ Preheating: An Exact Numerical Study
› The functional form of galaxy and halo luminosity and mass functions
› gateau: an observation simulator for ground-based submillimeter astronomy with integral field units and kinetic inductance detectors
› Deflection of a Filament Eruption with Three Parallel Flare Ribbons via Reconnection at an X-Point
› Testing Scalar Field Dark Matter models in M31 galaxy through the Rotation Curve analysis
› ArchGEM: an Advanced Data Analysis Tool for Analyzing Scattered Light Noise in LIGO
› STVG-MOG Cluster Dynamics and the Cosmological $1/r^2$ Force Law from Pairwise kSZ Data
› Direct Imaging Constraints on Binary Planets and Exomoons around Epsilon Indi A b
› The open-Universe signal: A model artifact rather than genuine curvature
› Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-\.Zytkow Objects
› High-Precision Ground Characterization of Test-Mass Magnetic Properties for the Taiji Gravitational Wave Mission via a Physics-Informed Neural Framework
› The Deep Newtonian Regime in Late-Time Blast Waves: Inevitable Transition and Distinct Flux Signatures
› CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
› Two Exciting High-redshift Galaxy Candidates Turn Out to Be Two Exciting Ultra-cool Brown Dwarfs
› The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
› Magnetic Activity Cycles and Rotation in Planet-hosting and Non-hosting Solar-type Stars
› A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model
› Diagnostic Disagreement as an Information-Projection Divergence: An Information-Theoretic Reading of the Quiet-Sun Temperature Ratio
› Beyond the Final Label: Exploiting the Untapped Potential of Classification Histories in Astronomical Light Curve Analysis
› SCAT Data Release 1: 1810 optical spectra of 1330 transients
› A GLIMPSE of the 99%: a census of the faintest galaxies during the epoch reionization and its implications for galaxy formation models
› Probabilistic Spectral Reconstruction of Trans-Neptunian Objects from Sparse Photometry: A Framework for Taxonomy, Survey Optimization, and Outlier Detection
› Alfven-winged pulsar
› With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies
› GRRMHD Simulations of State Transitions in Non-Jetted Tidal Disruption Events
› A very eccentric brown dwarf coplanar to a warm Jupiter and a hot super Earth
› Uncovering the Rapidly Evolving Orbits of the Dynamic TOI-201 System
› East Asian VLBI Network astrometry toward the star-forming region G040.96+02.48 in the Extreme Outer Galaxy
› Reconstructing the cosmic expansion with a generalized q(z) parameterization: A decelerating Universe from late-time constraints
› The Operation Control System for the Tianlai Experiment
› LStein: A new approach to visualizing sparse 2.5-dimensional data
› A sound-horizon-free measurement of the Hubble constant from DESI DR2 baryon acoustic oscillations using artificial neural networks
› Clash of the Trident and Tuning Fork: insights from bar and spiral strength in the (massive black hole)-stellar mass diagrams, and the `Triangal' galaxy evolution schema
› A Morphological Identification and Study of Radio Galaxies from LoTSS DR2. III. The Multiwavelength Analysis of Winged Radio Galaxies
› Physical Parameters of 146 Contact Binaries Derived from Light and Radial Velocity Curves
› The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from the Murchison Widefield Array (MWA) drift scan observations -- III. Improved upper limits at $z = 8.2$ from multiple pointings
› The Three Hundred project: cosmic web identification from 2D gas and Compton-$y$ maps of galaxy clusters outskirts
› The SOXS Spectrograph Instrument Control Software
› The Microchannel X-ray Telescope on board the SVOM mission: in-flight scientific performance
› The data analysis pipeline for the Microchannel X-ray Telescope on board the SVOM mission
› SVOM/VT: Instrument Overview, Science Objectives, and First-Year Performance
› ECLAIRs: the SVOM high-energy transient trigger camera
› The SVOM French Science Center Infrastructure
› SVOM Science User Support Services at Chinese Science Center
› SVOM Science User Support at FSC
› SVOM/ECLAIRs detection plane: main features and performance
› The SVOM / ECLAIRs Scientific Analysis Pipeline
› Overview of the ECLAIRs Trigger for SVOM gamma-ray burst detection
› SVOM/VT: Preliminary Calibration Analysis
› The SVOM mission, its profile and its system
› SVOM Ground Support System
› COLIBRI (SVOM/FM-GFT): Instrumentation and Performances on the SVOM Alerts
› Overview of Ground-based Wide-Angle Cameras array
› The coded mask of the ECLAIRs telescope onboard the SVOM space mission
› In-flight performance of the MXT Camera
› The VHF alert network of the SVOM mission
› Alert Chain and Observation Planning for Ground Wide Angle Camera Network
