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

view from south-west

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Temperature
4.1 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1025.4 hPa

Moon
Latest preprints on astro-ph:
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Unveiling photometric transients with the ILMT and their follow-up using DOT ›
TNGC-SIDM I: Evolution of massive cluster mergers under the self-interacting dark matter paradigm ›
How JWST is Revolutionizing Our View of Early Galaxy Formation ›
Identity Crisis: Untangling Mass-Ordering Artifacts from Compact-Object Pairing in Gravitational-Wave Populations ›
EMRIs in Kerr Spacetime: The Role of Inclination Diffusion ›
Any colour you like: The diverse chromaticities of white dwarfs ›
The Dance of the Little Red Dots: Spectroscopy of Two Blue Companions at z = 3.9 and 5.5 Reveals Young, Metal-Poor Starbursts Merging with Their LRDs within a Few Hundred Myr ›
Wave Cold Dark Matter Can Reproduce the Radial Acceleration Relation in X-ray Elliptical Galaxies ›
The Second Catalog of Low-Energy Fermi-LAT Sources ›
Audible curvaton: modulated phase transition as the origin of large-scale curvature perturbations and gravitational wave anisotropies ›
GroArnold: A Framework for Constructing Action-based Models for Triaxial Galaxies and Dark Matter Halos ›
A Nonlinear General Implicit Runge-Kutta Integrator for Multifluid Charged Dust and Gas ›
Forecasting a Cosmological 21 cm Stacking Detection with Early HIRAX Data ›
Thermodynamically consistent equation of state tables for use in giant planet and brown dwarf interior modeling ›
Substructure-enhanced Collisional Relaxation in Stellar Systems ›
Scalar-Assisted Growth of Supermassive Black Holes: Boson-Mass Windows and Observational Constraints ›
JWST observations of 47 Tucanae: I. The low-mass main sequence down to the hydrogen-burning limit ›
The mass functions of multiple stellar populations in 47 Tucanae ›
The convective-transition gap in 47 Tucanae with JWST ›
jax-SNANA: A GPU-accelerated Supernova Framework for the SBI Era ›
Kinetic Theory of the EFTofLSS : A Halo-Based Approach ›
First L-type substellar object discovered in the vicinity of the embedded cluster NGC 2023 ›
SPICY 30021: an embedded bona fide FUor with a mid-infrared precursor ›
The connection between massive galaxies and their dark matter haloes from $z=0.25$ to $z \sim 4$ from the combined COSMOS, XMM-LSS and ECDF-S fields ›
Velocity-field estimation techniques for on-disk solar coronal bright fronts (CBFs) and shock-wave propagation ›
The Atacama Cosmology Telescope: DR6 Constraints on Isotropic Time-Dependent Cosmic Birefringence from Axion-like Particles ›
Neural networks applied to forecasting the astroclimatic and meteorological parameters in an operational context ›
MOSS III: MeerKATs view on the galaxy populations in two massive galaxy clusters ›
Science-Driven Performance Requirements for UV Coronagraph Design: Implications for O$_3$ Detection in Earth-like Atmospheres ›
Understanding the Complex Morphology of a Coronal Mass Ejection. III: How to Create a Severe Geomagnetic Storm ›
A Distinct Type of Standstill in Ultra-Compact White Dwarf Binaries ›
Are Broad Mg II Galaxies Fading AGN? ›
SQuIGGLE: Radio AGN Found Predominantly in Young, Gas-rich Post-starburst Galaxies at z ~ 0.7 ›
Emergence of high-mass stars in complex fiber networks (EMERGE) VII. Multi-Tracer Column Density Synthesis ›
Galactic Outflows and Star-Formation Quenching: A JWST Perspective ›
Studying the Near-horizon Jet of M87 using Millimeter Balloon-borne VLBI stations ›
Chandra-JWST Probing the Effects of Moderate X-Ray Superflares on Protoplanetary Disks ›
Paleo-heat flux estimates across Enceladus derived from flexural response of the ice shell ›
Tracing Accretion and Inner-Disk Gas Evolution in the Orion Nebula via Br-alpha and CO ›
The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b ›
