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 north-east

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S Sky
Temperature
12.0 °C
Humidity
59%
Wind
3.2 km/h
Pressure
1014.6 hPa

Moon
Latest preprints on astro-ph:
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Supermassive Black Hole Winds in X-rays -- SUBWAYS. VI. Interplay between the soft X-ray excess and ultra-fast outflows ›
On the Nature of the BeWD System Nova FQ Circinus ›
Inferring the shapes of low-mass galaxies at $z>6$ from FIREbox$^{HR}$. Where are the disks? ›
Euclid Bypass end-to-end simulations for spectroscopic galaxy clustering performance assessment ›
PSR~B0355+54: An Unexpected Compendium of Nearly All Scintillation Arc Morphologies ›
Gamma-ray Bursts as Cosmological Probes Calibrated with Strongly Lensed Quasars and Neural Networks ›
The science case for an in-situ measurement platform in the Venus clouds ›
Graph Neural Networks for Astrophysics and Cosmology ›
The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at $z\sim7$ ›
Planets surviving common envelope evolution should be rare, massive, and orbit very close to their host star ›
How does a galaxy's quenching probability depend on its black hole's mass? ›
Metal-poor molecular clouds in dwarf galaxies at parsec-scale resolution ›
Small Collisions, Big Impact: The Sensitivity of Atmospheric Temperatures to Collision-Induced Absorption ›
ASTROLABE: A 3D Particle-Level Surrogate for Cosmology Simulation with Physical Flow Matching ›
Beyond static torques: Self-consistent migration and dynamical trapping of low-mass planets in dusty disks ›
Optical and Ultraviolet Emission from the Gas Photoionized by Gaia BH3: Archival Constraints and Predictions for the 2029 Periastron ›
Balmer breaks in accreting super-massive black hole binaries ›
Localizing binary neutron stars with the Einstein Telescope: a full Bayesian comparison of the triangular and 2L configurations ›
Dual and lensed AGN at sub-arcsecond separations uncovered by ERIS ›
DDELenS: Tomographic Weak Lensing Simulations with Dynamical Dark Energy ›
The SIMPLIFI Survey: Polarization of Dense Filaments with SOFIA III. Relative orientations of antenna temperature gradients with the magnetic field in the DR21 molecular cloud ›
Leviathan: a very massive, extended sub-millimetre galaxy spectroscopically confirmed at $\rm z = 4.05$ ›
Slowly Rotating Fully Convective Stars at $\lesssim$ 1 Gyr: Evidence from the Hyades and Praesepe ›
20,000 Rotation Periods in Nearby Open Clusters and Moving Groups from ZTF and ASAS-SN ›
Twenty-five years of XMM-Newton EPIC-MOS2 Unfocused Particle Background: Solar Cycle Modulation, Galactic Cosmic-Ray Correlation, and Implications for NewAthena ›
Ammonia-Hydrogen Phase Equilibria in Planetary Envelopes from First-Principles-Based Machine-Learning Molecular Dynamics ›
Numerical shock broadening and supernova neutrino conversion: implications for DUNE ›
A MUSE Study of Stellar and Ionized-Gas Kinematics in Central Group Galaxies ›
The GLEAM 4-Jy (G4Jy) Sample: V. Broadband spectral analysis ›
The Imprint of Core-collapse Asymmetries on Supernova Shock Breakout ›
Evolution of Massive Main-Sequence Stars in Binary Population Synthesis. II. Consequences for Black Hole High-Mass X-ray Binaries and Binary Black Holes ›
Analytical Chemistry at the Planetary Frontier ›
Ionized Gas Kinematics and Star-forming Clumps in Extremely Metal-poor Galaxies ›
Are Dynamical Dark-Energy Cosmologies Old Enough? ›
Large-scale Vortices in the Solar Photosphere: Statistical Properties and the Reliability of Local Correlation Tracking ›
Searching for Dense Perturbers in Cold Dark Matter Simulations ›
AI and The Enclosure of the Scientific Commons ›
J-PLUS: Identifying Outlier Spectral Energy Distributions in the Fourth Data Release Using Unsupervised Machine Learning ›
