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
6.8 °C
Humidity
95%
Wind
0.0 km/h
Pressure
1020.7 hPa

Moon
Latest preprints on astro-ph:
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MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57 ›
Modeling gravitational wave sources in the MillenniumTNG simulations ›
New ultralight scalar particles and the mass-radius relation of white dwarfs -- the important role of Sirius B ›
Beyond the stars: Linking H$\alpha$ sizes, kinematics, and star formation in galaxies at $z\approx 4-6$ with JWST grism surveys and $\texttt{geko}$ ›
A Deep Look into the Intermediate-Age Open Cluster NGC 2506: What Binary Systems Reveal About Cluster Distance and Age ›
Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective? ›
Preferential Accretion onto the Secondary Black Hole Strengthens Gravitational Wave Signals ›
Asymmetries in stellar streams induced by a galactic merger ›
Phase-resolved optical spectroscopy of the rapidly varying white dwarf ZTF 1851+1714 ›
A Walk on the Retrograde Side (WRS) project. II. Chemistry to disentangle in situ and accreted components in Thamnos ›
MEGATRON: Disentangling Physical Processes and Observational Bias in the Multi-Phase ISM of High-Redshift Galaxies ›
Are all Binary Black Holes Detected from LIGO-Virgo-KAGRA Follow the Universal Time-Delay Distributions? Likely Not ›
Evidence of violation of Case B recombination in Little Red Dots ›
JWST occultation reveals unforeseen complexity in Chariklo's ring system ›
The rise and fall of Little Red Dots could be driven by the environment ›
The first proper motion measurement of the acceleration regions in the large-scale jets of SS 433 powering the W50 nebula ›
Radiation magnetohydrodynamics modeling of an impulsively driven chromospheric jet in the solar atmosphere ›
CCAT: Readout of over 10,000 280 GHz KIDs in Mod-Cam using RFSoC Electronics ›
Ensemble seismic study of the properties of the core of Red Clump stars ›
Primordial Black Holes and their Mass Spectra: The Effects of Mergers and Accretion within Stasis Cosmologies ›
RFSoC receiver calibration system for 21-cm global spectrum experiments from space: The CosmoCube case ›
Revisiting the Orbital Dynamics of the Hot Jupiter WASP-12b with New Transit Times ›
Dual perspectives on GX 17+2: a simultaneous NICER and NuSTAR study ›
A chemodynamical study of $r$-process-enhanced stars ›
Ionized gas components in low surface brightness galaxy AGC 111629 ›
Formation of A Nuclear Star Cluster Through A Merger Event In The Low Surface Brightness Galaxy AGC 223218 ›
The Star-forming Main Sequence and Bursty Star-formation Histories at $z>1.4$ in JADES and AURORA ›
Spectropolarimetry of NGC 1275 reveals a narrow-line radio galaxy with polarization parallel to its radio jet axis ›
3D B-fieLds in the InterStellar medium and Star-forming regions (3D-BLISS): I. Using Starlight Polarization in Massive IRDC Filament G11.11-0.12 ›
Benchmarking AI-evolved cosmological structure formation ›
Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network ›
Identifying the secondary jet in the RadioAstron image of OJ~287 ›
Warm absorber outflows in radio-loud active galactic nucleus 3C~59 ›
A Sample of HeII {\lambda}4686 "Changing-Look" Quasars ›
Low-noise Fourier Transform Spectroscopy Enabled by Superconducting On-Chip Filterbank Spectrometers ›
A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane ›
Hard X-ray view of two $\gamma$-ray detected low-luminosity active galactic nuclei: NGC 315 and NGC 4261 ›
JWST observations of photodissociation regions: II. Warm molecular Hydrogen spectroscopy in the Horsehead nebula ›
MEGATRON: The environments of Population III stars at Cosmic Dawn and their connection to present day galaxies ›
Unlocking AGN Variability with Custom ZTF Photometry for High-Fidelity Light Curves and Robust Selection ›
The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies ›
Recasting the nature of INTEGRAL hard X-ray transients previously classified as active galactic nuclei ›
Textual interpretation of transient image classifications from large language models ›
Is the high-energy environment of K2-18b special? ›
Simulations of Globular Cluster Evolution with Multiple Stellar Populations ›
1FLAT: a Firmamento-based catalog of AGN in Fermi-LAT high Galactic latitude {\gamma}-ray sources ›
In-flight performance of the IXPE telescopes ›
Understanding an origin of palladium in metal-poor stars based on the non-LTE analysis of Pd~I lines ›
Protoplanetary disc population synthesis I. Constraining disc parameters to reproduce disc observations ›
Revealing the Temporally Stable Bimodal Energy Distribution of FRB 20121102A with a Tripled Burst Set from AI Detections ›
Modeling the formation of N2 and CH4 frost on Pluto's slopes ›
Machine Learning Techniques to Distinguish Giant Stars from Dwarf Stars Using Only Photometry -- Pushing Redwards ›
The formation of Gaia BH3 ›
Prolonged fallback and late-time rebrightening episodes in stellar tidal disruptions as imprints of a galactic environment ›
Machine Learning for Radial Velocity Analysis I: Vision Transformers as a Robust Alternative for Detecting Planetary Candidates ›
Polka-dotted Stars II: Starspots and obliquities of Kepler-17 and Kepler-63 ›
CURLING -- II. Improvement on the $H_{0}$ Inference from Pixelized Cluster Strong Lens Modeling ›
Disk fraction among free-floating planetary-mass objects in Upper Scorpius ›
Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations ›
Fomalhaut's debris disc is not dominated by primordial Plutos ›
