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-east

Cloud

Rainfall

S Sky
Temperature
2.1 °C
Humidity
94%
Wind
4.8 km/h
Pressure
999.8 hPa

Moon
Latest preprints on astro-ph:
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$\mathtt{Entity}$ -- Hardware-agnostic Particle-in-Cell Code for Plasma Astrophysics. II: General Relativistic Module ›
Detecting the signature of helium reionization through 3HeII 3.46cm line-intensity mapping ›
The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline ›
Hierarchical Interferometric Bayesian Imaging ›
Kepler-1624b Has No Significant Transit Timing Variations ›
Entity -- Hardware-agnostic Particle-in-Cell Code for Plasma Astrophysics. I: Curvilinear Special Relativistic Module ›
PROJECT-J: the shocking H2 outflow from HH46 ›
Evidence of 1:1 slope between rocky Super-Earths and their host stars ›
Neural posterior estimation of the line-of-sight and subhalo populations in galaxy-scale strong lensing systems ›
JADES: Low Surface Brightness Galaxies at 0.4 < z < 0.8 in GOODS-S ›
The Optical Evolution of the Tycho Supernova Remnant over Three Decades ›
Outflow Interaction in Cep-E: Numerical Simulation and Observational Manifestation ›
The Northern High Time Resolution Universe pulsar survey -- II. Single-pulse search set-up and simulations ›
Broadband X-ray observations of the periodic optical source ZTF J185139.81+171430.3 and its identification as a massive intermediate polar ›
An Overabundance of Radio-AGN in the SPT2349-56 Protocluster: Preheating the Intra-Cluster Medium ›
TIC 322208686: An Eclipsing System with $\gamma$ Doradus Pulsations and a Third Component on a Wider Orbit ›
Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon ›
Prospects for measuring the Doppler magnification dipole with LSST and DESI ›
Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars ›
A New FU Orionis Accretion Outburst in the W5 HII Region ›
Revisiting $\gamma$-Ray Orbital Modulation in the Redback Millisecond Pulsar PSR J2039-5617 ›
A stringent constraint on the fractional change of proton g-factor ›
Outbursts in ultra-compact AM CVn binaries ›
ACES: The Magnetic Field in Large Filaments in the Galactic Center ›
B[e]-star CI Cam: a high-resolution spectrum atlas in the range of 395$\div$780 nm ›
Verifying the failing supernova constraint on dark photons with two-dimensional hydrodynamic simulations ›
Full calibration of the tomographic redshift distribution from the HSC PDR3 Shape Catalog with DESI ›
Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI ›
Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from A Cosmic-Ray Transient ›
JWST COMPASS: Insights into the Systematic Noise Properties of NIRSpec/G395H From a Uniform Reanalysis of Seven Transmission Spectra ›
Tracing Quenching in Nearby Galaxies Through Inner Surface Mass Density and Cold Gas Content ›
Deep X-ray observation of NGC 3221: everything everywhere all at once ›
Curvature Perturbations from Higgs Modulated Reheating ›
A Bayesian statistical analysis of 897 pulsar flux density spectra ›
GRB 240715A: Revealing Novel Intrinsic Mechanism by Different Individual Pulse ›
Black Hole Spin Estimation with Time-variable Image of M87 During the Flaring State ›
On the bin sensitivity of the transverse BAO ›
Resolution and calibration effects in high contrast polarimetric imaging of circumstellar scattering regions ›
Approximate analytic model of the boundary layer around a low magnetic field neutron star at the disk accretion ›
A Catalog of Galactic Atomic Hydrogen Position-Position-Velocity Filaments ›
A Deep Multimodal Multi--Head Neural Network for Joint Estimation of Stellar Age, Lifetime, and Evolutionary Stage ›
Prospects for cosmological research using hundred-meter-class radio telescopes: 21-cm intensity mapping survey strategies with QTT, JRT, and HRT ›
Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves ›
Synthesis imaging with a lunar orbit array: I. global sky map and its systematics ›
The Albedo Problem and Cloud Cover on Hot Jupiters ›
Revealing the magnetization of the intracluster medium of Abell 3581 using background Faraday rotation measures from the POSSUM survey ›
Optimizing the potential of KM3NeT in detecting core-collapse supernovae ›
r-Process nucleosynthesis from hyperaccreting neutron stars in common envelopes ›
