ul. Podchorążych 2, 30-084 Kraków.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Obserwatorium Astronomiczne na Suhorze

Niebo nad obserwatorium

Chmury

Opady

Niebo
Temperatura
6.3 °C
Wilgotność
80%
Wiatr
12.9 km/h
Ciśnienie
1018.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Solar neutron and muon detection on November 11, 2025: First simultaneous recovery of energy spectra ›
SATMO: a Multi-Planet Thermal Analysis Tool for CubeSat Missions ›
The interstellar signature: A computational framework for open source interstellar tracking ›
Microlensing Signatures of Dyson Sphere-like Structures around Primordial Black Holes as Technosignatures of Extraterrestrial Advanced Civilizations ›
Evidence for evolving Dark Energy from a new cosmic probe ›
Probing the Warm Dark Matter mass with [C II] intensity mapping ›
Detection of 27 Candidate Circumbinary Planets Through Apsidal Precession of Eclipsing Binaries Observed by TESS ›
On the Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A ›
Detecting Neutrino Emission from Supernova Remnants: A Theoretically Motivated Target Catalog ›
The HIP 54515 b Superjovian Planet as an Early, Critical Look at the Roman Coronagraph's Performance in the Faint Target Star, Small IWA Limit ›
The mass-to-flux ratio in molecular clouds. What are we really measuring? ›
Heavy element enriched atmospheres and where they are born ›
On the missing dust of super-early galaxies: Supernova blowout and gas-dust venting in Blue Monsters ›
How is cold, star-forming gas in galaxies affected by magnetic fields? ›
The dynamic central environment of NGC 3516 revealed by XRISM ›
LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7 ›
Tracing Nitrogen Enrichment across Cosmic Time with JWST ›
Forecasting Dark Matter Subhalo Constraints from Stellar Streams using Implicit Likelihood Inference ›
Probing Infrared eXcess to Investigate Early-Universe Dust (PIXIEDust) ›
von Zeipel-Kozai-Lidov oscillations in nearby bright stars. I. Lambda Ophiuchi ›
Stellar Multiplicity via Speckle Interferometry with the 3.6 m Devasthal Optical Telescope ›
Chemical Signatures of AGB Mass Transfer in Gaia White Dwarf Companions ›
Danger Zone: Establishing Buffers for Enhanced Classification in BPT Diagrams ›
Growth and thermal evolution of icy planetesimals ›
Was the Solar System's dynamical instability triggered by a (sub)stellar flyby? ›
SAGAN-VI: When Jets Meet Filaments -- Environmental Imprints on the Growth of Giant Radio Galaxies ›
Analytical Solutions for the Dynamics of Planetary Nebulae with and without Common Envelope Evolution ›
Can meridional flow variations explain the observed rising/declining phase asymmetry in the solar cycle? ›
The Drivers of the Decline in Supermassive Black Hole Growth at $z ›
The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis ›
UVOIR spectrum, X-ray emission, and proper motion of the isolated neutron star RX J2143.0+0654 ›
Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z>6 Galaxy, the Strongly Lensed Cosmic Spear at z=6.2 ›
The Two-Infall Model Revisited: Constraints on Milky Way Bulge Assembly from >30,000 Galactic Chemical Evolution Models and Machine Learning ›
The SOFIA Massive(SOMA)Radio Survey. III. Radio Emission from Intermediate-Mass Protostars ›
The MAGPI Survey: forward modelled gas-phase metallicity gradients in galaxies at $z\sim 0.3$ ›
Improvements to the NSO Farside Mapping Pipeline: Noise Reduction Updates ›
Inferring main-sequence stage and buoyancy-glitch amplitudes from Fourier spectra of gravity-mode period spacings: Ensemble Analysis of 26 Slowly Pulsating B Stars ›
Estimation of the Hubble parameter from unedited compact object merger catalogues ›
NEOWISE data and Thermophysical Modeling of 98943 Torifune (2001 CC21) ›
Follow-up Observations of Candidate White Dwarf Planets with MIRI ›
Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XV. Reverberation Mapping of Mg II Emission Lines ›
First detection of X-ray polarization from the long-period X-ray pulsar 4U 1954+319 ›
Supernovae Shock Breakout from Red Supergiants in Two Dimensions ›
The Birth of Be Star Disks II. A High-Resolution Spectroscopic Campaign and TESS Observations of an Outburst of the Classical Be star {\lambda} Pavonis ›
The Head-on Collision of a Neutron Star with a White Dwarf ›
The Impact of Irradiation on the Radius and Thermal Evolution of Transiting Brown Dwarfs ›
The Milky Way Imaging Scroll Painting Survey: Data Release 1 ›
Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays ›
Magnetic activity of ultracool dwarfs in the LAMOST DR11 ›
Machine learning classification of baseband data of CHIME FRBs ›
PolySwyft: sequential simulation-based nested sampling ›
Extremely energetic EUV late phase of a pair of C-class flares caused by a non-eruptive sigmoid ›
Kick & spin: new probes for multi-messenger black-hole mergers in AGNs ›
Chemical analysis of the Milky Way's Nuclear Star Cluster: Evidence for a metallicity gradient ›
