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

In the dome

Cloud

Rainfall

S Sky
Temperature
13.9 °C
Humidity
53%
Wind
9.7 km/h
Pressure
1008.1 hPa

Moon
Latest preprints on astro-ph:
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Relaxation of a Vlasov gas to an inhomogeneous state due to phase space mixing in an axisymmetric potential: A Newtonian analogy of the Kerr orbital motion ›
Classification of X-ray Binaries in NGC 6946 with the use of Multiwavelength Data ›
An Assessment of the Triangulation Capabilities of a Multi-Site All-Sky Infrared Camera Array ›
Power-law Coupling and Mock Validation of a Surface-density Anisotropy Diagnostic for 85 Rich Galaxy Clusters ›
Deriving the Continuous $\beta$-FPUT Model for Decayless Solar Coronal Oscillations Directly from Resistive MHD ›
The variable mass-loss in low-mass red giant stars: Chromospheric motion across stellar evolution in 47 Tuc ›
BRICS Southern Observatory (BRICS-SO) Project: Invitation to African countries to invest in Chile ›
XuYi Interferometer Observation Simulator ›
A Technosignature Survey Of The Anti-Solar Point: The SETI Institute's Largest-Ever Campaign With The Allen Telescope Array ›
EMIR confirmation of the high-z Ly{\alpha} blob SHARDS20018464 ›
Armillary: A Label-Free Coordinate System for Stellar Spectra ›
Probing departures from Schwarzschild geometry with the S301 star and kilometre-baseline interferometry ›
First Direct Identification of a Multi-Star Microlens System Hosting a Planet ›
Optimal Photon Counting with Fast, Low Noise Astronomical Imagers ›
Cracking open the "dragon egg": ALMA 1.3mm observations of a compact, young high-mass core candidate at 30mas resolution ›
And Then There WEre Baryons (ATWEB): The Baryon Budget of the Universe in Halos and the IGM over 13 Billion Years of Cosmic Time ›
Unlocking new information in stellar circular polarisation with second-order least-squares deconvolution ›
Detecting multiple planets in Gaia data using Bayesian model selection ›
Uncovering the Physical Origins of Black Holes in the Milky Way for Astronomical Surveys ›
Power-Law Injection Spectrum from an Ensemble of Reconnecting Current Sheets ›
Discovery of a second-generation planet candidate accreting onto a white dwarf ›
DIGging into HII regions: the role of ionizing photon leakage and spectral hardening in coupling HII regions and diffuse ionized gas ›
Molecular hydrogen formation on dust: The impact of gas-dust drift on formation efficiency ›
Enhancing the Interpretability of Radial Velocity Analysis Using Leave-one-out Cross-validation ›
Spectroscopic Confirmation of the Milky Way Satellites Bo\"otes V and Leo Minor I and the LMC Satellite DELVE 2: Three Small Ultra-Faint Dwarf Galaxies ›
Hierarchical Black Hole Mergers at High Redshift: Predictions for LISA and LGWA from SEEDZ ›
Exploring the ultrahot Neptune LTT 9779 b with CRIRES+. Non-detection of helium transmission spectra and detection of H$_2$O on the dayside ›
Radial Modes of Hot Neutrino-Trapped Hybrid Stars ›
Lensing in the Blue IV: The First Weak Gravitational Lensing Maps from the Stratosphere ›
Chana: A GPU-Accelerated AMR GRRMHD Code ›
Multiple H I 21-cm absorbers towards blazar PKS 1158+007 ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) VII. First interstellar detection of fully deuterated methanol ›
Investigating X-ray Emission from Radio-detected Broad- and Narrow-line Seyfert 1 Galaxies ›
A spatially resolved view of Fast Radio Burst host metallicities with Integral-field Spectroscopy ›
A Classifier Framework for ALMA Bandpass Calibration Anomalies ›
The universal thickness of mid-infrared bubbles ›
SPECULATE: A synthetic spectral library, emulator and fitting package for accretion disc winds -- Infrastructure and application to CVs ›
Occam's Razor and a Three-Family Ultralight Fermionic Dark Matter Model ›
Tracing the main belt origins of S-complex near-Earth objects: From space mission targets to meteorite sources ›
