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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Latest preprints on astro-ph:
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Bayesian Inferences on Analytical Equations of State Approximations of Neutron Stars ›
$\Lambda$CDM in a courtroom ›
Inhomogeneous Cloud Coverage and Altitude-Dependent Heat Transport on the Hot-Jupiter NGTS-10 Ab from its Optical-to-Infrared Phase Curve ›
A Dark-matter Origin of Little Red Dots: Early Seeding and Super-Bondi Accretion ›
On the dynamical accessibility of twin stars ›
CMB-HD Foregrounds: Simulations, Source Detection, and Foreground Removal ›
Population III Host Candidates at $z\sim2$: Strong He II $\lambda1640$ and Absent UV Metal Lines in HETDEX Ly$\alpha$ Emitters ›
A pair of unequal jets imparted the kick velocity to the neutron star of Cassiopeia A ›
Dynamic Accretion Disk-Corona Connection and Broad Fe K$\alpha$ Variability in Mrk 766 Revealed by Time-Resolved High Resolution X-Ray Spectroscopic Analysis ›
Jet Feedback and the Self-Regulated Growth of Black Holes Embedded in AGN Disks ›
Optical Spectroscopy of a Candidate O-Star X-ray Binary in M33 ›
The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location ›
Forged in Quenching: Morphological Transformation across Star-forming and Quiescent Galaxies in EAGLE ›
JWST Observations of Starbursts: A Young Bubble in NGC 253's Central Starburst ›
Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions ›
Rescuing Kepler's False Positives: A Possible Habitable Zone Exoplanet in the Triple Star System KOI-1623 ›
Filament Formation via Collision-induced Magnetic Reconnection -- Kinematic Features ›
Gravitational Wave Bias in IllustrisTNG300 from Machine-Learned Population-Synthesis Calibrated Merger Rates ›
What the Solar System Can Teach Us About Rocky Exoplanets ›
Cosmic Noon Galaxies in the Hubble Ultra Deep Field with MIRI Wide-Field Slitless Spectroscopy ›
Formation of Merging Black Hole Binaries Inside Massive AGN Stars ›
The Post-Outburst Spectrum of L1415-IRS ›
Neutron Star Merger Universality Relations for a Quark--Hadron Crossover Equation of State ›
Disentangling Stellar Mass and Environmental Effects on eROSITA AGN Activity using multi-wavelength data from GAMA, WISE, GALEX, and DESI Legacy Survey ›
Determination of the Angular Distributions of Dynamical and Emission Parameters of GRB Relativistic Outflows ›
Using Gravity as an Age Indicator for Young Stars ›
NOCTURNE. II. Extreme radio variability in the heart of early-stage active galactic nuclei ›
Properties of the circumstellar matter around the pair-instability supernova candidate SN 2018ibb revealed by its light curve ›
Optomechanical design of an ADC and image rotator for the HJST Coud\'e Spectrograph at McDonald Observatory ›
Commissioning the AIP's ultrafast laser Inscription facility: defining the parameter space for type-I waveguide fabrication ›
SAMI and TNG-Cluster: tracing galaxy spin and environmental transformation across cluster phase-space and cosmic time ›
CNN-Based Inference of Gaseous Halo Properties from Synthetic X-ray and 21-cm HI Observations ›
RAMA: A new agile AO bench for the telescope FEELINGS ›
Right Energy, Wrong Profile: Why the 43 GeV Cluster Line Is Unlikely to Be Dark Matter ›
Characterizing bright $\delta$ Scuti pulsators using TESS light curves:II. Pulsation amplitude and energy distributions ›
The Variation of Circumstellar Parameters through Early Stellar Evolution ›
The Study of Detailed Morphology of Milky Way Dwarf Galaxies: Draco and Bo\"otes I ›
Design of an atmospheric dispersion corrector and double scrambler for improved fiber coupling and illumination uniformity for the HET HRS ›
Probing multi-state dark matter via optical absorption lines in DESI spectra ›
Multi-wavelength Constraints on Dust Dynamics and Size Evolution in Protoplanetary Disk Rings. II. Observational Implications ›
Supernova nucleosynthesis: a review ›
Radiation Pressure Instability-Driven Variability of Line-Driven Disk Winds in AGNs: Connection to Periodic Luminosity Variations and UFO Appearance ›
Probing the All-sky Distribution of Soft X-ray Emission Associated with the Milky Way ›
Cosmological information from field-level analysis in redshift space ›
Discovery of radio emission from the exoplanet $\beta$ Pictoris b ›
