Podchorazych 2, 30-084 Krakow, Poland.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Mount Suhora Astronomical Observatory

view from south

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Temperature
14.2 °C
Humidity
63%
Wind
4.8 km/h
Pressure
1024.9 hPa

Moon
Latest preprints on astro-ph:
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Multi-night photometric repeatability of STDWeb: an empirical error budget from a 14-night campaign on a single field ›
Radiative Transfer Modeling of Stripped-envelope Supernovae II: Neural Network Emulation of Light Curves ›
Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy ›
Explaining the X-ray Precursor, Ultra-long Prompt Emission, and Week-long Decay of GRB250702B with a Jetted Micro-TDE ›
The Last Crossing in Excursion-Set Theory of Cosmic Reionization ›
Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics ›
A Sulfur-Rich Atmosphere for the Young Jupiter Analog AF Lep b Reveals Significant Solid Accretion ›
A cosmic collision in the making: JWST/NIRISS reveals a merging and maturing protocluster core at z~3 around a red quasar ›
Flat Galactic Rotation Curves Interpreted as Evidence for the Mach's Principle ›
Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru 'Onohi'ula PFS-SSP ›
Filling the Gap: Calibrating Gyrochronology at 1.3 Gyr with the Benchmark Cluster NGC-752 ›
Lyman Break Galaxy selection and redshift measurement with supervised contrastive learning ›
An X-ray Absorption-Line Survey of the Circumgalactic Medium of M31 with XMM-Newton ›
Technology and Science Advancing Observations with Roman Coronagraph Informed by Ground-Based High-Contrast Imaging ›
SMA Observations Reveal Abundant HNC Chemistry in Transition Disks ›
Spiral Morphology and Radial Migration: Kinematically heating, cooling, and cold ›
From Cluster Core to Splashback: Linking Dynamical Structure to Multidimensional Galaxy Evolution in the Coma Cluster ›
3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves ›
Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors ›
Does IRS13 require an intermediate-mass black hole? ›
Evaporation of Primordial Black Holes with Multimodal Mass and Extended Spin Distributions: Cosmological Imprints on the Effective Number of Relativistic Species ›
The Carruthers Mission Concept and Performance ›
A Pre-Main Sequence Binary Viewed Through its Circumbinary Disk: A New Phase for KH 15D ›
Freezing the speckles: focal plane wavefront sensing with the spatially-clipped self-coherent camera ›
The eXtreme Wavefront Control Toolkit: High-Contrast Imaging Instrument Control for Ground and Space-Based Coronagraphs ›
CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies ›
The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: A Molecular Gas Line Search ›
CCD Rotation Rates From Regular Dispersion Solution Monitoring ›
Constructing X-ray Spectral Models of Galaxies: Varying Contributions from X-ray Binary Populations with Host Galaxy Properties ›
The Rotation Curve of the Milky Way: State of the Art, the Keplerian Decline Debate, and Implications for Dark Matter ›
Wavelength Calibration Accuracy Across the STIS CCD: Pipeline Update and User Guidance ›
Sensor fusion on MagAO-X: real time vibration control using accelerometers ›
Parametric Study of Torus Instability Threshold ›
The final design of GMagAO-X: high-contrast imaging at first-light of the GMT ›
Electron temperature and emission measure of HII regions in the central molecular zone (CMZ) from H40 \alpha recombination line and continuum emissions by ALMA CMZ Exploration Survey - ACES - ›
The Carbon Giant Population Revealed by Gaia DR3 ›
Astro+ database. I. Description and first results ›
Astrophysical Constraints on Hadron--Quark Crossover in Hybrid Neutron Stars ›
Tabular foundation models for the estimation of probabilistic quasar photometric redshifts in S-PLUS ›
Lunar Reflective Interferometry ›
windsoCC: reconstructing the wind-driven halo in MagAO-X images using wavefront sensor telemetry ›
Scaling Relations of Galactic Outflows Across Cosmic Time: New Insights from Cosmic Noon ›
Closed-loop Atmospheric Dispersion Correction for High-Contrast Imaging with MagAO-X ›