BRAHMa: Bar Recognition And Hatching using Machine learning -- a framework for oriented bounding box detection of galactic bars ›
Axial-Dipole and Equatorial-Dipole Coronal Holes: Congruent Magnetic Geometry, Divergent Evolution ›
Adaptive proposals for nonparametric equation-of-state inference with RIFT: iterative Gaussian-process refinement in a compressed sequence representation ›
Life in the Cosmic Neighbourhood: Galactic Habitable Zones in the EAGLE Simulations ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) III. CH$_3$OH isotopic fractionation in the low-mass protostar BHR71-IRS1 ›
The Rogue One: A Dark Matter-Dominated Dwarf in the Trail of Dark Matter-Deficient Galaxies ›
High-Angular-Resolution Survey of Stars within 18 pc of the Sun: Part I ›
The First Decade of Breakthrough Listen ›
Barium and europium abundances from the Gaia-ESO Survey using The Cannon ›
Stirred, not shaken: Dislodging $\omega$ Centauri from the Sausage galaxy through bar resonances ›
Discovery of 2 km ultra-fast rotating asteroid in Rubin DP2 catalog via varying Fourier order method ›
Radiation pressure powers quasar broad absorption line winds but fails to drive galaxy feedback ›
Hubble Space Telescope Observations of Active Asteroid (101955) Bennu ›
The Role of the Cosmic Web in Galaxy Evolution Across 0.4 ›
Very Long Baseline Interferometry with the SKA Observatory ›
A Graph Attention Network Framework for Simultaneous Prediction of Galaxy and Dark Matter Halo Properties in GAMA DR4 ›
COSMOS-3D: Spectro-photometric Confirmation of Shabgard, a Cool, Metal-poor Brown Dwarf in the COSMOS Field ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS): I. Overview of the ALMA Large Program ›
Stochastic Bubble Completion in de Sitter Space: Power Spectrum, Bispectrum, and Infrared Moment Hierarchies ›
Chaotic accretion can (still) explain early supermassive black hole growth ›
Optimizing Laguerre-Gaussian Mode Interferometry in Gravitational-Wave Detectors through Modal Degeneracy Breaking ›
Scalable and sequential inference of the neutron star equation of state with the Einstein Telescope ›
Fast and accurate differentiable code of the galaxy power spectrum based on Eulerian and Lagrangian one-loop perturbation theories ›
Does Diffusive Shock Acceleration Reach Steady State? Insights from a Near-Sun Shock Observed by Parker Solar Probe ›
Third-order scalar induced gravitational waves during a matter-dominated era: secular growth and implications for primordial black hole domination ›
HD 715 b, a Warm Jupiter Orbiting a Massive Subgiant Discovered from a Single TESS Transit ›
Probing beyond the Cosmic Horizon ›
Early galactic heavy element production - a phenomenological approach ›
Exploring an X1.8 flare and associated quasi-periodic pulsations using SDO and Aditya-L1 observations, alongside NFFF extrapolation ›
Ariel Tier 3 Observations: An Opportunity to Explore both Stellar and Planetary Variability through Broad Wavelength Time-domain Spectroscopy ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) VI. Discovery of a class I methanol maser transition and its association with acetaldehyde ›
Evolution of neutrino distributions under repeated electron scattering ›
Starspots on weak-lined T Tauri stars in the sigma Orionis cluster ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) II. Approach to data reduction and products for line-rich broadband (sub)millimeter spectra ›
Blinding Lights: Simulation-Based Evidence for Terrestrial Giant Impacts as Astronomically Observable Events ›
X-ray spectral scaling of black hole mass in quasi-periodic eruptive source RX J1301.9+2747 ›
Probing turbulence in the ionized interstellar medium using young pulsars. I. Dispersion measure variations ›
ApPolLO: Apertif counterparts of Polarised LOFAR sources ›
The $\mathrm{[O\ III]}\lambda5007$ Equivalent Width as an Ionization-Parameter Diagnostic Across Cosmic Time ›