From Simulations to Surveys: Domain Adaptation for Galaxy Observations ›
The Plane Quasar Survey: An Ionized Extension of the Magellanic Stream on the Northern Side of the Galactic Plane ›
Milky Way galaxy-analogs and isolated galaxies with bars: environmental density in the Local Volume ›
Insights into jet-NLR energetics in PMN J0948+0022 ›
How Primordial Black Holes Change BBN ›
Disc breaking and parametric instability in warped accretion discs ›
How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements ›
Fast Radio Bursts from White Dwarf Binary Mergers: Isolated and Triple-Induced Channels ›
Tracing the Trace Anomaly of Dense Matter inside Neutron Stars ›
Hierarchical Bayesian estimation of population-level torque law parameters from $68$ young radio pulsars observed with the Murriyang telescope ›
A Smooth Transition from Giant Planets to Brown Dwarfs from the Radial Occurrence Distribution ›
The Dynamical Interaction between Low-mass Planets and Dust Coagulation ›
Numerical Non-Adiabatic Tidal Calculations with GYRE-tides: The WASP-12 Test Case ›
Icy worlds: Moons and Dwarf Planets ›
TDLight: A Framework for Incremental Light Curve Management and Smart Classification ›
Measurement of Milli-Charged Particles with a running electromagnetic coupling constant at IceCube ›
The dawn is quiet II: Gaia XP constraints on the Milky Way's proto-Galaxy from very metal-poor MDF tails ›
BSN-V: The First Detailed Light Curve Modeling of Eight Totally Eclipsing Contact Binary Stars Using Ground-Based and TESS Observations ›
STORMY : A Real-time Triggering Framework using Yamagawa Solar Spectrograph for Active Solar Emission Observations with the MWA ›
Improved constraints on ultralight axions using latest observations of the early and late Universe ›
On the planetary forcing of the Solar dynamo: Evidence from a Lagrangian framework ›
The variability of blazars throughout the electromagnetic spectrum ›
The complex inner disk of the Herbig Ae star HD 100453 with VLTI/MATISSE ›
Resolving the flat-spectrum conundrum: clumpy aerosol distributions in sub-Neptune atmospheres ›
Enhancing Fast Radio Transient Detection with Mask R-CNN Image Segmentation ›
Lost and Found - A gallery of overlooked optical nuclear transients from the ZTF archive ›
Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts ›
Chondrule formation by collisions of planetesimals containing volatiles triggered by Jupiter's formation ›
Multi-height probing of horizontal flows in the solar photosphere ›
Time-dependent Turbulent Electron Acceleration and Transport in Solar Flares ›
Spectrophotometric evidence for a metal-bearing, carbonaceous, and pristine interstellar comet 3I/ATLAS ›
Observations of sulfuretted species in HL Tau ›
Separating the Inseparable: Constraining Arbitrary Primordial Bispectra with Cosmic Microwave Background Data ›
A search for photometric variability towards the globular cluster M3 with the TWenty Inch Survey Telescope ›
Towards testing gravity with LSST using $E_G$ ›
Observing bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution ›
Inclinations and Position Angles for Disc Galaxies in the SGA sample ›
Centennial solar EUV irradiance from ionospheric currents: Varying sunspot-EUV irradiance relation and modified spot-facula ratio ›
What do gravitational-wave observations tell us about Luminous Red Novae? ›
The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos ›
The TEQUILA catalog of variables in TESS full-frame images: Differential photometry light curves from the first two years of observations ›
Revisiting model-independent constraints on spatial curvature and cosmic ladders calibration: updated and forecast analyses ›
Systematic assessment of the Hubble tension via Bayesian jackknife testing ›
Kinematics show consistency between stellar mass and supermassive black hole parent population jet speeds ›
Historical Reconstruction of Solar Surface Magnetism from Cycle 1-24 Using the Synthetic Active Region Generator (SARG) and the Advective Flux Transport (AFT) Model ›
Limits on GeV-scale WIMP Annihilation in Dwarf Spheroidals with IceCube DeepCore ›
Guesswork in the gap: the impact of uncertainty in the compact binary population on source classification ›
Probing the Formation Environment of Strongly Lensed Black Hole Mergers: Implications for the AGN-disk Channel ›
