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

widok od południa

Kamerka S

Kamerka N

Niebo
Temperatura
14.1 °C
Wilgotność
65%
Wiatr
0.0 km/h
Ciśnienie
1018.2 hPa

Księżyc
Najnowsze prace na astro-ph:
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First detection of the moving lens effect with ACT and DESI LS ›
The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization ›
The pre-infall bias of subhalos ›
Bulgeless Evolution And the Rise of Discs (BEARD) II. The role of mergers in shaping the Milky Way analogues in TNG50 ›
Mars as an Exoplanet: Lessons from a Planet at the Edge of Habitability ›
Planetary formation tracks on the Hertzsprung-Russell diagram: Visualising the processes of giant planet growth ›
Mapping 3-D Explosive Nucleosynthesis with Type II Supernova Infrared Emission Lines ›
Astrometric exoplanet detection survives solar-like stellar contamination ›
Automating the detection of polarization angle rotations in blazars. Re-analysis of RoboPol data reveals 27 new rotations ›
Directly tracking the re-brightening of a supermassive black hole accretion disk ›
Hyrax: An Extensible Framework for Rapid ML Experimentation and Unsupervised Discovery in the Era of Rubin, Roman, and Euclid ›
Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. III: Hunting for electron-capture supernovae using nebular spectroscopy ›
Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies ›
Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass ›
GRB 260310A/SN 2026fgk: Photometric and Spectroscopic Evolution of a Nearby GRB-Supernova and an Exceptionally Bright Afterglow at z=0.153 ›
Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues ›
Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies ›
How High-Specific-Energy Winds Regulate the Circumgalactic Medium of Dwarf Galaxies ›
High-resolution X-ray spectroscopy with XRISM/Resolve reveals super-Solar abundance ratios in Virgo/M87 ›
Summary of Discussion Sessions from "The Dusty Universe 2025: The Fifth Pandust Conference" ›
Blue Straggler Stars in Old Open Clusters and the Kraft Break ›
Exoplanets in ancient stellar populations: occurrence constraints and hot-Jupiter candidates in the Galactic halo ›
Detection of propadiene (CH$_2$CCH$_2$), propene (C$_3$H$_6$) and non-detection of propane (C$_3$H$_8$) in Jupiter's northern polar stratosphere ›
Optimal mitigation of random telegraph noise for improved photometry at high frame rates ›
IceCube Second Track Data Release IceTracks-DR2: Data from 2008-2022 for Neutrino Source Searches ›
Magnetohydrodynamics Simulations ›
VarWISE: Infrared Variability via NEOWISE Single Exposure Photometry ›
JWST Observations of Starbursts: Molecular Hydrogen Excitation and Disequilibrium in M82 ›
Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact ›
Radiative PIC simulations of relativistic pair plasma: multiple interacting current sheets and turbulent evolution ›
A Cloud-Based Tool for Meteorite Recovery Using Drones and Machine Learning ›
Lossless Compression of Cosmological Information from Type Ia Supernova Distance Measurements ›
Temporal evolution of the circumstellar disk orientation in the transient X-ray pulsar GRO J1008-57 ›
Taking Inventory of the Most Promising Lensed Radio Sources for Constraining Fundamental Properties of Dark Matter ›
Faraday Complexity and Depolarization in LOFAR Two-metre Sky Survey (LoTSS-DR2) Polarized Radio Sources ›
Peculiar velocities at low Galactic latitude ›
Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets ›
Correlation between baryonic process and galaxy assembly bias ›
Constraints on the Crystallinity of Water Ice in Planet-forming Disks from Infrared Scattered-Light Spectra ›
AMPM I. A Targeted Search for Asteroid Mass Primordial Black Hole Microlenses ›
A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau ›
Recombination Thickness as an Uncertainty in Inflationary Observables ›
AMPM II. A Lunar-Mass Primordial Black Hole Microlensing Candidate in the Milky Way Halo ›
Gaia21bja: pre-main sequence star with quasi-periodic bursts ›
Dwarf and Intermediate-Mass Galaxies in MaNGA: Evidence for Different Evolutionary Trends ›
Formation of a nuclear star cluster through the inspiral of globular clusters: A case study of the dwarf elliptical galaxy UGC 7346 ›
Spectro Capture: A Software System for Automated Small-Observatory Spectroscopy ›
Memory burden effect of regular primordial black holes ›
Chromospheric resonator model for sunspot revealed by multi-height observation of umbral wave ›
Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion ›
Prospect of Measuring the Cosmic Dipole by Strongly Lensed Gravitational Waves Associated with Galaxy Surveys ›
Methodological Synergies between Technosignature and UHE Neutrino Searches ›
The Astro2Geo Project I. Radio astrometric offsets correlated with Gamma-ray brightness ›
A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10 ›
Towards inertial-mode helioseismology: Direct sensing of solar rotation at 75 deg latitude and 0.8 Rsun ›
Recent Findings from the Telescope Array Experiment ›
From mass-loss histories to lightcurves: a generalised framework for interaction-powered transients ›
Reassessing the Statistical Necessity of Stellar Velocity Anisotropy in Strong-Lensing Cosmology with Lens-by-Lens Photometric Constraints ›
Mare versus highland lunar impact flash light curve dichotomy ›
Evidence for Intermediate-Mass Black Holes From Microlensing Signatures in CHIME/FRB catalog 2 ›
The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs ›
COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0 ›
Solar Atmospheric Abundances in Space & Time ›
The Small Phased Array DEmonstrator (SPADE) -- Description and first results ›
A Parameterized YSO Accretion Disk Model with Increasing Accretion Rate: Predicted Outburst Lightcurves ›
Magnetized neutron stars: perturbative versus fully-numerical approaches ›
