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

Dome at sunrise

Cloud

Rainfall

S Sky
Temperature
8.3 °C
Humidity
78%
Wind
9.7 km/h
Pressure
1018.5 hPa

Moon
Latest preprints on astro-ph:
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Pulsar Detection with Deep Learning ›
Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars ›
The kSZ optical depth degeneracy and future constraints on local primordial non-Gaussianity ›
The Ray Tracing Sampler: Bayesian Sampling of Neural Networks for Everyone ›
Updated dark pixel fraction constraints on reionization's end from the Lyman-series forests of XQR-30 ›
Unveiling Extended Components of 'Little Red Dots' in Rest-Frame Optical ›
Model-Independent Inference of Galaxy Star Formation Histories in the Local Volume ›
Exploring the quasar disc-wind-jet connection with LoTSS and SDSS ›
Demystifying flux eruptions: Magnetic flux transport in magnetically arrested disks ›
Figuring Out Gas & Galaxies In Enzo (FOGGIE) XI: Circumgalactic O VI Emission Traces Clumpy Inflowing Recycled Gas ›
Cosmological Simulations of Weakly Collisional Plasmas with Braginskii Viscosity in Galaxy Clusters ›
Spiral Structure Diversity in Milky Way Analogs from TNG50: The Role of Gas and Disk Dynamics ›
WOCS XCIII: NGC 7789: the Evolution of Li, Stellar Rotation, and Extended Main Sequence Turnoffs ›
New Pipeline for Efficient Analysis of Large Spectroscopic Samples of OB Stars ›
Resolved HII regions in NGC 253: Ionized gas structure and suggestions of a universal density-surface brightness relation ›
25 Years of Groundbreaking Discoveries with Chandra ›
Chemical separation of stellar populations: analytic solutions for chemical evolution models with metallicity-dependent yields ›
A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region ›
Mitigating gain calibration errors from EoR observations with SKA1-Low AA* ›
Atmospheric collapse and re-inflation through impacts for terrestrial planets around M dwarfs ›
On the Universality of the Relation Between Magnetic Fields and Star Formation in Galaxies ›
TRIShUL: Technique for Reconstructing magnetic Interstellar Structure Using starLight polarization ›
NEOForCE: Near-Earth Objects' Forecast of Collisional Events ›
Potential Thermal Profiles of The Third Interstellar Object 3I/ATLAS ›
Lyman-$\alpha$ radiation pressure regulates star formation efficiency ›
A Natural Language Interface for Efficient Data Retrieval in SDSS ›
HS-ANET: Star Spectral Type Enhanced Astrometric Calibration for Hyper Spectral Space Imaging ›
How does ice shell geometry shape ocean dynamics on icy moons? ›
Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations ›
Ram pressure shaping HVC droplets -- FAST HI observations of HVC AC-III and theoretical interpretation ›
Hot Jupiter Origin and Tidal Evolution Constrained by a Broken Age-Frequency Relation ›
Accretion rates of stellar-mass compact objects embedded in AGN discs ›
Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443 ›
Direct Numerical Simulations of Oxygen-Flame-Driven Deflagration-to-Detonation Transition in Type Ia Supernovae ›
Multi-Faceted Emission Properties of PSR J2129+4119 Observed with FAST ›
Rotation Measure Analysis of Shocks and Sloshing Fronts in a Galaxy Cluster Merger Simulation ›
A new particle-based code for Lagrangian stochastic models applied to stellar turbulent convection ›
Stellar Parameters and Evolutionary Pathways of the Subgiant system HIP 72217 ›
A Triple-GEM Time Projection Chamber for Wide Field-of-View Hard X-ray Polarimetry: First Results ›
Theoretical models for the Late Thermal Pulse in post-AGB stars: the case of DY Cen ›
The SOMA MM Survey. I. An Astrochemical Census of Massive Protostars ›
The role of black hole feedback on galaxy star formation and the degeneracy with halo quenching ›
Apsidal Motion in O-Star Binaries: GENEC rotating binary models put to the k2-test ›
Interstellar Comet 3I/ATLAS: Evidence for Galactic Cosmic Ray Processing ›
Weak-Lensing Detection of Intercluster Filaments in Three Nearby Cluster Systems ›
