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

Before observations ...

Cloud

Rainfall

S Sky
Temperature
-3.3 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1007.6 hPa

Moon
Latest preprints on astro-ph:
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Ultramassive Black Holes and the Three $M$-$\sigma$ Relations ›
CMB Spectral Distortions from Resonant Conversions in Atomic Dark Sectors ›
Modeling Globular Cluster Stellar Streams with a Basis-Expansion N-body Code ›
Dyad: a binary-star dynamics and statistics library for Python ›
Characterizing Lyman alpha emission from high-redshift galaxies ›
Constraining Binary Neutron Star Populations using Short Gamma-Ray Burst Observations ›
ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium ›
ARCHITECTS II: Impact of subgrid physics on the observable properties of the circumgalactic medium ›
MeerKAT discovery of a high-redshift strongly-lensed hydroxyl gigamaser ›
Revising the Milky Way Cepheid Calibration: Quantifying and Correcting for Previously Undetected Distance Modulus Errors in the Gaia-based Multi-Wavelength Period-Luminosity Relations ›
The Interplanetary Habitable Zone ›
LHAASO observation of Mrk 421 during 2021 March - 2024 March: a comprehensive VHE catalog of multi-timescale outbursts and its time average behavior ›
Updated Sensitivities of the Five STIS L-mode Gratings ›
The Signature of Strong High-Redshift Radio Backgrounds on the Cosmic Dawn 21-cm Bispectrum ›
Dust Morphology Under Changing Dust Mass Ratios in Protoplanetary Discs ›
Surveying the Giant HII Regions of the Milky Way with SOFIA: VIII. W43 Main ›
Searching for Neutron Star Mergers in the Absence of Gravitational Waves with Optical Afterglow Emission ›
Superorbital Phase Evolution and a Soft-Hard X-ray Phase Shift in LMC X-4 ›
The Cosmological Parameters (2025) ›
New Dynamical Measurements from a Lensed Quasar Sample: Joint Analysis Constrains the Mass Profile Evolution of Lens Galaxies ›
Modelling the non-equilibrium chemistry of the Milky Way's cold nuclear wind ›
Unprecedented Multipoint Observation of Spatially Varying ICME Turbulence of Different Ages during October 2024 Extreme Solar Storm at 1 AU ›
Solar active region scaling laws revisited ›
AT 2025abao: the fourth luminous red nova in M 31 ›
Modelling the Break in the Specific Angular Momentum within the Envelope-Disk Transition Zone ›
Pulsars and Millisecond Pulsars III: Tracing Compact Object Dynamics in Globular Clusters with NBODY6++GPU ›
Detection of Cyclotron Absorption in the Radio Emission of GPM 1839-10 ›
Dust and Ices in the SNR ›
Dynamical Preconditions for Ice Formation in Supernova Remnant and Cloud Interactions: A 2D MHD Study ›
Estimatingthe Contribution of Galactic Neutrino Sources ›
Habitable Zones Around Massive Stars: From the Main Sequence to Supergiants ›
J-PAS: Semi-Supervised Sim-to-Obs Transfer for Robust Star--Galaxy--Quasar Classification ›
The James Webb Space Telescope Absolute Flux Calibration. V. Near-Infrared Camera Wide Field ›
Three-dimensional kink modes in solar coronal slabs: group velocities and their implications for impulsively excited waves ›
Nonlinearity in H4RG-10 Near-Infrared Detectors at Elevated Temperatures: Characterization and Data-Driven Correction Method ›
Dense Molecular Clumps with Large Blue Asymmetries: Evidence for Collapse ›
Superhumps and their Relation to the Disk Instability Model ›
Optimal polarization modulation and calibration schemes ›
Image instabilities and polarization cross-talk ›
Pulsar Timing Array in the past decade ›
Constraining Lorentz Violation using 21cm and CMB Cross Correlations ›
VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova ›
S-PLUS: Beyond Spectroscopy IV. Stellar Parameters and Elemental-abundance Ratios for Six Million Stars from DR4 and First Results for the Magellanic Clouds ›
Effective Magnetic Susceptibility of Dust Grains with Superparamagnetic Inclusions and Implications ›
Kinematic Evidence for Open Cluster Origins of Galactic Binary Neutron Stars ›
High Energy Emission from the Galactic Center ›
In-orbit Demonstration of X-ray Pulsar Navigation with NinjaSat ›
LIGHTS. The Thin Encircling Stellar Stream of NGC 3938 ›
Diversities and similarities exhibited by multi-planetary systems and their architectures: II. Radii of singles and multis ›