Probing the cosmological 21~cm global signal from the Antarctic ice sheet ›
AppleCiDEr II: SpectraNet -- A Deep Learning Network for Spectroscopic Data ›
High-energy variability of the gravitationally lensed blazar PKS 1830-211 ›
Testing new-physics scenarios with the combined LHAASO and Carpet-3 fluence spectrum of GRB 221009A: axion-like particles and Lorentz-invariance violation ›
JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b ›
Beyond diagnostic-diagrams: A critical exploration on the classification of ionization processes ›
The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; varying hydrodynamic models, dust, and wide-field, narrow-band imaging detection ›
A Comoving Framework for Planet Migration ›
Confirming Near- to Mid-IR Photometrically-Identified Obscured AGNs in the JWST era ›
Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts ›
Diffuse continuum emission and large extended sources at MeV energies ›
Rolling with modular symmetry: quintessence and de Sitter in heterotic orbifolds ›
Magnetic Helicity, Magnetic Monopoles, and Higgs Winding ›
Vision Transformer for Transient Noise Classification ›
A comprehensive look into the accuracy of SpEC binary black hole waveforms ›
Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable twin stars ›
Influence of Solar Sails on Magnetic Field Measurements in Space Plasmas ›
A Review of 10 Years of ProtoSpace: Spacecraft CAD Visualization in Collaborative Augmented Reality ›
Measurement of the $^{35}Cl(n, p)^{35}S$ cross-section at the CERN n\_TOF facility from subthermal energy to 120 keV ›
When vacuum breaks: a self-consistency test for astrophysical environments in extreme mass ratio inspirals ›
Unified Dark Matter and Dark Energy in a model of Non-Canonical Scalar-Tensor Theory ›
GW231123: extreme spins or microglitches? ›
On Inflation and Reheating Features in the Higgs-$R^2$ Model ›
Tracing satellite planes in the Sculptor group: II. Discovery of five faint dwarf galaxies in the DESI Legacy Survey ›
Distribution of Europium in The Milky Way Disk; Its Connection to Planetary Habitability and The Source of The R-Process ›
A Semi-analytic Framework of Population III and Subsequent Galaxy Formation on Cosmological N-body Simulations ›
The Southern Photometrical Local Universe Survey (S-PLUS): searching for metal-poor dwarf galaxies ›
AGN ruled out as the dominant source of cosmic reionization ›
Foreground Removal in Ground-Based CMB Observations Using a Transformer Model ›
Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold ›
Dark sirens and the impact of redshift precision ›
Investigating dusty Red Supergiant outflows in Westerlund 1 with 3D Hydrodynamic simulations ›
Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations ›
Determining the 3D Dynamics of Solar Flare Magnetic Reconnection ›
Gravitational Wave Memory of Primordial Black Hole Mergers ›
Prospects for disentangling dark matter with weak lensing ›
Cosmic Ray Perpendicular Superdiffusion and Parallel Mirror Diffusion in a Partially Ionized and Turbulent Medium ›
Are magnetic fields in cosmic voids primordial? ›
The hot circumgalactic medium in stacked X-rays: observations vs simulations ›
Direct reconstruction of the Reionization history from 21cm 2D Power Spectra ›
Requirements on bandpass resolution and measurement precision for LiteBIRD ›
Type Ibn supernovae from ultra-stripped supernova progenitors ›
Thick Disks around White Dwarfs viewed 'Edge-off': Effects on Transit Properties and Infrared Excess ›
Synthesizer: a Software Package for Synthetic Astronomical Observables ›
Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts ›
Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear ›
Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometers ›
The source of the cosmic-ray excess in the Centaurus region -- constraints on possible candidates, mass composition and cosmic magnetic fields ›
Matter power spectrum reconstruction with KiDS-Legacy: Improved internal $\Lambda$CDM consistency and preference for strong baryonic feedback ›
Supergranulation and poleward migration of the magnetic field at high latitudes of the Sun ›
Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information ›
Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization ›
Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy ›
Abundance of strontium in the Galactic globular cluster 47 Tuc ›
A Link Between Rocky Planet Density and Host Star Chemistry ›
M5 -- Mars Magnetospheric Multipoint Measurement Mission: A multi-spacecraft plasma physics mission to Mars ›
Sharpening the dark matter signature in gravitational waveforms I: Accretion and eccentricity evolution ›
Background-dependent and classical correspondences between $f(Q)$ and $f(T)$ gravity ›
Prospects of future MeV telescopes in probing weak-scale Dark Matter ›
Unveiling a New $\beta$-Scaling of the Tearing Instability in Weakly Collisional Plasmas ›
The Dark Matter Diffused Supernova Neutrino Background ›
Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature ›
Modeling Gravitational Wave Modes from the Inspiral of Binaries with Arbitrary Eccentricity ›
Universality of gravitational radiation from magnetar magnetospheres ›
Flavour interferometry in Reissner-Nordstrom background ›
The impact of Alfvenic shear flow on magnetic reconnection and turbulence ›
High-Quality Axion Dark Matter at Gravitational Wave Interferometers ›
Regression of Suspension Violin Modes in KAGRA O3GK Data with Kalman Filters ›
Extra Radiation Cosmologies: Implications of the Hubble Tension for eV-scale Neutrinos ›
WISPFI Experiment: Prototype Development ↓↑