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

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Temperature
4.8 °C
Humidity
68%
Wind
0.0 km/h
Pressure
1022.1 hPa

Moon
Latest preprints on astro-ph:
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A Sub-Parsec Origin for Rapid Accretion-State Transitions in Radio-Loud AGN ›
A combined PRIMER+MINERVA study of the evolution of $\mathbf{[O\mbox{III}]+H\beta}$ equivalent width from $\mathbf{z=3}$ to $\mathbf{z=8.5}$ ›
DarkMatterFM-Registry: A Machine-Readable Registry of Dark-Matter Models Extracted from the arXiv Literature ›
Primordial or Post-Inflationary: Distinguishing the Origin of Scale-Dependent Features in the CMB ›
Anisotropic three-point statistics of the peculiar velocity and galaxy density fields: modelling in Fourier and configuration space ›
Constraining Dust Attenuation Curves in Star-Forming Galaxies at Cosmic Noon Using Multiple Emission Line Ratios ›
FORGE'd In The Early Universe II: Constraining The Pop III Initial Mass Function ›
Magnetically Arrested Accretion and Black Hole Spin in a Semi-Analytic Model of Galaxy Formation ›
FORGE'd in Fragments: Pop III star formation in a Milky Way-like progenitor halo ›
Hydrodynamic Natal Kicks and Formation of Black Hole Binaries ›
Jeans Dynamical Constraints on the IMF in Massive Quiescent Galaxies at $z\sim0.7$ from JWST/NIRSpec ›
VENUS: Strong Lens Mass Models and Einstein Radii of 60 Galaxy Clusters ›
Short-term optical monitoring of quadruply imaged quasars ›
Nonstandard Dark Matter at Nonlinear Scales ›
Digging into the Interior of Hot Cores with ALMA (DIHCA). VIII. Feeding a high-mass binary system in the making ›
Testing influence of tides on gravitational wave emission with SPH code PHANTOM ›
TRGB Distances to the Andromeda Dwarf Satellites from the INT Monitoring Survey ›
Expanding the Volatile Abundance Inventory for High-Priority K-Dwarf JWST Exoplanet Systems ›
TitanMPAS - a new global and regional Titan atmospheric circulation model. Part I: Global model results ›
Modified Newtonian Dynamics and galaxy clusters ›
Coherent radio emission at 45 MHz from the nearby planet-hosting star GJ 725A ›
Constraining the Merger Fraction and the Upper Mass Limit of Ultramassive White Dwarfs ›
Neutrino pair annihilation in curved spacetime: a fast moment method and the geometry of flavour conversion ›
The Complex Magnetic Anatomy of a White Dwarf Chromosphere ›
Bicoherence States from QPO-Accretion Flow Coupling in Black Hole X-ray Binaries ›
Interferometric survey of stellar parameters. Reliable methodology for a direct measurement of the angular diameter in exoplanet host stars ›
KCWI Observations of Type 2 Quasar-driven Ionized Outflows at z~0.1 ›
Unlocking Pandora's Secrets: Probing the Thermodynamics of Abell 2744 ›
Modeling of the X-ray Flux and Polarization Energy Spectra of Black Hole X-Ray Binaries with the KerrC Code ›
Predicting Continuum Emission in Massive Star-Forming Regions with Embedded HII Regions - Dust, Free-Free, and Anomalous Microwave Emission with POLARIS ›
Tidal Braking Does Not Dominate Open-Cluster Slow Rotators ›
System noise temperature measurements of a 19-element phased array feed ›
Identifying Chemically Coherent Stellar Families in the Galactic High-{\alpha} Disk with Low-Resolution Spectroscopy ›
Dynamical formation of Gaia neutron star binaries in star clusters as a phase-dependent process ›
Phosphorus-rich star formation in giant molecular clouds hosting primordial globular clusters ›
SEDust: A DUSTY-Based SED-Fitting Pipeline for Dust and Mass-Loss from AGB and LPV Stars ›
Probing Dark Matter via the Migdal Effect in LUX-ZEPLIN Data ›
Estimations for strong and weak hot Jupiter magnetism: A Python package with interpolators and scaling laws ›
New optimisations for exact, scalable 2D Gaussian process inference, with applications to astronomical time-series ›
Chromospherically Active Stars in the MeerKAT Galactic Plane Survey ›
Quasi-spherical fallback in binary neutron-star mergers: fuel and obstacle for extended emission ›
Suppression of water-ice UV photodesorption on cosmic dust analogs ›
The N/O-O/H relation across large-scale environments ›
Successive Decimetric Bursts Associated with Breakout Magnetic Reconnection during the Decay Phase of an M-Class Flare ›