Twisted Pseudodisk and Asymmetric Mass Accretion on the Circumstellar Disk II: Parameter Survey ›
The Contribution of Mergers and Accretion to Dark Matter Halo Assembly: An Excursion Set Theory Approach ›
Transients and Stellar Activity as Revealed by Ultraviolet Diagnostic Tracers ›
Deep X-ray View of a Distant Protocluster Anchored by a Quasar at $z=6.63$: No Evidence for Enhanced X-ray AGN Activity ›
A JWST View of Cosmic Star Formation from $z\sim0$ to 9 with Hydrogen Recombination Lines in the COSMOS and GOODS-N fields ›
Hot Molecular Hydrogen in Galaxies at Redshift ~ 0.2-1.5 Revealed by JWST ›
Large-scale Environmental Dependence of AGN Activity Revealed by JWST Pa$\alpha$ Emitters ›
ExoEcho: Exoplanet Ephemerides Change Observations. III. A JWST Survey for Transit Timing Variations of 37 Exoplanets ›
Search for Sub-Solar Mass Binaries in the First and Second Part of LIGO's Fourth Observing Run O4a-O4b ›
Magnetic Reconnection Governs the Entire Lifecycle of Solar Eruptive Magnetic Flux Rope ›
Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity ›
Simulations of Dust Content and Attenuation in $z=5-15$ Galaxies ›
Optimal Design of Shaped Pupil Lyot Coronagraph for China's Large Segmented Telescope ›
Barflow: Modeling Gas Kinematics of Bar-Driven Flows ›
A possible evolutionary connection between high-mass X-ray binary pulsars and isolated rotation-powered pulsars ›
Cosmology with strong gravitational lenses ›
Development and characterization of a millimeter-wave circular polarization observation method using a quarter-wave plate with Simons Array ›
Correlation of galactic very-high-energy gamma-ray sources detected by LHAASO with high-energy neutrinos ›
Post-merger rotational evolution of magnetised single hot subdwarfs results in slow rotation due to magnetic braking ›
Constraint on particle mass of dark matter based on XTE J1814-338 observation and DANS model ›
Microcaustics: Fast GPU-Accelerated Dynamical Microlensing of Time-Dependent Extended Sources ›
Evidence for Suppressed Non-thermal Broadening in a Flare Ribbon from Stereoscopic Observations ›
High-Frequency Transverse Waves in Chromospheric Fibrils Revealed by DKIST ›
Identifying Planetary Nebulae Candidates from IPHAS and VPHAS+ Surveys via YOLO Deep Learning Models ›
Large dust grains escaping from a supernova remnant ›
Strong gravitational lensing with Euclid ›
A heterogeneous set of unusual quasars selected from astrometry and broad-band photometry ›
specwizard: A Public Python Framework for Creating Synthetic Absorption Spectra from Hydrodynamical Simulations ›
LiDO: The Large inclination Distant Objects Survey ›
Linear Polarization of Synchrotron Radiation from Very-small-pitch-angle Electrons ›
Black Hole Binary Mergers in Galactic Nuclei: Combined Effects of Secular Dynamics and Stellar Flybys ›
PDRs4All XXIII. JWST-MIRI template spectra of PAHs in the Orion Bar obtained with blind signal separation ›
Low-cost neural summaries for cosmological inference: an ensemble of convolutional neural networks trained on approximate simulations ›
On-sky performance and prospects of near-infrared CMOS detectors in exoplanet detection: first year of SPIRIT ›
RPCA: a Resolved PSF reconstruction method for undersampled images ›
Sleeping or Dead? Probing the Quenching Mechanism of JWST Dormant Galaxies at z > 3 with ALMA ›
The Role of Environment in Shaping the Assembly Timelines of Massive Quiescent Galaxies at Cosmic Noon ›
The physical and chemical structure of TMC-1. The spatial distribution and excitation conditions of carbon, oxygen, and sulfur bearing species: Depletion of CO and CS ›
Galactic Morpholography: Linking present-day galaxy compactness to assembly history and relic formation in the COLIBRE simulations ›
Nova shells in 3D: I. A catalog of integral field spectroscopic observations ›
Testing Departures from the $\Lambda$CDM model in f(T) Gravity with DESI DR2 ›
Stationary Resistive MHD Solutions Near an Isolated Three-Dimensional Magnetic Null ›
