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

ponad chmurami

Kamerka S

Kamerka N

Niebo
Temperatura
10.8 °C
Wilgotność
55%
Wiatr
6.4 km/h
Ciśnienie
1017.8 hPa

Księżyc
Najnowsze prace na astro-ph:
›
Multi-mission Observations of GS 1354-64 during the 2025-26 Outburst: First Results ›
Astronomy Open Science Competence Centre in Europe ›
SPHEREx confirms predictions for artificial satellite trail pollution in Low Earth Orbit ›
BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso-scale: Morphology and thermodynamics ›
BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Morphology and thermodynamics ›
BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Variability and kinematics ›
BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Morphology and thermodynamics ›
BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso scale: Variability and kinematics ›
Reconstructing the Globular Cluster Initial Mass Function from Present-Day Globular Cluster Systems ›
The strength of Type-C quasi-periodic oscillations in black hole X-ray binaries correlates with the jet inclination ›
BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Variability and kinematics ›
DebrisWatch II: Digging deeper for geosynchronous debris ›
TRINITY: A coupled model of winds, radiation, and photoionised gas in molecular clouds. I. Methods and validation ›
The Ellis and Baldwin test of the Cosmic Dipole: Exploring the impact of multiple flux density cuts ›
Probabilistic Data-Driven Modelling of Astrophysical Transients: The Neural Process Family for Ultrafast and Class-Agnostic Light Curve Reconstruction with NightLANP ›
VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for QU-Fitting ›
MAGAZ3NE: Spatially Resolved Ages and Chemical Abundances of Ultra-Massive Quiescent Galaxies at z $\sim$ 3.5 using JWST/NIRSpec IFU ›
A Semi-Supervised Variational Autoencoder for Generating Neutron Star Equations of State ›
Hydrodynamic Response of Mildly Evolved Common Envelope Donors in Luminous Red Novae ›
Reading between the rings: observed dust ring properties as probes of planet masses ›
The Celestial Reference Frame at K Band: The CRF-K-2025 Catalog ›
Bar-driven gas redistribution suppresses star formation in spiral galaxies: Evidence from dust lanes in NGC 3351 ›
A Probabilistic Calibration Procedure for the CORSAIR Polarimeter ›
The dynamical structure of the Earth co-orbital region and implications for the near-Earth asteroid population ›
The Ultraviolet View of Star and Planet Formation: Disks, Accretion, and Outflows with the Hubble Space Telescope into the 2030s ›
Study of the 1/f spectrum using virtual spacecraft sampling in MHD turbulence ›
Can COSI detect $\gamma$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process? ›
Comparing explodability predictions from a parameter-optimized semi-analytic model with structure-based progenitor criteria ›
Double Dots: Compact Pairs Mark Little Red Dots and High-Redshift Broad-line AGNs ›
Transient axion streams from disrupted miniclusters ›
Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66 ›
Detection of a large-scale organized 2 kG order magnetic field in the Herbig Ae star HD179218 ›
Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the $52^{\circ} ›
cBHBd: A fast code for the evolution of tidally limited star clusters and their binary black hole mergers ›
Hybrid neural denoising for resource-efficient near- and sub-threshold radio triggering of extensive air showers ›
FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays ›
Mass and radius measurements of the neutron star 47~Tuc X7 -- A new bias-free method ›
Noise Suppression and Radio Frequency Interference Rejection for Self-Triggered Radio Detectors of Extensive Air Showers ›
Spectroscopic metallicities and first {\alpha}-element abundances of RR Lyrae stars in Baade's Window ›
Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters ›
Unsupervised Morphological Characterization of Gravitational-Wave Glitches in LIGO O4a Using Frozen DINOv2 Features ›
GINKAKU: Scalable Cosmological Structure Formation Simulation Code and Post-processing Pipeline ›
Dark Quest II: A Wide-Coverage Neural Network Emulator of the Nonlinear Matter Power Spectrum Across Extended Cosmologies ›
Comparing telluric removal methods in their capability to recover injected exoplanet atmosphere signals with high resolution emission spectroscopy ›
Triaxial shapes and densities of G!k\'un||'h\`omd\'im\`a, Haumea, and Varda from stellar occultations ›
Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering ›
Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks ›
Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts ›
Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks ›
A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$\lambda$ Trends in Three Gas-Giant Mass Regimes ›
MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods ›
Hidden worlds: a non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163 ›
Cluster-centric trends in bar size and pattern speed: the case of Abell 2199 ›
The unique ability of the Hubble Space Telescope to characterize young exoplanet environments ›
Evolution of the dusty nova QY Mus from eruption to quiescence ›
The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback ›
Entropic backreaction from cosmic structure formation: a thermodynamic approach to the late-time cosmological tensions ›
Whispers of Supergravity in Gravitational Wave Backgrounds: Determining the Gravitino Mass from Cosmic Thermal History ›
Fewer simulations, sharper covariances: Reducing mock covariance noise with Zeldovich approximation control variates ›
