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-west

Cloud

Rainfall

S Sky
Temperature
1.8 °C
Humidity
91%
Wind
4.8 km/h
Pressure
1018.6 hPa

Moon
Latest preprints on astro-ph:
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Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows ›
Globules and pillars in Cygnus X IV. Velocity-resolved [OI] 63 mu map of a peculiar proplyd-like object ›
Effects of Resolution and Local Stability on Galactic Disks: I. Multiple Spiral Mode Formation via Swing Amplification ›
Asteroseismic detection of an internal magnetic field in the B0.5V pulsator HD 192575 ›
APEX survey of interstellar HCl: $^{35}$Cl/$^{37}$Cl isotopic ratios in dense cores and outflows ›
Statistical Properties of Cold Streams In Massive Star-Forming Halos in IllustrisTNG-50 ›
The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration ›
A Paradigm Shift in Exoplanet False Positive Identification with HIP-44302 ›
The impact of magnetic fields during tidal disruption events ›
Little Red Dots host Black Hole Stars: A unified family of gas-reddened AGN revealed by JWST/NIRSpec spectroscopy ›
J-PAS: A value-added catalogue of optical line intensities for nebular emission galaxies (JOLINES) ›
Probing Exotic Astrophysical Dark objects through Astrometric Microlensing from Gaia ›
LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background ›
The HITRAN2024 methane update ›
The LMT 2 millimeter receiver system (B4R). II. Science demonstration observations toward Orion-KL/OMC-1 ›
Evaluating Star-Planet Interactions with Zeeman Doppler Imaging: Case Study in YZ Ceti ›
Intrinsic galaxy alignments in CAMELS simulations and the significant impact of baryon model ›
Gravitational Waves as a Probe of Core Collapse Supernova Progenitor Structure ›
Modeling Galaxy Formation in Cosmological Simulations with CRK-HACC ›
The relations between dust properties and galaxy global / integrated quantities in the nearby Universe ›
Data span and frequency coverage requirements for robust detection and inference in PTAs: A case study with EPTA DR2 ›
The Atacama Cosmology Telescope: $B$-mode delensing with DR6 data and external tracers of large-scale structure ›
Vibrationally excited H2 mutes the He i triplet line at 1.08 {\mu}m on warm exo-Neptunes ›
Interferometric view into RT Pav's long secondary period. binary vs oscillatory convective modes ›
Numerical implementation of flat FLRW models of cosmic expansion with Planck 2018 cosmological parameters ›
A Catalogue of Mid-infrared Variable Sources from unTimely ›
Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak ›
Deep insights into Abell 2163: unveiling the treasure trove of ICM plasma physics ›
Constraining the Properties of GRB Accreting Magnetar with $R/I$ Evolutionary Effects Using \emph{Swift}/XRT Data ›
A Novel Comb Generator for Frequency Phase Transfer ›
Probing CMB Polarization Gaussianity with the Statistics of Unpolarized Points: Non-Gaussianity of Planck Data and Prospects for Future B-Mode Measurements ›
Forecasting Primordial Non-Gaussianity from UNIONS Lyman-Break Galaxies and Planck CMB lensing ›
Galaxy rotation curve based on RGB stars from the Gaia DR3 catalogue ›
Recovering Intrinsic Pulsar Profiles and Scattering Parameters with a CLEAN-Based Algorithm for High-Precision Timing ›
Astrophysical constraints from future measurements of the kinetic Sunyaev-Zel'dovich power spectrum ›
The life of central radio galaxies in clusters: AGN-ICM studies of eRASS1 clusters in the ASKAP fields ›
The First Scientific Flight and Observations of the 50-mm Balloon-Borne White-Light Coronagraph ›
Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images ›
Manifestation of the stellar wind cycle in infrared images: Example of the heliosphere ›
Galaxy and Mass Assembly (GAMA): The Properties of Quasar Host Galaxies: Star Formation Histories and Stellar Populations ›
Differentiable N-body code for Galactic Dynamics -- Odisseo ›
The Solar Close Observations and Proximity Experiments (SCOPE) mission ›
Clustering in dynamical dark energy: observational constraints from DESI, CMB, and supernovae ›
Classical Cepheids in the Galactic thin disk. I. Abundance gradients through NLTE spectral analysis ›
Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data ›
Needle in a Poissonian haystack -- An X-ray astronomer's guide to QPE fishing ›
Spiral excitation in protoplanetary disks through gap-edge illumination: Distinctive kinematic signatures in CO isotopologues ›
Towards Understanding the Origin of Swift Gamma-Ray Bursts Driven by Magnetars ›
Laboratory Detection and Rotational Spectroscopy of $trans$-HNSO: Implications for Astronomical Observations ›
Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters ›
The network analysis of the cosmic web as a tool to constrain cosmology and cosmic magnetism ›
ALMACAL. XV. Band 3 ALMA Survey and Number Counts ›
Forecasting Constraint on Primordial Black Hole Properties with the CSST $3\times2$pt Analysis ›
Skew-spectra: a generalization to spin-$s$ ›
The NANOGrav 12.5-year Data Set: Chromatic Noise Characterization & Mitigation with Time-Domain Kernels ›
Identifying Transient Hosts in LSST's Deep Drilling Fields with Galaxy Catalogues ›
Non-Gaussianity in SMICA ›
Tracing Structure: Shape and Centroid Deviations in 39 Strong Lensing Clusters as a Test of Cluster Formation Predictions ›
Structure-Preserving Unpaired Image Translation to Photometrically Calibrate JunoCam with Hubble Data ›
Vortex Dynamics in the Neutron Star Inner Crust ›
The Parkes Observatory Pulsar Data Archive ›
Evading the dust fragmentation barrier with the streaming instability in protoplanetary disks ›
EMU and Euclid: Detection of a radio-optical galaxy clustering cross-correlation signal between the Evolutionary Map of the Universe and Euclid ›
Closing the gap: Follow-up observations of peculiar dusty objects close to Sgr A* using ERIS ›
The Hubble Ultracool Multiplicity (HUM) Survey. I. Characterizing Sensitivity to Companions at Sub-Diffraction Limit Separations with HST WFC3/IR ›
The Shear-to-Cosmology Paradigm I: Hybrid Field-Level and Simulation-Based Framework for Weak Lensing Surveys ›
BSN: The First Multiband Light Curve Analysis of the W UMa-type Contact Binary System EM Tucanae ›
SN 2021ukt: A Transitional Supernova with a Short Plateau and Persistent Interaction ›
Collapse of Axion Domain Wall Induced by Helical Primordial Magnetic Fields ›
Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Analytical Model to Predict Cloud-Scale Star Formation Rate ›
Incorporating neutron star physics into gravitational wave inference with neural priors ›
Blending-induced beating and emission in the symbiotic star Terz V 2513 ›
ExoJAX Retrievals of VLT/CRIRES Spectra of Luhman 16AB: C/O Ratios and Systematic Uncertainties ›
High-resolution cosmological simulations of primordial dark matter clustering under long-range and fractional forces ›
The observation of Ground Level Enhancement GLE 77 by the neutron detectors of the Experimental Complex NEVOD ›
Constraining dark matter halo profiles with symbolic regression ›
$\delta$ Circini: A massive hierarchical triple system with an eclipsing binary ›
Predictions from $s$-process AGB models of the isotopic variations of zirconium and neodymium for comparison to bulk meteorites ›
Consequences of radially correlated rotation curves for galaxy mass models ›
Young M dwarfs flare activity model: Towards better exoplanetary atmospheric characterisation ›
Blazar classification from multi-wavelength data using Deep Learning ›
Sulfur monoxide as a tracer of the Galactic $^{32}$S/$^{34}$S gradient ›
Large-amplitude Variability Driven by Giant Dust Storms on a Planetary-mass Companion ›
Bursty star formation, chemical enrichment, and star cluster formation in numerical analogues of GN-z11 ›
An improved formalism for measuring the dark matter subhalos mass by its gravitational wake ›
Primordial Black Holes as Dark Matter and the Tachyonic Trap During Inflation ›
Predictions on gravity mode pulsations of collisional blue straggler stars in globular clusters ›
Witten-O'Raifeartaigh potential revisited in the context of Warm Inflation ›
SlotFlow: Amortized Trans-Dimensional Inference with Slot-Based Normalizing Flows ›
Tools and Advancements towards Data Standardization of the MAGIC Collaboration ›
Macroscopic Dark Matter under siege: from White Dwarf Data to Gravitational Wave Detection ›
Simulating AGN feedback in galaxy clusters with pre-existing turbulence ›
Properties of Core Collapse Supernovae from Binary Population Synthesis ›
A Detection of Sulfur-Bearing Cyclic Hydrocarbons in Space ›
Calcium versus silicon ejecta velocities and decline rates in supernovae Ia: The role of high-velocity features ›
Stellar streams around dwarf galaxies in the Local Universe ›
CO observations in rotating circumbinary post-AGB disks ›
Synchrotron Self-Compton Model of TeV Afterglows in Gamma-Ray Bursts ›
Investigating the Impacts of AGN Activities on Dwarf Galaxies with FAST HI Observations ›
The Kinematic Properties of T\.ZO Candidate HV 11417 with Gaia DR3 ›
Identifying bars in galaxies using machine learning ›
Consensus based Algorithm for Nonparametric Detection of Star Clusters (CANDiSC) ›
Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect and Pairwise Velocity with DESI DR1 Galaxies and ACT DR6 and Planck CMB Data ›
Inflation Driven by Scalar-Neutrino Coupling in a Mass-Varying Neutrino Framework ›
Variation of Microphysical Parameters in Reverse-shock Scenario ›
The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries ›
A measurement of $H_0$ from DESI DR1 using energy densities ›
From metallicity distributions to mutual information: A new perspective on stellar halo assembly ›
Baryon fraction from the BAO amplitude: a consistent approach to parameterizing perturbation growth ›
Kinetic Mixing and the Phantom Illusion: Axion-Dilaton Quintessence in Light of DESI DR2 ›
A Comprehensive Study of WIMP Models Explaining the Fermi-LAT Galactic Center Excess ›
Bubble Nucleation from Boson Star Collapse ›
High Mass Dark Matter Searches With the High Speed Flux From the Large Magellanic Cloud ›
GANDALF: A hardware-agnostic spectral solver for kinetic reduced MHD turbulence ›
Gravitational waves from the late inspiral, transition, and plunge of small-mass-ratio eccentric binaries ›
Searches for Post-Merger Gravitational Waves with CoCoA: Sensitivity Projections Across Large Template Banks for Current and Next-Generation Detectors ›
On the Relation between Source Region and In-situ Variability of Low $\delta B$ Solar Wind Streams ›
QCD axions and domain walls in dense matter under compact stellar conditions ›
Lorentz Violation in Emergent Gravity and Its Cosmological Consequences ›
Kerr black holes as circular polarizers ›
Data-driven informative priors for Bayesian inference with quasi-periodic data ›
Net Charge Accretion in Magnetized Kerr Black Holes ›
Multipole moments do not uniquely characterise spacetimes beyond general relativity ›
Misalignment dynamics of Scalar Condensates with Yukawa coupling: Particle and Entropy Production ›
3D Modeling of Solar Oscillations with Hybridizable Discontinuous Galerkin Method ›
Inflation, black holes with primary hair, and regular planar black holes from an infinite tower of regularized Lovelock-Proca corrections ›
Constraining of Nuclear Matter Equations of State With Rotating Neutron Stars ›
Scalar field effective potentials in de Sitter spacetime ›
Statistical analysis and correction of the pile-up effect in MAPMT single photoelectron counting with the SPACIROC-3 ASIC: application to the Mini-EUSO experiment ›
Vector-field spontaneous baryogenesis with Lorentz invariance violation ›
Multipartite entanglement features of primordial non-gaussianities ›
Klein Bottle Cosmology ›
Observational constraints of diffusive dark-fluid cosmology ›
Total and dark mass from observations of galaxy centers with Machine Learning ›
Where do stars explode in the ISM? -- The distribution of dense gas around evolved massive stars in M33 ›
Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis ›
LINX: A Fast, Differentiable, and Extensible Big Bang Nucleosynthesis Package ›
Deep Investigation of Neutral Gas Origins (DINGO): Options for the Processing and Storage of Radio Astronomy Data for robust Deep Spectral Line Imaging in the SKA-Era using uv-Grids ›
The galaxy-IGM connection in THESAN: observability and information content of the galaxy-Lyman-$\alpha$ cross-correlation at z$\geq$6 ›
Stochastic gravitational wave background anisotropies from inflation with non-Bunch-Davies states ›
Cosmological Model Independent Constraints on Lorentz Invariance Violation with Updated Gamma-Ray Burst Observations: An Artificial Neural Network Approach ›
Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology ›
The dynamical and thermodynamic effects of turbulence for the cosmic baryonic fluid ›
A new approach for simulating PBH formation from generic curvature fluctuations with the Misner-Sharp formalism ›
Ultra-diffuse galaxies in the EAGLE simulation ›
A multi-messenger window into galactic magnetic fields and black hole mergers with LISA ›
A New Wavelet Scattering Transform-Based Statistic for Cosmological Analysis of Large-Scale Structure ›
Collisionless relaxation to equilibrium distributions in cold dark matter halos: origin of the Navarro-Frenk-White profile ›
JWST Spectroscopy of a Blue Binary Cold Classical Kuiper Belt Object ›
Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals ›
Sulphur abundances in star-forming regions from optical emission lines: A new approach based on photoionization models consistent with the direct method ›
CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer ›
Cosmological abundance of primordial black holes in mixed dark matter scenarios incorporating Kaluza-Klein dark matter ›