Lower central dark matter densities in nearby galaxies than predicted by simulations ›
Population synthesis of low-mass binaries with wind-accreting neutron stars ›
The study of AF And. I. Hydrogen abundance constraints and dynamically-consistent wind model of the hot state ›
H$_2$O emission as tracer of pebble drift: insights from coupling transport and thermochemical models ›
Testing a Pre-Supernova Contribution to $^{44}$Ti in Cassiopeia A ›
The asymmetric limbs of HD 209458 b observed with JWST NIRCam F322W2/F444W ›
Triple coronal hard X-ray source observed by STIX during a failed filament eruption ›
Impact of Equation of State on Black Hole Accretion Flows and Radiative Properties ›
Supernova Kinetic Yield oN galactic Emission Tracers (SKYNET) I. Contribution of radiative supernova remnants to Galactic N + emission ›
Gravitational lensing of gravitational waves by galaxy clusters ›
Promise and pitfalls of plasma emission as an exo-space-weather tool ›
An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: II. The nature of FIR-bright quasars ›
The UV-to-FIR environments of nearby Type Ia supernovae with the DustPedia Galaxy Catalogue -- I. Local versus global host properties ›
Hardware-efficient neural networks for FPGA-based radio triggering of extensive air showers ›
Pushing HST to the limit: Detection completeness and morphology robustness of faint galaxies in the EGS field ›
Lyman-$\alpha$ forest 1D flux power spectrum constraints on QSO-assisted reionization models ›
Around the water snowline: I. Effects of dynamical and chemical interplay on mid-infrared water spectra of protoplanetary discs ›
Optimal exposure time for satellite imaging? A trade-off between residual tip-tilt and registration accuracy ›
The evolution of discs and the epoch of formation\newline of giant planets around solar type stars ›
Saturns Are Not Large Neptunes: The effect of removing inflated giants from empirical mass-radius relations ›
How Small is Large Enough? Determining Minimal Cluster Sizes for Molecule Adsorption on Interstellar Amorphous Ice ›
Stellar age is not disk age ›
Determining elemental composition in laboratory meteorite ablation spectra through radiative transfer modeling ›
Investigating past high-energy fluxes with paleo-detectors ›
No statistically significant evidence for a correlation between stellar and planetary composition ›
Count-based spectral component imaging (CCI) of solar flares in X-rays ›
The WEFT project: I. The emergence of turbulence in a cosmic filament ›
Glycine in the interstellar medium revisited: Resolving conformational complexity kinetically ›
PyExoCross 2.0: A Python Framework for LTE and non-LTE Spectra, Cross Sections, and Spectroscopic Post-processing of Atomic and Molecular Line Lists ›
A fast radio burst from a non-targeted low-frequency survey ›
Caught by its own light: Wimpzillas, the LHAASO knee and the diffuse $\gamma$-ray sky ›
A self-consistent orbital architecture for GG Tau A. I. Simultaneous orbital fitting of the hierarchical triple ›
Large ${\rm Pm}$ small-scale kinematic dynamo in protoneutron stars ›
Characterization of IBEX LmAPD detectors at CEA for future low-noise NIR astronomy instruments ›
DewTwin-Coin: an onboard autonomous framework for lunar water-ice prospecting using Chandrayaan-3 LIBS and ChaSTE data ›
Assessing ionospheric effects on image quality in the LOFAR Decametre Sky Survey ›
X-ray to Mid-IR Spectral Energy Distributions: A Catalog of X-ray Selected AGNs in the XMM-COSMOS Survey ›
Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy ›
The Equivalence Principle in the Dark Sector in light of DESI ›
Spontaneous wandering of the magnetic axis in pulsars: 3D magneto-thermal simulations and the imprint on braking indices ›
Stellar Ages of M Dwarf Hosts of Temperate Sub-Neptunes ›
Constraints on the central engine of merger-driven long gamma-ray bursts ›
Secular evolution of viscous and self-gravitating protoplanetary discs with magnetic winds ›
$B$-sure. Part II. Scattering transforms as robustness test for tensor-to-scalar ratio detection from CMB observations ›
Dark Radiation Sticks Together: Dark QCD and the Hubble Tension ›
Multiple-Mediator-Affected Ultra-High-Energy Neutrino Attenuation: Hints for 5D ${U(1)}_{L_\mu - L_\tau}$ in IceCube ›