Gamma-ray Time Delay and Magnification Ratio in the Gravitationally-Lensed Blazar PKS 1830-211 ›
Exploring the universal $\bar{\mathcal{I}}-\mathcal{C}$ relations for relativistic stars in $f(Q)$ gravity ›
Post-Supernova Accretion of Light Elements onto a New-Born Neutron Star and NS 1987A ›
Classification of Transient Astronomical Object Light Curves Using LSTM Neural Networks ›
Vision-Guided Optic Flow Navigation for Small Lunar Missions ›
WavePID: Studies of DOM-level waveform timing for track vs. cascade discrimination in IceCube at 5-100 GeV ›
The $\mu$-deformed Einstein field equations with $\mu$-dependent effective cosmological constant ›
Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector ›
Constraining linear form of $f(\mathcal{R,G,T})$ gravity from astrophysical observations of the Pulsar U1724 ›
Hawking-radiation-ignited autocatalytic formation of primordial black holes ›
Detection prospects for the Cosmic Neutrino Background using matter interferometers ›
Constraint on massive vector field with extreme-mass-ratio inspirals around a slowly rotating black hole ›
Hyperspectral Variational Autoencoders for Joint Data Compression and Component Extraction ›
From LIGO to Fiber- Compact Sagnac Interferometer for Gravitational-Wave Detection ›
Dynamical interplay between coupled scalar dark sectors and gravity ›
Enhancing low energy reconstruction and classification in KM3NeT/ORCA with transformers ›
Black hole binaries in shift-symmetric Einstein-scalar-Gauss-Bonnet gravity experience a slower merger phase ›
Ghost instabilities and strong coupling in quadratic non-metricity theories ›
Inflation in theories with broken diffeomorphisms ›
Neural surrogates for designing gravitational wave detectors ›
Gravitational Wave Probe of Singlet-Doublet Dark Matter Induced Radiative Neutrino Mass ›
Predicting partially observable dynamical systems via diffusion models with a multiscale inference scheme ›
Refractive neutrino masses in the solar DM halo: Can the dark-LMA solution be revived? ›
Axion Cosmology with Multi-Branch Yang-Mills ›
Gravitational waves from dark domain walls ›
Residual neural networks to classify the high frequency emission in core-collapse supernova gravitational waves ›
Inferring Magnetic Field Morphology and Dust Scattering Geometry from Mid-IR Polarimetry: the Extended Aitken Method ›
Constraints on the Hubble and matter density parameters with and without modelling the CMB anisotropies ›
TXS 0506+056-like blazar sources and their role as possible neutrino emitters ›
Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars ›
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars ›
Study of primordial non-Gaussianity $f_{\mathrm{NL}}$ and $g_{\mathrm{NL}}$ with the cross-correlations between the scalar-induced gravitational waves and the cosmic microwave background ›
Constraining Axion Dark Matter with Galactic-Centre Resonant Dynamics ›
Constraining the Hubble Constant with a Simulated Full Covariance Matrix Using Neural Networks ›
A method for statistical research on binary stars using radial velocities ›
Quantifying the Impact of LSST $u$-band Survey Strategy on Photometric Redshift Estimation and the Detection of Lyman-break Galaxies ›
PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). II. Phase-Resolved Cross-Correlation Transmission Spectroscopy of KELT-20b ›
Over-Luminous Type Ia Supernovae and Standard Candle Cosmology ›
Dark Matter (S)pins the Planet ›
The Compton-Getting origin of the large-scale anisotropy of Galactic cosmic rays ›
Constraints on the lepton asymmetry from DESI DR2 BAO data ›
V965 Cephei revisited: evidence for a binary system ›
Diverse reddening distributions in sight lines to type Ia supernovae ›
A black hole in a near-pristine galaxy 700 million years after the Big Bang ›
The Pandora project. II: how non-thermal physics drives bursty star formation and temperate mass-loaded outflows in dwarf galaxies ›
Primordial black holes with mass ratio-modulated initial clustering: merger suppression and projected constraints ›
The Detection-vs-Retrieval Challenge: Titan as an Exoplanet ›
JADES and BlackTHUNDER: rest-frame Balmer-line absorption and the local environment in a Little Red Dot at z = 5 ›
Cancellation of one-loop correction to soft tensor power spectrum ›
Sensitivity of the redshifted 21 cm signal from the Dark Ages to parameters of primordial magnetic fields ›