Tracking a solar energetic eruption and associated energetic particles from Sun to spacecraft ›
Flares and flux ropes: an entangled story ›
HD 152384: A 5 Myr old debris disk system showing a gaseous ring of refractory elements at the dust sublimation radius ›
Optical constraints on intranight variability in TeV HBLs from a two-year Asiago Schmidt monitoring campaign ›
Uncovering the origin of complex velocity distributions in edge-on disc galaxies ›
R&D activity in INAF on light instrumentation for continuous optical turbulence monitoring ›
Search for High-Energy Neutrinos from Infrared Flares ›
Galaxy-to-galaxy stochasticity has a limited impact on reionization and the 21-cm signal at fixed mean emissivity ›
Revisiting the Optical F-corona from the Artemis II Total Solar Eclipse with RAW Data: How Far Can Consumer JPEG Images Be Trusted for Astronomical Photometry? ›
Exact map-space beam convolution via spin-mapmaking ›
Constrain the Size of Broad Line Region in NGC 1068 Using Sub-millimeter Excess ›
HD 120678: a classical Be star with a tilting heartbeat disk ›
The ringing Large Magellanic Cloud: evidence for a recent dwarf-dwarf collision ›
Geometrical and Optical Design of the GUEST Laser-Ranged Test Masses for the Detection of Gravitational Waves in the $\mu$Hz range ›
Thermalization of the Primordial Stochastic Gravitational-Wave Background ›
IRAC-Excess Galaxies in the NIRSpec Wide Survey: physical properties of bright EELGs at $z\sim7$ and implications for Reionization ›
Bouncing Bianchi Type I Universes with Interacting Vacuum ›
Origin of the red spectral tilt in Inflation without an Inflaton ›
Probing Planet Formation within 10 au: Dust Substructures in Extremely Compact Protoplanetary Disks ›
Rotochemical heating of neutron stars in 2D ›
Updates to STIS NUV Dark Calibration ›
Joint Line Intensity Recovery from Multi-Tracer Cross-Correlations ›
The contact frontier in Galactic civilization networks: radial structure and the Galactic habitable zone ›
LHAASO Constraints on New-Source Cosmic Rays:Abundance Scenarios and Injection Spectral Indices ›
A Parsec-Scale Transient High-Frequency-Peaked Radio Source in the Very Large Array Sky Survey Brightening and Fading over a Decadal Timescale ›
A Step-Like Transition Underlying the Life and Death of Galaxies ›
Modelling the 6.7 GHz Methanol Flaring in G358.93-0.03 Using the Maxwell-Bloch Framework ›
Can bosenovae deplete the galactic dark matter? ›
Revealing the Spatial Distribution of Dust and Plasma Solitary Waves in Jupiter's Innermost Magnetosphere Using Juno Waves Observations ›
Dynamics of a switchback-like magnetic deflection induced by a propagating coronal jet ›
Refurbishment and Cryocooler Upgrade of the CPAPIR Wide-Field Near-Infrared Camera: Design, Integration, and Lessons Learned ›
Binary-lens amplification of starlight: from magnification flares to quasi-periodic tracking of orbital evolution ›
GRB 181201A: Spectropolarimetric Constraints on Prompt Emission and Magnetic Field Structure ›
International Astrophysical Consortium for High-energy Calibration: Summary of the 18th IACHEC Workshop ›
Nonlinear Perturbations of Relativistic Stars ›
Spinformation: do gravitational-wave events carry information beyond effective spins? ›
Strong-Field Gravitational-Wave Lensing from Ray-Traced Arrival-Time Surfaces ›
Black Hole Fine Structure ›
The WDM time-frequency transform in gravitational-wave data analysis II: Evolutionary spectrum and noise covariance ›
Magnetically Charged Black Holes from Grand Unified Theory ›
Radion/Dilaton portal freeze-in dark matter in extra-dimensional theories ›
Quantum noise and torque correlations in a torsion-bar Sagnac speed meter ›
Testing Charged Black Holes Embedded in Anisotropic Matter and Surrounded by Plasma through Gravitational Lensing: Bounds from the Sloan Lens ACS Survey ›
All Quiet on the Vector Front: Scalar Growth and Perturbative Control in Horndeski--Weyl-squared Gravity ›
