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

Suhora w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
-- °C
Wilgotność
--%
Wiatr
-- km/h
Ciśnienie
-- hPa

Księżyc
Najnowsze prace na astro-ph:
›
Towards Mitigating Systematics in Large-Scale Surveys via Few-Shot Optimal Transport-Based Feature Alignment ›
Non-Parametric Reconstruction of the Hubble Parameter from the Fourth Gravitational Wave Transient Catalog and DESI Baryonic Acoustic Oscillations ›
Hydrodynamic instabilities in long-term three-dimensional simulations of neutrino-driven supernovae of 13 red supergiant progenitors ›
Rock vapour is opaque: implications for dynamics and observations of lava planets ›
Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancy ›
LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS ›
KDP as a thermal blocking filter - Deep near IR observations with a warm narrow band filter ›
Inflation without an Inflaton II: observational predictions ›
On the coincidence between the close passage of HD7977 and the Pliocene-Pleistocene transition ›
The Transition from Giant Planets to Brown Dwarfs beyond 1 au from the Stellar Metallicity Distribution ›
ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at $z = 3.1$ ›
Infrared Signatures of Dusty Tori Formed by MHD-Driven Outflows ›
Modeling X-ray photon pile-up with a normalizing flow ›
A new estimate of the zero-point shift of the Gaia DR3 parallaxes obtained from a comparison with VLBI measurements of masers and radio stars ›
Disk mass predictions for binary neutron star mergers: limitations of proposed symbolic regression models ›
The Atmospheric Response to Large Electron Beam Fluxes in Solar Flares III: Comprehensive Modeling of the Brightest Observed Near-Ultraviolet Continuum Source in an X9 Solar Flare ›
PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies ›
Through the Heliospheric Lens: Directional Deflection of High-Energy Cosmic-Ray Electrons and Positrons ›
Euclid Quick Data Release (Q1): Identification of massive galaxy candidates at the end of the Epoch of Reionisation ›
SourceREACH (Source REconstruction of Arcs behind Cluster Halos): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses ›
Functionality of Ice Line Latitudinal EBM Tenacity (FILLET). Protocol Version 1.1 ›
Formation of Close Binaries through Massive Black Hole Perturbations and Chaotic Tides ›
First Light And Reionisation Epoch Simulations (FLARES) XX: Comparing semi-analytic models at high-redshift ›
He-star donor pathway for the hypervelocity star D6-2 ›
The Impact of Orbital Anisotropy Assumptions in Lensing-Dynamics Modeling ›
Gravitational wave standard sirens from GWTC-3 combined with DESI DR2 and DESY5: A late-universe probe of the Hubble constant and dark energy ›
Dual core system candidates: a sample of objects with large velocity offset between absorption and narrow emission lines ›
3D extinction maps of the Milky Way disc from Gaia GSP-Spec parameters ›
Chemically primitive dwarf accretion reignites the inner disk assembly of Malin 1 ›
Doppler imaging combined with high-cadence photometry. I. Revisiting the surface of a pre-main-sequence flare star ›
High-impact Scientific Software in Astronomy and its creators ›
Metallicity Effects on Machine Learning Classification of Dusty Stellar Sources in the Magellanic Clouds ›
Implications of Mini-EUSO measurements for a space-based observation of UHECRs ›
Pre-Supernova Multiple Giant Eruptions in Massive Stars ›
Clustering effects on the Dark Siren determination of $H_0$: A simulation study ›
AstroMLab 5: Structured Summaries and Concept Extraction for 400,000 Astrophysics Papers ›
QuaRT: A toolkit for the exploration of quantum methods for radiation transport ›
Characterization of type Ibn SNe ›
The X-$\gamma$ detector onboard the POEMMA-Balloon with Radio payload ›
Examining Turbulence in Galactic Molecular Clouds - II: Continuity of Turbulence Cascading in a Portion of the Local Arm ›
Made-to-Measure Outperforms Schwarzschild's Method ›
The influence of AGN feedback on star formation in red spiral galaxies ›
Spectral-Timing Evolution of a Black hole X-ray binary Swift J1727.8-1613: Linking Disk Reflection and Type-C QPO Frequency During the 2023 Outburst ›
Detection of disk-jet co-precession in a tidal disruption event ›
Mock Observations for the CSST Mission: Multi-Channel Imager--Instrument Simulation ›
