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

Big Dipper over the dome

Cloud

Rainfall

S Sky
Temperature
14.6 °C
Humidity
57%
Wind
11.3 km/h
Pressure
1026.2 hPa

Moon
Latest preprints on astro-ph:
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The Preprint Evolution: The Rise of Unreviewed Drafts on arXiv and its Implications for Astronomy ›
Reconstructing Implicit Scientific Knowledge: Evaluating LLM Agents through End-to-End Reproduction of Astronomy ›
Photoelectron and electron microscopy investigation of laboratory grown Mg-silicate space dust analogues ›
Massive Population III Galaxies Near a GN-z11 Analog: The Role of the Baryon-Dark Matter Streaming Velocity ›
GA-NIFS view of LAP1: Assembly of Pop~III stellar clusters during EoR ›
Discovery of the Infrared Counterpart of the Rapid Burster with JWST ›
LIMFAST. V. Probing Reionization with the Synergy Between 21 cm and Photometric Galaxy Surveys ›
Discovery of over a thousand variable stars in Terzan 5 and Liller 1 with JWST ›
Current and Future Constraints on the Primordial Power Spectrum ›
SIFARI: Self-Supervised Interferometric Fitting for Astronomical Radio Imaging ›
GameDev: GPU-accelerated model for dust evolution ›
The 1.6 $\mu\mathrm{m}$ $\rm{H^{-}}$ bump as a diagnostic of TP-AGB contributions and recent quenching. I. Insights from stellar population models ›
JWST lensed quasar dark matter survey V: Hints of self-interacting dark matter from 29 quadruply imaged quasars ›
Toddlers in Resonance I: low masses and eccentricities of the 17 Myr giant planets HIP 67522 bc from transit timing variations ›
The long period radio transient ASKAP J1448-68 is a cataclysmic variable ›
Improved Modeling for Moving Sources of Radio Frequency Interference and Impact on Flagging Strategies ›
COSMOS-3D: Diverse Environments and Hot-dust Signatures among Dusty Star-forming Galaxies at $z$ = 4.9-7.2 ›
Satellite stellar-to-halo mass relations in primordial black hole universes ›
Divergence-free magnetohydrodynamics on a moving mesh ›
Enhanced density fluctuations: consequences for stellar dynamics and dark matter substructure ›
CHAMPS: The COSMOS High-Redshift ALMA-MIRI Population Survey - A New Census of the Dusty Early Universe ›
Hierarchical Bayesian Inference on the intrinsic event rate of Type I gamma-ray bursts from the {\it Fermi}/GBM catalogue ›
Bayesian Evidence for Inspiraling Hotspot Motion in the Galactic Center ›
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 ›
An Off-Nuclear Tidal Disruption Event Discovered At Late Times: The Case Of TDE 2023mfm ›
Beyond what's observed: hierarchical inference of Gaia astrometric compact-object binaries ›
Cosmological-perturbation equations from the total-angular-momentum formalism ›
Connecting the Dots: Prospects for Detecting Multi-Source Inflation through Scale-Dependent and Stochastic Bias of Little Red Dots ›
MOCSS: Multi-Object Coronagraphy for JWST/NIRSpec Slitless Spectroscopy ›
Snapshots of r-process production in the Milky Way disk ›
The Dense, Rocky Core of Haumea Revealed by Satellite Dynamics ›
First Detection of the Doppler Shift of X-ray Photons Due to a Telescope's Orbital Motion ›
CHAMPS: Data Reduction and Detection of ~3300 Dusty Galaxies at 1.2 mm ›
Constraining Reionization with Persistent Homology: a Novel Summary Statistic for Wide-Field Lyman-$\alpha$ Emitter Observations ›
Comparing Active Anomaly Detection Frameworks: From Light Curves to Images ›
Binary tidal evolution as a sculptor of circumbinary planet architectures ›
Fast Radio Bursts from Induced Upscattering. I. Magnetar Polar Fireballs ›
MEGATRON: The Physical Origins of Steep UV Slopes at High Redshift ›
PHAROS: Panchromatic spectral energy distributions of solar-like stars across evolutionary stages ›
What We Have Learned from NICER About Neutron Star Radii ›
