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

Stars over the dome

Cloud

Rainfall

S Sky
Temperature
0.2 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1025.5 hPa

Moon
Latest preprints on astro-ph:
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Agentic Systems for Calibrating Cosmological Simulations ›
Likely Metal Scarring in the Magnetic White Dwarf LHS 2534 ›
SEAMLESS Survey: A Closer Look at Seven Local Volume Dwarf Galaxies in Diverse Environments ›
Hints of self-interacting dark matter from strong gravitational lensing ›
Chaos and loss: reevaluating the loss-cone formalism in the context of chaotic diving orbits in flattened potentials ›
When precise inference is wrong: Diagnosing model misspecification with applications to cosmic dawn and reionisation ›
Surprisingly normal? GW241011 and GW241110 in the context of hierarchical merger classification ›
Missing Mergers: On the Unexpected Delay-Time Distribution of Binary Neutron Star Mergers ›
Bridging Scales: Multi-Zone GRMHD-Informed Anisotropic AGN Feedback in Galaxies ›
Model-independent and reconstruction-free evidence for cosmic acceleration from DESI baryon acoustic oscillations ›
Cosmic merger rates and population evolution of binary black hole mergers in AGN disks ›
How to feed your dragon: the role of turbulence in AGN activity ›
Learning Galaxy Kinematics from Spatially Unresolved Spectra ›
The assembly of dusty galaxies at $z \geq 4$: grain growth and the evolutionary origin of the dust-to-stellar-mass scatter ›
Kinematic Decomposition of the BCG and ICL in Abell S1063 and MACS J1206 ›
NGDEEP: Anchoring the $0.5 < z < 3.5$ Star-Forming Main Sequence at Low Stellar Masses with Ultradeep JWST/NIRISS WFSS ›
From Quantum Field Fluctuations to High-Redshift AGN: Semiclassical Origins of Halo Mass Function Constraints in the JWST Era ›
FOMO-Z. Optimal galaxy classification, photometric redshifts, and reconstruction of population distributions ›
The Importance of Curium-250 to the $\gamma$-Ray Signature of $r$-Process Remnants ›
The Size-Mass Relation and Inside-Out Quenching of Massive Quiescent Galaxies at $2 ›
Optimizing Prompt Radio Counterpart Searches for Gravitational-Wave Events with the Deep Synoptic Array ›
Completeness and dynamical stability in exoplanet occurrence rates ›
GRB 241113B: the first SVOM and EP gamma-ray burst A soft GRB likely seen on-axis, from soft X-rays to gamma-rays ›
Machine Learning Sensor Fusion for Water Vapor Radiometry based Tropospheric Delay Calibration ›
An Assessment of Water Vapor Radiometry Landscape in ngVLA Context ›
Vacuum Phase Transition and Decay to Cross the Phantom Divide ›
Spectral Information Content of Diffraction-Limited Images ›
MAGIKS: Multimodal Alignment and Gravitational-Wave-Conditioned Interaction for Kilonova Search ›
HAWC, Fermi-LAT and Chandra Detections of High Energy Particles in the S106 Star Forming Region ›
Effect of quark-hadron phase transitions on the neutron star mass distribution ›
The Effect of Large Apertures on Atmospheric Noise Spectra for Millimeter-wave Telescopes ›
Spectroscopic observations of periodic bursty ejections during a dome-spire-shaped jet ›
Stellar Bars Reshape the Spatial Distribution of UV-bright Clumps in Nearby Galaxies ›
Relative Influence of Coronal Properties of CME in their Evolution and Geo-effectiveness ›
Kinematic Map of the Galactic Bulge Using HST Proper Motions ›
Resolving the Complex Line-Locking Structure in Quasar J004613+010425 with VLT/X-shooter Spectroscopy ›
Identifying a High-confidence Candidate of Stellar Coronal Mass Ejection on an M~dwarf ›
Enhanced Detectability of Very-High-Energy Gamma Rays from Off-Axis Short Gamma-Ray Bursts: Impacts of Structured Jets and External Inverse-Compton Scattering ›
Cryogenic Optical Characteristics of S-FPL51 and S-LAH71: Refractive index, Transmission and Thermal expansion ›
OASIS I: Spectroscopy of Mini-Quenched and Lulling Galaxies Constrains the Quiet Side of Bursty Star Formation at z > 4 ›