Antimatter in the universe and Milky Way ›
Estimating the local star formation rate density from ASKAP RACS ›
Evidence for Enhancement in the Rate of Fast Radio Bursts Toward Galaxy Clusters ›
An Optically Motivated Gamma-ray Study of Fermi-LAT Novae ›
PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation ›
JWST Spectroscopy of Type Ia Supernova 2025rbs from Maximum Light to the Nebular Phase ›
Two new highly scattered fast radio bursts: evidence for scatter broadening by the circumsource medium ›
Electromagnetic responses driven by gravitational-wave memory in magnetar-flare outflows ›
Comparing realtime optical gain measurement and methods on MagAO-X ›
Mapping the Inner Milky Way with Infrared-Derived Distances to AGB Stars ›
Transmutation Timescales for Dark Matter Induced Collapse of Compact Stars into Black Holes ›
Toward a unified framework for helium observations and interpretation of atmospheric escape ›
A Wandering 35,000-Solar-Mass Black Hole Fed by a Gravitational Wake ›
Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? ›
Exploring the long-term temporal variability in polarization through multi-epoch optical spectro-polarimetry - Part I: A sample of Herbig Ae/Be and classical Be stars ›
Synchrotron-Regulated Relativistic Magnetohydrodynamic Turbulence: Emission, Polarization, and Faraday Rotation ›
SIRIUS Project: Dynamical Evolution of Primordial Binaries during Star Cluster Formation ›
Exploring the long-term temporal variability in polarization through multi-epoch optical spectro-polarimetry - Part II: A sample of symbiotic and red-giant stars ›
Application of continuous corrections in widefield imaging obtained with the IDGCAL calibration method ›
Bernhard-1: An Eccentric Binary Periodically Obscured by its Misaligned Circumbinary Disk ›
Evolution of Neutron Star Environment in the Galactic Halo : Implications for Dark Matter Accretion ›
Wavefront Profiling via correlation of GLAO open loop telemetry ›
Evidence for Solar-Cycle Modulation of the Alpha-to-Proton Temperature Ratio in Solar Wind ›
ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models ›
Wind-confined jet collimation revealed by the acceleration-phase photosphere of GRB 220426A ›
Spectroscopic Binary Detection as Agent-Callable Tools: Detecting 40,000+ Main-Sequence Binary Candidates from SDSS DR19 APOGEE Spectra ›
Observational Insights into Post-Main-Sequence Rotation and Magnetism: 20 Years of Science, from the Subgiant to the White Dwarf Phase ›
The Radcliffe Wave is not alone in the Local System ›
Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems ›
Fitting trends in quasar emission and absorption line redshifts ›
Fine-tuning in mixed Dark Matter models with Primordial Black Hole relics ›
Gravity modes and potential evidence for Rossby Waves in late O-type supergiants ›
Opposition effect of comet 28P/Neujmin observed with Subaru Hyper Suprime-Cam ›
Intense but Harmless: Exo-Space Weather Around an M Dwarf with a Single-Hemisphere Dynamo ›
High-temperature photovoltaics for solar-electric Oberth maneuvers: ton-class payload feasibility for interstellar-precursor missions ›
Eclipses by Artificial Satellites to Measure the Angular Sizes of Stars ›
Beyond Feedback: Disentangling Baryonic Effects with tSZ$\times$FRB Cross-Correlations ›
The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae ›
A fast, differentiable neural-network surrogate for precessing binary black-hole waveforms ›
The iSTORM Instrument for Airborne Measurements of Gamma-Ray Emissions from Thunderstorms ›
Dipole-Field Magnetic Windows for Radio-Frequency Transmission Through Hypersonic Plasma Sheaths: A Reduced-Order Scaling Model ›
Mysterious Transients in the Palomar Observatory Sky Survey (POSS-1) as profound manifestation of the Dark Matter physics ›
Eliminating photon transport in long-baseline optical interferometry using quantum memories ›
A $U(1)_{(B-L)_3}$ model for dark matter and the $B^+\to K^+\nu\bar{\nu}$ excess reported by Belle II ›
Heavy neutral leptons beyond the BBN bound: probing the lepton asymmetry of the Universe ›
Scalar baryons in neutron stars ›