Nonlinear diffusive shock acceleration with upstream escape reproduces DAMPE observations ›
Tracing Fe K X-ray reverberation lag in the energy-resolved spectra of Narrow-line Seyfert 1 galaxy Ton S180 ›
PeV neutrons as origin of separated SS433 TeV signals ›
Pre-perihelion Volatile Evolution of Interstellar Comet 3I/ATLAS Indicating Significant Contribution from Extended Source in the Coma ›
I-Band Asymptotic Giant Branch (IAGB) Stars: I. Exploring a New Standard Candle for the Extragalactic Distance Scale ›
Gaia FGK Benchmark Stars: Selecting Infrared Lines for Abundance Determination ›
Production of Jets before Neutron Star Mergers ›
I-Band Asymptotic Giant Branch (IAGB) Stars: II. A First Estimate of their Precision and a Differential Zero Point ›
Gravitational waves from supercooled phase transitions and pulsar timing array signals ›
Formation and Survival of Complex Organic Molecules in the Jovian Circumplanetary Disk ›
Predicting New Concept-Object Associations in Astronomy by Mining the Literature ›
Atmospheric constraints on GJ 1214 b from CRIRES+ and prospects for characterisation with ANDES ›
Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations ›
Quintessence with tachyonic resonance and late-time cosmic-microwave-background and gravitational-wave signals ›
The Physical Properties of PS1-12sk and the Implications to Its Progenitor System ›
Circular orbits and observational features of the rotating Simpson-Visser black hole surrounded by a thin accretion disk ›
Back to Normal Again: Possible Destinies of JWST overmassive SMBHs and "Little Red Dots" in the View of Shin-Uchuu Simulation ›
Zel'dovich smearing approximation of the BAO feature for model-agnostic cosmological inference ›
Multiscale feature integration network for inpainting of full-sky CMB $B$-modes ›
Human versus Artificial Intelligence; various significant examples in astrophysics ›
Seismic detection of core magnetic fields in red giants using the gravity offset ›
Infrared spectra of methane-containing ice mixtures for JWST data analysis ›
Large-scale and local environmental drivers of quenching: tracing H$\alpha$ concentration in X-ray and optical galaxy groups ›
Bayesian Cosmic Void Finding with Graph Flows ›
H.E.S.S. detection of the PSR J0855-4644 nebula ›
4U 1556-60 as a very faint neutron star X-ray binary at 700 pc with an undetected radio jet ›
Bounds on Lorentz invariance violation from muon fluctuations at the Pierre Auger Observatory ›
Exploring Non-minimal coupling using ultra-diffuse galaxies ›
Pulsar based modeling of point spread function of Fermi Large Area Telescope ›
Infrared period-luminosity relations of Galactic Miras based on multi-epoch photometry and the Gaia parallax uncertainty ›
Evidence for the merger hypothesis in V4332 Sgr: a low $^{12}$C/$^{13}$C ratio and multiple outbursts ›
Carbon chain diversity in L1544 and IRAS 16293-2422: an astrochemical pathfinder study for the SKAO ›
The Habitable Worlds Observatory in Historical Context ›
The impact of the formation channel on gravitational-wave-galaxy cross-correlations ›
A universal critical accretion rate for black hole jet formation ›
Statistical Validation and Vetting of Exoplanet Candidate TOI 7475.01 ›
Reduction of bar fraction in paired galaxies in the SDSS ›
Exploring the magnetic field of the ultraluminous X-ray pulsar NGC 4631 X-8 ›
Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at $z=1.5$ ›
Recalibrating the Sensitivities of the STIS First-Order, Medium-Resolution Modes ›
First detection of the TiO i1Pi-a1Delta system in stellar spectra and its laboratory characterization ›
Microphysical Model of Jupiter's Great Red Spot Upper Chromophore Haze ›
[C/N] Ages and Extra-Mixing for [Fe/H] ›
Multi-frequency mapping of the S255IR region at a wavelength of 1~mm ›
Improved frequency hierarchy treatment for anisotropic spectral distortions ›
The radial velocity curve for HeII emission cannot be used for component mass determination in SS433 ›
Geodetically Anchored 0.30m Digital Elevation Model of the Chandrayaan-3 Vikram Landing Site from Chandrayaan-2 Orbital High Resolution Camera (OHRC) Stereo Imagery ›
Generalization from Low- to Moderate-Resolution Spectra with Neural Networks for Stellar Parameter Estimation: A Case Study with DESI ›
Gravitational Wave Echoes of the First Order Phase Transition in a Kination-Induced Big Bang ›