Cool, Cloudy Nights on an Ultrahot Neptune: A Panchromatic NIRISS/NIRSpec Transmission Spectrum of LTT 9779 b ›
Assessing the detectability and identification of pulsar halos with H.E.S.S. and CTAO ›
How well do integral-of-motion distribution functions describe Milky Way-analogue halos? ›
Whole-disk Photometric and Colorimetric Phase Curves of Earth with the Clementine Lunar Orbiter ›
JWST/MIRI Spectroscopy of the Quiescent Black Hole X-ray Binary XTE J1118+480: Constraints on Jet and Circumbinary Dust Contributions to the Mid-infrared Emission ›
Probing Baryons with the Kinematic Sunyae Zel'dovich Effect and Machine Learning Derived Peculiar Velocities using DESI DR2 and ACT DR6 ›
Properties of Circumfacular Regions derived from H$\alpha$ and Ca II K synoptic observations of the Sun ›
Everything Everywhere All At Once: A Hierarchical Framework for Mapping Anisotropies in the Local Universe ›
ECLIPSE-X: Plate-Scale Calibration as the Binding Constraint on Relativistic Astrometry with Spacecraft Navigation ›
Combined constraints on the diffuse flux of cosmic neutrinos between 10^16 eV and 10^26 eV ›
An Ionized Superstructure at Cosmic Dawn Revealed by a Foundation Model for Astrophysical Research ›
A Bayesian Inference Framework for Binary Lens Events Fully Incorporating Higher-Order Effects ›
High-CO2 Climates and Observables in the Outer Habitable Zone ›
Population search for dark matter spikes in megamaser rotation curves ›
Broadband reverberation mapping of quasars at cosmic noon ›
Testing KMTNet--PRIME Optical--Near-Infrared Source-Color Constraints in KMT-2024-BLG-0211 and KMT-2024-BLG-1522 ›
Dynamical friction vs. subhalo heating in Cold Dark Matter haloes ›
Morphological Identification of Dynamical Regimes in MHD Turbulence with ScaleAware-JEPA ›
LUMA: A CNN for Strong Gravitational Lens Searches in Astronomical Imaging ›
Cross-correlating Squared kSZ and HI Intensity Fields: A Map-level ACT--MeerKAT Forecast ›
Weak Lensing Measurements from the Lyman-$\alpha$ Forest ›
LISA Double White Dwarfs in Triple Systems ›
Detecting Extragalactic Exoplanets With Fast Radio Burst Nanolensing ›
Re-interpreting the GRS 1915+105 observations within the variable TADAF scenario ›
First laboratory demonstration of iEFC for high-contrast imaging at small angular separation on ELT scales ›
Astrometric Evidence for Outer Giant Planets in Known Exoplanet Systems ›
Chondrule size averaging in two and three dimensions ›
On the frequency-dependent time lags of the intermediate polar V709 Cas ›
MEGATRON: Dwarf Galaxy Quenching in the Epoch of Reionization ›
Multi-wavelength polarization degree dependence of Mrk 421 for different particle energy distributions ›
A halo-based intrinsic-alignment model for simulation-based inference ›
Homogeneous Nucleation of Water Vapor Evidenced by Elongated Clouds on Mars ›
On the origin of carbon- and oxygen-rich hot subdwarfs: an sdB merger scenario ›
The ALPINE-CRISTAL-JWST Survey: Investigating the role of interstellar dust, gas and stars in high-z galaxies at kpc-scales ›
Search for dark matter annihilation in the Sun using the full ANTARES dataset ›
Caught in the act: diffuse stellar and Ly$\alpha$ emission around a halo-less quasar in the assembling cluster CARLA J0800+4029 at z=2 ›
The Occurrence Rate of Planets Around Subgiant Stars from TESS Photometric Survey ›
Carving out the Multifield Cosmological Collider Landscape ›
TOI-6981 b: a transiting sub-Neptune at the water ice line ›
Fooled by mass? Recovering the $\Gamma-\lambda_{Edd}$ relation of quasars from their X-ray variability ›
Abundance analysis of three new extremely metal-poor stars, including one CEMP-s star ›
GA-NIFS: sRMS, a new method for disentangling resolved and unresolved emission in integral field spectroscopy. Application to distant quasars ›
X-ray measurements of the elemental abundances for the diffuse emission in the nuclear starburst galaxy NGC 3079 ›