The Future of Gamma-Ray Bursts as Probes of the Epoch of Reionization in the Era of JWST and the Extremely Large Telescope ›
The presence and order of QCD phase transitions from gravitational-wave observations of neutron star mergers ›
Globular Clusters GMRT Pulsar Survey (GCGPS) III: ORION - a multi-beam acceleration search pipeline ›
Source velocities of fast radio bursts constrained by their dispersion measure variations ›
SN 2023iop: An Extreme 1987A-like Supernova and the Death of Very Massive Stars ›
Core-Collapse Supernova Rates in the Dark Energy Survey ›
Size, Albedo, and Taxonomy of Asteroid (1201) Strenua from Stellar Occultation and ATLAS Photometry ›
Exomoonlight Sonata: On the Fate of Exomoons Around Migrating White Dwarf Planets ›
Constraining the FRB Central Engine from Flux Variations of Persistent Radio Sources: FRB 20240114A as the First Attempt ›
A $\wedge$-like metallicity profile in the disk of the Sagittarius dwarf galaxy ›
A Radiation-Hardened, Fault-Aware Quantized Neural Network That Self-Heals ›
Probing Nearby Electron Sources and Local Diffusion with the TeV All-Electron Spectrum ›
Short-timescale X-ray variability of the blazar 1ES 1959+650 observed with AstroSat/SXT ›
Gaussian process-based Bayesian imaging of bolometric (sub-)millimetre data ›
Estimator Precision and Selection for Up-the-Ramp Sampling with a High-Read-Noise InGaAs Camera ›
An improved self-gravity treatment in general relativistic smoothed particle hydrodynamics ›
Cosmic-ray melt windows in interstellar ice make a four-carbon ketose but not the sugar pattern of G+0.693-0.027 ›
When the core ate the atmosphere ›
Probing the Optical/UV Continuum Variability of Active Galactic Nuclei with the Damped Random Walk Model ›
What Shapes the Ultraviolet Spectra of Type Ia Supernovae? ›
The chemical evolution of the LMC from APOGEE abundances: a hybrid two-infall OMEGA+ analysis ›
Single-Parameter Exponential Model Outperforms Standard Dark Matter and Modified Newtonian Frameworks in Predicting Galactic Rotation Curves ›
A bright X-ray flaring event from the intermediate supergiant fast X-ray transient IGR J00370+6122 observed with NuSTAR ›
The environments of type Ibn supernovae: evidence for a strong Wolf-Rayet star component ›
Probing Minihalos in the Late Dark Ages through Velocity Acoustic Oscillations in the 21-cm Power Spectrum ›
Constraining Solid HNCO and Its Environment in Open JWST Data with Laboratory Spectra ›
VVV CL001: A strong candidate for the most ancient star cluster in the Galaxy ›
Understanding the formation of alpha-Fe bimodality in the Milky Way using constrained cosmological simulations of the Local Group ›
Phakoseismology: Asteroseismology of gravitationally microlensed stars ›
An improvement to the spatial discretisation in the Astrophysical Weighted Particle Hydrodynamics method ›
Kinematically isolating intracluster light in AS1063: a distinct stellar population tracing the dark matter core ›
Rapid Variability of Radiative Signatures from Driven Relativistic Reconnection ›
On the superbursts as photodisintegrators of ashes from the rp-process -- Numerical simulations of superbursts with MESA II ›
Constraints on Dark Matter Annihilation from Starlight-Induced Inverse Compton Emission in Omega Centauri ›
Pulsar J1909+0749 and Supernova Remnant G42.1-0.2: A case of a pulsar that has exited the shell of its associated supernova remnant ›
The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres ›
Deriving Interplanetary Sector Boundary Crossings using Potential Field Source Surface Modeling ›
Detection and Statistics of large-scale Sector Boundary Crossings in the Solar Wind: The SBCross Catalog ›
Hidden engines in tidal disruption events: multimessenger signatures in a lepto-hadronic framework ›
