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

over the clouds

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S Sky
Temperature
-0.8 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1010.5 hPa

Moon
Latest preprints on astro-ph:
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Distinguishing life from non-life via molecular frontier orbital energy gaps ›
Experimental and numerical modeling of liposome congregation in meteorite craters of Early Earth ›
Periodic Wobble of the Post-Perihelion Jet Structure Around 3I/ATLAS ›
Simultaneous Double Transits of Phobos and Deimos as Seen from the Martian Surface: A Millennium Catalogue ›
The Chemical Homogeneity of Single-Lined Spectroscopic Binaries in Open Clusters ›
POSEIDON I: The Dynamical Origins of Transiting Neptunes ›
Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors ›
Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z=7, up to z= 14 ›
The ionised interstellar medium of DSFGs revealed by JWST/NIRSpec and ALMA: Super-solar metallicity, low ionisation parameters and, typical electron densities ›
Inferring the population properties of galactic binaries from LISA's stochastic foreground ›
A dedicated survey of fast-rotating near-Earth asteroids with the Two-meter Twin Telescope. I. Observational strategy and first results ›
Abundance Calculations of Neon Isotopes in the Predicted Lifetime of the Sun ›
The impact of electron precipitation on Earth's thermospheric NO production and the drag of LEO satellites ›
The 2021 Hot-type Symbiotic Outburst of YY Herculis: An Optical Follow-up Study ›
Magnetic structure of coronal dark halos ›
The Impact of Degraded Charge Transfer Efficiency on Extended Sources in ACS/WFC ›
One Halo, Two Boundaries: Relating Accretion Shocks and Splashback Radii in Galaxy Clusters ›
The Physics of Solar Energetic Particles ›
Solar cycle irregularity study ›
Accretion disks in (repeating) partial tidal disruption events: rapid state transitions, UV plateaus and flares from disk-remnant collisions ›
Fast reconnection in a coronal torn plasma sheet ›
Assessing Zeeman Measurements of Magnetic Fields in Synthetic HI Observations ›
Massive Black Hole formation in proto-stellar clusters via early gas accretion ›
Diverse properties of electron Forbush decreases revealed by the Dark Matter Particle Explorer ›
Variable Red Giants Exploration with MASTER Robotic Net: Main Algorithms and Study of Three Mira-type Targets ›
Cosmological constraints from a joint DESI DR1 Full-Shape and DR2 BAO ›
Discovery of burst oscillations in the newly discovered millisecond X-ray pulsar SRGA J144459.2$-$604207 ›
The Martian mid-latitude subsurface ice is the remnant of a past ice sheet ›
Exploring the Universe Expansion History with f(R,T) Gravity: Constraints on Cosmological Parameters ›
Characterization of Residual Morphological Substructure Using Supervised and Unsupervised Deep Learning ›
Variational views for self-supervised learning in radio astronomy ›
The ngVLA Band-4 Water Vapor Radiometry Concept ›
Tempawral: A Time-Resolved Retrieval Framework for Variable Brown Dwarfs and Exoplanets ›
SN 2017hcc and SN 2023usc a comparative spectroscopic study of type IIn supernovae ›
Evidence of Nuclear Urca Process in the Ocean of Neutron-Star Superburst MAXI J1752$-$457 ›
Evidence for Log-Periodic Modulation in High-Redshift Compact Object Abundance Consistent with Cyclic Condensate Collapse ›
The Optical Properties of Host Galaxies of Radio Sources in the Coma Cluster ›
Gravitational Baryogenesis in $f(R)$ Cosmologies ›
Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy ›
Astrometric properties of reference frame sources as a function of redshift ›
Magnetic-field Order in the Southwestern Rim of RCW 86 Constrained Using X-Ray Polarimetry ›
The Apparent Asymmetric Outflows of TeV Particles from Pulsar Winds ›