Photochemistry of interstellar ice forming Complex Organic Molecules ›
Collisional rate coefficients for OH-H$_2$ at high temperatures ›
Self-lensing flares from black hole binaries V: systematic searches in LSST ›
Photon Dynamics and Collision Risks in Relativistic Spaceflight: A Comparative Study of Methods and Implications ›
Delving into the depths of NGC 3783 with XRISM III. Birth of an ultrafast outflow during a soft flare ›
Globular Cluster Systems in Dwarf Galaxies: Catalogs and Comparisons ›
J-PAS: First Identification, Physical Properties and Ionization Efficiency of Extreme Emission Line Galaxies ›
Relativistic MHD simulations of merging and collapsing stars and effects on GRB transient ›
Investigating ionising sources and the complex interstellar medium of GHZ2 at $z=12.3$ ›
Supervised Classification of LEO Debris Families Using Multi-Set Proper Elements ›
Radiation pressure instability: from heart-beat states in black hole binary systems to Quasars and Changing-Look AGN ›
Small-scale bright point characteristics at high-resolution with the Daniel K. Inouye Solar Telescope ›
Measuring the diffuse Galactic synchrotron spectral index and curvature between 45 and 2300 MHz ›
A Search for Transit Duration Variations in M dwarf Multi-Planet Systems ›
NICER Perspective on TeV Blazar Mrk~421: X-ray Variability and Particle Acceleration ›
Astrometric Reconnaissance of Exoplanetary Systems (ARES). I. Methodology validation with HST point-source images of Proxima Centauri ›
High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA ›
The Two-Dimensional Structure of Circumplanetary Disks and their Radiative Signatures ›
HI-detected Dwarf Galaxies in the FASHI Survey: Insights from Single- and Double-Peaked Emission-Line Samples ›
Predicting Quasar Counts Detectable in the LSST Survey ›
Pulsars identified in the LOFAR Two-metre Sky Survey at 144 MHz ›
Stochastic gravitational-wave background search using data from five pulsar timing arrays ›
Low-Mass Neutron Stars and Effective Phase Transitions from a Hybrid Van der Waals-Polytropic Equation of State ›
A magnetar outburst with atypical evolution: the case of Swift J1555.2-5402 ›
The frame-dragging vector potential on galaxy scales from DM-only Newtonian $N$-body simulations ›
Thermal design of focal plane assembly of wavefront camera for exoplanet imaging corona module ›
Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections ›
Neutrino mass constraints in the context of 4-parameter dark energy equation of state and DESI DR2 observations ›
Backwards Gamma-Ray Bursts: Searching for Exploding Primordial Black Holes in Short-Duration GRB Catalogs ›
Neutrino pair bremsstrahlung due to electromagnetic collisions in neutron star cores revisited ›
The Radius of PSR J0437-4715 from NICER Data ›
Predicting Infall Time of Milky-Way Satellites via Machine Learning ›
Euclid Quick Data Release (Q1): Euclid spectroscopy of QSOs. 1. Identification and redshift determination of 3500 bright QSOs ›
FIRESTORM I: Stellar Feedback and Gas Kinematics in the Evolved W40 Hub-Filament System ›
Probing the environment around GW170817 with DESI: insights on galaxy group peculiar velocities for standard siren measurements ›
Exploring the binary origin of B and Be rapid rotators ›
A search for successful and choked jets in nearby broad-lined Type Ic supernovae ›
Near-IR CO and CN in classical Cepheids ›
Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy ›
The impact of lunar topography on the 21-cm power spectrum for grid-based arrays : Insights for the Dark-ages EXplorer (DEX) ›
Foreground Mitigation for CMB Lensing with the Global Minimum Variance Quadratic Estimator ›
Resolving the (Debate About) Nozzle Shocks in Tidal Disruption Events ›
Hot Jupiters are Inflated Primarily by Shallow Heating ›
Core-halo scaling relations in self-interacting scalar field dark matter ›
Impact on orbital period of X-ray Binary system attached to a cosmic string ›
Infrared Freeze-In of Magnetic Dipole Dark Matter ›
Inflationary Particle Production and the Swampland ›
Open Effective Field Theory and the Physics of Cosmological Collider Signals ›
Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement ›
Noble gravitational atoms: Self-gravitating black hole scalar wigs with angular momentum number ›
High-overtone ringdown fits: start time, no-hair tests, and correlations ›
Probing Cosmic Strings via Black Hole Quasinormal Modes in Gravitational Wave Astronomy ›
Careless Whispers: A population of sub-threshold post-merger gravitational waves constrains the hot nuclear equation of state ›
On the existence of bound states in SIMP dark sectors ›
Time-Averaged Template for Stochastic Gravitational-Wave Background Detection in Space-Based Interferometers ›
Superluminal constraints from ultra-high-energy neutrino events ›
Dark Photons in the Early Universe: From Thermal Production to Cosmological Constraints ›