Orbital Parameters for 65 Wide Binary Systems: no evidence for gravitational anomaly at low acceleration ›
The Effect of Field Line Tracing Height on Wang-Sheeley-Arge Solar Wind Predictions at Earth ›
Real-Time 24-hour Ahead Forecasting of Solar Energetic Particle Events with SEPNET-PRISM-R ›
Coevolution of Dust Growth and Gravitational Instability in Massive Protostellar Disks ›
Data-Driven Ages from Asteroseismology for FGK Dwarfs ›
Revisiting the Unknown Unknowns in Transient Astrophysics with the SKA Telescopes ›
Photometric variability of blue supergiants: Constraints on stellar masses and evolutionary stages ›
KMOS Spectroscopic Follow-up of 16 Star Cluster Candidates of the Sagittarius Dwarf Galaxy ›
Identifying a jet-shaped point-symmetric morphology in the supernova remnant HB9 ›
Tight asteroseismic upper limits on hot subdwarf magnetism ›
The "Rubin 2036: Opportunities for Discovery" Workshop: A Community Roadmap for the Future of the Vera C. Rubin Observatory After the LSST ›
A Solar Optical Clock ›
Resonant three-mode coupling in asteroseismology I: Bifurcations, chaos, and DAV white-dwarf outbursts ›
The clumpy fraction of galaxies at $z=1-9$ with JADES: evidence for a mass-dependent transition in clump origin ›
Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields ›
TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance ›
A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274) ›
Large fluctuations and cusp-core transformation in dwarf galaxies ›
Resolving the extended interstellar medium of infrared galaxies II. Fine-structure line emission ›
Resolving the extended interstellar medium of infrared galaxies I. Polycyclic aromatic hydrocarbon emission ›
Automated optimization of solar energetic particle acceleration and transport parameters against five-spacecraft observations of the 9 October 2021 event ›
Community Lessons from builders of infrared multi-object spectrographs ›
Slow-Roll Inflation at Arbitrary Order ›
Dynamical stability of Magnetic Supramassive Neutron Stars ›
Constraints on Millimeter-wave Extragalactic Transient Populations from 4 Years of SPT-3G data ›
Search for Compact Binary Coalescences with Sub-solar Mass Components in Data from the Second Part of LIGO-Virgo-KAGRA's Fourth Observing Run ›
Adaptive Model-Switch Thermodynamic Integration: A Bayes Factor Estimator ›
Ion Heating in Pair-loaded Relativistic Turbulence ›
Floquet Instability of Photon-Axion Conversion ›
Elementary-Symmetric Ricci Gravity: Metric Formulation ›
Annihilation feedback on elastic scattering in self-interacting dark matter ›
A Natural Dark Matter-Dark Energy Interaction from Axion-Monopole Dynamics ›
Deglobalising the fit: how to search for physics beyond vacuum General Relativity in LISA catalogues ›
Cosmic birefringence from a stiff axion field and its cosmological implications ›
Modular Bayesian Inference for Partially Misspecified Mixtures with Uncertain Class Labels ›
Self-interacting dark matter from radiative bound-state-formation feedback ›
Illuminating Light Dark Matter with Fixed-Target Experiments ›
A Multipole Technique for the Simulation and Analysis of Gravitational Waveforms from Extreme Mass Ratio Inspirals ›
High-cadence GW astrometry in the $\mu$Hz gap ›
P-ONE-1: the first detector line of the Pacific Ocean Neutrino Experiment ›
Stability Analysis of Axion Dark Energy Model ›
Untangling Extreme Mass Ratio Inspirals and Massive Black Hole Binaries in LISA Data ›
Axion detection in the non-Markovian noise ›
Two-Component Dark Matter and Strongly First-Order Electroweak Phase Transition via a Two-Step Mechanism in the Inert Doublet plus Real Singlet Model ›
Direct Urca process facilitated by non-Fermi-liquid quantum criticality ›