Shock-driven heating in the circumnuclear star-forming regions of NGC 7582: Insights from JWST NIRSpec and MIRI/MRS spectroscopy ›
Tracing the evolution of brightest galaxies and diffuse light in galaxy groups ›
{\sc ampere}: A tool to fit heterogeneous observations consistently ›
oMEGACat. VIII. A Subpopulation Census of {\omega} Centauri ›
Model-independent late-universe measurements of $H_0$ and $\Omega_\mathrm{K}$ with the PAge-improved inverse distance ladder ›
$\Lambda$vCF: Extending $\Lambda$CDM into a Unified Model with Particle Creation ›
The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions ›
XRISM Observations of The Prototypical Cold Front in Abell 3667 ›
Joint Analysis of Optical, Near-Infrared And Mid-Infrared Variability of 4 Quasars at Redshift < 1 ›
Optimizing Long-term Variability of AGN Light Curves. I. A Case Study with ZTF Observations in the EGS Field ›
Neon is an inhibitor of CO hydrogenation in pre-stellar core conditions ›
The dance of dust: Investigating young stellar object dipper variability ›
The rotation speed of the spiral pattern in the Milky Way galaxy ›
In space there will be no need to scream - Limits to the presence of giant planets in the $\zeta^2$ Ret system ›
A summary of instruments proposed for observing pulsating variables from the Mt. Abu Observatory ›
CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA ›
A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter ›
Combined Orbital and Thermal Evolution of Oort Cloud Comets ›
The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field ›
A Star's Death by a Thousand Cuts: The Runaway Periodic Eruptions of AT2023uqm ›
The magnetic fields of the dusty nuclei and molecular outflows of Arp 220 ›
Hybrid Physical-Neural Simulator for Fast Cosmological Hydrodynamics ›
The second data release of the Indian Pulsar Timing Array: Investigating the Effect of Coronal Mass Ejection on PSR J1022+1001 and a Possible Mode Change of PSR J2145-0750 ›
The chemical DNA of the Magellanic Clouds IV. Unveiling extreme element production: the Eu abundance in the Small Magellanic Cloud ›
Tidal disruption events with SPH-EXA: resolving the return of the stream ›
The 2024 July 16 Solar Event: A Challenge To The Coronal Mass Ejection Origin Of Long-Duration Gamma-Ray Flares ›
Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM ›
An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise ›
The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection ›
Stellar Spectroscopy Using Diffraction Grating, CMOS Monochrome Sensor, and Reflecting Telescopes ›
Flinch: A Differentiable Framework for Field-Level Inference of Cosmological parameters from curved sky data ›
Active Dwarf Galaxy Database II: Connections between Host Galaxy Properties and Black Hole Accretion Signatures ›
The Weighing Halos Accurately, Locally, and Efficiently with Supernovae (WHALES) Survey Overview and Initial Data Release ›
Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA ›
Compact Accretion Disks in the Aftermath of Tidal Disruption Events: Parameter Inference from Joint X-ray Spectra and UV/Optical Photometry Fitting ›
The Library of Exoplanet Atmospheric Composition Measurements: Population Level Trends in Exoplanet Composition with ExoComp ›
Boosting the cosmic 21-cm signal with exotic Lyman-$\alpha$ from dark matter ›
Beyond general relativity: gravitational waves in non-minimally coupled theories ›
Ensuring Outcome-Based Curriculum Coherence through Systematic CLO-PLO Alignment and Feedback Loops ›
Beyond GRMHD: A Robust Numerical Scheme for Extended, Non-Ideal General Relativistic Multifluid Simulations ›
KM3-230213A and IceCube Neutrino Events from Metastable Dark Matter of Primordial Black Hole Origin ›
Testing the type-II seesaw mechanism with gravitational waves ›
Generative Artificial Intelligence for Air Shower Simulation ›
Mapping Anisotropies in the Stochastic Gravitational-Wave Background with space detector networks ›
Study of neutrino spin oscillations in a gravitational field with a differential equations method ›
