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

w kopule

Chmury

Opady

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

Księżyc
Najnowsze prace na astro-ph:
›
A Correlation Between Black Hole Mass and Dark Matter Halo Concentration in Cosmological Simulations ›
CoBiTS: Single-detector discrimination of binary black hole signals from glitches using deep learning ›
Bridging stellar evolution and planet formation: from birth, to survivors of the fittest, to the second generation of planets ›
Diffusive or Ballistic? Distributions and Spectra of PeV Cosmic Rays around Microquasars ›
Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots ›
First-Principles Formalism for Simulating Self-Interacting Dark Matter ›
The Clustering of Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter ›
Time-resolved X-ray spectra of Proxima Centauri as seen by XMM-Newton ›
Widespread Shocks in an Odd Radio Circle Host Galaxy ›
Monitoring and Evaluating Astronomy-for-Development Initiatives ›
Characterization of telecentric dual-etalon Fabry-P\'erot systems from observational data. Properties of the CRISP2 instrument at the Swedish 1-m Solar Telescope ›
Constrained Brownian-bridge prior for neutron-star equation-of-state inference ›
Designing the Community Infrastructure for ESO's Next Transformational Facility. Equitable Governance and Sustainable Teams for 2040s Astronomy ›
Precision Spectroscopy for 1.9 Million Galaxies from SDSS-IV: Improved Spectral Measurements and Catalogs for eBOSS ›
A recurrent 70-100 minute quasi-periodic pulsation in the intermediate-aged mid-M dwarf GJ 3512 ›
The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates ›
The Impact of the MAST Data Archive ›
Double Hot Jupiter Formation through Mirrored ZLK Migration in Binary Star Systems: The Case of WASP-94 ›
A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array ›
Continuous Wide-Field Optical Monitoring for Very Early-Phase Transient Discovery ›
Red noise-based false alarm thresholds for astrophysical periodograms via Whittle's approximation to the likelihood ›
Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUs ›
Discovery of a Luminosity-dependent Continuum Lag in NGC 4151 from Photometric and Spectroscopic Continuum Reverberation Mapping ›
Measurements of quasar proximity zones with the Lyman-$\alpha$ forest of DESI Y1 quasars ›
Robust and scalable simulation-based inference for gravitational wave signals with gaps ›
On Lorentz Variability of Magnetically Dominated Relativistic Outflows ›
The size of 3I/ATLAS from non-gravitational acceleration ›
Standard Sirens in 2040s: Probing the Cosmic Expansion History with Gravitational Waves and Spectroscopic Galaxy Surveys ›
Energy-Dependent Shifts of Medium-Scale Anisotropies in Very-High-Energy Cosmic Rays Observed by LHAASO-KM2A ›
The evolution of obscured AGN across cosmic time -- A large quasar survey for the 2040s ›
Unveiling Long-Period Variables in M33's Central Region: Insights into Stellar Evolution and Star Formation via Near-Infrared Photometry ›
Imaging the LkCa 15 system in polarimetry and total intensity without self-subtraction artefacts ›
Observed Low-Plasma-$\beta$ Temperature Anisotropy Constraint Driven by $\alpha$-Particle Drift ›
Searches for Prompt Low-Frequency Radio Counterparts to Gravitational Wave Event S250206dm with the OVRO-LWA Time Machine ›
Harmony of the Spheres: Extension to All Points of an Algorithm for Producing a Density Field with Given Two-, Three-, and Four-Point Correlation Functions ›
Detecting stellar flares in the presence of a deterministic trend and stochastic volatility ›
Formation of Be stars via wind accretion: Case study on Black hole + Be star binaries ›
The Extended Baryonic Tully-Fisher Relation for MaNGA Galaxies ›
Linear Analyses of Thermal Instability in Stratified Medium ›
Solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport indicated by type II and type N radio bursts ›
Photospheric horizontal magnetic field decrease preceding a major solar eruption ›
Towards Understanding the Milky Way's Matter Field and Dynamical Accretion History based on AI-GS3 Hunter ›
Towards Unveiling the Origins of the Milky Way Bulge through Multi-band-Messenger Sky Surveys ›
Addendum to "Cygnus~X-3 as a semi-hidden PeVatron'' discussing the LHAASO 2025 data ›