On the Stability of Tolman Oppenheimer Volkoff Fireholes ›
Hybrid Stars with Different Amount of Quark Matter ›
Exponential Growth of Turbulent Cross Helicity in Shear-Flow-Driven Turbulence ›
MadStree: automated evaluation of tree-level de Sitter correlators ›
Lagrangian perturbation theory for modified gravity ›
Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory ›
Unveiling dark forces with measurements of the Large Scale Structure of the Universe ›
Causality and perturbative-QCD constraints on first-order phase transitions in neutron stars ›
Kratos-polrad: Novel GPU system for Monte-Carlo simulations with consistent polarization calculations ›
MAMMOTH-LyC: Investigating the Role of Galaxy Mergers in a Strong Lyman Continuum Leaker at $z=2.39$ ›
Formation and Evolution of [Wolf-Rayet] Planetary Nebulae through a Late Thermal Pulse ›
An empirical derivation of the average dust attenuation law at 2 ›
Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study ›
The Life and Death of Stars That Capture Primordial Black Holes ›
The Effect of Adiabatic Index on Radius Evolution and the Mass Loss ›
A New Scaling of Neutron Star Tidal Deformability for Directly Probing the Central Equation of State Parameter ›
Search for Diffuse Supernova Neutrino Background in the Full KamLAND Dataset with Neural-Network-Based Event Classification ›
Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors ›
Infrasound Newtonian Noise Estimation at the Einstein Telescope Candidate Site Sos Enattos ›
Observational Evidence for Anisotropic Metal Excess around Galaxies ›
VAPOLA - A multiyear, multiband polarization survey of AGNs and Sgr A* at millimeter wavelengths with ALMA II. Spectropolarimetric properties and their evolution from 2017 to 2023 ›
Periodic activity on the (sub)mm surface of the AGB star Mira A ›
Wide Field Localization Using Fixed Modulation Collimators ›
Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey ›
Solar spicule population properties inferred from IRIS Mg II k off-limb spectra using likelihood-free Bayesian inference ›
Galaxy Protoclusters as Drivers of Cosmic Reionization: II. Te-Based Metallicities of Lyman-{\alpha} Emitters ›
Collisional excitation of SiC$_6$ by helium: cross sections, rate coefficients, and astrophysical implications ›
A faint dust ring beyond the compact disk of Sz 76 ›
Structure and evolution of cosmic voids within DESI DR1 ›
Optical constraints on intranight variability in TeV HBLs from a two-year Asiago Schmidt monitoring campaign ›
Consistently Reproducing Early Galaxy Observations and 21-cm Signal during the Epoch of Reionization ›
Beyond the Disc--Spheroid Dichotomy at $0.6 < z < 8.0$: Evidence for a Morphological Indeterminacy Regime from JWST ›
The DARWIN Project: Cosmological Simulations of Galaxy Formation down to Dwarf Scales in Diverse Environments ›
The Central Molecular Zone of our Galaxy, a chemical complexity factory: first interstellar detections of molecules towards G+0.693 ›
New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis ›
Inflationary Particle Production and the Swampland ›
Probing freeze-in dark matter using Bose-Einstein condensate in neutron star ›
Energy extraction from NED-deformed rotating black holes via the Comisso-Asenjo reconnection process ›
Detecting Tidal Resonances in Binary Neutron Stars ›
A dark-matter-sensitive orientation clock near rotating black holes ›
Resonant lunar tides of Earth's core and basal magma ocean ›
Gravitational-wave responses and noise correlations in geometric time-delay interferometry ›
Exact 1D Nonlinear Solutions for Proton-Driven Plasma Wakefields ›
Entropic Chaplygin-Gas cosmology and late-universe tension diagnostics ›
Penrose process in radiating Kerr-Vaidya black holes: efficiency, energy transport, and the viability boundary ↓↑