Mock Observations for the CSST Mission: Integral Field Spectrograph--Instrument Simulation ›
The first AKRA mass map reconstruction from HSC Y1 data ›
Unraveling eMSTO in NGC 2355: Stellar Rotation and Binaries ›
The homogeneity scale in the Local Universe: model-independent estimate from S-PLUS DR4 blue galaxies ›
Sub-millimeter galaxies in hierarchical models: revisiting the need for a top-heavy stellar initial mass function with Bayesian optimisation ›
Simulations of structured upflows from plumes and their connection to the solar wind ›
IdentYS: A Python-Based Tool for Identifying Young Stars in Star-Forming Regions ›
The Chandra Strong Lens Sample: Measuring the Dynamical States and Relaxation Fraction of a Sample of 28 Strong Lensing Selected Galaxy Clusters ›
Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping" ›
From Images to Physics: Probabilistic Inference of Galaxy Parameters and Emission Lines via VAE & Normalizing Flows ›
Observations of Five Southern-Hemisphere Cataclysmic Binary Stars ›
On the Temporal Variability in the Magnetic Dichotomy of Late M Dwarf Stars ›
Orbital Eccentricities Suggest a Gradual Transition from Giant Planets to Brown Dwarfs ›
Modeling stellar convective transport with plumes : II. Transport Properties of Locally and Non-locally driven Convection ›
Near-infrared [P II] and [Fe II] line mapping of Galactic supernova remnants ›
SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material ›
Orbit Elements from Kepler Solutions in Projective Coordinates ›
Helical Magnetic Field in the Acceleration--Collimation Zone of the M87 Jet ›
AGN feedback in merging galaxies with a SMUGGLE multiphase ISM ›
Thermal infrared characterization of spatially unresolved resident space objects: Prospects from analytical two-component modeling ›
Reheating and Inflationary dynamics driven by an inverse tangent potential ›
The B[e] Phenomenon in Supergiants. A Result of Mass Transfer in Binaries, Mergers, or What? ›
Topological Signatures of Heating and Dark Matter in the 21 cm Forest ›
Wide-Field X-ray Polarimetry for High Energy Astronomical Transients: First results of the pathfinder CXPD Cubesat Mission ›
Prospects for detecting periodic or sharp fast-time features in the supernova neutrino lightcurve with IceCube ›
Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo ›
Infrared photometry and CaT spectroscopy of the most metal-poor in-situ globular cluster VVV-CL001 ›
Spectral component imaging of solar X-ray flares ›
Probing the Nature of Dark Matter Self-Interactions Through Observations of Massive Black Hole Mergers ›
Natural gradient descent for improving variational inference based classification of radio galaxies ›
The Spontaneous Genesis of Solar Prominence Structures Driven by Supergranulation in Three-Dimensional Simulations ›
Vortex creep heating in neutron star cooling with direct Urca processes in heavy neutron stars ›
TransFit-CSM: A Fast, Physically Consistent Framework for Interaction-Powered Transients ›
Unveiling the nature of the Einstein Probe transient EP 241021a ›
Multiple Components and Spectral Evolution of BL Lacertae as Revealed by Multiwavelength Variability and SED Modeling ›
Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions ›
Stray Light Correction for the Helioseismic and Magnetic Imager ›
Constraining the Neutral Hydrogen Fraction from SKA Simulated Observation using a Double-Gaussian Decomposition Technique ›
Constraining r-process nucleosynthesis with multi-objective Galactic chemical evolution models ›
An Unusual Velocity Field in a Sunspot Penumbra ›
PDRs4All XX. Haute Couture: Spectral stitching of JWST MIRI-IFU cubes with matrix completion ›
Cosmic Expansion Driven by Gravitational Particle Production: Toward a Complete Cosmological Scenario ›
Learning Cosmology from Nearest Neighbour Statistics ›
The PAH 3.4 micron feature as a tracer of shielding in the Orion Bar and NGC 6240 ›
Investigating magnetic activity cycles in solar-like oscillators using asteroseismic data from the K2 mission ›
Magnetic fields in the close neighborhood of LDN 328 core ›
Shaping the Mantle: The Role of Superheated Cores After Giant Impacts ›
The bulk metal content of WASP-80 b from joint interior-atmosphere retrievals: Breaking degeneracies and exploring biases with panchromatic spectra ›