› SVOM Real-time Response and Collaboration System
› SVOM/VT: Overview of data processing and GRB identifications with X-band data
› GRM Scientific Pipeline
› SVOM/VT: Flight Model Verification and Pre-launch Testing
› SVOM/VT: Real-Time Onboard Data Processing
› SVOM/VT: On-ground processing of VT-VHF data
› SVOM/C-GFT: Instrumentation and Performances on the SVOM Alerts
› The GRB joint scientific analysis pipeline of the ECLAIRs and GRM instruments on board SVOM
› Thermal instability in coronal loops: linking eigenvalue spectra to time-dependent evolution
› The FLAMINGO simulations data release
› Recovering extra-tidal open cluster members via multi-elemental chemical tagging
› Fates of the sub-stellar objects (FOSSO) II. Evidence for Suppression of Metal Pollution in White Dwarfs by Close Substellar Companions
› pyTANSPEC v1.0 and HxRGproc: Updated packages to Clean and Reduce TANSPEC data
› The long-term outburst(s) of GPSV16: from an intermediate to a FUor classification
› The formation of circumbinary planets through disc fragmentation
› Propagating data-driven galaxy redshift distribution uncertainties in 3$\times$2-pt analyses
› CSST Preparations: Galaxy Completeness and S\'ersic Profile Fitting across the Wide, Deep, and Extreme Fields
› Robust Angles-Only Initial Relative Orbit Determination Using Polynomial Optimization
› Mapping the Milky Way with Gaia Bp/Rp spectra-IV: the broken and asymmetric density profile of the stellar disk traced by a large sample of red clumps
› An archive of reduced and telluric-corrected CRIRES+ L- and M-band spectra with slit-tilt and wavelength calibrations
› Machine learning technique for morphological classification of galaxies from SDSS. IV. Visual inspection vs CNN for merging, irregular, edge-on, barred, ringed, and with dust lanes galaxies at 0.02
› Hidden oscillations in plain sight: identification of seismically unresolved red-giant asteroseismic binary candidates
› Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation
› Analyses on Wassenius' Report for Total Solar Eclipse in 1733: Quantifications of the Solar Radius and the Earliest Reported Prominences
› Aromatic rings in the Central Molecular Zone: Benzonitrile
› StarCLR: Contrastive Learning Representation for Astronomical Light Curves
› The spin state of asteroid Apophis and a prediction of its change during the 2029 close encounter with Earth
› Investigating interstellar dust along the line of sight of GX 13+1 using different dust size distributions
› A Theoretical Study of the Structure and Elemental Abundances of HD 20794
› Mars Thermospheric Polar Warming at Aphelion: Dynamical Processes Studied Using M-GITM
› Accurate distances of the Galactic spiral arms from dust-scattered X-ray emission of gamma-ray bursts
› Nonparametric Variational Inference Reconstruction of the Cosmic Expansion History from SNe Ia -- the \texttt{charm2} code
› Measurement of the Weyl Potential Evolution and $E_G$ Statistic from KiDS-1000, BOSS and 2dFLenS
› \texttt{SWIM}: Stochastic Warm Inflation Module to generate and analyse Warm Inflationary power spectrum
› Halfway to the Peak: Kinematic Signatures of Stable Rotating Disks in Luminous Infrared Galaxies at z=0.5-0.6
› Dynamical Modeling of the Broad-Line Region with High-Mass Active Galactic Nuclei and Constraints on the Virial Factor
› Analysis of the Gaia DR3 planetary nebula candidates and the possible symbiotic stars among them
› Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
› Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
› The lifetime of 100,000 molecular clouds in the nearby Universe
› Cosmological Impact of Redshift-Dependent Type Ia Supernovae Calibration
› Integrated Lander-Propulsion-GNC Framework for Autonomous Lunar Powered Descent
› Effect of total dose proton irradiation on the performance of Kinetic Inductance Detectors for far-Infrared space observatory
› Physics informed operator learning of parameter dependent spectra
› Pre-localization of Massive Black Hole Binaries in the Millihertz Band
› Tests of scalar polarizations with multi-messenger events
› A systematic evaluation of vision-language models for observational astronomical reasoning tasks
› Fokker-Planck entropic force interpretation of galactic rotation curves
› Predicting Potential Host Galaxies of Supermassive Black Hole Binaries Based on Stellar Kinematics in Archival IFU Surveys
› Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
› Effect of Thermal Emission in Isotropic Scattering Atmospheres: An Invariant-Embedding Extension of Chandrasekhar's $H(\mu)$-Function
› Interstellar dust production, destruction and effects of dust depletion in galaxies
› Stochastic Inflation with Interacting Noises
› VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets
› Kilonovae and Long-duration Gamma-ray Bursts