Modeling isolated magnetar spin-down evolution and implications for long-period radio transients ›
Prospects of Indirect Detection of Dark Matter via Primordial Black Hole Induced Gravitational Waves ›
Evolution of Linear Perturbations under Time-Dependent Hubble Friction I: SR-USR-SR Inflation ›
Agent Mars: Multi-Agent Simulation for Multi-Planetary Life Exploration and Settlement ›
Holographic Dark Matter ›
Leveling of MHD turbulence imbalance in shear flows ›
Description of 4 Spacecraft, Moving on Elliptic Kepler Orbits ›
Harmonic Analysis on Correlation for Gravitational-Wave Backgrounds of Arbitrary Polarization from Interfering Sources in Generic Dispersion Relation ›
MarsRetrieval: Benchmarking Vision-Language Models for Planetary-Scale Geospatial Retrieval on Mars ›
Polarization fringes in optical systems: a compendium ›
Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective ›
On the Cuspy Structure of Rotating Wormhole Shadows ›
The initial states of high frequency gravitons ›
Measuring neutrino mixing above 1 TeV with astrophysical neutrinos ›
Local Short-Time Acceleration and deSitter Spacetime induced Extra Spectral Broadening: a Simple Interpretation of Modified Inertial in MOND ›
Accelerating Posterior Inference from Pulsar Light Curves via Learned Latent Representations and Local Simulator-Guided Optimization ›
Investigating the impact of quasi-universal relations on neutron star constraints in third-generation detectors ›
Excavation of a 69-m diameter and 94-m high cavern for the Hyper-Kamiokande detector ›
Gauge-independent gravitational waves from a minimal dark $U(1)$ sector with viable dark matter candidates ›
Dynamics of powerful radio galaxies ›
Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A ›
Detecting prompt and afterglow jet emission of gravitational wave events from LIGO/Virgo/KAGRA and next generation detectors ›
A reassessment of LVE method and hemispherical power asymmetry in CMB temperature data from Planck PR4 ›
Cool-Core Destruction in Merging Clusters with AGN Feedback and Radiative Cooling ›
GA-NIFS: interstellar medium properties and tidal interactions in the evolved massive merging system B14-65666 at z=7.152 ›
Galaxy mergers classification using CNNs trained on S\'ersic models, residuals and raw images ›
Compression fronts from fast radio bursts ›
Periodicities in radio emissions from the Jupiter's magnetosphere and consequences for radio emissions from star-exoplanet systems ›
Free Cosmic Density Bispectrum on Small Scales ›
Comparative biosignatures with systemic retrievals ›
Gamma-Ray Millisecond Pulsars: Off-pulse Emission Characteristics, Phase-Resolved Pseudo-Luminosity--Cutoff Energy Correlation, and High-energy Pulsed Emission ›
Superfluid Dark Matter ›
Modeling YSO Jets in 3D II: Accretion-Fed, Star-Anchored Poynting Jets in the Low-Density Polar Cavity Powered by Disk-Magnetosphere Interaction ›
MUSE-DARK-I: Dark matter halo properties of intermediate-z star-forming galaxies ›
The spin-orbit alignment hypothesis in millisecond pulsars ›
Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx ›
A normalizing flow approach for the inference of star cluster properties from unresolved broadband photometry I: Comparison to spectral energy distribution fitting ›
Impact of thermal effects on prompt-collapse binary neutron star mergers ›
New Insight from the James Webb Space Telescope on Variable Active Galactic Nuclei ›
Hypothesis of a bi-isotropic-like plasma permeating the interstellar space ›
Addressing Dipole Tension via Clustering in $\Lambda$CDM and beyond ›
Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation ›
Exploring the spatially-resolved capabilities of the J-PAS survey with Py2DJPAS ›
Two unseen massive white dwarf candidates in close binaries ›
Star-forming galaxies in the cosmic web in the last 11 Gyr ›
SymBoltz.jl: A symbolic-numeric, approximation-free, and differentiable linear Einstein-Boltzmann solver ›
CCAT: Magnetic Sensitivity Measurements of Kinetic Inductance Detectors ›
Spectral Properties of Anomalous Microwave Emission in 144 Galactic Clouds ›
DIPLODOCUS II: Implementation of transport equations and test cases relevant to micro-scale physics of jetted astrophysical sources ›
Astrophysical uncertainties challenge 21-cm forecasts: A primordial black hole case study ›
