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

Sunset view from dome

Cloud

Rainfall

S Sky
Temperature
6.6 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1019.5 hPa

Moon
Latest preprints on astro-ph:
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Finite temperature effects on g-modes of inviscid neutron stars ›
Sensitivities of Black Hole Images from GRMHD Simulations ›
JWST Observations of Starbursts: Dust Processing in the M82 Superwind ›
An XMM-Newton Analysis of the Supermassive Black Hole Binary Candidate MCG+11--11--032 ›
Spectral index evolution of the limb-brightened jet in 3C 84 ›
A Deep ALMA Survey of the Redshift Distribution of Dusty Star-forming Galaxies ›
A sample of short-lived Galactic radio transients from ASKAP VAST ›
SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations ›
Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy ›
Distinct First-to-Second Peak Yield Ratios and Timescales Reveal a Sub-dominant Prompt Channel ›
Consistency of the dark matter halo perturbation parameter from morphological and kinematic lopsidedness of galaxies ›
The Shocking Origin of the Flat $EE/BB$ Ratio ›
A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06 ›
Beyond the Diffusion Coefficient: Propagators and Memory in Cosmic Ray Transport ›
Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0 ›
Hybrid Simulations of Supersonic Shear Flows: II) Cosmic Ray Viscosity ›
JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI ›
Introducing $\Delta V_{\star-g}$: a new universal kinematic disturbance parameter ›
Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars ›
A Forward, Analytic, Differentiable, Geometric (But Inflexible) Lens Model ›
An Atmosphere on the Ultra-Short Period super-Earth HD 3167 b ›
Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends ›
How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs ›
The role of small-scale environments in the quenching of massive galaxies at $1 ›
No Country for Old Stars -Spectroscopic confirmation of the first intermediate-age RR Lyrae in the open cluster Trumpler 5 ›
Reconstructing chemical enrichment pathways in disc galaxies: A phylogenetic approach ›
Relativistic Effects on Circumbinary Orbit Stability ›
OB runaway stars originating in the Vel OB1 association ›
Effective field theory of a single scalar pion field for large scale structure in the Universe ›
Beyond the Standard Model of Cosmology: Testing new paradigms with a Multiprobe Exploration of the Dark Universe ›
Constraints on Coupled Dark Energy in the DESI Era ›
Homogeneous accretion of the Earth in the inner Solar System ›
Mapping the emission and spectral properties of the FRI radio galaxy 3C 449 with LOFAR and the VLA ›
The exponential growth of infinitesimal perturbations in the long-term evolution of simulated galaxies ›
Astrophysical parameters of LS 437 and the nature of X0726-260 ›
Disk instability model incorporating a variable inner disk radius in SS Cyg and U Gem ›
Active moons in our Solar System and beyond -- Io, Europa, Enceladus, Triton, and exomoons ›
Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility ›
On the possibility of chemically driven convection in red giants. Implications for the He-core flash and mixing above the Red Giant Branch Bump ›
Inspecting Cloudy Substellar Atmospheres with JWST MIRI Synthetic Magnitudes from Spitzer Mid-infrared Spectra ›
A First Principles Approach to the 100,000-year Problem ›
Spatially Resolved Kinematics of SLACS Lens Galaxies. II: Breaking Degeneracies with Lensing and Dynamical Models ›
Probing Collapsed Dark Matter Halos with Fast Radio Bursts ›
21 cm Power Spectrum Analysis of North Celestial Pole Observations with the Tianlai Dish Pathfinder Array ›
JWST/MIRI Hydrocarbon and Water Absorption in the Wind of a Young Disk: Signatures of Pebble Drift and Carbon Grain Sublimation ›
In Situ Interferometric Spatial Mapping Of A Microwave Kinetic Inductance Detector Array ›
FRTSearch: Unified Detection and Parameter Inference of Fast Radio Transients using Instance Segmentation ›
Detection and analysis of white-light emission in solar flares through light curve diagnostics ›
KIC 3868420: A high-amplitude $\delta$ Scuti-$\gamma$ Dor hybrid star crossing the Hertzsprung gap ›
Enhancing Ly{\alpha} Emitter Identification in HETDEX with a Convolutional Neural Network ›
Accretion-Mode Transition: The Driver Behind Spectral Changes in Changing-Look AGNs ›
The $\mu$ Herculis system solved after nearly three centuries ›
Multiwavelength Study of Blue Straggler Stars in Tombaugh 2: Evidence for Binary Mass Transfer and Constraints on Cluster Dynamical State ›
Interaction-powered Type Ibn Supernovae as a Transient PeVatron Candidate: The Case of SN 2023uqf ›
Acoustic instability at shock-wave precursors ›
POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean ›
Evidence for a bloated massive protostar in IRAS20126+4104 ›
M1-92: AGB interruption and isotopic ratio paradox. Chemistry and morpho-kinematics from improved shapemol modelling ›
Deriving volume density profiles of filaments from observed surface densities ›
Primordial Black Holes Formation Beyond the Standard Cosmic QCD Transition ›
Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation ›
Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow ›
Kelvin waves over a differentially rotating spherical shell ›
Metal enrichment in the galaxy group IC 1262 ›
Dark Matter's influence on Evolution of MBHB in Dwarf Galaxies: A Case Study of Leo I dSph ›
Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics ›
The undetectable fraction of core-collapse supernovae in luminous infrared galaxies -- II. GSAOI/GeMS dataset ›
Self-Lensing Signals in Binary Systems Containing White Dwarfs with Neutron star or Stellar-mass Black hole Companions ›
Illuminating the Local Universe: Large-Scale Structure from ZTF Type Ia Supernovae ›
A Search for Hydroacoustic Signals from Bolides ›
Constraining Electron-Impact Ionization of O$_2$ Through UV Aurora Observations at Ganymede ›
Solar Orbiter observations of solar energetic electron events associated with hard microflares ›