OASIS II: The Ionized Gas Traces Feedback-Driven Declines into the Quiet Side of Bursty Star Formation at z > 4 ›
OASIS III: Bursty star formation drives observed galaxy sizes at $z\geq4$ ›
As a matter of reconstruction -- varying the magnetic Prandtl number in implicit large eddy simulations ›
Disk-Corona Energy Balance Evolves with Flux State in the Quasar PDS 456 ›
Dark Halos, Intermediate-Mass BH and Nuclear Stellar Clusters in Dwarf Spheroidals ›
Demographics and growth of the astronomy and astrophysics community ›
The JWST/PASSAGE Survey: Metallicity Radial Gradients in Emission-Line Galaxy Pairs at Cosmic Noon with NIRISS ›
Co-evolution of AGN and Host Galaxies across Cosmic Time Using JWST data ›
HWP-synchronous signal induced by misalignment of the sapphire crystal axis ›
The Broad-Line Region Size-Luminosity Relation in AGN Constrained by the Viewing Angle with the FRADO Model ›
From Anoxic to Oxic Earth: Detectability of Atmospheric Biosignatures across Stellar Hosts with ELT/ANDES ›
The Evolution of the Circumgalactic Medium after a starburst in DESI Post-Starburst Galaxies ›
SN 2025dys: A luminous supernova explosion from a partially stripped helium star ›
The Pristine Survey. XXX. Mapping substructures in the inner and outer halo with blue horizontal branch stars ›
Long-term variability of the 35-day cycle in Her X-1 ›
Gamma-Ray Emission from LS 5039: A 30-500 GeV Excess and Phase-Resolved Broadband Spectral Modeling ›
Inferring dominant acceleration mechanisms using the longitudinal spread of solar particle intensities: 28 May 2021 event ›
Decay of space plasma turbulence downstream of bow shocks: MMS magnetosheath unbiased campaign observations ›
First Light with the Dark100 Array of PANOSETI Telescopes at Palomar Observatory ›
The Dynamical Mass Profiles of Galaxy Groups - Application to IllustrisTNG-300 ›
Primordial black holes and gravitational waves from aligned axion inflation ›
The multiple origins of spurs in stellar streams: a challenge for dark matter diagnostics ›
A multi-wavelength view of PSR J0437-4715 with NICER and other missions: Radius measurements from far-ultraviolet to hard X-ray pulse profile modeling ›
Bar likelihood in local galaxies: the joint role of stellar mass, morphology and environment ›
Collisional excitation of HMgC$_3$N by He: rate coefficients and astrophysical implications ›
The Unusual X-ray Spectrum of R Mon ›
The 943 MHz radio-SFR relation of nearby galaxies observed with ASKAP ›
Two-loop matter power spectrum from FFTLog and kite integrals ›
Stellar Kinematics and Molecular Gas toward NGC 6357: An Overlooked Earlier Stellar Generation ›
Current Sheets and Magnetic Reconnection statistics by Solar Orbiter at few to tens of Ion Inertial Lengths I: Energy Dissipation ›
An exploration of in-band spectral index techniques for extended radio sources with EMU ›
Cosmology with post-EoR 21 cm Intensity Mapping surveys: power spectrum measurements in the last decade ›
Formation of Micron-sized Presolar Graphite Grains in Low-energy Supernova Ejecta ›
An end-to-end CNN search for ultra-short-period planets in TESS: from the blend ceiling to the independent validation of TOI-6662 b ›
Distinguishing N$_2$-Dominated from O$_2$-Dominated Atmospheres on Terrestrial Exoplanets with Reflected-Light Spectroscopy ›
Elastic boundaries in Stochastic Inflation ›
Tests of equivalence principle violation in doubly coupled dark energy ›
Nova V1674 Her as a fast magnetic rotator ›
Model-Independent Assessments of Tidal Alignment and Density-Weighting Dependence in Galaxy Intrinsic Alignments ›
Two-peak gravitational wave spectra from supercooled two-field phase transitions ›
Gravitational Lensing Signatures of a Black Hole in Mimetic Euler-Heisenberg theory ›
Leaking Sound Waves: Gravitational Waves From Dark Sectors Weakly Coupled to the Standard Model ›
Effects of Eddington-inspired Born-Infeld Gravity on Black Hole Accretion ›
Stress-enhanced diffusion in Yukawa crystals ›
Equipartition between Alfv\'enic turbulence and energetic ions as the origin of the -5 common spectrum in the heliosphere ›