Wavefront Curvature and Transverse Atomic Motion in Time-Resolved Atom Interferometry: Impact and Mitigation ›
Charged Rotating Black Hole and the First Law ›
Supermassive black holes from inflation constrained by dark matter substructure ›
Constraining binary mergers in AGN disks using the non-observation of lensed gravitational waves ›
Resurrecting Gravitational Vector Modes and their Magnetogenesis ›
Timescales of Quasar Accretion Discs from Low to High Black Hole Masses and a Turnover at the High Mass End ›
EELG1002: A Record-Breaking [OIII]+H$\beta$ EW $\sim 3700$\AA~Galaxy at $z \sim 0.8$ -- Analog of Early Galaxies? ›
Radiation-driven dusty outflows from early galaxies ›
The role of equation of state on the spin-up of millisecond pulsars ›
Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model ›
COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of Spectroscopy ›
Probing the cosmic baryon distribution and the impact of AGN feedback with FRBs in CROCODILE simulation ›
Capturing Small-Scale Reionization Physics: A Sub-Grid Model for Photon Sinks with SCRIPT ›
What Determines the Brightness of the Magnetically Open Solar Corona?: Insights from Three-dimensional Radiative Magnetohydrodynamic Simulations and Observations ›
Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch ›
A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy ›
Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals ›
Planetary Obliquity Excitation Through Pre-Main Sequence Stellar Evolution ›
A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array ›
Application of interpretable data-driven methods for the reconstruction of supernova neutrino energy spectra following fast neutrino flavor conversions ›
Beyond monoculture: Polydisperse moment methods for sub-stellar atmosphere cloud microphysics II. A three-moment gamma distribution formulation for GCM applications ›
Cosmological Preference for a Positive Neutrino Mass at 2.7$\sigma$: A Joint Analysis of DESI DR2, DESY5, and DESY1 Data ›
SN 2024gy: Multi-epoch Spectroscopic Features Suggestive of Delayed Detonation in a Type Ia Supernova ›
The role of migration traps in the formation of binary black holes in AGN disks ›
In-Situ Formation of the Cold Classical Kuiper Belt ›
Numerical simulations of oscillations for axisymmetric solar backgrounds with differential rotation and gravity ›
SDSS-V LVM: Detectability of Wolf-Rayet stars and their He II ionizing flux in low-metallicity environments I. The weak-lined, early-type WN3 stars in the SMC ›
AGN-heated dust revealed in "Little Red Dots" ›
Acceleration of Heavy Ions at Non-Relativistic Collisionless Shocks ›
Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function ›
Exploring the Early Universe with Deep Learning ›
Understanding the Origins of Super-Puff Planets: A New Mass-Loss Regime Coupled to Planetary Evolution ›
SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations ›
Magrathea v2: A planetary interior modeling platform in C++ ›
Probing the Physical and Chemical Characteristics of an Extremely Early Class 0 Protostar in G204.4-11.3A2-NE ›
Evolution of accretion disc-corona in the TDE Candidate AT 2019avd ›
Filamentary accretion flows in high-mass star-forming clouds ›
Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals ›
AnomalyMatch: Discovering Rare Objects of Interest with Semi-supervised and Active Learning ›
Constraints to Lorentz violation and ultrahigh-energy electrons in D-foamy space-times ›
Constraining the Deviation of Kerr Metric via Bumpy Parameterization and Particle Swarm Optimization in Extreme Mass-Ratio Inspirals ›
Spinning black holes in astrophysical environments ›
Multi-scale optimal control for Einstein Telescope active seismic isolation ›
Numerical computation of electromagnetically sourced nonlinear tails ›
Precision gravity constraints on large dark sectors ›
Observable spins in gravitational waves from compact binary mergers ›
Illuminating the lantern: coherent, spectro-polarimetric characterisation of a multimode converter ↓↑