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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Latest preprints on astro-ph:
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A Novel Technique for Long-term Timing of Redback Millisecond Pulsars ›
The Spin-Orbit Alignment of 8 Warm Gas Giant Systems ›
GalSBI: Phenomenological galaxy population model for cosmology using simulation-based inference ›
PICS: Planetary Nebulae in Cosmological Simulations -- Revelations of the Planetary Nebula Luminosity Function from Realistic Stellar Populations ›
A grand-design spiral galaxy with an ordered magnetic field at redshift 2.6 as resolved with ALMA and gravitational lensing ›
SLOW IV: Not all that is Close will Merge in the End. Superclusters and their Lagrangian collapse regions ›
The 3D morphology of open clusters in the solar neighborhood III: Fractal dimension ›
On the Use of Letters of Recommendation in Astronomy and Astrophysics Graduate Admissions ›
$\texttt{UFig v1}$: The ultra-fast image generator ›
Probing the major driver of stellar population properties over sub-galaxy scales with SDSS MaNGA IFU spectroscopy ›
$\texttt{galsbi}$: A Python package for the GalSBI galaxy population model ›
What do we learn by mapping dark energy to a single value of $w$? ›
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: I. Free-floating MLPs ›
Magnetic Fields in Massive Star-forming Regions (MagMaR). V. The Magnetic Field at the Onset of High-mass Star Formation ›
Non-topological Solitons of Dark Matter and Gravitational Wave Signals ›
DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration ›
Beyond the Goldilocks Zone: Identifying Critical Features in Massive Black Hole Formation ›
Modeling Mg II resonance doublet spectra from galaxy haloes at z $\sim$ 1 ›
Resolved and unresolved Galactic gamma-ray sources ›
Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581 ›
Discoveries and Properties of EL CVn-type Binaries in the TESS Survey ›
ESpRESSO -- Forward modeling Roman Space Telescope spectroscopy ›
Geometrical Distances of Extragalactic Binaries through Spectroastrometry ›
Binary Evolution Pathways to Blue Large-Amplitude Pulsators: Insights from HD 133729 ›
The Long-term Evolution of the Solar Transition Region ›
An empirical model of the extragalactic radio background ›
Stellar parameter prediction and spectral simulation using machine learning ›
Interacting dark energy models ›
Towards Galactic Archaeology with Inferred Ages of Giant Stars From Gaia Spectra ›
A comprehensive numerical study on four categories of holographic dark energy models ›
Insights into the Properties of Type Ibn/Icn Supernovae and Their Progenitor Channels through X-ray Emission ›
Probing the low-energy particle content of blazar jets through MeV observations ›
Substellar candidates at the earliest stages: the SUCANES database ›
Molecular chemistry induced by J-shock toward supernova remnant W51C ›
Spectroscopic observations of flares and superflares on AU Mic ›
Betwixt Annihilation and Decay: The Hidden Structure of Cosmological Stasis ›
Chemodynamic evolution of Sun-like stars in nearby moving groups ›
Modified gravity in galaxy clusters: Joint analysis of Hydrostatics and Caustics ›
Chemical Evolution of R-process Elements in Stars (CERES). III. Chemical abundances of neutron capture elements from Ba to Eu ›
herakoi: a sonification experiment for astronomical data ›
Constraining Schwarzschild Models with Orbit Classifications ›
Quantifying Roche Lobe Overflow in the Formation of Merging Black Hole Binaries ›
Magnetic Reconnection between a Solar Jet and a Filament Channel ›
Evolution, speed, and precession of the parsec-scale jet in the 3C 84 radio galaxy ›
Fast-rotating A- and F-type stars with H{\alpha} emissions in NGC 3532, candidate UV-dim stars? ›
Journey of complex organic molecules: Formation and transport in protoplanetary disks ›
A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC ›
Constraining primordial black hole abundance with Insight-HXMT ›
A first glimpse at the MeerKAT DEEP2 field at S-band ›
Long term optical variations in Swift J1858.6-0814: evidence for ablation and comparisons to radio properties ›
Is cosmological data suggesting a nonminimal coupling between matter and gravity? ›
Using nebular near-IR spectroscopy to measure asymmetric chemical distributions in 2003fg-like thermonuclear supernovae ›
Insights from Modeling Magnetar-driven Light Curves of Stripped-envelope Supernovae ›
Galaxy Morphological Classification with Manifold Learning ›
Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82 ›
A BCool survey of stellar magnetic cycles ›
Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars ›
Radial evolution of a density structure within a solar wind magnetic sector boundary ›
Meteoroid Ablation within the Jovian Atmosphere: Implications on the Oxygen Delivery to the Gas Giant's Atmosphere ›
FBQ 0951+2635: time delay and structure of the main lensing galaxy ›
On the Relation between the Inclination Angle of the Accretion Disk and the Broad-line Region in Active Galactic Nuclei ›
Revisiting the Galactic Winds in M82 I: the recent starburt and launch of outflow in simulations ›
On the evolutionary nature of massive B-type supergiants: a modern empirical reappraisal using data from IACOB, Gaia and TESS ›
Constraints on Pre-Big-Bang Cosmology from Advanced LIGO and Advanced Virgo's First Three Observing Runs ›
SIRI-2 Detection of the Gamma-ray Burst 221009A ›
A Comparative Test of the LCDM and R_h=ct Cosmologies Based on Upcoming Redshift Drift Measurements ›
FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields ›
Primary Beam Chromaticity in HIRAX: I. Characterization from Simulations and Power Spectrum Implications ›
A new and flexible design method for Symmetric Quadrature Hybrid Couplers using Markov Chain Monte Carlo ›