Thermally irreversible sulfur chemisorption on silicate grains as a major sulfur reservoir in molecular clouds ›
Common Envelope Evolution: Too stochastic to be deterministic ›
Fast and furious -- High-velocity features of Ca and Si in the spectra of Type Ia supernovae ›
Detecting atmospheres in the presence of stellar contamination: an empirically calibrated framework applied to four JWST/NIRSpec PRISM transits of TRAPPIST-1c ›
On-sky commissioning and technical performance of Proto-NUX at Pic du Midi ›
Shaping binary black hole merger efficiency with gravitational wave observations ›
Near-infrared periodicity in the SPICY catalog. True young stellar objects versus contaminants ›
ALMA - CTAO synergies ›
Solar spicule population properties inferred from IRIS Mg II k off-limb spectra using likelihood-free Bayesian inference ›
An End-to-End Numerical Framework for Tidal Disruption Events with AthenaK ›
A Full-Sky SPHEREx Map of Integrated 3.3 and 3.4 {\mu}m PAH Emission ›
Detection of fine-structured radio bursts during a superflare on EQ Peg ›
Joint Mass-Radius and Magnetic-Geometry Inference of PSR J0740+6620 ›
Torsionally excited methanol in massive young stellar objects: The role of the mid-IR radiation field ›
Constraining exoplanet population parameters with Kepler and simulation-based inference ›
Improved Constraints on the Surface of LHS 3844 b from its Mid-Infrared Spectrum ›
Radiation Hydrodynamics of Self-gravitating Protoplanetary Disks II. Accretion, Migration, Spin, and Internal Structure of GI Fragments ›
Science Using Single-Pulse Exploration with Combined Telescopes: II. Pulse profile evolution and single-pulse modulation ›
Detecting HI Self-Absorption using Neural Networks ›
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 ›
Very High-Energy GRB Afterglow Fits with Neural-Network Emulation and Bayesian inference ›
Gravitational-wave dark sirens as astrophysical probes: inferring galaxy-merger relations and identifying individual hosts ›
Atmospheric dynamics and variability of periodically irradiated tidally locked planets ›
LYRA: The formation and growth of nuclear star clusters in dwarf galaxies ›
Low Frequency Gravitational Wave Detection with Gravito-Magnetism ›
Constraining dark matter using 20-year INTEGRAL/IBIS observations II: Sub-GeV dark matter ›
Black Hole Quasinormal Mode Resonances and Reconnections in Coupled Systems ›
Stochastic gravitational-wave background from subsolar neutron stars in collapsar disks ›
LMC-Perturbed LZ Dark Matter Landscape ›
What Fraction of Extreme Mass Ratio Inspirals That Merge After the LISA Mission Ends Are Detectable? ›
Computing gravitational radiation from highly eccentric bound binaries in the small-mass-ratio limit ›
An Energy-Conserving Unstaggered Electromagnetic-Potential Particle-in-Cell Method, Part II: Fully Relativistic Formulation with an Adapted Higuera--Cary Pusher ›
Does the High-Energy LUX--ZEPLIN Event Suggest Hyperfine Atomic Dark Matter? ›
The Irreversible Depletion of Dark Matter Spikes by Extreme-Mass-Ratio Inspirals ›
Gravitational-Wave Inference For Noise PSD Jumps Across Data Gaps ›
The alternative scalar field dark sector of the Universe: Cosmological inflation, quintessence and ekpyrotic model in the framework of scalar-tensor cosmology ›
Scaling RIFT 1: Extending RIFT to third-generation gravitational-wave analyses ›
An autonomous approach to model daytime behavior of sub-ionospheric VLF signals over short and medium propagation paths in India ›
Effects of Alfv\'enicity on the Compressible Energy Cascade in Magnetohydrodynamic Solar Wind Turbulence: Evidence from Parker Solar Probe, Solar Orbiter, and WIND observations ›
Bayesian Constraints on Bosonic Dark Matter in Neutron Stars within a Covariant Density-Functional Equation-of-State Ensemble ›
Fast and Flow-rious: Gravitational Wave Background Bayesian Model Comparison using Normalizing Flows and Nested Sampling ›