CMB lensing imprints of cosmic voids in DESI Legacy Survey DR9 LRGs with photometric redshift calibration ›
Inflaton Accretion onto Primordial Black Holes During Reheating ›
Domain-wall Quintessence ›
How long can you trust a Starlink TLE? An empirical comparison of SGP4 and high-fidelity propagation against operator-updated truth across a megaconstellation ›
Facing the phase: Gravity-mode offset and buoyancy glitches in red--giant branch stars ›
Latitudinal variations in Neptune's temperature profile observed with ALMA ›
The first IXPE view of the eclipsing ADC source 4U 1822-37 ›
Arm morphology in off-centre barred galaxies ›
New NanoSIMS Multielement Isotope Data Reveal CO Novae As Key Sources Of 13C-rich Presolar Silicon Carbide Grains ›
Probing String-Theory-Inspired Topologies of the Early Universe through CMB Temperature and Polarization Anisotropies ›
Simulating the Convective Urca Process with Multiple Urca Pairs in a Simmering White Dwarf ›
ComPACT: Mass-Redshift Properties of the galaxy cluster catalogue ›
Interacting Dark Sector field theory with phantom crossing ›
TIC 295741342: A Triply-Eclipsing Triple Star System with a Giant Tertiary ›
Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity ›
The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter ›
Galaxy Proximate Damped Lyman-Alpha Systems and HI Reionization Topology in TECHNICOLOR DAWN ›
Spectral classification of brown dwarfs using machine learning ›
The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations ›
Exceptional Points and Resonance in Black Hole Ringdown ›
Structure of the $^8$B and $^8$Li nuclei and the astrophysical $S_{17}(0)$-factor of the $^7$Be($p,\gamma$)$^8$B direct capture process within a three-body model ›
The Majoron Cosmological Window: Dark Matter and Thermal Leptogenesis ›
Magnetic Prandtl number dependence of plasmoid-mediated reconnection ›
Quasinormal modes of Proca and Maxwell fields in $d$-dimensional Schwarzschild-AdS black holes ›
Affine ANEC selects the closed FRW branch for geodesically complete cosmology ›
GstLAL O4 Online Results Paper ›
Elemental Stoichiometry as an Ecological Biosignature with Applications to Life Detection ›
Locality in effective field theory for inflationary soft modes ›
The stability of color-flavor-locked quark matter and massive CFL quark stars ›
Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability ›
A new analysis of the "hep" S-factor and the "hen" cross section ›
A novel pre-inflationary model in view of the lack of angular correlation of CMB ›
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO ›
WIMP-like Dark Matter Without Thermalization At Freeze-Out ›
Direct T_e-based Metallicities of z=2-9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon ›
The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths ›
Sulfur on Venus: Atmospheric, Surface, and Interior Processes ›
Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection ›
Cosmic Ray Ionization of Low-Excitation Lines in Active Galactic Nuclei and Starburst Galaxies ›
Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. I: Luminosity Function, Volumetric Rate ›
DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy ›
Low-Luminosity Type IIP Supernovae from the Zwicky Transient Facility Census of the Local Universe. II: Lightcurve Analysis ›
A Census of Variable Radio Sources at $3\,$GHz ›
The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10 ›
$f$-mode Oscillations for Hyperons and H-dibaryons in Neutron Stars ›
Primordial black holes versus their impersonators at gravitational wave observatories ›
Cosmic-ray impact on optical and mid-infrared emission line diagnostics in NGC 5728 ›
Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A ›
Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra ›
Under Pressure: Decoding the Effect of High Densities on Derived Nebular Properties ›
Addressing prior dependence in hierarchical Bayesian modeling for PTA data analysis II: Noise and SGWB inference through parameter decorrelation ›
Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations ›
High-Precision Amplitude-Modulated Continuous-Wave Lunar Laser Ranging ›
The impact of strong feedback on galaxy group scaling relations ›
Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations ›
A radially broad collisional cascade in the debris disk of $\gamma$ Ophiuchi observed by JWST ›
Propulsion Trades for a 2035-2040 Solar Gravitational Lens Mission ›
Detection horizon for the neutrino burst from the stellar helium flash ›
Constraining Neutrino Mass with the Void Weak Lensing Effect ›
Reconstructing the Type Ia Supernova Absolute Magnitude with Two-Probe Physics-Informed Neural Networks ›
Orbital Debris in Earth Orbit: Operations, Stability, Control, and Market Formation ›
Oxygen and nitrogen isotopologues on cold COCONUTS-2b observed with MIRI/MRS ›
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies ›
Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption ›
From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system ›
Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries ›
Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties ›
On binary pulsars and the force of gravity ›
Classical and Semiclassical Stability of Emergent Universes in Jordan-Brans-Dicke Theory ›
Reviving WIMP dark matter with temperature-dependent couplings ›
The Muonic Portal to Vector Dark Matter:connecting precision muon physics, cosmology, and colliders ›
Data-driven exploration of the neutron $^3\text{P}_2$ pairing gap using Cassiopeia A neutron star observational data: Direct $\chi^2$ minimization ›
Minimal Freeze-in Dark Matter: Reviving electroweak doublet dark matter with Boltzmann suppressed freeze-in ›
GR from RG: Gravity Is Induced From Renormalization Group Flow In The Infrared ›
Modifications of CMB Temperature and Polarization Quadrupole Signals in Thurston Spacetimes ↓↑