The impact of feedback and cosmology on Cosmic Infrared Background cross-correlations ›
Rapid Sequence Cost Evaluation for Multi-Spacecraft Rendezvous: A Permutation-Invariant Set Transformer ›
Predicting High-Energy neutrino emission from X-ray absorption in CSM-interacting SNe ›
Reflex instabilities I: Boundaries makes grid-based disc simulations frame-dependent ›
Reflex instabilities II: The reflex motion of the central object drives at least seven instabilities in accretion discs ›
The Potential Contribution of Radiative Supernova Remnants to the Local Cosmic Ray Spectrum ›
Mapping of interstellar ices with JWST in protostellar envelopes: Spatial variations of $^{13}$CO$_2$, $^{12}$CO$_2$, CO, OCN$^-$ and H$_2$O ice ›
Assessing transitional pulsar candidates through a quantitative estimation of their light-curve similarity ›
Stochastic effect on ultralight dark matter searches with astronomical polarized sources ›
SOPHIE and TESS characterization of fourteen TESS Objects of Interest: nine planetary systems and five low-mass stellar companions ›
It Takes Two: nucleosynthesis in core-collapse supernova simulations of binary-star progenitors ›
Unveiling the Accretion Architecture of GS 1354--64: A Broadband X-ray and Polarimetric Study of its 2025--2026 Outburst ›
Nancy Grace Roman Space Telescope Wide Field Instrument: Grism Saturation Response to Bright Sources during Thermal-Vacuum Testing ›
Boosted Odds: Lower-Point Probes of Parity Violation with Momentum Fields ›
Galaxy merger-driven signatures in massive black hole pair hosts across cosmic time ›
When, Why, and How CMB Compression Fails ›
Halo Mass Function Constraints on Early Galaxy and AGN Populations in the JWST Era ›
Space-based Cosmic Neutrino Measurements ›
Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) -- IV. Methyl cyanide isotopologues toward BHR71-IRS1 ›
Coronal Mass Ejections from the Young Sun: Deceleration-Powered Solar Energetic Particles as a Self-Extinguishing Forcing of the Early Earth ›
Parameter degeneracy and information loss in inverse flavor mapping for high-energy astrophysical neutrinos ›
The pseudospectrum for gravitational perturbations in Kerr spacetimes ›
Lunar radio emission from dark photon dark matter ›
Coherent versus incoherent amplification: from parametric resonance to the kinetic regime in stimulated axion decay ›
Magnus: neutrino oscillation probabilities for any Hermitian Hamiltonian, any number of flavors, and any matter profile ›
Spectator Dark Matter and the Higgs Portal ›
Time-Frequency Analysis for LISA: Galactic Foreground Modulation ›
Axion Pyramid ›
The neutrino magnetic moment and supernovae with strong magnetic fields ›
Flavor decoherence and washout timing in nonthermal leptogenesis after inflation ›
Gravitational Waves and Nambu-Goldstone Bosons from Infrared-Finite Cosmic Strings ›
Decoy and disclosure radii of invariant shape descriptors ›
Line-of-sight Acceleration Driven Effects in Eccentric Compact Binary Coalescences ›
Line-of-Sight Acceleration-driven waveform corrections for unequal-mass compact binary coalescences ›
Universal Relations Meet Causality: Bounding the Dynamical Love Number of Neutron Stars ›
Constraining the gravitational-wave breathing mode with LVK antenna patterns and GWTC data ›
LISA Sensitivity and SNR Calculations ›
Superluminous supernova search with PineForest ›
Extreme superluminal expansion traces an ultra-narrow GRB jet across relativistic regimes ›
Black Holes in the Red-sequence Elliptical Galaxies at Redshifts $\sim 0.7-2.5$: Not Dark Energy Source but Remnants of Little Red Dots ›
A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666 ›
Exploring a Cosmic-Ray Inverse-Compton Origin to the SZ-to-X-Ray Pressure Deficit in the Cool Core Cluster ZwCl 3146 ›
Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants ›
Euclid: Impact of halo mass-conversion model assumptions on galaxy cluster number-count analyses ›
High-Precision Differential Radial Velocities of C3PO Wide Binaries: A Test of Modified Newtonian Dynamics (MOND) ›