Bridging the chirp-mass gap: searching for gravitational waves from inspiraling ultra-compact binaries using LIGO O4ab data ›
Charging of rotating black holes: kinetic simulations of black hole magnetospheres ›
Bridging Between Statistical Mechanics and Black Hole Evolution: Theoretical Formalism ›
Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field ›
Impact of the Host Galaxy on the Search for Gravitational-Wave Microlensing by Compact Objects ›
Adding slow magnetoacoustic mode to the HLL-type multi-state approximate Riemann solution ›
Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ Event ›
Vanilla Scotogenic Model at the future Muon Collider ›
Strong magnetic field inside degenerate relativistic plasma and the impacts on the neutrino transport in Core-Collapse Supernovae ›
The Cocytos Stream: A Disrupted Globular Cluster from our Last Major Merger? ›
Combined tracer analysis for DESI 2024 BAO ›
Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI ›
XID+PRIMA, II: Stepping Through Hyperspectral Imaging to Deblend PRIMAger Beyond the Extragalactic Confusion Limit ›
Induced Scattering of Fast Radio Bursts in Magnetar Magnetospheres ›
Mixing-induced thermal instabilities and coronal condensations ›
The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure ›
The Curious Case of Centaurus A: On the Subject of the Quenched satellites ›
Ly{\alpha} forest bounds on sterile neutrino production via neutrino self-interactions ›
On gravitational baryogenesis in inflationary $f(R)$ Cosmologies ›
Pad\'e semi-cosmographic reconstruction of residual dark energy in decaying dark matter cosmology: DESI DR2 BAO constraints and mock 21 cm forecasts ›
Metal Mayhem at z~7-10: Diversity and Evolution of Gas-Phase Metallicity Gradients ›
FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis ›
DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Overdensities ›
A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State ›
Discovery of a Compact Hub-Filament System in G286.21+0.17 with JWST and ALMA: Insights into Protocluster Formation and Competitive Accretion ›
Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics ›
Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae ›
Temporal Invariance Is an Illusion: Time-Dependent Influences of the Galactic Magnetic Field on UHECR Observations ›
A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations ›
Time-dependent cosmic-ray escape from wind bubbles: hard spectra formation ›
Effects of Super-rotating Jets on Phase-Resolved Transmission Spectra at High Spectral Resolution ›
Traversing the Galactic Centre in space and time ›
Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics ›
Optically Selected Superthin Galaxies Remain Thin in the Near-infrared ›
Robust Heteroskedastic Matrix Factorization: A Generalization of PCA that Flags Outliers and Handles Missing Data ›
Using Ringed Disks to Determine Fundamental Parameters of Planet Formation ›
Implementation of frequency-correlated noise in CMB component separation: Method, Validation, and Early Applications ›
Conformally Interacting Dark Energy with Early and Late-Time Measurements ›
Why Azimuthal Averaging Works in Halo Lensing: Symmetry and Power Counting for Nonlinear Shear and Magnification ›
Active galactic nucleus activity in brightest cluster galaxies at intermediate redshifts in Sunyaev-Zel'dovich--selected clusters ›
Host Galaxy UV Emission and Dust Reddening in Little Red Dots ›
Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM ›
Evolution of the High-Energy Excess in Swift J1727.8-1613 during Its 2023 Flare State ›
Forecasting Coupled Dark Energy Parameters with the One-Loop Galaxy Power Spectrum ›
Spectator Composes a Gravitational Canon: Spectator-field-triggered Phase Transition During Inflation and its Anisotropic Gravitational Wave Signals ›
Probing the Kinematic Dipole with LISA: an analytical treatment ›
Structure of the $^8$B and $^8$Li nuclei and the astrophysical $S_{17}(0)$-factor of the $^7$Be($p,\gamma$)$^8$B direct capture process within a three-body model ›
Neutrino helicity oscillations in astrophysical environments: A many-body approach ›
Parametrized beyond-Teukolsky framework in the time domain ›
DANSur_HM: Modularly incorporating higher modes in a deep learning based gravitational-wave surrogate ›
A distance-independent constraint on the axion-electron coupling from RGB stars ↓↑