Potential periodic signals in blazars: significance, forecasting and deep learning ›
Feedback shaped the galaxy morphological sequence in presence of mergers ›
Safety Acquisitions: Redundancy for non-repeatable multi-orbit STIS visits ›
Parameter Estimation Limits in Blazars ›
Probing the maximum energy of fast radio bursts using thousands of sources from the Second CHIME/FRB Catalog ›
Certified Uncertainty for Surrogate Models of Neutron Star Equations of State via Mondrian Conformal Prediction ›
Photometry of Fireballs using High Frame Rate Cameras ›
BayeSED-GALAXIES II. Bayesian full spectrum analysis of galaxies and application in the CSST wide-field slitless spectroscopy survey ›
Long Photometric Cycles in Double Periodic Variables from Nodal Precession of a Tilted Accretion Disk ›
Surface Properties, Orbital Dynamics, and Thermophysical Modeling of the Primitive Asteroid (269) Justitia ›
The Hydrostatic Mass Bias and the $\sigma_8$ Tension: A Multi-Probe Forecast for Stage-IV/V Surveys ›
SMMAN: quasi-Simultaneous Multi-wavelength Monitoring of gamma-ray-loud AGNs with the Nanshan 26-m radio telescope ›
A Realistic Pulsar - Supermassive Black Hole Timing Model ›
Probing dark matter distributions with the pericentre precession of the stellar orbits near the Galactic Centre black hole ›
A unified study of nuclear physics and dark matter constraints through gravitational-wave observations of binary neutron star mergers ›
MEDUSA I. Tracing magnetic field structures in tidal arms of the dwarf-dwarf merger NGC 1487 ›
Searching for and characterizing halo substructures with the GALAH DR4 survey ›
Weak S-type asteroids compared to C-type explain the observed size distribution of the main belt ›
Exo Skryer: A JAX-accelerated sub-stellar atmospheric retrieval framework ›
Influence of Cross-sectional Expansion on Coronal Emissions from a Radiatively Cooling Solar Flare Loop ›
Chemodynamical properties of gas-rich galaxies: a comparison of observations and simulations ›
MIGHTEE: Discovery of a triple-double radio galaxy ›
The morphological stability of open clusters: a new 2D perspective ›
Young system development in a cometary globule: An investigation into the eccentric disk around AT Pyx in terms of planet-formation and interaction with its surrounding environment ›
Direct comparison of SiPMs and PMTs in operation with a bright background and prospects of using SPADs as truly digital sensors ›
Primordial Black Hole Formation in Rastall Gravity: Shifted Collapse Threshold and Exponential Abundance Sensitivity ›
Observational Evidence Linking Loop Length and Thermal-Nonthermal Peak Timing in Solar Flares ›
Apophis source population and Earth encounter frequency of Apophis-like bodies ›
Probing the Milky Way Halo with RR Lyrae Stars from Gaia Data Release 3 ›
A Bayesian Method for Air-Shower Reconstruction using Information Field Theory ›
Winds of Change: XRISM Resolve X-ray spectroscopy of NGC 4051 ›
Investigating polarization signatures from GRB models ›
Optical observations of the fast nova V1674 Herculis ›
Probing Dust in the MWC 480 Disk from Millimeter to Centimeter Wavelengths ›
Energy and mass transport associated with impulsive spicular flows in solar coronal holes ›
Multivariate time-series forecasting of ASTRI-Horn monitoring data: A Normal Behavior Model ›
LRG-BEASTS: Detection of sodium and evidence for water absorption in the hot Saturn HAT-P-44b ›
Bar Formation During a Gaia-Sausage-Enceladus-like Merger Event ›
Simulation of proton radiolysis of H2O and O2 ices with the Nautilus code ›
The major merger-active galactic nucleus connection up to the cosmic noon ›
The Orbital Eccentricity--Radius Distribution for Warm, Single Planets in TESS ›
Cosmic strings and domain walls: the impact of CMB $B$-mode data ›
21,864 Unresolved, Low-mass Binaries Identified via their Overluminosity in \textit{Gaia} DR3 and a Catalog of 347,440 Systems within 100 pc of the Sun ›