Two-Fluid Radial Stability of Dark-Matter-Admixed Compact Objects: Dark Compact Planets, Dark White Dwarfs, Dark Neutron Stars, and Dark Oysters ›
More Eccentric, Not Always Less Detectable: High Mass Holds Its Ground, Low Mass Loses Reach ›
Conceptual Design of a Compact Magnetic Spectrometer for Space Radiation Measurement ›
New Effects in Multifield Cosmology Coupled to the Gauss-Bonnet Term ›
From thermogravity to thermocosmology with a running non-conservation scale ›
Topological Multi-Natural Inflation ›
SAPPHIRES: Extremely Metal-Poor Galaxy Candidates with $12+{\rm log(O/H)} ›
ZTF SNe Ia DR2: Towards cosmology-grade ZTF supernova light curves using scene modeling photometry ›
Reprocessing of X-rays emission in Ultra-Luminous X-ray sources ›
The Multiphase Circumgalactic Medium of DESI Emission-Line Galaxies at z~1.5 ›
ECOGAL I. Project design and the first catalogue ›
GLIMPSE-DDT spectroscopic properties of faint-end galaxies at $z\sim6$: Towards first metal enrichment, dust production, and ionizing photon production ›
The Geometric Crisis in Cygnus~X-3: Limitations of Wind-Fed Accretion and the Case for Roche-Lobe Overflow ›
VINTERGATAN-GM: long-lived satellite planes induced by a massive GSE-like merger ›
The pulsar population of Omega Centauri: New TRAPUM searches, timing, and cluster dynamics with MeerKAT and Parkes ›
Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6 ›
Curvature-Radiation Geometries Across the Second CHIME/FRB Fast Radio Burst Population ›
Interaction-induced star formation boosts stellar mass assembly in $z\sim5$ galaxies ›
The Status of Single Scalar Field Dark Energy ›
Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging ›
Lambda as a Probe of Lensing Consistency ›
What becomes of JWST/NIRCam-selected high-redshift massive galaxies? ›
Corrected detector-level reconstruction of inclined radio air showers from trigger-level ADC waveforms ›
Ultra-long simulations of collisionless relativistic shocks in front-comoving frame: evidence for a steady state and its properties ›
Gravitational-Wave Sky Mapping with Pulsar Timing Arrays: The Full Earth-Pulsar Response and Resolution Operational Regimes ›
Supergranulation as a Tracer of Solar-Cycle Variability ›
Optimizing the extraction of information from redshift probability distribution functions ›
Column-density estimation from the equivalent widths of absorption doublets ›
Prospects for Direct Detection of Ultralight Dark Matter candidates in deci-Hz Band with IndIGO-D ›
A Framework for Evaluating Forward Contamination Risk for Bio-ISRU Microorganisms ›
An efficient approach to resistive GRMHD simulations of binary neutron star mergers ›
MEGATRON: Dwarf Galaxy Quenching in the Epoch of Reionization ›
On The Scaling Relations Between Black Holes And The Galaxy/Bulge Mass And Their Connections With The Black Hole Occupation Fraction ›
Running cosmological constant in light of recent CMB-BAO data ›
Hoag-type Galaxies: A Photometric Study of the Cores and Rings of Thirty Systems from the DESI Legacy Survey ›
Searching for Ultra-Light Axions with Twisted Cavity Resonators of Anyon Rotational Symmetry with Bulk Modes of Non-Zero Helicity ›
Local-equilibrium theory of neutrino oscillations ›
What do the fundamental constants of physics tell us about life? ›
Sterile neutrino dark matter in conformal Majoron models ›
On the curlometer measurement of field-aligned and perpendicular currents in low Earth orbit: Swarm observations and whole geospace simulations ›
Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions: A generalization ›
Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions ›
Bayesian nonparametric estimation of correlated gravitational wave detector network noise using matrix-gamma process priors ›
Solar Magnetic Configuration Control over Radiation Belt Electrons ›
cWB-space: A time-frequency unmodelled transient-search pipeline for LISA ›
Searching for gravitational wave echo with group equivariant neural posterior estimation ↓↑