› A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos
› Cross-correlations between the CLAMATO Lyman-alpha forest and galaxies within the COSMOS field
› 3I/ATLAS: In Search of the Witnesses to Its Voyage
› Constraints of dynamical dark energy models from different observational datasets
› Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments
› Harrison-Zeldovich attractor: From Planck to ACT results
› The CatWISE2020 Quasar dipole: A Reassessment of the Cosmic Dipole Anomaly
› Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension
› Evolution of action-space coherence in a Milky Way-like simulation
› Constraining interacting dark energy models with black hole superradiance
› Tachyonic dark energy- Constraints from current observations
› DESI-DR1 $3 \times 2$-pt analysis: consistent cosmology across weak lensing surveys
› Pulsed radio emission from a Central Compact Object
› SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
› Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN
› Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks
› What Understanding Means in AI-Laden Astronomy
› Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
› Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass
› The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
› Weak Lensing Low Multipoles
› The kinematic cosmic dipole beyond Ellis and Baldwin
› Cosmology with one galaxy: An analytic formula relating $\Omega_{\rm m}$ with galaxy properties
› Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies
› Fermi-LAT 16-year Source List
› A dynamical attractor in the evolution of dwarf spheroidal galaxies
› Fundamental properties of protoplanetary discs determined from simultaneous fits to thermal dust images and spectral energy distributions
› Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
› The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas
› Modeling the Accretion of High-Velocity Clouds from a Rotating Halo
› Distribution function-based modelling of discrete kinematic datasets, in application to the Milky Way nuclear star cluster
› A Five-Stage Framework for Slitless Grism Spectra: Demonstrated on Euclid Q1 Strong-Lens Candidates and Ported to CEERS NIRCam
› The Distribution of Cosmic Ray Electrons in Star-Forming Galaxies
› Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
› Plasma Dynamics of Radiative Cooling Accretion Flow in AM Herculis with XRISM
› Secular Light Curve of Exocomet 3I/ATLAS, and its Location on a Comet Evolutionary Diagram
› A Path to Constraints on Common Envelope Ejection in Massive Binaries: Full Evolutionary Reconstruction of Three Black Hole X-ray Binaries
› The demise of the synchronous moon that gave Mars its triaxiality. The role of solar tides and a palaeo ocean
› Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints
› The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
› Kardashev's Conundrum: Statistical Falsification of the Standard Kardashev Model and the Kardashev--Sagan--Nakamoto Resolution
› Ice as a Photochemical Shield: Adsorption Energetics and Spectroscopic Modulation of Interstellar Thiocyanates HCSCN and HCSCCH in TMC-1
› Study on the detector energy response of SVOM/GRM
› The Gamma-Ray Monitor onboard the SVOM satellite
› Stability of Multiplanet Systems Through Hot Jupiter Destruction
› Purely Quadratic Non-Gaussianity from Tachyonic Instability: Primordial Black Holes and Scalar-Induced Gravitational Waves
› Ancient 'ghost' planetary nebulae discovered with amateur telescopes
› Cosmological Gravitational Waves from Ultralight Vector Dark Matter
› An Analytic Threshold for LESA-Driven Negative ELN Flux Directions in Core-Collapse Supernovae: Derivation and Population Census
› Signature of iron line profile from a Kerr-like wormhole
› Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy
› First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST
› Cosmological Implications of Affine Gravity
› Spinfoams, $\gamma$-duality and parity violation in primordial gravitational waves
› Scalar Thermal Field Theory for a Rotating Plasma
› A Quantal Theory of Restoration of Strong CP Symmetry
› Magnetic field dynamics in presence of Hall conductivity and thermal diffusion
› Complete reflection of nonlinear electromagnetic waves in underdense pair plasmas enabled by dynamically formed Bragg-like structures
› High-Quality Axion Dark Matter at Gravitational Wave Interferometers
› Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary
› Dark Matter Freeze-in from a $Z^\prime$ Reheaton
› Extreme-mass ratio inspirals in Schwarzschild - de Sitter spacetime I: Weak-field orbits
› New benchmarks for direct detection of freeze-in dark matter in vector portal models
› Reshaping the inner shadow of a Kerr black hole by a torn accretion disk

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