High Resolution Observations of CO(3-2) in Haro 2: Cool Molecular Outflows of a Ly$\alpha$ Emitter ›
A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy ›
High-Precision Multi-Period Analysis of the Ellipsoidal Variable Candidate TIC~470127886 from TESS Photometry ›
Statistical analysis of eclipsing binaries with monotonic orbital-period variations: A-type W UMa contact systems ›
Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet ›
Sense and Sensitivity - I. Uncertainty analysis of the gas-phase chemistry in AGB outflows ›
JWST observes the assembly of a massive galaxy at z~4 ›
High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4 ›
A model-independent assessment of the late-time dark energy density evolution ›
Investigating the Dark Energy Constraint from Strongly Lensed AGN at LSST-Scale ›
The hard ultraluminous state of NGC 5055 ULX X-1 ›
The physical properties of post-mass-transfer binaries ›
The Scatter of the Many Outweighs the Scatter of the Few: Systematic Error Asymmetry in Steeply-Falling Mass Functions for High-Redshift JWST Galaxies ›
Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs ›
On Bayesian inference considerations and other issues concerning Drake's equation of Astrosociobiology ›
Kerr-Bertotti-Robinson Black Holes Surrounded by a Cloud of Strings ›
Relativistic Maxwell-Bloch Equations with Applications to Astrophysics ›
Testing general relativity with amplitudes of subdominant gravitational-wave modes ›
Symmetric Bimetric Cosmology: A Minimal Extension of {\Lambda}CDM ›
Upper Bound on the Cosmic Baryon Chemical Potential from Lepton-Flavor Asymmetry ›
Spin precession effects in the phasing formula of eccentric compact binary inspirals till the second post-Newtonian order ›
The Engineering and Programming Methods Used in Manufacture of Astrolabes and Errors Resulting ›
Quintessence: Quadratic potentials ›
From the Virgo interferometer calibration to the bias and uncertainty of the h(t) detector strain during the O4 run ›
Auto-encoder model for faster generation of effective one-body gravitational waveform approximations ›
Thermal Quarkyonic Matter and Its Implications for Neutron Star Structure ›
The Great January Comet of 1910 (C/1910 A1): A Key Opportunity Missed by New Zealand Astronomers ›
Efficient Reconstruction of Matched-Filter SNR Time Series from Nearby Templates ›
Chiral Magnetic Effect induced Spectator Process for Leptogenesis ›
Towards an anomaly detection pipeline for gravitational waves at the Einstein Telescope ›
Sub-Solar Mass Intermediate Mass Ratio Inspirals: Waveform Systematics and Detection Prospects with Gravitational Waves ›
The Birth of Gravitational Particle Creation: the Enduring Legacy of Leonard Parker's 1966 Thesis ›
Bimodular Gravity: Unimodularising Bimetric Scalar-Tensor Gravity ›
Variable-temperature attenuator calibration method for on-wafer microwave noise characterization of low-noise amplifiers ›
Gravitational--Electromagnetic Coupling on Kerr Spacetime ›
In-orbit background and sky survey simulation study of POLAR-2/LPD ›
Redshift Drift fluctuations from N-body simulations ›
Discovering High-$z$ BL Lacs Using Swift/UVOT and SARA Observations with the Dropout Technique ›
3D Modeling of Moist Convective Inhibition in Idealized Sub-Neptune Atmospheres ›
Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems ›
The 3D pulsar magnetosphere with machine learning: first results ›
Water-rich sub-Neptunes and rocky super Earths around different Stars: Radii shaped by Volatile Partitioning, Formation, and Evolution ›
Constraints on the $z\sim6-13$ intergalactic medium from JWST spectroscopy of Lyman-alpha damping wings in galaxies ›
The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers ›
Complementary signatures of $\alpha-$attractor inflation in CMB and cosmic string Gravitational Waves ›
A Bayesian estimator for peculiar velocity correction in cosmological inference from supernovae data ›
The role of triple evolution in the formation of LISA double white dwarfs ›
The role of turbulence in setting the phase of the ISM and implications for the star formation rate ›
Precision cross-sections for advancing cosmic-ray physics and other applications: a comprehensive programme for the next decade ›
A Multi-Site Study of Radio Environment for Cosmology Experiments ›
A possible correction of the Saha curve for non-equilibrium states ›