CMB Injection Bounds on Moduli Fields ›
Exact bispectra in strongly mixed multifield inflation ›
Superfluidity in the Interiors of Neutron Stars ›
LMC-induced Perturbations in the Milky Way Halo:I. HaloDance Simulation Suite and Observational Forecasts ›
MEGATRON: Reproducing the Diversity of High-Redshift Galaxy Spectra with Cosmological Radiation Hydrodynamics Simulations ›
Complex dynamical regimes of the Tayler-Spruit dynamo ›
Euclid preparation. Testing analytic models of galaxy intrinsic alignments in the Euclid Flagship simulation ›
The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs ›
Seasonal Variation of Polar Ice: Implications for Ultrahigh Energy Neutrino Detectors ›
A Comparative Study of the Streaming Instability: Unstratified Models with Marginally Coupled Grains ›
Hydrodynamic escape from the proto-lunar disk and the origin of the Earth-Moon volatile dichotomy ›
A modern halo streaming model for redshift space distortions ›
A spatial filter for mitigating radio interference and its application to CHIME/FRB Outriggers ›
Gravitational Waves from Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA, and LISA ›
Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries ›
The Radio-FIR Correlation in the Context of Deep Radio Source Counts ›
Temporal Invariance Is an Illusion: Time-Dependent Influences of the Galactic Magnetic Field on UHECR Observations ›
The Effects of Cosmic Ray Protons on Galactic Nonthermal Filaments ›
SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics ›
The Chirp-Mass Ladder: A New Rung Emerges ›
Resolved Ages and Stellar Metallicities in Progenitors of Milky Way Analogs: A Closer Look at their Star Formation Histories since $z=5$ ›
SN 2023rve: A Type II Supernova with No Nebular Oxygen ›
On-Orbit Calibration of Danuri/PolCam. II. Image Artifact Correction ›
LMC-induced Perturbations in the Milky Way Halo II: Bridging Field-level Inference and Summary-level Simulation-Based Inference ›
Constraining the $z \approx 1$ neutral hydrogen (HI) distribution ›
HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager ›
How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition ›
Constraining spinning primordial black holes with interstellar dust heating ›
Generating the wide sequence of Diffuse Galaxies with de Broglie waves of Dark Matter ›
The interplay between active galactic nucleus photoionization, radio jet, and star formation in the z $\sim$ 3.5 radio galaxy 4C +03.24 ›
Comparative spectro-temporal study between 1A 1246$-$588 and 4U 0614$+$091 using AstroSat ›
Pulsed Accretion onto Eccentric Binaries in Highly Misaligned Circumbinary Disks ›
The July 2023 Outburst of Comet 12P/Pons-Brooks: Observations and Modeling of Dust Coma and Arc Structure ›
Discovery of a 62-min long-period transient with near-orthogonal rotator geometry ›
Planetesimal formation facilitated by streaming instability in weak pressure bumps ›
Refactoring the SIXTE simulator: Towards a more modular code base ›
Fast radio burst - persistent radio source systems III. The relation between PRS luminosity and FRB rotation measure ›
From Stars to Waves: Stochastic Inference of Microlensed Gravitational Waves ›
Sommerfeld enhancement from unstable final-state particles in dark matter annihilation ›
The Depletion of Collisionless Dark Matter Spikes ›
Kaon Portal to Freeze-in Dark Matter ›
Hybrid Expansion Cosmology in f(T) Gravity: Late-Time Evolution and Observational Bounds ›
Probabilistic Causality from Graviton Fluctuations ›
A Common Antimatter Response in AMS-02 Positrons and Antiprotons ›
Primordial black hole formation in bulk-viscous cosmology ›
Multiple-Mediator-Affected Ultra-High-Energy Neutrino Attenuation: Hints for 5D ${U(1)}_{L_\mu - L_\tau}$ in IceCube ›
A Systematic Study of Resonance-Driven Flux Modifications in Extreme-Mass-Ratio Inspirals ↓↑