Recurrence plot analysis of blazar gamma-ray light curves: Exploiting the time-domain capabilities of Fermi-LAT ›
Spider-Webb: Spatially-Resolved Evidence of Inside-Out Quenching in the Spiderweb Protocluster at $z \sim 2$ ›
Nanohertz Gravitational Waves ›
Accretion geometry in neutron star low-mass X-ray binaries during the hard spectral state ›
Detecting false positives with PLATO using double-aperture photometry and centroid shifts ›
Orbital classification in rotating bar potentials using an empirical proxy of the second integral of motion ›
Solar Vortex Detection With Velocity Field Normalisation: Eliminating False Positives ›
Constraints on the polarization angle oscillations of the Crab Nebula with the Simons Array and its applications to the search for axion-like particles ›
EuroHPC SPACE CoE: Redesigning Scalable Parallel Astrophysical Codes for Exascale ›
Optical SETI at ESO in the 2040s ›
Weak Lensing Mass Calibration of the ACT DR5 Galaxy Clusters with the DES Year 3 Weak Lensing Data ›
Validating the CROCODILE model within the AGORA galaxy simulation framework ›
Fragmenting Filaments and Evolving Cores -- Insights from Dust Polarisation Study of a filament in Northern Orion B ›
$\Omega_1\Omega_2$-$\Lambda$CDM: A promising natural extension of the standard model of cosmology ›
On the Diversity of Pulsar's Frequency-Dependent Circular Polarization ›
The Milky Way Bulge Extra-Tidal Star Survey: NGC 6569 ›
Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae ›
The Simons Observatory: Detector Polarization Angle Calibration using Sparse Wire Grid with Initial Data Sets of the Small Aperture Telescope ›
GW231123: A Case for Binary Microlensing in a Strong Lensing Field ›
Height and Energy Evolution of X-ray Double Sources in a Solar Flare ›
DESI DR2 Constraints on the $R_h=ct$ Universe: Model Viability and Comparison with $\Lambda$CDM ›
Raman Spectroscopy of Salt Deposits from the Simulated Subsurface Ocean of Enceladus ›
ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud (LMC): N79 South GMC ›
Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure ›
The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591 ›
Enhanced Non-Thermal Line Broadening inside Coronal Cavities above Solar Prominences revealed by Spectral Imaging CoronaGraph ›
Outburst Characteristics of Transient Low Mass X-ray Binary 4U 1608-52 ›
Multi-wavelength study of the pre-eruption dip in the recurrent nova T Coronae Borealis preceding imminent nova eruption ›
Orbital Stability of Moons Around the TRAPPIST-1 Planets ›
Disentangling the hemispheres of Teegarden's Star b with LIFE ›
Identifying Quasi-Periodic Micropulses in Pulsars with FAST Using Convolutional Neural Networks ›
Dynamically close galaxy pairs from the unWISE survey: Testing the merger-AGN-star formation connection ›
Towards DM-free search for Fast Radio Bursts with Machine Learning -- I. An implementation on multibeam data ›
Sensitivity of CTAO to axion-like particles from blazars: a machine learning approach ›
Observations of the 21 cm HI Line from the Milky Way galaxy using Pyramidal Horn Radio Telescope ›
Search for Axion-Like Particles from Nearby Pre-Supernova Stars ›
Optical Follow-Up Strategies for the Next Neutrino-Detected Galactic Core-Collapse Supernova ›
Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment ›
Machine learning for the early classification of broad-lined Ic supernovae ›
Diagnosing the AGN population origin of TeV neutrinos with their spatial correlation ›
Dynamics of clusters of galaxies in the presence of dark energy: Virgo cluster ›
GALATEA: The 15-m Galactic Archaeology Spectroscopic Surveyor ›
Confining nonlinear electrodynamics black holes: from thermodynamic phases to high-frequency phenomena with accretion process ›
Revealing the intricacies of radio galaxies and filaments in the merging galaxy cluster Abell 2255. II. Properties of filaments using multi-frequency radio data ›
Low-redshift 3D Lyman-{\alpha} Forest Correlations with China Space Station Telescope ›
Strong model-agnostic constraints for twin-star solutions ›
Predicting coronal mass ejection travel times using enhanced model-guided machine learning ›
Shock-induced magnetic reconnection driving Ellerman bomb emission and a spicule ›