GW230729\_082317 and GW231118\_005626: A Candidate of Hierarchical Triple Mergers ›
Activity of the ejected galactic nuclei and cosmic rays ›
Existence of Distinct Strong and Weak Shear Regimes of Self-Generated Turbulent Magnetic Reconnection ›
Primordial non-Gaussianity as a large-scale cosmic-web bias ›
The OpenMULTI3D stellar analysis package. A 3D non-LTE spectrum synthesis code for AFGKM-type stars within the DISPATCH framework ›
Where the red rise stops: JWST/MIRI reveals a near-infrared turnover in the Little Red Dot Abell2744-QSO1 ›
CO gaps in cold transition disks around low-mass stars ›
Validation of Habitable Zone Limits with a New Radiative-Convective Equilibrium Climate Model ›
Constraints on Cosmic-Rays and the MeV Emission from Jupiter's Atmosphere ›
Violent relaxation redux ›
Through Ups and Downs: the Transient Lensing Behaviour of SIDM halos undergoing Core Collapse ›
A joint astrometric, eclipse timing and radial velocity orbit for the hierarchical triple V819 Herculis ›
XMM-Newton observations of the highest field polar AR UMa: An extreme case of soft-blobby accretion ›
SQUALO II: Probing Accretion Through CO Molecular Outflows in Massive Star-forming Clumps ›
Fundamental Noise Processes in Pulsar Timing ›
A possible connection between the ridge and hypotenuse in the bispectrum of black hole X-ray binaries through quasi-periodic modulation ›
Advances in High-Precision Astrometry for Exoplanet Detection for Astrometric Missions ›
Forecasting Fundamental-Plane Tests of Intermediate-mass Black Holes in Radio-selected Dwarf Galaxies ›
Does DESI point towards transient cosmic acceleration? ›
Superorbital period evolution of Hercules X-1 ›
Odd Loops: What Structures Can Produce a Parity-Violating Inflationary Trispectrum? ›
Ensemble Individual Mode Frequency Modeling of Kepler Giants - Extending the IACgrid towards the red-giant branch ›
The AIDA-TNG project: Galactic bar pattern speeds in self-interacting dark matter ›
Lessons from double-plane lenses for galaxy profiles, the Hubble tension, and the mass-sheet degeneracy ›
Multi-phase Carbon Structure and Dynamics in NGC 6334: Insights from CO, [C I], and [C II] ›
SN 2026ahvu in NGC 1433 May Be a Prompt Type Ia Supernova with a Delay Time Under 100 Myr ›
VLT and Keck recovery and characterisation of 2025 SC$_{79}$: linking 'Ayl\'o'chaxnim and Atira asteroids ›
Predicting next-week VIIRS fire detections in Bolivia: a reproducible benchmark with temporal and geographic evaluation ›
Entanglement in Collective Neutrino Oscillations on a Quantum Computer ›
Phentax: A JAX implementation of the IMRPhenomTHM waveform model ›
A pipeline for identifying astrophysical signals and instrumental glitches in LISA data ›
Baryon Number Susceptibilities of Hot and Dense Nuclear Matter in Relativistic Mean-Field Models ›
Probing flavor-dependent neutrino-dark matter interactions with the flavor composition of high-energy cosmic neutrinos ›
Mathematical foundations and numerical simulations of BDNK hydrodynamics: from heavy-ion collisions to astrophysics ›
Effects of a Nuclear Detonation in Low Earth Orbit ›
Challenges for minimal warm inflation in the Standard Model and beyond ›
Extragalactic photon-ALP conversion at CTA energies ›
Galaxy and Halo Root Systems: Fingerprints of Mass Assembly ›
Correcting for the effects of the point spread function in intra-halo light measurements and application to deep Hyper Suprime-Cam data ›
Early X-ray emission of short Gamma-Ray Bursts: insights into physics and multi-messenger prospects ›
Exoplanetary radio emission predictions and detectability in the SKA era ›
How Significant are Cosmological Collider Signals in the Planck Data? ›
New Constraints on Cosmic-ray boosted Sub-GeV Dark Matter via Light Mediators ›
An information-theoretic framework for quantifying coherence in the cosmic density field ›
An efficient model of cosmology dependence in the covariance matrix of the matter power spectrum ›
Cosmic Ray Inter-Station Fluctuations as Precursors of Geomagnetic Storms: Causal Baseline Analysis and Forecasting Limitations ›
Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres ›
The Baryon Budget of Galaxies across the First Billion Years ›
Estimation of the magnetic field strength from ALMA dust polarization in the protocluster G327.29 ›
Universal Dark-matter Density Profiles of Cosmic Filaments ›