Non-conservation and time non-locality of biased tracers ›
Analytical Fluxes from Generic Schwarzschild Geodesics ›
Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE ›
GenSBI: Generative Methods for Simulation-Based Inference in JAX ›
On the Validity of the Effective Theory of (Multi-)Field Inflation ›
Neutrino-antineutrino superfluidity ›
Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves ›
From WIMP to FIMP during reheating: collider vs non-collider probes for p-wave annihilation ›
Reconstructing ACT-compatible and GW170817-compatible Einstein-Gauss-Bonnet Inflation from the Observational Indices ›
Dynamical Resolution of the Cosmic Coincidence Problem in Non-Interacting Holographic Dark Energy via Einstein-Cartan Torsion ›
Fermionic Bubble Loop in Cosmological Collider Revisited: Exact signals from spectral and Mellin-Barnes methods ›
Using the Pericentre Precession of LAGEOS II to Constrain Quadratically Coupled Ultralight Dark Matter ›
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess in $\mathrm{U}(1)_{L_\mu-L_\tau}$ model ›
First-Order Perturbations of Covariant Maxwell Equations in Gravitational Waves ›
Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM ›
Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars ›
Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference ›
Inflation with vector fields revisited: non-Gaussianities ›
Three-dimensional orbital-free density functional theory description of nuclear pasta in the inner crust of neutron stars ›
Detecting Gravitational Wave Bursts From Stellar-Mass Binaries in the Milli-hertz Band ›
Stochastic Gravitational Wave Background from Highly-Eccentric Stellar-Mass Binaries in the Milli-hertz Band ›
Formation of neutron stars via accretion-induced collapse and core-merger-induced collapse inside planetary nebulae from white dwarf binaries ›
Extracting Astrophysical Information of Highly-Eccentric Binaries in the Millihertz Gravitational Wave Band ›
We Must Preserve Hubble given its Unique Complementarity to Webb, Roman, and Euclid ›
Euclid: Photometric redshift calibration with the clustering redshifts technique ›
Turbulence in Primordial Dark Matter Halos and Its Impact on the First Star Formation ›
The Low-mass Dwarf Host Galaxy of Nonrepeating FRB 20230708A ›
Interpreting the Hubble tension with a cascade decaying dark matter sector ›
Constraints on DBI dark energy with chameleon mechanism ›
Prototyping of 6.2-mm-Pitch Fiber Positioner Modules for Stage-V Telescope Instrumentation ›
Influence of Dark Matter on Hybrid and Twin Stars ›
Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE ›
How precisely can we measure the ages of subgiant and giant stars? ›
Numerical Studies on the Radio Afterglows in TDE: Forward Shock ›
RGC: a radio AGN classifier based on deep learning. I. A semi-supervised multiclass model for VLA images ›
Implication of multiple source populations of Galactic cosmic rays from proton and helium spectra ›
Forecasting Constraint on Primordial Black Hole Properties with the CSST $3\times2$pt Analysis ›
GASTRO library II: Exploring Chemical Bimodalities in Disk Galaxies with GSE-like Mergers and Massive Star-forming Clumps ›
The quenched fraction of satellites around simulated Milky Way-mass galaxies ›
A Convolutional Neural Network for the Recovery of Transfer Functions From Velocity-Resolved Reverberation Mapping Data ›
Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering ›
Evolution of Cosmic Voids: Structure, Galaxies, and Dynamics ›
Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes? ›
BLUEPRINT: Blue-dominant Lyman-alpha (Ly$\alpha$) emission as evidence of gas inflow in ultra-low-mass galaxies at z = 3 ›
Self-Limited Accretion onto Embedded Binaries in a Uniform Medium ›
Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLAS ›
Andromeda XXXVI: discovery of a new ultra-faint dwarf galaxy towards M31 ›
Imaging magnetically driven astrospheres: a forward modelling approach ›
A Generalized Algorithmic Framework for Detecting Faraday Rotation Measure Flares in Repeating Fast Radio Bursts ›
Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data ›
Quantifying the Reconstructability of Astrophysical Methods with Large Language Models and Information Theory: A Case Study in Spectral Reconstruction ›
Impact of stellar population models on the estimated physical properties of galaxies ›
The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres ›
Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era ›
Probing the faint end of simulated galaxy counts at z>3 ›
Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact ›
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona ›
Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena ›
The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization ›
Universe in a black hole in Einstein$-$Cartan gravity ›
GRTresna: An open-source code to solve the initial data constraints in numerical relativity ›
Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies ›
Probing Quadratically Coupled Ultralight Dark Matter with Pulsar Timing Arrays ›
Impact of conversion-driven processes on singlet-doublet Majorana dark matter relic ›
Exploring New Propagation Scales With Galactic Neutrinos ›
Search for Annual Modulation in Combined ANAIS 112 and COSINE 100 Data using Bayesian Model Comparison ›
Terrestrial Test of Shapiro Time Delay: Forth test of Einstein General Theory of Relativity ›
Part I: Low Energy Galactic Neutrinos ›
Early-universe constraints on the electron mass ›
May Negative Mass Objects exist in the sky? ›
On The Nonthermal Power Laws In Magnetized Turbulent Plasmas ↓↑