Do low-redshift observations open the doors to an open universe? ›
Deep Learning for Primordial $B$-mode Extraction ›
Non-local-in-time structure formation and sixth-order galaxy bias ›
Impact of Galaxy Cluster Environment on the Stellar Mass Function of Galaxies ›
Period Change of the Binary System WR+O V444 Cyg: Updated Ephemeris Formula ›
Deep H{\alpha} survey of the Coma cluster: The Catalog ›
InterACTing dark radiation models after ACT ›
High-Precision Differential Radial Velocities of C3PO Wide Binaries: A Test of Modified Newtonian Dynamics (MOND) ›
A High-Resolution NUV Transmission Spectrum of KELT-9b: Mg II and Fe II Escaping from the Hottest Known Giant Planet ›
A cosmologist's take on Little Red Dots ›
Are Primordial Black Holes Truly Fine-Tuned? ›
Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultra-Deep Rest-Frame Optical Spectroscopy of JADES-GS-z14-0 ›
Magnetically supramassive and hypermassive compact stars ›
Effects of helium sedimentation on late star formation in galaxy clusters ›
Constraints on gravitational waves from the 2024 Vela pulsar glitch ›
New Multi-messenger Probe of Dark Matter-Nucleon Interactions from Ultra-high Energy Cosmic Ray Acceleration ›
Superfluid fraction in the crystal phase of the inner crust of neutron stars ›
Revisiting Mars' Induced Magnetic Field and Clock Angle Departures under Real-Time Upstream Solar Wind Conditions ›
A Framework for Lorentz-Dirac Dynamics and Post-Newtonian Interaction of Radiating Point Charges ›
Traversable wormholes inside anisotropic magnetized neutron stars: physical properties and potential observational imprints ›
Energetically-dominant Sunward-Propagating Alfv\'en Waves Near 1 au and Their Relation to Large-scale Magnetic Switchbacks ›
Optical appearance, Hawking radiation, and Barrow thermodynamics of Letelier black hole in electromagnetic universe ›
Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies ›
Gravitational Production of Massive Spin-2 Particles During Reheating ›
Bose-Einstein Condensate dark matter with logarithmic nonlinearity ›
The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123 ›
Ultra-high precision high voltage system for PTOLEMY ›
Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession ›
The tidal gap: causality bound on exotic compact objects with applications in the solar and sub-solar mass range ›
Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties ›
Probing Dark Sectors with Exploding Black Holes: Gamma Rays ›
The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth ›
Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset? ›
ContEvol formalism: numerical methods based on Hermite spline optimization ›
Time Non-locality in Dark Matter and LSS ›
Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study ›
Constraining primordial black hole abundance with Insight-HXMT ›
On the Role of Chapman's Hydrostatic Solar Wind Mechanism in Parker's Hydrodynamic Solar Wind Model ›
Stellar Stripping and Disruption in Disks around Supermassive Black Hole Binaries: Repeating nuclear transients prior to LISA events ›
Cosmological search for sterile neutrinos after DESI 2024 ›
The Ultraviolet Type Ia Supernova CubeSat (UVIa): Science Motivation & Mission Concept ›
Multi-copy Axion Transfer Function and Observational Implications of Effective de Broglie Scales ›
Periodicities in radio emissions from the Jupiter's magnetosphere and consequences for radio emissions from star-exoplanet systems ›
Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm? ›
Challenges in the detection of gases in exoplanet atmospheres ›
A Detailed Investigation of HD 209458 b HST & JWST Transmission Spectra with SANSAR ›
The ambiguous AT2022rze: Changing-look AGN mimicking a supernova in a merging galaxy system ›
Accurate and efficient likelihood modeling for large-scale CMB data ›
TDCOSMO 2025: Cosmological constraints from strong lensing time delays ›
Indicator Functions: Distilling the Information from Gaussian Random Fields ›
The link between galaxy merger, radio jet expansion and molecular outflow in the ULIRG IRAS 00183-7111 ›
An Enhanced Thermodynamic Framework for Third-Order Galaxy Correlation Functions: A Physically Motivated Closure and Observational Test ›
Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook ›
