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

Kamerka S

Kamerka N

Niebo
Temperatura
7.1 °C
Wilgotność
93%
Wiatr
0.0 km/h
Ciśnienie
996.2 hPa

Księżyc
Najnowsze prace na astro-ph:
›
Variations of angular momentum $L_z$ as an indicator of orbital chaos of globular clusters in the central region of the Galaxy with a bar ›
Spectropolarimetric Evolution Reveals Dual-Axis Ejecta in the Atypical Magnetar-Powered SN 2012au ›
Practical Author Name Disambiguation under Metadata Constraints: A Contrastive Learning Approach for Astronomy Literature ›
Reaching for the Edge II: Stellar Halos out to Large Radii as a Tracer of Dark Matter Halo Mass ›
Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH ›
An Analytical Model for the Eccentricity Cascade: Hot Jupiter Formation via S-type Instability ›
Large-Scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to $z \sim 7$ with the Largest JWST Survey ›
Widening of Binaries via Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System ›
The signature of major mergers on the hydrostatic mass bias of galaxy clusters ›
TESS Investigation -- Demographics of Young Exoplanets (TI-DYE) IV: a Jovian radius planet orbiting a 34 Myr Sun-like star in the Vela association ›
Intra-night optical polarization monitoring of blazars ›
KOALA, a new ATLAS9 database -- I. Model atmospheres, opacities, fluxes, bolometric corrections, magnitudes and colours ›
Hybrid Simulations of Supersonic Shear Flows: I) Particle Acceleration ›
The Quiescent Merging Nature of the Coma Cluster Revealed by ICM Velocity Structure ›
REBELS-IFU: Steeply rising star formation histories and the importance of dust obscuration in massive $z \simeq7$ galaxies revealed by multi-wavelength observations ›
REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization ›
XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi ›
Indirect forces in disc-planet interaction ›
Hydrogen-Poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source ›
Hydrogen-line profiles from accreting gas giants and their CPDs ›
Jeans Model for the Shapes of Self-interacting Dark Matter Halos ›
Optimization of lenslet arrays for PRIMA Kinetic Inductance Detectors ›
Historical Surveys to Rubin First Look: Absolute Colors of trans-Neptunian objects ›
The Dawes Review 13: A New Look at The Dynamic Radio Sky ›
The impact of supermassive black holes on exoplanet habitability: I. Spanning the natural mass range ›
What's Inside Matters: The Effect of Oxygen Fugacity and Initial Volatile Abundance on the Atmospheres of the TRAPPIST-1 Planets ›
Mock Observations for the CSST Mission: Main Surveys -- the Mock Catalogue ›
ALMAGAL V. Relations between the core populations and the parent clump physical properties ›
Ubiquitous high-frequency waves and disturbances in the active region corona observed with DKIST/Cryo-NIRSP ›
Unveiling the Chemical Complexity and C/O Ratio of the HD 163296 Protoplanetary Disk: Constraints from Multi-line ALMA Observations of Organics, Nitriles, Sulfur-bearing, and Deuterated Molecules ›
Evolutionary Map of the Universe: A pilot survey to detect high Galactic latitude pulsars in variance images with ASKAP ›
In situ Evidence of 5-minute Oscillations from Parker Solar Probe ›
PRIMA General Observer Science Book Volume 2 ›
A High-Precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multi-Layer Internal Structure Models ›
EUSO-SPB2 Cherenkov Telescope: Overview and First Neutrino Constraints ›
Discovery of an X-ray bridge between the comma-shaped gas and the main cluster in MCXC J0157.4-0550 ›
A proposal to construct the dark-matter-only counterpart of the observed Universe combining weak lensing and baryon censuses ›
Accuracy and Applicability of the Hartle-Thorne and Komatsu-Eriguchi-Hachisu Methods for Modeling Rotating Neutron Stars ›
SPICE -- modelling synthetic spectra of stars with non-homogeneous surfaces ›
Surface figure metrology for reflective membrane mirrors based on phase-measuring deflectometry ›
Measurement of cosmic-ray muon flux at CJPL-II ›
Highly Polarized Intrinsic Emission and its Orthogonal Counterpart in Vela X-1 ›
The Spatial Evolution of Star Clusters in NGC 628 with JWST ›
A Simulation Platform for Small Solar System Bodies using the Einstein-Elevator ›
Galactic foreground residual biases in CMB lensing convergence reconstruction and delensing of B-mode maps ›
Constraints on the canonical single-field slow-roll inflation model from observations ›
Empirical prediction of plasma emission measure distributions and X-EUV spectra of late-type stars ›
Evidence for the Keplerian orbit of a close companion around a giant star ›
Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization ›
Formation and disruption of resonant chains of super-Earths: Secular perturbations from outer eccentric embryos ›
Close-in compact super-Earth systems emerging from resonant chains: slow destabilization by unseen remnants of formation ›
A glitch in the millisecond pulsar J0900$-$3144 ›
Recalibrating Inflation: Insights from Starobinsky Gravity ›
Shadow-Induced Warps in Protoplanetary disks ›
Boost operator approach to the relativistic polarized SZ effect ›
Modeling the Multi-Wavelength Afterglow of Short Gamma-Ray Bursts with a Plateau Phase ›
Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations I: Hydrodynamics ›