HelioSpectrotron 5000: An Interactive Multi-Resolution Solar Spectral Atlas ›
The Universal Eccentricity Distribution for Dynamical Gravitational-Wave Merger Channels ›
IceCube's convex all-sky neutrino spectrum consistent with the magnetically powered corona scenario for active galactic nuclei ›
Topography-Induced Stationary Waves and the Onset of Nightside Warming on Rocky Planets around M-dwarf Stars ›
Improved constraints on modified Newtonian gravity from Cassini radio tracking data ›
Dark Matter in Zwicky's Cosmology: Towards an Epistemological Reconstruction ›
Cosmological Constraints on Long-Lived Particles Using Dimension-Six Effective Operators ›
Scaling solutions for varying tension strings ›
Dark Glueball Direct Detection ›
Testing the Spacetime Geometry of Sgr A* with the Relativistic Orbit of S2 star ›
The Role of Inhomogeneities in the Turbulent Accretion of Black Holes ›
Nuclear Pasta and Crustal Quasi-Periodic Oscillations in Neutron Star ›
Improving calibration accuracy with torque coupled gravity field calibrator for sub-Hz gravitational wave observation in CHRONOS ›
Chaotic imprints of dark matter in extreme mass-ratio inspirals ›
GPU-Native Compressed Neighbor Lists with a Space-Filling-Curve Data Layout ›
Leptophilic scalar dark matter in U(1)$_{L_\mu-L_\tau}$: Evading direct detection and prospective neutron star heating ›
Addressing leakage and mode suppression in angular power spectrum estimation for gravitational-wave backgrounds using pulsar timing arrays ›
Development of a Cherenkov-Based Time-of-Flight Detector Using Silicon Photomultipliers ›
Prompt And Delayed Radio Bangs At Kilohertz By SN 1987A: A Test For Graviton-Photon Conversion ›
Inverse Compton Scattering on laser beam and monochromatic isotropic radiation ›
Leptonic originated High energy neutrinos from astrophysical objects ›
Lecture Notes in Cosmology ›
Machian Gravity: Confronting Galaxy Cluster Mass Profiles ›
Multi-energy diffuse neutrino fluxes originating from core-collapse supernovae ›
Joint Optical and Infrared Observations of N and O Reveal the Dust-Obscured Gas in Haro 3 ›
Helium features are inconsistent with the spectral evolution of the kilonova AT2017gfo ›
Why Do Stars Turn Red? I. Post-Main-Sequence Expansion Mechanism ›
Helium as an Indicator of the Neutron-Star Merger Remnant Lifetime and its Potential for Equation of State Constraints ›
Measuring the Stellar-to-Halo Mass Relation at $\sim10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses ›
From particles to precision. Simulating subsonic turbulence with Smoothed Particle Hydrodynamics ›
Resonant amplification of multimessenger emission in rotating stellar core collapse ›
Effective field theory of coupled dark energy and dark matter ›
Post-glitch Recovery and the Neutron Star Structure: The Vela Pulsar ›
Why Do Stars Turn Red? II. Steady-State Envelope Solutions ›
Chemical Signatures of Population III Stars in Damped Lyman-$\alpha$ Absorption Systems at $z \approx 6$ ›
The Low Mass Dwarf Host Galaxy of Non-Repeating FRB 20230708A ›
Non-linear Dynamics and Primordial Black Hole Formation During Kination ›
Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample ›
The NEID Earth Twin Survey. IV. Confirming an 89 d, $m\sin i=10~\mathrm{M_\oplus}$ Planet Orbiting a Nearby Sun-like Star ›
The COLIBRE project: cosmological hydrodynamical simulations of galaxy formation and evolution ›
Intrinsic alignments of galaxies in multiple projections ›
Probing Hernquist dark matter with black hole shadows: A comprehensive study of various accretions ›
The Metallicity Dependence of PAH Emission in Galaxies II: Insights from JWST/NIRCam Imaging of the Smallest Dust Grains in M101 ›
From X-rays to High-Energy Gamma-rays: A Comprehensive Multi-Wavelength Study of Early Gamma-Ray Burst Afterglows ›