HOLISMOKES XVIII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data ›
Dissecting Reionisation with the Cosmic Star Formation and Active Galactic Nuclei Luminosity History ›
Direct correlation of line intensity mapping and CMB lensing from evolution along the lightcone ›
MUSEQuBES: The Column Density, Covering Fraction, Mass, and Environmental Dependence of Cool HI Gas Around Low-Redshift Galaxies ›
The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation ›
Impact of Resonance, Raman, and Thomson Scattering on Hydrogen Line Formation in Little Red Dots ›
Field-level Reconstruction from Foreground-Contaminated 21-cm Maps ›
VIPCALs: A fully automated calibration pipeline for very long baseline interferometry data ›
Constraining deviations from $\Lambda$CDM in the Hubble expansion rate ›
SN2023syz and SN2025cbj: Two Type IIn Supernovae Associated with IceCube High-energy Neutrinos ›
Rethinking mass transfer: a unified semi-analytical framework for circular and eccentric binaries. I. Orbital evolution due to conservative mass transfer ›
The Hubble constant from the improved lens modeling of cluster-lensed supernova Refsdal with new spectroscopic redshifts and the Jackknife method ›
Sibling Sub-Neptunes Around Sibling M Dwarfs: TOI-521 and TOI-912 ›
A novel reverberation mapping method for blazars ›
Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity ›
Impact of the latest 22Ne+{\alpha} reaction rates on nucleosynthesis in massive stars and galactic chemical evolution ›
A Less Terrifying Universe? Mundanity as an Explanation for the Fermi Paradox ›
Evidence for increasing dark energy in DESI from the Local Distance Ladder ›
Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics ›
The Tidal Torque Theory Revisited: II. Rotational Halo Properties ›
Measurements of the Birks' coefficient of GAGG:Ce using hard X-rays ›
SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations ›
Mode Composition Shapes Magnetic Anisotropy in Solar Wind Turbulence ›
Cosmic voids and the kinetic analysis. V. Hubble tension, the cosmological constant and aperiodic filaments ›
Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature ›
Recoil-Enabled Energy Transfer from Coherent Neutrino Scattering in Core-Collapse Supernovae ›
Galaxy Clusters from the DESI Legacy Imaging Surveys. III.Star-forming Fraction of Brightest Cluster Galaxies ›
REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization ›
PRIMA General Observer Science Book Volume 2 ›
Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data ›
Deep Investigation of Neutral Gas Origins (DINGO): Options for robust Deep Spectral Line Imaging in the SKA-Era ›
Measurement of Milli-Charged Particles with a running electromagnetic coupling constant at IceCube ›
Broad-band temporal and spectral study of TeV blazar TXS 0518+211 ›
Quantifying the differences in transmission and emission spectra for hot irradiated gaseous exoplanet atmospheres: A comparison of 1D and 3D modeling using JWST ›
Compton-induced $\gamma$-ray Cascade Emissions in Radio Galaxy NGC 1275 ›
Wideband search for axionlike dark matter using octupolar nuclei in a crystal ›
A Catalog of First-Order Electroweak Phase Transitions in the Standard Model Effective Field Theory ›
Post-adiabatic waveform-generation framework for asymmetric precessing binaries ›
Cosmological perturbation theory with trinity of scalar fields ›
Waveform models for the gravitational-wave memory effect: II. Time-domain and frequency-domain models for nonspinning binaries ›
Thermodynamics of magnetized BPS baryonic layers and the effects of the Isospin chemical potential ›
Gravitational waves in minimal Maxwell $f(R)$ gravity ›
Leptophilic dark matter in $U(1)_{L_{i}-L_{j}}$ models: a solution to the Fermi-LAT Galactic Center Excess consistent with cosmological and laboratory observations ›
QCD corrections to Minimal Dark Matter annihilations ›
Unified Framework for Geodesic Dynamics with Conservative, Dissipative, and GUP Effects ›
Gravity and the Hierarchy Problem ›
Bound State Perturbations in the Interior of Black Holes ›
Probing the nonstrange quark star equation of state with compact stars and gravitational waves ›
WallGo investigates: Theoretical uncertainties in the bubble wall velocity ›
Gravitational Bound State Perturbations Inside Black Holes and Isospectrality ›
Numerical tiling-based simulations of decoherence in multifield models of inflation ›
Ghost instabilities and strong coupling in quadratic non-metricity theories ›
$\mathbb Z_2$-Stable Dark Matter via Broken $\text{SU}(5)$ Gauge Bosons ›
A Bottom-Up EFT Approach To Superdense Baryonic Matter ↓↑