Evidence for cloud-to-cloud variations in the ratio of polarized thermal dust emission to starlight polarization ›
Detailed Abundance Determination of Metal-Poor Stars with X-Shooter I. Unusual Chemistry in Halo Stars ›
Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations ›
Mock Observations for the CSST Mission: Integral Field Spectrograph--GEHONG: A Package for Generating Ideal Datacubes ›
Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem ›
Ginnungagap -- a massively parallel cosmological initial conditions generator ›
Indirect forces in disc-planet interaction ›
JADES: Low Surface Brightness Galaxies at 0.4 < z < 0.8 in GOODS-S ›
Beyond the Simple Power Law: A Bayesian Analysis of 897 Pulsar Spectra ›
Multi-Resonant-Line Radiative Transfer: Lyman-Alpha Fine Structure and Deuterium Coupling ›
The DESI DR1 peculiar velocity survey: growth rate measurements from the galaxy power spectrum ›
Probing AGN Feedback in Dwarf Galaxies with Spatially Resolved NIR Coronal Lines from JWST ›
Frequency- and phase-resolved polarimetry of millisecond pulsars and its application to timing ›
Globular Clusters GMRT Pulsar Search (GCGPS) II: Discovery of five MSPs in M69 and M70 ›
Mode Energy Partition in Partially Ionized Compressible MHD Turbulence ›
Graph Neural Networks for Interferometer Simulations ›
Quantifying sunspot group nesting with density-based unsupervised clustering ›
Asymptotic behaviour of galactic small-scale dynamos at modest magnetic Prandtl number ›
Cygnus~X-3 as a PeVatron and the LHAASO 2025 data ›
A Linearized Approach to Radial-Velocity Extraction. II: Shot-Noise-Limited Precision via Spectral Factorization ›
Probabilistic modeling of Cherenkov emission from particle showers ›
Dense gas linked to star-forming regions photoionised by embedded gamma-ray bursts ›
Revisiting the Great Attractor: The Local Group's streamline trajectory, cosmic velocity and dynamical fate ›
The miniJPAS survey: Dissecting galaxy properties across environments with spatially resolved photometry ›
Data Mining-Based Cislunar Escape-Family Analysis in The Multi-Body Models ›
Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics ›
Constraining Black Hole Parameters from Shadow and Inner-Shadow Morphology Considering Effects from Thick Disk Accretion Flows ›
Densities of small planets around the M dwarfs TOI-4336 A and TOI-4342 with ESPRESSO: Three sub-Neptunes, one super-Earth, and a Neptune-mass candidate ›
Two late-T dwarfs at kiloparsec distances revealed by JWST UNCOVER survey ›
The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure ›
Imaging Venus-like Worlds: Spectral, Polarimetric, and UV Diagnostics for the Habitable Worlds Observatory ›
The local void model for the Hubble and BAO tensions ›
Searching for dark matter signals with high energy astrophysical neutrinos in IceCube ›
NovaMoon: A Strategic Lunar Reference Station for Positioning, Timing, and Largely Enhanced Science in the Earth-Moon System ›
Statistical isotropy of the universe and the look-elsewhere effect ›
Velocities of Free Floaters in a Sea of Stars ›
Direct pathway to the Early Supermassive Black Holes: A Red Super-Eddington Quasar in a Massive Starburst Host at $z=7.2$ ›
Cosmological Simulation with Population III Stellar Feedback and Metal Enrichment I: Model Description And Convergence Test ›
Upper limit on HF(1-0) absorption in a dusty star-forming galaxy at $z = 6$: Constraints on early fluorine enrichment ›
STEP survey: III. STEPping stones between the clouds: the star formation history of the Magellanic Bridge ›
Fate of false vacuum in non-perturbative regimes: Gravity effects ›
Hydrodynamics of Relativistic Superheated Bubbles ›
Gravitational Waves from Phase Transitions ›
Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study ›
About electroweak domain walls in Majoron models ›
Maximal parameter space of sterile neutrino dark matter with lepton asymmetries ›
Affleck-Dine Leptoflavorgenesis ›
A relativistic treatment of accretion disk torques on extreme mass-ratio inspirals around non-spinning black holes ›
Resonant Loop Interferometers for High-Frequency Gravitational Waves ›
Tracing Inflationary Imprints Through the Dark Ages: Implications for Early Stars and Galaxies Formation ›
Kinematic Anisotropies in PTA Observations: Analytical Toolkit ›
The measurable impact of the 2pN spin-dependent accelerations on the jet precession of M87$^\ast$ ↓↑