Centrifugal instability of Taylor-Couette flow in stratified and diffusive fluids ›
Single-field D-type inflation in the minimal supergravity in light of Planck-ACT-SPT data ›
The Strong-$CP$ Problem and its Gauge Axion solution as Evidence for Fundamental Strings ›
A Bayesian Approach Study of Hybrid Neutron Stars ›
Near-infrared Variability Detected in the Young Star-Forming Dwarf Galaxy SBS 0335-052E ›
Particle acceleration and multi-messenger radiation from Ultra-Luminous X-ray Sources: A new class of Galactic PeVatrons ›
Andromeda's tenuous veil: A likely Milky Way nebula projected toward M31 ›
Exploring sub-GeV Dark Matter Physics with Cosmic Ray and Future Telescopes ›
Euclid: Quick Data Release (Q1) - A photometric search for ultracool dwarfs in the Euclid Deep Fields ›
Smooth sailing or ragged climb? -- Increasing the robustness of power spectrum de-wiggling and ShapeFit parameter compression ›
Isotropy Test with Quasars Using Method of Smoothed Residuals ›
Shapes and orientations of massive halos in the statistically anisotropic universe ›
Core Collapse Beyond the Fluid Approximation: The Late Evolution of Self-Interacting Dark Matter Halos ›
Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for $3 ›
Testing stellar yield prescriptions in OMEGA+: Implications for rising sodium abundances in young thick disc stars ›
Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk ›
Thermochemical models of outer core convection with heterogeneous core-mantle boundary heat flux ›
Robust Extraction of Global 21 cm Spectrum from Experiments with a Chromatic Beam Based on Physics-Motivated Error Modeling ›
Transient QPOs of Fermi-LAT blazars with Linearly Multiplicative Oscillations ›
Assessing Universal Relations for Rapidly Rotating Neutron Stars: Insights from an Interpretable Deep Learning Perspective ›
The Mass of Cosmic Rays of Ultra High Energy ›
Hot, cold, and multi-component accretion flows around supermassive black hole binaries ›
SMILES Data Release II: Probing Galaxy Evolution during Cosmic Noon and Beyond with NIRSpec Medium-Resolution Spectra ›
Molecular Hydrogen in High-redshift Damped Lyman-{\alpha} Absorbers ›
Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background ›
Disentangling Multiple Gas Kinematic Drivers in the Perseus Galaxy Cluster ›
Enhanced radio emission between a galaxy cluster pair ›
A Thick Volatile Atmosphere on the Ultrahot Super-Earth TOI-561 b ›
CECILIA: Gas-Phase Physical Conditions and Multi-Element Chemistry at Cosmic Noon ›
Probing potential redshift-dependent systematics in the Hubble tension: Model-independent $H_0$ constraints from DESI R2 ›
Hunting Very High-Energy ($>$100 GeV) Emitting High-Synchrotron Peaked Blazars ›
Neutrinos from stars in the Milky Way ›
Photo-$z$ Estimation with Normalizing Flow ›
Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A and EP250207b ›
Relativistic reflection within an extended hot plasma geometry ›
The Hidden Story of Chemical Evolution in Local Star-Forming Nuclear Rings ›
SPHEREx: Aromatics, Aliphatics and PAH Size across the Iris Nebula ›
Sco X-1 as a continuous gravitational waves source: modelling the secular evolution using MESA ›
Is The Trace Anomaly at its Minimum Value at Neutron Star Centers? ›
Accretion Geometry of the New Galactic Black Hole Candidate AT2019wey in the Hard State ›
The Transition from Giant Planets to Brown Dwarfs beyond 1 au from the Stellar Metallicity Distribution ›
Shaping the Mantle: The Role of Superheated Core After Giant Impacts ›
A model-independent assessment of the late-time dark energy density evolution ›
From Flash to Crater: Morphological and Spectral Analysis of the Brightest Lunar Impact on 11 September 2013 using LRO Data ›
The Albedo Problem and Cloud Cover on Hot Jupiters ›
Dynamical Dark Energy in light of DESI BAO and Full-Shape Data ›
Multi-Wavelength Afterglows as Diagnostic Probes of Dense Circumburst Medium in GRBs ›
DESI Strong Lens Foundry V: A Sample of HST-Observed Strong Lenses Modeled with GIGA-Lens ›
Neural Surrogate HMC: On Using Neural Likelihoods for Hamiltonian Monte Carlo in Simulation-Based Inference ›
Superheavy Supersymmetric Dark Matter for the origin of KM3NeT Ultra-High Energy signal ›
Power-Law Bounces in $f(R)$ Gravity: Analysis of the Ekpyrosis and Accelerating Regimes ›
Comparing a Compact-Binary Mass-Shell Model with Select Observed Gravitational Waves ›
Exact Taub-NUT-like Black Holes in Einstein-bumblebee gravity: their thermodynamics and thermodynamic topology ›
Semianalytic calculation of the gravitational wave spectrum induced by curvature perturbations ›
Einstein gravity extended by a scale covariant scalar field with Bekenstein term and dynamical mass generation ›
Holographic Constraints on the String Landscape ›
Cosmological perturbations on an averaged background ›
A theory-agnostic hierarchical Bayesian framework for black-hole spectroscopy: a case study on GW250114 in Einstein-dilaton-Gauss-Bonnet gravity ↓↑