Eccentric Disks With Self-Gravity ›
Beware of the running $n_s$ when producing heavy primordial black holes ›
Exploring Joint Observation of the CSST Shear and clustering of astrophysical gravitational wave source measurements ›
Constraining and Comparing the Dynamical Dark Energy and f(R) Modified Gravity Models with Cosmological Distance Measurements ›
CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA ›
Damping of dynamical friction force in self-interacting ultralight dark matter and Fornax timing problem ›
Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System ›
Modeling the Multi-Wavelength Afterglow of Short Gamma-Ray Bursts with a Plateau Phase ›
Constraining properties of dust formed in Wolf-Rayet binary WR 112 using mid-infrared and millimeter observations ›
Metal-loaded outflows in sub-Milky Way galaxies in the CIELO simulations ›
Game Theory in Cosmology ›
Constraints on the intergalactic magnetic field from Fermi-LAT observations of GRB 221009A ›
Skykatana: a scalable framework to construct sky masks for the Vera Rubin Observatory and large astronomical surveys ›
Magnetic plasmoid explosions in the context of magnetar giant flares and fast radio bursts ›
Exploring the formation mechanisms of tidal structures in globular clusters of extragalactic origin ›
Fading into darkness: A weak mass ejection and low-efficiency fallback accompanying black hole formation in M31-2014-DS1 ›
Dust Properties of the Interstellar Object 3I/ATLAS Revealed by Optical and Near-Infrared Polarimetry ›
BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion ›
The Characteristic Mass and Energy Conversion Efficiency in the Cusp-Core Transition of Dark Matter Haloes: Implications for Scaling Relations and Supernova feedbacks ›
Thermal emission spectra of the ultra-hot Jupiter WASP-33 b ›
Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework ›
Status of the $S_8$ Tension: A 2026 Review of Probe Discrepancies ›
Precursors in tidal disruption events: repeating, fast, and AGN-hosted TDEs ›
Infrared spectra of methane-containing ice mixtures for JWST data analyses ›
The Montreal Open Clusters and Associations (MOCA) Database: A Census of Nearby Associations, Open Clusters, and Young Substellar Objects within 500 pc of the Sun ›
Little Red Dots as Globular Clusters in Formation ›
Investigating Nonlinear Quenching Effects on Polar Field Buildup in the Sun Using Physics-Informed Neural Networks ›
Gravitational Wave-Induced Freeze-In of Fermionic Dark Matter ›
Krylov complexity of thermal state in early universe ›
The Numerics of VMEC++ ›
Stamps of state on structure: Probing the state of ultralight dark matter via its density fluctuations ›
An Open System Approach to Gravity ›
From $U(1) \times U(1)$ Symmetry Breaking to Majoron Cosmology: Insights from NANOGrav 15-year Data ›
Distinguishing gravity theories with networks of space-based gravitational-wave detectors ›
Probing scalar field with generic extreme mass-ratio inspirals around Kerr black holes ›
(Non-)Perturbative Dynamics of a Light QCD Axion: Dark Matter and the Strong CP Problem ›
A User-Friendly Python Interface for the Numerical Relativity Code AMSS-NCKU ›
The Stochastic Schwinger Effect ›
Constraining a de Broglie--Bohm quantum bounce cosmology with Planck data ›
Optical design and sensitivity optimization of Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS) ›
On flying near the base of a pseudo-streamer ›
Ghost-free non-local $F(R)$ Gravity Compatible with ACT ›
Neutrino production mechanisms in strongly magnetized quark matter: Current status and open questions ›
When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity ›
The measurable impact of the 2pN spin-dependent accelerations on the jet precession of M87$^\ast$ ›
Characterization of an MPPC-Based Scintillator Telescope and Measurement of Cosmic Muon Angular Distribution ↓↑