A parametrized test of general relativity for inspiralling eccentric binaries in LISA ›
On the nature of oscillating modes of proto-neutron stars ›
The generalized second law as a thermodynamic selection criterion for dynamical dark energy ›
Two-Fluid Schwarzschild Solution ›
Baryogenesis and CMB spectral distortion from Axions ›
All You Need is not $\Omega_\mathrm{gw}$: Beyond the Mean of the Cross-Correlation Estimator when Searching for an Astrophysical Gravitational-Wave Background ›
Advancing Stellar Streams as a Dark Matter Probe -- I: Evolution of the CDM subhalo population ›
Updated Constraints on the Injection Energy of Positrons Generating the Galactic 511 keV $\gamma$-ray line ›
Quantum cosmological perturbations in bouncing models with mimetic dark matter ›
r-Process Nucleosynthesis With Ab Initio Nuclear Masses Around The N=82 Shell Closure ›
The impact of internal versus external perturbations on close-in exoplanet architectures ›
Protoplanetary disc population synthesis I. Linking mass-dependent viscosity, star formation history and environment to observations ›
How Flat is a Plateau? Evolution of Late-Time TDE Disks ›
Nuclear parameter inference with semi-agnostic priors ›
Comprehensive study of solar type II radio bursts and the properties of the associated shock waves ›
Core Scouring Dynamics and Gravitational Wave Consequences: Constraints on Supermassive Black Hole Binary Hardening ›
Thermodynamic characteristics of a Fermi gas with an invariant energy scale and its astrophysical implications ›
The CGM with local universe FRBs: evidence of strong AGN feedback in a massive elliptical galaxy ›
Shock-induced chiral magnetic effect ›
The capture of halo material by orbiting subhaloes ›
PACHA: Probing AGN Coronae with High-redshift AGN ›
An Enriched Methane D/H Ratio in the Interstellar Object 3I/ATLAS ›
A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy ›
The Effect of Expansion and Instabilities in the Thermodynamic Regulation of the Young Solar Wind Plasma ›
Explaining Neural Networks on the Sky: Machine Learning Interpretability for Cosmic Microwave Background Maps ›
Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not ›
Habitability Study of Terrestrial Planets: Application to Venus-like Worlds ›
Impact of Primordial Black Hole population on 21 cm observables at high redshift ›
The GMRT High-Resolution Southern Sky Survey for pulsars and transients -- VIII: Orbital Variability and the Evolution of a 1-Day He-WD Millisecond Pulsar J2101-4208 ›
Upstream neutrino production and delayed jet emission in the blazar GB6 J1542+6129 ›
Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing ›
The Small-scale Structures in the Wind of Messier 82 ›
Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation ›
Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array ›
GRACE-DG: A Discontinuous Galerkin Method-Based Code for General Nonlinear Coagulation-Fragmentation Equations ›
Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds ›
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy ›
Search for Planetary-mass Black Holes with an Improved Viterbi Algorithm ›
Updating the SCExAO/CHARIS polarimetric calibration following the Nasmyth beam-switcher upgrade ›
Effective reheating in Gauss--Bonnet inflation with $\mu(\phi,X)$ coupling ›
Integrated cosmological memory: A dark-siren method to probe dark energy ›
The Lunar Polar Icy Regolith and Possible Moonflows ›
Circumgalactic CIV Absorption Found Only Within 30 Degrees of the Minor Axis of Present-Epoch Galaxies ›
Reconstruction of ASO-S/HXI Solar Flare Hard X-ray Source Images with Physics-Constrained Deep Networks ›
Constraints on the Inert Doublet Model of dark matter with very high-energy gamma-ray observatories ›
Induced Gravitational Waves as Cosmic Tracers of Leptogenesis ›
Black hole spectroscopy: from theory to experiment ›
Circular orbits in spherically symmetric spacetimes and BSW effect with nonzero force ›
Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects ›
Boson star-black hole binaries: initial data and head-on collisions ›
Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis ›
Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound? ↓↑