Star clusters in the gamma-ray sky ›
Planetary nebulae as tracers of stellar population properties: a pilot study with MUSE ›
A 34.6-day transiting sub-Neptune in the TOI-1422 planetary system ›
Looking at infrared background radiation anisotropies with Spitzer II. Small scale anisotropies and their implications for new and upcoming space surveys ›
Mutated Hilltop Inflation in the Era of Present and Future CMB Experiments ›
Probing the era of giant collisions: millimeter observations of the HD 166191 system ›
An optical--mid-infrared color evolution tool for nova identification using WISE data ›
Testing the cosmological Euler equation: viscosity, equivalence principle, and gravity beyond general relativity ›
Implicit inference of the reionization history with higher-order statistics of the 21-cm signal ›
Characterization of the ionization response of argon to nuclear recoils at the keV scale with the ReD experiment ›
Keeping It Renormalizable: Minimal Baryogenesis induced Asymmetric Dark Matter ›
In-situ environmental radiation background measurement in the second phase of CJPL ›
NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration ›
Dark Matter Capture in a Core-Collapse Supernova Revives Dark Photons ›
Influence of Rotation on Fingering Convection in Planetary Cores ›
Intrinsic Dimension Estimation for Radio Galaxy Zoo using Diffusion Models ›
\textit{Euclid}: From Galaxies to Gravitational Waves -- Forecasting Stochastic Gravitational Wave Background Anisotropies and Their Cross-Correlation ›
First Use of GPS Satellites for Beam Calibration of Radio Dish Telescopes ›
Gamma-Ray Burst Light Curve Reconstruction: A Comparative Machine and Deep Learning Analysis ›
Anatomy of Parity-violating Trispectra in Galaxy Surveys ›
Establishing a Connection Between the Jet and the Corona in Black Hole Low Mass X-Ray Binaries ›
Molecular Dynamics Simulations on Nuclear Recoils in Silicon Crystals towards Single Electron-Hole Pair Ionization Yields ›
Accurate $N$-body simulations with local Primordial non-Gaussianities: initial conditions and aliasing ›
Transformers for Stratified Spectropolarimetric Inversion: Proof of Concept ›
Braking index of the frequently glitching PSR J0537$-$6910 ›
Multi-Model Framework for Reconstructing Gamma-Ray Burst Light Curves ›
Survival of higher overdensity cold gas in a turbulent, multiphase medium ›
EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger? ›
The Impact of Spectroscopic Redshift Errors on Cosmological Measurements ›
Probing the Cosmological Principle with CMB lensing and cosmic shear ›
Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey ›
Euclid preparation LXXIX. Using mock low surface brightness dwarf galaxies to probe Euclid Wide Survey detection capabilities ›
Recovering the Coupled Treatment of Redshift-Space Distortions and the Lightcone Effect after Diffuse Foreground Removal ›
Interstellar Dust-Catalyzed Molecular Hydrogen Formation Enabled by Nuclear Quantum Effects ›
Multi-modal atmospheric characterization of $\beta$ Pictoris b: Adding high-resolution continuum spectra from GRAVITY ›
CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. V. Chemical composition gradients as a function of the galactocentric radius ›
The evolution of the bar fraction and bar lengths in the last 12 billion years ›
FlowLensing: Simulating Gravitational Lensing with Flow Matching ›
Probing Anisotropic Cosmic Birefringence with Foreground-Marginalised SPT B-mode Likelihoods ›
Galactic X-ray Transients in the First eROSITA All Sky Survey ›
Connecting outflows with radio emission in active galactic nuclei at cosmic noon ›
ZTF25abjmnps (AT2025ulz) and S250818k: A Candidate Superkilonova from a Sub-threshold Sub-Solar Gravitational Wave Trigger ›
Constraints on Cosmic Birefringence from SPIDER, Planck, and ACT observations ›
Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared ›
Kinematic scaling relations of disc galaxies from ionised gas at $z\sim~1$ and their connection with dark matter halos ›
Global Distribution of the Key Species on the Surface of Europa ›
Dark Photons in the Radio Sky: I. Resonant Conversions in Halos ›
Dark Photons in the Radio Sky: II. Resonant Conversions in the Intergalactic Medium ›
A Bayesian Perspective on Evidence for Evolving Dark Energy ›
Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer ›
Flavor Matters, but Matter Flavors: Matter Effects on Flavor Composition of Astrophysical Neutrinos ›
Bridging the Rossby number gap in rapidly rotating thermal convection ›
Demonstration that Differential Length Changes of Optical Cavities are a Sensitive Probe for Ultralight Dark Matter ›
Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities ›
Earth-Scattering Induced Modulation in Low-Threshold Dark Matter Experiments ›
Precision calculation of $N_{\text{eff}}$ with Neutrino Direct Simulation Monte Carlo ›
The periastron regression of 2M1510 AB, the jet precession of M87* and Telisto/Planet Nine: three different scenarios for a possible common cause ›
Euler-Heisenberg action for fermions coupled to gauge and axial vectors: Hessian diagonalization, sector classification, and applications ›
Stochastic Limit of Growing Gravitational Wave Memory from Sources in the Early Universe and Astrophysical Sources ↓↑