Kinetic magnetohydrodynamics and Landau fluid closure in relativity ›
TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars ›
Origin and evolution of NiI and FeI in the coma of the interstellar comet 3I/ATLAS throughout its trajectory ›
Rapid and robust simulation-based inference for kilonovae ›
Identifiability of $g$ mode Resonances in Eccentric Binary Neutron Stars with Multidetector Observations ›
Cancellation of one-loop time dependence in superhorizon curvature perturbations from all scales ›
Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event ›
Set them free: extending RAMCOAL to model massive black hole triplets in hydrodynamical simulations of galaxies ›
Effects of Solar Wind Plasma Noise on Stochastic Gravitational Wave Background Searches with a Space Based Interferometer Network ›
Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins ›
Alcock-Paczynski Blinding Scheme for the Ly-$\alpha$ Forest Analysis ›
Primordial tensor mode from the neutrino sector ›
Gas-Phase Metallicity and Nitrogen Abundances in Low-Mass Galaxies Down to $M_\star\simeq10^{6.6}\,M_\odot$ at $z\simeq4.5$--$9.8$ from JWST Lensing Cluster Surveys ›
The Extended Ultrahigh-energy Gamma-Ray Emission in the Vicinity of PSR J2238+5903 ›
Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy ›
A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction ›
Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations ›
3D Hydrodynamic Simulations of Micro-Tidal Disruption Events Favor a Narrow, Ultra-relativistic Jet for GRB250702B ›
WindsoCC: reconstructing the wind-driven halo in MagAO-X images using wavefront sensor telemetry ›
An Optically Motivated Gamma-ray Study of Fermi-LAT Novae ›
Towards Genuine Coexistence: Per-Satellite Emission and Radiation Limits to Protect Radio Astronomy and Geodetic VLBI at 1-14 GHz from Satellite Constellations ›
ASKAP discovery of a pair of large radio bubbles: on the origin of odd radio circles ›
Finding and using interpretable latents in a neutrino foundation model with sparse autoencoders ›
PIFFLE: Characterizing Foreground Dispersion Measure Contributions Across 4 Decades in Halo Mass in the FRB20230907D Field ›
Amortized Opacity Marginalization Improves C/O Interval Calibration for Brown-Dwarf Retrievals ›
Rapid Growth of Intermediate-Mass Black Holes through Disk-induced Stellar Disruptions ›
ALMA Chemical Evolution (ACE) survey: the dust content of subsolar metallicity galaxies at cosmic noon ›
Resolving the Galactic Center Region's Gamma-Ray Emission and Searching for its Neutrino Counterpart with HAWC and IceCube ›
The Science Potential of Characterizing Gas Giant Exoplanets with HWO ›
Grid Optimization for Wide Field Modulation Collimators ›
Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units ›
Gravitational waves from strong first-order phase transitions in an expanding Universe ›
Late Epoch Infrared Spectroscopy and Two-Component 3D Photoionization Modeling of Classical Nova V5668 Sgr ›
Dynamical plausibility of triple-assisted interaction in Be-star multiple systems ›
FOMO-Z. Optimal galaxy classification, photometric redshifts, and reconstruction of population distributions ›
Tracking the evolution of sub-Neptunes. II. The radius valley on gyrochronological ages ›
Targeting the future of spectroscopic galaxy surveys -- A cosmological study case with the Wide-field Spectroscopic Telescope ›
How bursty star formation shapes spectral diversity at high redshifts: breaking degeneracies in early galaxy formation ›
Rotational Excitation of HC$_5$NH$^+$ by He: Collision Dynamics and Astrophysical Applications ›
Tidal Deformability of Neutron Stars in Scalar-Tensor Theories of Gravity ›
Asymmetric Dark Matter from Low-Scale Spontaneous Leptogenesis ›
Challenging the Weak Cosmic Censorship with Phantom Fields ›
Relativistic mode sums for neutron-star tidal response ›
Graviton Floor ›
New Universal Relations for Magnetized Neutron Stars ›
On the nature of oscillating modes of proto-neutron stars ›
Constraining the Quadratic-mode Amplitude Coupling in GW250114 ›
Optimal Strategies for Gravitational-Wave Memory Detection with Noise Marginalization in Pulsar Timing Arrays ›
Rotation slows the instability of Ellis-Bronnikov wormholes ›
Sensitivity of the IceCube atmospheric muon rate to decadal trends in the effective atmospheric temperature ↓↑