On the statistical convergence of N-body simulations of the Solar System ›
Effects of Lorentz invariance violation on charged particles and photon production in astrophysical sources ›
Reconnection-driven Flares in M87*: Proton-Synchrotron-powered GeV Emission ›
Equation vs. AI: Predict Density and Measure Width of molecular clouds by Multiscale Decomposition ›
SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis ›
Mitigating incoherent excess variance in high-redshift 21 cm observations with multi-output cross-Gaussian process regression ›
A comprehensive spectroscopic reference of the solar system and its application to exoplanet direct imaging ›
Blade Antenna-SDR System Prototype for the CANTAR Global 21-cm Experiment: Simulations, Measurements, and In-Situ Results ›
Modeling spectral filtering effects on color-matching functions: Implications for observer variability ›
Mysteries of Capotauro: investigating the puzzling nature of an extreme F356W-dropout ›
Active galactic nuclei-heated dust revealed in "little red dots" ›
Hurst Index of Gamma-Ray Burst Light Curves and Its Statistical Study ›
Predicting stellar collision outcomes of main sequence stars ›
MCI: Multi-Channel Imager on the Chinese Space Station Survey Telescope ›
Exponential quintessence with momentum coupling to dark matter ›
Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology ›
Ultra-long Gamma-ray Bursts from Micro-Tidal Disruption Events: The Case of GRB 250702B ›
The Colors of Ices: Measuring ice column density through photometry ›
The very faint X-ray transient Swift J174610-290018 at the Galactic center ›
On the statistical characterization of the synchrotron multi-zone polarization of blazars ›
Transverse Velocities in Real-Time Cosmology: Position Drift in Relativistic N-Body Simulations ›
Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes ›
TOI-3288 b and TOI-4666 b: two gas giants transiting low-mass stars characterised by NIRPS ›
Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics ›
Polarization based direction of arrival estimation using a radio interferometric array ›
The Lensing Counter Narrative: An Effective Description of Small-Scale Clustering in Weak Lensing Power Spectra ›
Mitigating Nonlinear Systematics in Weak Lensing Surveys II: Stability and Diagnostics with Intrinsic Alignment ›
Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break ›
Validation of optical pathlength stability in a LISA test-bench demonstrator ›
JWST Exoplanetary Worlds and Elemental Survey (JEWELS) I: High-Precision Chemical Abundances of 20 FGK Planet-Hosting Stars from JWST Cycle 2 ›
Spectroscopic characterization of a remarkable temporally varying, triple-lensed quasar at z=2.67 ›
GLIMPSE-D: An Exotic Balmer-Jump Object at z=6.20? Revisiting Photometric Selection and the Cosmic Abundance of Pop III Galaxies ›
DESI-DR1 $3 \times 2$-pt analysis: consistent cosmology across weak lensing surveys ›
The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000 ›
Understanding the Neutron Star Population with the SKAO telescopes ›
Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center ›
The contribution from small scales on two-point shear analysis: comparison between power spectrum and correlation function ›
Observations of AGN-driven feedback: dynamics and ionization of the filaments in M87 ›
Boosted dark matter from primordial black holes produced in a first-order phase transition ›
The effect of split endcaps on the flow dynamics in a tall Taylor-Couette setup ›
Sound waves from primordial black hole formations ›
The Possibility of Formation of Compact Boson Stars via Cosmological Evolution of a Background Scalar Field ›
Revisiting Isocurvature Bounds on the Minimal QCD Axion ›
Boosted dark matter versus dark matter-induced neutrinos from single and stacked blazars ›
Dark wounds on icy moons: Ganymede's subsurface ocean as a dark matter detector ›
Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries ›
Observing Double White Dwarfs with the Lunar GW Antenna ›
Electron Inertia and Magnetic Reconnection ›
Streamlined Supergravity ›
The meaning of "Big Bang" ›
Can the 3 neutrino masses really be found using SN 1987A data? ›
Quantum Walks and Exact RG in de Sitter Space ›
Delayed Scaling of Multi-Type Cosmic F- and D-strings in VOS Models ↓↑