Banana Split: Improved Cosmological Constraints with Two Light-Curve-Shape and Color Populations Using Union3.1+UNITY1.8 ›
Unraveling the mysteries of Jets in peculiar NLSy1 galaxies through multi-wavelength variability ›
Searching for outbursts from Symbiotic Binaries in GOTO and ATLAS data ›
Gravitational self-lensing of Fast Radio Bursts in neutron star magnetospheres: II. Applications to strong repeaters and the CHIME population ›
Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS ›
Simulating the jittering-jets explosion mechanism: circum-jet rings account for observed core-collapse supernova remnant morphologies ›
Homogeneous stellar parameters for 717,807 TESS FGK stars using Gaia DR3 ›
A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers ›
Exploring the Impact of Tilted Magnetic Dipoles on the Atmospheric Dynamics of Hot Jupiters: Towards an Improved Magnetohydrodynamic Framework ›
Alleviating the Hubble Tension Using Coupled Dark Energy - Dark Matter Interaction ›
Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models ›
Whispers of Supergravity in Gravitational Wave Backgrounds: Determining the Gravitino Mass from Cosmic Thermal History ›
Probing Direct Contributions of Galaxies and AGN to Cosmic Reionization in a Quasar Field J0226+0302 with JWST NIRCam and NIRSpec ›
PHANTOM: A MATLAB and Octave Toolbox Connecting Linear Field Statistics to Dark Matter Halo Observables ›
Detection of relativistic orbital deformation from improved timing of PSR J1757$-$1854 ›
Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics ›
Radio and X-ray Observations of the Transitional Supernova 2019yvr: Insights into the Progenitor Mass-Loss History ›
The Treble Clef radio phoenix and its old nonthermal filaments ›
Companion architectures of sub-Saturns: Distinct migration pathways across the Neptunian landscape ›
Fast and accurate bandpass integration of complex SEDs with neural networks ›
A Data-Driven Model for $r$-Process Production Patterns ›
The ALMA View of the Edge-on Gomez's Hamburger System: A Highly-Dynamic, Asymmetric Protoplanetary Disk Reveals the Earliest Phases of Giant Planet Formation ›
The New Dark Matter Density Profile from JWST JADES Galaxies ›
Just a Phase? Weakening Vertical Shear Instability Explains Class II Disk Morphologies: Simulations with dust coagulation, sedimentation, thermal relaxation, and backreaction ›
The long period radio transient ASKAP J1448-68 is a cataclysmic variable ›
A Systematic Assessment of Total Stellar Mass Measurements with Spatially Resolved Photometry and Medium Bands at 1 < z < 9: The Impact of Mass-to-Light Variations and Outshining ›
Improved Constraints on the Surface of LHS 3844 b from its Mid-Infrared Spectrum ›
Discovery of the Lyman-$\alpha$ Forest in a Star-Forming Galaxy at $z \approx 7.57$: Implications for the Timing and Topology of Cosmic Reionization ›
Deep radio characterization of the supernova remnant G343.1-00.7 ›
Vector field dark matter search with Sagnac interferometer ›
Pulsations and constraints on time lags in two distinct ULXs: NGC 5204 X-1 and NGC 55 ULX-1 ›
Irradiated Atmospheres VII. Effect of Mixing Energy Flux on Atmosphere-Interior Coupling ›
From the Milky Way to the Early Universe: How Metallicity Shapes the Formation of Double Neutron Stars ›
Einstein ring fingerprint around supermassive black holes illuminated by broad line region spectral lines ›
Rotation of the polarization plane in axion fields: application to neutron star polar cap regions ›
Analytic Approximations for Fermionic Preheating ›
Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum ›
Polarization Analysis of Ringdown Signals ›
Detector orientation matters: Consequences for gravitational-wave background detectability ›
Stochastic template banks for GW searches using low-discrepancy sequences ›
Building a Better Beta: Nucleation and Timescales in Cosmological Phase Transitions ↓↑