A universal and physically motivated threshold for Hessian-based cosmic web identification: V-Web case ›
Kinetic simulations of the Kruskal-Schwarzchild instability in accelerating striped outflows I: Dynamics and energy dissipation ›
Nonlinear evolution of fluting oscillations in coronal flux tubes ›
How Many Bursts Does it Take to Form a Core at the Center of a Galaxy? ›
A glitch in gravity: cosmic Lorentz-violation from fiery Big Bang to glacial heat death ›
Asymmetric Temperature Variations In Protoplanetary disks: I. Linear Theory and Corotating Spirals ›
JWST PRIMER: strong evidence for the environmental quenching of low-mass galaxies out to $\mathbf{\textit{z} \simeq 2}$ ›
Influence of gravity on the quantum speed limit in neutrino oscillations ›
Gravitational Influence on the Quantum Speed Limit in Flavor Oscillations of Neutrino-Antineutrino System ›
On the construction of fuzzy dark matter halos with arbitrary initial velocities ›
Efficient Gravitational Wave Parameter Estimation via Knowledge Distillation: A ResNet1D-IAF Approach ›
Lectures in Quantum Gravity ›
Visions in Quantum Gravity ›
Axion mass prediction from adaptive mesh refinement cosmological lattice simulations ›
Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift ›
Status and Perspectives on Axion Searches ›
Bayesian evidence for two peaks in the sound speed in cold dense QCD ›
Evidence of enhanced two-level system loss suppression in high-Q, thin film aluminum microwave resonators ›
Characterizing hole trap production due to proton irradiation in germanium cross-strip detectors ›
Scalar perturbations on the normal and self-accelerating branch of a DGP brane and $\sigma_8$ ›
Controlling the asymptotic bias of the unadjusted (Microcanonical) Hamiltonian and Langevin Monte Carlo ›
High Quality QCD Axion via Electric-Magnetic Duality ›
Intrinsic Torsion, Extrinsic Torsion, and the Hubble Parameter ›
Fast Flavor Pendulum: Instability Condition ›
Exploring nuclear force with pulsar glitch observation ›
Electromagnetic radiation from a relativistic jet induced by a plane gravitational wave ›
Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars ›
Limits on dark matter, ultralight scalars, and cosmic neutrinos with gyroscope spin and precision clocks ›
Probing a diffuse flux of axion-like particles from galactic supernovae with neutrino water Cherenkov detectors ›
Primordial black hole formation from cosmological fluctuations ›
Signatures of Star-planet Interactions ›
Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) ›
A Simple Analytic Treatment of Neutrino Mass Impact on the Full Power Spectrum Shape via a Two-Fluid Approximation ›
Calibrating baryonic feedback with weak lensing and fast radio bursts ›
A Thorough Search for Short Timescale Periodicity in Four Active Repeating Fast Radio Bursts ›
Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid ›
Extracting $H_{0}$ and $r_{d}$ in Pacif Parametrization Models through Late-Time Dataset ›
On the Hubble expansion in a Big Bang quantum cosmology ›
Evaluating the Potential to Constrain Dark Matter Annihilation with Fermi-LAT Observations of Ultra-Faint Compact Stellar Systems ›
JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe ›
Modeling Multiple X-Ray Reflection in Super-Eddington Winds ›
Impact of star formation models on the growth of simulated galaxies at high redshifts ›
EDGE: Dark matter core creation depends on the timing of star formation ›
The protostars in Orion: Characterizing the properties of their magnetized envelopes ›
Discovery of Polarized X-Ray Emission from the Accreting Millisecond Pulsar SRGA J144459.2-604207 ›
Study of a Tilted Thin Accretion Disk around a Kerr-Taub-NUT black hole ›
Superflare on a rapidly-rotating solar-type star captured in X-rays ›
Simultaneous Multiband Photometry of the Early Optical Afterglow of GRB 240825A with Mephisto ›
Dusty substructures induced by planets in ALMA disks: how dust growth and dynamics changes the picture ›
JWST captures a sudden stellar outburst and inner disk wall destruction ›
Formation of giant radio sources in galaxy clusters ›
The nature of low-luminosity AGNs discovered by JWST based on clustering analysis: progenitors of low-$z$ quasars? ›
Analysis of biasing from noise from the Nancy Grace Roman Space Telescope: implications for weak lensing ›
Searching for Planets Orbiting Vega with the James Webb Space Telescope ›
Relativistic reconnection with effective resistivity: I. Dynamics and reconnection rate ›
Insights into the Long-Term Flaring Events of Blazar PKS 0805-07: A Multi-Wavelength Analysis over the 2009-2023 Period ›
Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not ›
Post-common-envelope planetary nebulae ›
An NGC 1068-Informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056 ›
votess: A multi-target, GPU-capable, parallel Voronoi tessellator ›
Probabilistic Galaxy Field Generation with Diffusion Models ›
The Temperature versus Orbital Period relation of AM CVns: Insights from their Donors ›
Strong signature of right-handed circularly polarized photoionization close to the cyclotron line in the atmosphere of magnetic white dwarfs ›
Gravitational waves from patterns of electroweak symmetry breaking: an effective perspective ›
On the structural stability of a simple cosmological model in $R+\alpha R^{2}$ theory of gravity ›
Thermalization and hotspot formation around small primordial black holes ›
Ringdown of a postinnermost stable circular orbit of a rapidly spinning black hole: Mass ratio dependence of higher harmonic quasinormal mode excitation ›
Evaluating Near-Real Time Thermospheric Density Retrieval Methods from Precise Low Earth Orbit Spacecraft Ephemerides During Geomagnetic Storms ›
Constraining accretion physics with gravitational waves from eccentric extreme-mass-ratio inspirals ↓↑