Correlation between gravitational wave frequencies as a signature of new black hole physics ›
Biases in Ringdown Tests of General Relativity from Gravitational-Wave Microlensing ›
$^{16}$O(p,$\gamma$)$^{17}$F Reaction and the C and O Isotopic Ratios in Red Giant Branch Stars ›
Transient PULSE: Code for the Transient Propagation of UltraLight (pseudo)Scalars to Earth ›
Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking for the MagLim++ lens sample ›
Evidence of galaxy cluster rotation and intrahalo gas motions in the cosmic microwave background ›
A Very Rich Bimodal Galaxy Cluster Merger: RXC J0032.1+1808 ›
Validation of Satellite Lifetime Predictions at Leonid Space ›
The stellar-to-halo mass relation of central galaxies across three orders of halo mass ›
CHRONOS Science Program ›
Probing the magnetic field of a coronal mass ejection with PSR J1022+1001 ›
Identifying heating processes in simulations with an entropy-based scheme: A single jet episode in a galaxy cluster ›
Delayed Radio Flares in Neutrino-associated Blazars: The Case of TXS 0506+056 ›
Probing scalar-tensor-induced gravitational waves in the nHz band: NANOGrav and SKA ›
The DESIRED strong-line calibrations: I. New empirical metallicity relations for the local and high-redshift universe ›
Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO ›
Astrophysical Parameters of 5056 Open Star Clusters from Bayesian Nested Sampling with PARSEC Isochrones ›
Cosmo-PINN: A Physics-Informed Neural Network for Cosmological Reconstruction ›
Time-reversed stochastic inflation in the quantum well ›
Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability ›
WaveDM.jl: An Adaptable Simulation Framework for Dynamics of Baryonic and Wave Dark Matter on Galaxy Scales ›
Testing the prevalence of hydrogen-silicate miscibility in young sub-Neptunes ›
Investigation and Mitigation of a Prominent Off-Axis Stray Light Path in Rubin Observatory Commissioning ›
Enhanced Astrometry of the Rapid ASKAP Continuum Survey: Mid and High Frequency Epochs ›
Volcanic Satellites and Ion Escape in the Magnetospheres of Ultra-Cool and Brown Dwarf Stars ›
Physical Characterization of Moon Impactor 2025-010D ›
Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares ›
Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array ›
pynucastro 3: A community library for nuclear astrophysics ›
Continuum Variability in AGN: Evidence for Systematically Suppressed Fluctuations in the BAL Population ›
Modelling Fourier filtering wavefront sensors for PSD-based methods: the AOPERA tool ›
Field-Level Baryon Acoustic Oscillation Reconstruction of the DESI DR1 Luminous Red Galaxies with Linear Field Transformer (LiFT) ›
The Study of Detailed Morphology of Milky Way Dwarf Galaxies: Draco and Bo\"otes I ›
Evolving dark energy and a younger Universe from cosmic inhomogeneity ›
A forest of emission lines observed by Sunrise III/SUSI above the solar limb ›
Vector field dark matter search with Sagnac interferometer ›
Rotational excitation of SiC$_6$ by collisions with helium: cross sections, rate coefficients and non-LTE modeling ›
Axial-Dipole and Equatorial-Dipole Coronal Holes: Congruent Magnetic Geometry, Divergent Evolution ›
How much can shape degeneracies affect the Hubble constant measurement? ›
Scaling Up: A Global Optical/X-ray Correlation For Reprocessing Across Black Hole Masses ›
3D Global Climate Simulations of Synthetic Mars Warming ›
Searching for Ultra-Light Axions with Twisted Cavity Resonators of Anyon Rotational Symmetry with Bulk Modes of Non-Zero Helicity ›
Cosmic Rays as an Interdisciplinary Earth Observation Tool: From Particle Physics and Atmospheric Processes to Geosciences and Urban Science ›
Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment ›
Collider Probes of Dark Energy Microphysics ›
Axion Misalignment Across First-Order Phase Transitions ›
Quantum Field Theory Of Cosmological Perturbations Induced By Ultralight Dark Matter ↓↑