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
8.0 °C
Wilgotność
50%
Wiatr
8.0 km/h
Ciśnienie
998.7 hPa

Księżyc
Najnowsze prace na astro-ph:
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High-resolution near-IR spectroscopy of the B[e] supergiant LHA 115-S 18: discovery of hot water vapor emission ›
LISA science ground segment conventions ›
SDSS-V LVM: A spatially resolved study of the physical conditions and the chemical abundance discrepancy in the Lagoon Nebula (M 8) ›
Shaping the diffuse X-ray sky: Structure, Variability and Visibility ›
MEOW: The increase in the obscured AGN fraction in mid-infrared from 0 < z < 6 with JWST MIRI ›
Second Order Closures for the Radiative Transfer Equation: Some Are Unstable ›
Where within the 3C 84 jet are $\gamma$-rays produced? ›
Reinterpreting the puzzling properties of z>6 galaxies within a variable IMF framework ›
Phantom-Crossing Dark Energy and the $\Omega_m$ Tug-of-War ›
Unified Formation Channel of Hot and Warm Jupiters via Planet-Planet Scattering ›
Detailed Analysis of the NGC 2168 Cluster, Leveraging Gaia DR3 ›
A systematic study of AGN feedback in a disk galaxy II: MACER prediction of X-ray surface brightness profile and comparison with eROSITA observations ›
Primordial Non-Gaussianity and the Field-Level Cramer-Rao Bound ›
CHANG-ES. XXXVIII. A Thin Radio Halo Shaped by Slow Cosmic-Ray Transport in the Quiescent Galaxy NGC 4565 ›
The Crimson Kiss of Two Giants: Helium Detonation and High-Energy Neutrino Production ›
A large population of over-massive black hole quasars at z=0.3-0.8 revealed by eROSITA ›
Planet-Planet Scattering Explains the Mass-Eccentricity Relation of Warm Jupiters ›
Magnetic Connectivity in the Time-Dependent Corona and Heliosphere ›
Carbon Nitride Monolayer Nanosheets: Astrochemical Insights into the Fate of Interstellar Hydrogen ›
The GRAVITY young stellar object survey -- XV. The star-disk interaction region of the T Tauri star DO Tau ›
More Than Power: Revisiting the CMB Hemispherical Power Asymmetry with Morphological Descriptors ›
Cross-spectra likelihood for robust $\tau$ constraints from all satellite polarisation data ›
Impact of eccentricity on the population properties of neutron star - black hole mergers ›
Optical Spectroscopy of the IR Source CPM 19 and Surrounding Objects ›
Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation ›
Ecological modelling of hycean worlds ›
Model validation and tolerancing of scalar vortex masks in the High Contrast Imaging Testbed (HCIT) facility ›
Turning the knobs on dust evolution: Comparing codes, parameters and their effects on planet formation and disc observables ›
Dimpled scalar vortex coronagraph laboratory demonstration ›
A Multi-messenger Search for Ultra-high-energy Gamma Rays in Coincidence with Neutrinos ›
Automatic search for transiting planets in TESS-SPOC FFIs with RAVEN: over 100 newly validated planets and over 2000 vetted candidates ›
The Radio-wave Observations at the Lunar Surface of the photoElectron Sheath (ROLSES) instrument onboard the Intuitive Machines-1 Mission to the Moon ›
Subsurface ocean salinity and dissipation rate inferred from Enceladus ice shell morphology ›
Multi-Sensor Trajectory Reconstruction of the 24 April 2025 Alaska Fireball and Implications for Planetary Defense ›
The Two Component Circumgalactic Medium Emission around z~2 Radio-loud Quasars ›
Cluster Infall for Mass Calibration in the Stage-IV Era ›
HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI) ›
A Slit Mask Integral Field Unit for the Robert Stobie Spectrograph on the Southern African Large Telescope: I. Instrument Development ›
SGR 1935+2154's Quiet Local Environment: Clues for Its Progenitor ›
Sometimes You Just Can't Put a Ring on It: Setting Constraints on Rings around Moons from Magnetic Fields ›
Enhancing cosmological constraints with nonlinear tanh transformations of Hermite-Gaussian Derivative fields ›
Probing the Bias of Large-Scale Structure with Unlocalized Fast Radio Bursts ›
The Fate of the Milky Way--Andromeda System: To Merge or Not? ›
Orbital motion detected in gamma Cas Fe K emission lines ›
Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge ›
Extinction curves, extinction laws, and the failure of interstellar dust models ›
How well does MAGPHYS recover galaxy properties? A test using EAGLE simulated star-forming galaxies ›
MAGIC observations of NGC 4278. The first low-luminosity radio galaxy with compact jets detected at TeV energies ›