A weak Ly$\alpha$ halo for an extremely bright Little Red Dot: Indications of enshrouded SMBH growth ›
Displacement of ultra-high-energy cosmic ray source images by the intergalactic magnetic field: the cases of Cen A and M83 ›
Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background ›
TasVisAn and InsPy -- Python Packages for Triple-Axis Spectrometer Data Visualization, Analysis, Instrument Resolution Calculation, and Convolution ›
The fate of Quasi-Exponential inflation in the light of ACT-DR6 ›
Reconstructing dark energy with model independent methods after DESI DR2 BAO ›
Asteroids fail to retain cometary impact signatures ›
Ruling Out Dark Energy Model induced by de-Sitter Regions of Non-Singular Black Holes with Planck2018, DESI BAO, and Union3 Supernovae ›
The Distribution of Atomic Hydrogen in the Host Galaxies of FRBs ›
Estimating cluster masses: a comparative study between machine learning and maximum likelihood ›
2D End-to-End Modeling of Kilonovae from Binary Neutron Star Merger Remnants ›
A Turbulent Framework for Star Formation in High-Redshift Galaxies ›
Radio Observations of a Candidate Redback Millisecond Pulsar: 1FGL J0523.5-2529 ›
The Dark Energy Camera All Data Everywhere cosmic shear project V: Constraints on cosmology and astrophysics from 270 million galaxies across 13,000 deg$^2$ of the sky ›
Universal Structure of Turbulent Radiative Mixing Layers ›
MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z${\sim}$2 ›
No evidence for local $H_0$ anisotropy from Tully--Fisher or supernova distances ›
Bayesian Framework for the E1 and E2 Astrophysical Factors at 300 keV from Subthreshold and Ground-State Asymptotic Normalization Coefficients ›
Detailed theoretical modelling of the kinetic Sunyaev-Zel'dovich stacking power spectrum ›
Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation ›
New Evidence for Extragalactic Einstein Probe Transients associated with Long Gamma-ray Bursts ›
Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A & EP250207b ›
Energetics of star-planet magnetic interactions: Novel insights from 3D modelling ›
Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model ›
Mock Observations for the CSST Mission: Main Surveys-the Slitless Spectroscopy Simulation ›
JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios ›
The Deepest GLIMPSE of a Dense Gas Cocoon Enshrouding a Little Red Dot ›
Effect of molecular hydrogen self-shielding modeling on early Reionization Era galaxies in radiative hydrodynamic cosmological simulations ›
Stellar Populations with MaNGA: Iron Kink and Nitrogen Fuzz ›
Probing Time-Dependent Physics with Phase-Folding CMB Maps ›
JWST View of the Supernebula in NGC 5253. II. Nebular Lines ›
Ginnungagap -- a massively parallel cosmological initial conditions generator ›
A new multiprobe analysis of modified gravity and evolving dark energy ›
Hydrogen-line profiles from accreting gas giants and their CPDs ›
A 34.6-day transiting sub-Neptune in the TOI-1422 planetary system ›
Tests of General Relativity with GWTC-3 ›
The need for a nonlocal expansion in general relativity ›
Complementarity between Cosmic String Gravitational Waves and long-lived particle searches in a laboratory ›
Dynamical Solution to the Eta Problem in Spectator Field Models ›
Non-interacting holographic dark energy with Torsion via Hubble Radius ›
Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions ›
Quintessential Inflation in Palatini $F(R,X)$ gravity ›
Black hole quasinormal mode resonances ›
Insights on the Cosmic Origin of Matter from Proton Stability ›
MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity ›
The Fast and the Frame-Dragging: Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly-spinning black holes ›
High-Precision Relativistic Time Scales for Cislunar Navigation ›
Automated Algorithmic Discovery for Scientific Computing through LLM-Guided Evolutionary Search: A Case Study in Gravitational-Wave Detection ›
Modified Black Hole Potentials and Their Korteweg-de Vries Integrals: Instabilities and Beyond ›
Is the $\Lambda$CDM Model in Crisis? ›
Importance of being nonminimally coupled: Scalar Hawking radiation from regular black holes ›
Conserved Quantities in Expanding G\"odel Cosmology ›
Imaging and polarization patterns of various thick disks around Kerr-MOG black holes ↓↑