Variability classification of TESS targets in LOPS2, the first long-term pointing field of PLATO. Version 1 of the public variability catalogue ›
Gravitational Gertsenshtein-Zeldovich mechanism for the Association between GW190425 and FRB 20190425A ›
The spectrum of the persistent radio source associated with FRB 20190417A ›
A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution ›
The role of accretion efficiency, natal kicks, and angular momentum transport in the formation of the Gaia black holes ›
JWST observations of photodissociation regions. IV. Carbonaceous emission band sub-components in NGC 7023 have distinct spatial distributions ›
Hot blue progenitors of stellar-mass black holes ›
The $R$-Process Alliance: Actinide Abundances, Variation, and Evolution in Metal-Poor Stars ›
Revisiting the angular size-redshift cosmological test with milliarcsecond radio structures in active galactic nuclei ›
Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? ›
High-energy Processes in the Bubbles of Wolf-Rayet Stars: The case of WR 102 ›
How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE ›
Probing Scalar-Tensor-Induced Gravitational Waves in the nHz Band: $\texttt{NANOGrav}$ and SKA ›
Reassessing planetary composition: Evidence of rock-dominated envelopes in Uranus and Neptune ›
Obscured at the Core: Evidence for Nuclear Dust in Reddened Type-1 AGN ›
A note on Gurzadyan theorem ›
Frequency & Radiative Analysis of Random Yagi-UHF/VHF Phased Array ›
Amerigo Vespucci and the discovery of the Southern Sky ›
Astrophysical Signatures of Einstein-Skyrme Anti-de Sitter Black Holes: Epicyclic Frequencies and QPO Constraints ›
RAPRAL v1.0: RAdiation Prediction using RAy tracing and Line-by-line methods for hypersonic air flows ›
Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors ›
Novel ringdown tests of general relativity with black hole greybody factors ›
Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects ›
MMS Insights into CME Driven Sub-Alfv\'enic Solar Wind at 1 AU ›
Fe-H melting curve below 3 GPa: Implications for hydrogen in the lunar core ›
Graviton Production from Inflaton Condensate: Boltzmann vs Bogoliubov ›
Dark matter heating of Planet 9, and its observational implications ›
Infrared Spectral Gap in a Gluonic Dark Sector as the Origin of the Galactic Acceleration Scale ›
Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints ›
Jets and spectral states with three-components of accretion flow around a black hole ›
Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D ›
The molecular chemistry of nanoscale organic matter in asteroid Ryugu ›
Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascades ›
VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability ›
Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6 ›
Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias ›
Relativistically-strong electromagnetic waves in magnetized plasmas ›
The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos ›
Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses ›
The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12 ›
EFT of Dark Energy with Cosmic Chronometers: Reconstructing Background EFT Functions ›
A search for successful and choked jets in nearby broad-lined Type Ic supernovae ›
A Shocked Wind Interpretation of an Odd Radio Circle ›
The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates ›
The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-$\chi_{\rm eff}$ correlation ›
Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars ›
Revealing the diversity of Type IIn supernova progenitors through their environments ›
POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload ›
An Open-Source High-Level Graphical Signal Processing Language with Simulation and HDL Generation ›
Self-resonance preheating in deformed attractor models: oscillon formation and evolution ›
Measurement prospects for the pair-instability mass cutoff with gravitational waves ›
$\texttt{GPUmonty}$: A GPU-accelerated relativistic Monte Carlo radiative transfer code ›
Testing models for fully and partially stripped low-mass stars with Gaia: Implications for hot subdwarfs, binary RR Lyrae, and black hole impostors ›
Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate ›
Comment on: "Third-order corrections to the slow-roll expansion: Calculation and constraints with Planck, ACT, SPT, and BICEP/Keck [2025 PDU 47 101813]" ›
New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences ›
Formation and disruption of wide binaries in star clusters revealed by N-body simulations ›
The multi-age stellar populations of Terzan 5 as revealed by JWST ›
AI-Assisted Spectral Decomposition of Euclid Q1 Gravitational Lenses: Extended-Coverage NISP Extraction with Vision-Language Model Quality Control ›
DeepDISC-Euclid: Source Classification and Photometric Redshifts in Euclid Deep Field North With a Pixel-Level Deep Learning Approach ›
A Statistical-AI Framework for Detecting Transient Flares in SDSS Stripe 82 Quasar Light Curves ›
Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune System ›
The environmental imprint on molecular layering in the dusty streamer of M512 ›
Scalar-Induced Electromagnetic Radiation: Comparison with Axion-Like Particles and Implications for Modified Gravity ›
Non-degenerate pumping of superconducting resonator parametric amplifier with evidence of phase-sensitive amplification ›
BHaHAHA: A Fast, Robust Apparent Horizon Finder Library for Numerical Relativity ›
A Match Made in Heaven: Linking Observables in Inflationary Cosmology ›
Properties of the neutron star crust informed by nuclear structure data ›
Testing the Dark Universe through the Layzer-Irvine Equation ›
Relativistic Maxwell-Bloch Equations with Applications to Astrophysics ›
GREA and Dark Energy: A holographic correspondence ›
Searches for Post-Merger Gravitational Waves with CoCoA: Sensitivity Projections Across Large Template Banks for Current and Next-Generation Detectors ›
Is the Conventional Picture of Coherence Time Complete? Dark Matter Recoherence ›
The emergent Big Bang scenario ›
Photon Propagation through Magnetar-Hosted Axion Clouds: Time Delays and Polarimetric Constraint ↓↑