3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra ›
Revisiting Constraints on Primordial Curvature Power Spectrum from PBH Abundances ›
Low-Frequency Stochastic Gravitational-Wave Background in Gaia DR3 catalogue ›
The time-delay model and its applications to galactic archaeology ›
A High-frequency Geodetic VLBI Experiment for Optical Clock Comparison ›
Anomalously Strong Localized First Ionization Potential Effect Associated with a Solar Subflare ›
The Persistent Radio Sources and Multi-wavelength Counterparts of Fast Radio Bursts in Massive Binary Systems ›
Intracluster light is a close tracer of the dark matter halo shape ›
First Detection of the Glycine Isomer Glycolamide in Hot Molecular Core ›
Unlocking accretion rate diagnostics for high-mass protostars using JWST/MIRI HI lines ›
Identification of low redshift groups and clusters of galaxies in the X-CLASS survey and the X-ray luminosity-temperature relation ›
Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging ›
How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background ›
Perihelion observations of interstellar comet 3I/ATLAS with the IRAM 30-m telescope ›
Semi-cosmographic constraints on decaying dark matter and dynamical dark energy: DESI DR2 BAO and 21\, cm intensity-mapping forecasts ›
Upper Limits to Long-Term Variability of Solar-Type Stars from Observations of the Open Cluster M67 ›
The Lyman-alpha Emission in Solar Flares. II. A Statistical Study on Its Relationship with the White-light plus Soft X-ray Emission ›
Formation of spirals in early stage protoplanetary discs ›
3D CMZ V: A new orbital model of our Galaxy's Center, informed by data across the electromagnetic spectrum ›
Signatures of localised particle acceleration at a global coronal shock wave ›
Data-calibrated point spread function prediction: General description of the method and demonstration on MUSE-NFM ›
Photometric and late-time spectropolarimetric observations of GRB 250129A afterglow ›
An Opacity-Free Test of the Cosmic Distance Duality Relation Using Strongly Lensed Gravitational Wave Signals with Space-Based Detector Networks ›
Investigating peculiar prompt emission properties of the multi-Peaked GRB 250129A ›
Microlensing by Cluster of Primordial Black Holes ›
Solving the Cosmic Coincidence Problem: The Locally Pumped Dark Energy Model ›
Ca2+ transient detection and segmentation with the Astronomically motivated algorithm for Background Estimation And Transient Segmentation (Astro-BEATS) ›
What does it take to have $N_{\rm eff} < 3$ at CMB times? ›
Kinetic Isocurvature Perturbation ›
Slow-down of expanding bubbles in the early Universe ›
Inside the Black Box of Big Bang Nucleosynthesis: Parameter Sensitivity Studies in Light of new LBT Data ›
Analyzing Fermionic Dark Matter scenarios with anomalous compact objects ›
First measurements of deuteron production spectra in p+p collisions at beam momentum of 158 GeV/c at NA61/SHINE ›
Wave-particle equilibria with heavy ions in weakly collisional space plasmas ›
Dark graviton sensing with magnetically levitated superconductors ›
$\beta$-decay Measurements Near the $N=40$ Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts ›
Cosmic Ray Boosted Dark Matter in COSINUS: Modeling and Constraints ›
Astrophysical aspects of string compactifications ›
Dark Matter Detection through Rydberg Atom Transducer ›
Discovery of a radio jet in the Cloverleaf Quasar at z = 2.56 ›
Millisecond Pulsars in Globular Clusters and Implications for the Galactic Center Gamma-Ray Excess ›
Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620 ›
On the spatial distribution of luminous blue variables in the M33 galaxy ›
A Potential Link between Nuclear Winds and Cold Gas Outflows on Kiloparsec Scales in Reionization-Era Quasars ›
In the grip of the disk: dragging the companion through an AGN ›
Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020 ›
Cosmology in Extended Parameter Space with DESI Data Release 2 Baryon Acoustic Oscillations: A 2$\sigma$+ Detection of Nonzero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly ›
On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation ›
Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory ›
An SDSS-V 3D Tomographic Na I Map of the ISM: An Initial Study Towards the Smith Cloud ›
Improved reconstruction of the century-long solar magnetic field by incorporating morphological asymmetry in sunspots ›
Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network ›
GPU-Accelerated X-ray Pulse Profile Modeling ›
Spin-Orbit Misalignments of Eccentric Black Hole Mergers in AGN Disks ›
Effect of stochastic kicks on primordial black hole abundance and mass via the compaction function ›
Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter ›
Probing the wind and evolutionary state of the quiescent luminous blue variable Var$\,$2 in the Galaxy M33: constraints from self-consistent non-LTE modeling ›
Evidence for Neutrino Emission from X-Ray-bright Active Galactic Nuclei with IceCube ›
Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal ›
Searching for Exotrojans in Pulsar Systems ›
Graph-Based Light-Curve Features for Robust Transient Classification ›
Measuring cosmic dipole with the GRB luminosity-time relation ›
It's always the quiet ones: Single Degenerate Double Detonation Type Ia Supernova from Quiescent Helium Accretion ›
Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies ›
Prospects for Observing the Microquasar SS 433 with the LACT Array ›
Equation-of-state-informed pulse profile modeling ›
Searching Within Galaxies for the Earliest Signs of Quenching With Spatially Resolved Star Formation Histories in UVCANDELS Galaxies at z< 0.3 ›
The Scoured Spike: Suppression of Indirect Dark Matter Signals by a Hidden Companion ›
Fast Radio Bursts from White Dwarf Binary Mergers: Isolated and Triple-Induced Channels ›
The broad-lined type Ic supernova 2020lao experienced an energetic explosion with no central-engine signatures ›
How Dark Sector Equations of State Govern Interaction Signatures ›
Detection of 27 candidate circumbinary planets through apsidal precession of eclipsing binaries observed by TESS ›
Stochastic gravitational-wave background search using data from five pulsar timing arrays ›
Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes ›
KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies ›
The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591 ›
Abundance of cosmic voids in EFT of dark energy ›
A global view of post-interaction white dwarf-main sequence binaries ›
Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes ›
Cosmogenic 10Be as a Tracer for Recent Heliospheric Encounters with Interstellar Cold Clouds ›
Time delay measurements with Broken Power Law model ›
The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies ›
A redshift survey of the nearby galaxy cluster Abell 2199 : No upturn of the faint-end slope of galaxy luminosity function ›
Searching for the Shortest-wavelength Aromatic Infrared Bands: No Evidence for the Predicted 1.05 $\mu$m Polycyclic Aromatic Hydrocarbon Feature ›
Revisiting CPL with sign-switching density: To cross or not to cross the NECB ›
The impact of strong lensing on Hubble constant measurements with gravitational-wave dark sirens ›
Bridging the Prandtl number gap: 3D simulations of thermohaline convection in astrophysical regimes ›
The Stellar Mass Function for Nine Massive Galaxy Clusters in the Local Universe ›
A hot, nebular-dominated galaxy interacting with a pristine PopIII system uncovered by JWST ›
Identifying AGNs from X-ray detections-I: Metallicity calibrations in AGNs with X-ray luminosity as the primary input parameter ›
The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6 ›
Searching for Fast Astronomical Transients in Archival Photographic Plates ›
A turbulence index independent framework for deriving solar wind speed and coronal electron density from radio spectral broadening ›
Parallel adaptive reweighting importance sampling for Bayesian astrophysics ›
The full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT ›
Little Red and Blue Dots: simply stratified Broad Line Regions ›
Detecting light dark matter with prompt-delayed events in neutrino experiments ›
Time as a test-field: the no-boundary universe in motion and a smooth radiation bounce ›
Gravitational waves from supermassive right-handed neutrinos produced at preheating ›
Anomalous Dynamical Screening of Relativistic Plasma in a Magnetic Field ›
The tidal response of a relativistic star ›
Structure Formation with Dark Magnetohydrodynamics ›
astroCAMP: A Community Benchmark and Co-Design Framework for Sustainable SKA-Scale Radio Imaging ›
Shocks, compressible perturbations, and intermittency in the very local interstellar medium: Voyager 1 and 2 observations and numerical modeling ›
Detection prospects of solar $g$-modes with LISA ↓↑