A theoretical prediction for the dipole in nearby distances using cosmography ›
Bouncing Grains Keep Protoplanetary Disks Bright ›
20 GeV halo-like excess of the Galactic diffuse emission and implications for dark matter annihilation ›
MUSE IFU observations of galaxies hosting of Tidal Disruption Events ›
Testing signatures of phantom crossing through full-shape galaxy clustering analysis ›
The IACOB project XV. Updated calibrations of fundamental parameters of Galactic O-type stars ›
A Targeted Gamma-Ray Search of Five Prominent Galaxy Merger Systems with 17 years of Fermi-LAT Data ›
Bayesian Inference of Gravity through Realistic 3D Modeling of Wide Binary Orbits: General Algorithm and a Pilot Study with HARPS Radial Velocities ›
The Cosmic Dance: Observational Detection of Coherent Spin in Galaxy Clusters ›
Machine learning classification of black holes in the mass--spin diagram ›
Analytic Model for Scattered Ly$\boldsymbol{\alpha}$ Emission in the Post-reionization Intergalactic Medium ›
Precise Measurement of the Absolute Sky Brightness at 60 to 350 MHz ›
Anisotropic Cosmic Ray Transport in strong MHD Turbulence due to Magnetic Mirroring and Resonant Curvature Scattering ›
Stellar Feedback Effects on the Mass Distribution of Clouds and Cloud Complexes ›
How two-dimensional are planet-disc interactions? II. Radiation hydrodynamics and suitable cooling prescriptions ›
HST Confirms Sub-5 kpc Dual Quasar Pairs at Cosmic Noon ›
Trade-off Analysis for Lunar Augmented Navigation Service (LANS) Constellation Design ›
Head-tail molecular clouds falling onto the Milky Way disk ›
Particle acceleration at radiative supernova remnant shocks ›
Nearly Monochromatic Primordial Black Holes as total Dark Matter from Bubble Collapse ›
Systematics mitigation for catalogue-based angular power spectra ›
Revisiting Very High Energy Gamma-Ray Absorption in Cosmic Propagation under the Combined Effects of Axion-Like Particles and Lorentz Violation ›
StarDICE IV: correcting visible photometry from atmospheric gray extinction using thermal infrared observations ›
Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared ›
Dynamical Masses and Radiative Transfer Modeling of HD 698: a Be Binary in Evolutionary Transition ›
Euclid Quick Data Release (Q1): Hunting for luminous z > 6 galaxies in the Euclid Deep Fields -- forecasts and first bright detections ›
The Type Ia Supernova 2021hem: A 2003fg-like Event in an Apparently Hostless Environment ›
Detection of Lensed Gravitational Waves from dark matter halos with deep learning ›
Topmetal-L: A Low Noise Charge-Sensitive Pixel Sensor for POLAR2/LPD ›
Where Galaxies Point: First Measurement of the Large-Scale Axial Intrinsic Alignment ›
ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at $z = 3.1$ ›
A new estimate of the zero-point shift of the Gaia DR3 parallaxes obtained from a comparison with VLBI measurements of masers and radio stars ›
Investigating the Dark Energy Constraint from Strongly Lensed AGN at LSST-Scale ›
Ultralight Dark Matter Statistics for Pulsar Timing Detection ›
Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation ›
Frequency contamination from new fundamental fields in black hole ringdowns ›
Radial and Non-Radial Oscillations of Protoneutron Stars with Hyperonic Composition ›
Unitarity-Conserving Non-Minimally Coupled Inflation and the ACT Spectral Index ›
Ring formation from black hole superradiance through repeated particle production on bound orbits ›
Generation of axions and axion-like particles through mass parametric resonance induced by scalar perturbations in the early universe ›
New models of nonsingular black hole dark matter from limiting curvature ›
Thermodynamic stability of superflows in General Relativity and Newtonian gravity ›
Transition to Petschek Reconnection in Subrelativistic Pair Plasmas: Implications for Particle Acceleration ›
Bouncing Cosmologies in modified gravity with space time torsion ›
ReplicationBench: Can AI Agents Replicate Astrophysics Research Papers? ›
Wavefront Curvature and Transverse Atomic Motion in Time-Resolved Atom Interferometry: Impact and Mitigation ›
Equivalence of scalar-tensor theories and scale-dependent gravity ›
Impact of reactor antineutrinos on the neutrino floor in low-mass WIMP-like dark matter searches ↓↑