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 to Mt. Babia Gora

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Latest preprints on astro-ph:
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Environmental Noise Challenges for the Einstein Telescope - A Review ›
Constraints on magnetic monopoles from X-ray observations of neutron stars ›
Deus ex $H_0$ -- Is evidence for dynamical dark energy conditioned on early cosmology? ›
GLOW I: Comprehensive Measurements of Gas-Rich, Star-Forming, Low-Mass Galaxies in the Nearby Universe ›
Wild behaviour near the finish line: the Type Ibn SN 2020able and its stratified environment ›
GLOW II: A Census of Oxygen in Low-Mass Galaxies ›
Probability of gravitational-wave lensing by intermediate-mass black holes and globular clusters ›
First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models ›
Scattering from Dusty Outflows in Hot Dust-Obscured Galaxies with Blue Excess Emission ›
Radial Stellar Age Gradients in 42 Local Volume Dwarf Galaxies ›
The large-scale ordered magnetic field in the Galactic halo and the Local Bubble ›
X-Ray Observation of Type II Supernova 2024ggi ›
Fast and Accurate Prediction of Neutron Star Structure with Deep Neural Networks ›
Axion dark matter search with a photonic bandgap cavity haloscope and dielectric tuning rod over 10.25-10.45 GHz ›
Capture Driven Evolution of Asymmetric Dark Matter in Non-rotating Neutron Stars ›
Mapping gas accretion and stellar kinematics to sub-kiloparsec scales in NGC 4696 with JWST/NIRSpec ›
Spectrally dispersed non-redundant aperture-masking interferometry in the thermal infrared with LBTI/ALES ›
The Circumgalactic Medium of Present-Epoch Luminous Galaxies as Probed by CIV Absorption ›
Do Accretion Disks Get Bent Out of Shape? Investigating the Origin of Rapid Fluctuations in the Tails of Long Thermonuclear X-ray Bursts ›
On-sky capabilities and performance of the Keck All Sky Precision Adaptive Optics system ›
Neutrino quantum kinetics for fast flavor conversion in a time-dependent environment ›
A Systematic Study of Type Ia Supernova Remnants: Using Nucleosynthesis to Probe their Supernova Progenitors ›
The Impact of Splashback Galaxies on Galaxy Assembly Bias ›
The $\delta$ Scuti pulsator occurrence as a function of age, $T_{\rm eff}$, rotation, and metallicity ›
Inflationary Axion Isocurvature in the CMB across All Ultralight Masses ›
Overview and status of BICEP Array's BA4-90/150 CMB polarimeter ›
Insights into the Pulsar Timing Array hypothesis space ›
What can Planetary Ice Shells Teach Us about Ocean Mixing and Life, and Why Salt Matters ›
NATA: a chemical-picture equation of state for stellar merger hydrodynamics ›
Anisotropic Particle Transport from a Pulsar Wind Nebula Revealed by Einstein Probe and LHAASO ›
Spec-S5: A Next-Generation All-Sky Spectroscopic Facility Enabling Large-Scale Surveys for Cosmology and Astrophysics ›
A Two-level Radial-velocity Zero-point Calibration for LAMOST MRS with Gaia and APOGEE and a Value-added RV Catalogue ›
JWST Reveals a Galaxy-Wide Association of Red Supergiants with OB Stars in NGC 5584 ›
Implicit Likelihood Inference and $z$-Binned Reconstruction of Dark Energy $w(z)$ ›
First detection of C2H+ in the interstellar medium ›
Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15 ›
Diagnosing the Fe line complex of the intracluster medium by XRISM high-resolution spectroscopy ›
A New Window on the H{\alpha} Luminosity Function and Star Formation Rate Density from 1.2 < z < 6.6 from JWST Medium-Band Photometry ›
Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient ›
On the Physical Origins of Long Period Radio Transients ›
From Light to Sound: Spectroscopic Evolution & Sonification of the flaring Nova V612 Scuti ›
The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data ›
Design evolution for the Wide-field Spectroscopic Telescope ›
Design and simulation of a photonic lantern-inspired astrophotonic chip for spectral sensing ›
KCWI Discovery of a Spatially Resolved Kpc-Scale Ionized Outflow in NGC 1275 ›
GATOS: Distinct Feedback Modes in AGN Central Regions Revealed by Spatially Resolved JWST Spectroscopy ›
The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae ›
Constructing a Hydrogen Line Library for Ly{\alpha} Emitters at Low Redshifts (z < 0.4): Estimating Dust Extinction and Assessing Paschen line Detectability with SPHEREx ›
A Catalog of Giant Radio Source Candidates from TGSS ADR1 Using a Deep Learning--based Pipeline ›
Three-Dimensional Expansion of Iron Ejecta in Cassiopeia A with Chandra and XRISM ›
FORTVSH: A Fortran Module For Vector Spherical Harmonics Computations ›
Plasmoid-Mediated 2D Magnetic Reconnection in Partially Ionized Plasmas ›
Slow Cosmic-Ray Diffusion in Supersonic and Super-Alfv\'enic Turbulence ›
Coronal Rain Driven by Low-Frequency Impulsive Heating: Dependence of Dynamics and Morphology on Coronal Heating and Magnetic Field ›
Exploration of UV-bright sources in Globular cluster NGC 3201 using UVIT observations ›
Sun-to-Earth Coronal Mass Ejection Simulations From a Vector Magnetogram ›
QUIJOTE scientific results - XX. Commissioning and First Results from the Thirty and Forty Gigahertz Instrument (TFGI) ›
The James Webb Space Telescope Absolute Flux Calibration. VI. Near-Infrared Camera Imaging and Coronagraphy ›
Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds ›
Timing and statistical analysis of single-pulse search pulsar discoveries from the PALFA survey ›
A Hybrid R-Theta Fiber Positioning Robot Using a Piezoelectric Bender for Radial Motion ›
Synthetic Fe XIII 1074.7 nm Observations of Torsional Alfv\'{e}n Waves in Coronal Waveguides ›
Gas Flows and Mass Accretion Rates in Eight Dippers: HD 142666, HD 143006, HD 145718, V935 Sco, DoAr 25, EPIC 204638512, EPIC 205151387, and EPIC 203850058 ›
Atmospheric Diversity of Giant Planet Analogs from 3-5um with SPHEREx ›
An Identifiability Audit of One-Parameter Structural Corrections to the Radial Acceleration Relation in SPARC ›
Locating the missing baryons in the warm-hot intergalactic medium with fast radio bursts and the Sunyaev-Zel'dovich effect ›
Unveiling Metal Mixing in a Grand-Design Spiral: A UV-optical multiphase spatially resolved study of M83 ›
Multi-tracer mass bias in matched cosmic voids from SDSS DR7 and the ELUCID constrained simulation ›
Foreground Subtraction with a Tensor-Based Oriented Singular Value Decomposition Method for HI Experiments ›
Statistical inference of fast radio burst environments using galaxy number density ›
Optimizing Wavefront-Deformation Sensor Placement for Active Radio-Telescope Surfaces ›
The Role of Extended-Source Geometry and Diurnal Cycles on Exoplanetary Thermal Baselines: Reconciling the Brightness Temperature of 55 Cancri e ›
Pointing Model Meets Deep Learning: A Retrospective Study on a MeerKAT+ Telescope Applying Deep Learning Methods for Blind Pointing Corrections ›
Impact of disk magnetic fields on the propagation of stellar-scale jets in the magnetically arrested accretion disks of active galactic nuclei ›
AGN activity in nearby disk galaxies: the roles of bar strength and spiral-arm morphology ›
Astrophysical origins of TeV features in the cosmic-ray lepton spectrum ›
Kratos-linerad: GPU-accelerated Monte Carlo radiative transfer of lines with efficient imaging ›
Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014 ›
A Machine Learning Based Search for Lunar Anomalies ›
Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology ›
Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares ›
A Partial Lyman Limit Absorber in the Halo of a Galaxy Pair: A Possible Signature of Gas Inflow ›
The Environmental Dependence of Star Cluster Demographics ›
CMB Spectral Distortion Anisotropies from Acoustic Damping with primordial non-Gaussianity ›
Global simulations of accretion flows onto perturbers embedded in magnetized disks -I. MRI and jet formation in ideal MHD ›
Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 ›
Searching for low-surface-brightness galaxies with compact neural networks A parameter-efficient approach to first-pass selection of diffuse galaxy in HSC-SSP imaging ›
Sector-based morphological analysis of four planetary nebulae (J 320, NGC 2610, A 6672 and PRTM 1) observed with UVIT/ASTROSAT ›
Ubiquitous Interstellar Neutral Helium Detected with JWST ›
A Chemical Inventory of the Disk around the Class 0 Protostar L1527 IRS with ALMA ›
Unsupervised Domain Adaptation for Multitask Image Analysis in Realistic Context with Extreme Label Shift; Application to the CTAO first Large Sized Telescope ›
Reconstruction of ASO-S/HXI Solar Flare Hard X-ray Source Images with Physics-Constrained Deep Networks ›
Wigner interferometry ›
Recoiling Black Holes I. Burst of Observables ›
TOI-7475 spectroscopic follow up - detection of a massive hot Jupiter on an eccentric orbit ›
Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe ›
Exploring the multi-wavelength properties of the high energetic event ZTF20abbiixp/GRB 200524A: from prompt emission to afterglow ›
Not R Kurvature: Beating Large-Scale White Noise ›
Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis ›
Quasi-automatic software support for Gaia ground based optical tracking ›
SGNAX: a unified matched-filter and excess-power pipeline for gravitational-wave detector characterization ›
An emerging baryon cycle in a galaxy 500 million years after the Big Bang ›
NASA ASTRA Initiative White Paper: Space-Based Mission for Ultrahigh Energy Particles ›
The Galactic Neutrino Sky: Predictions from Gamma-ray Source Populations ›
A bestiary of low-level electrical artifacts in SPHEREx flight data ›
Infrared Spectroscopy and Photochemistry of Aromatic Nitriles in Para-Hydrogen Matrices ›
Peak 'Nebular' Emission and Early Flux Excesses in Ca-strong Supernovae ›
Nascent Embedded-protostar Survey in Taurus (NEST) II: Measuring Dust Mass, Disk Size, and Gas Mass ›
The Fate of Large Scale White Noise in Second-Order Cosmological Perturbation Theory ›
IPA: Morphology and Kinematics of Molecular Hydrogen Winds in Five Young Protostars across the Mass Spectrum Observed with JWST ›
Realization Variance of Gravitational Wave Background Anisotropies from Shot Noise for Pulsar Timing Arrays ›
Baryogenesis via the CKM Matrix with Minimal Flavor Violation ›
Real-time physics inversion for retrieval of sub-pixel wildfire temperatures from VSWIR imaging spectroscopy ›
Celephais: efficient spectral initial data code for precessing compact binaries ›
The G347.3-0.5 outlier from O3: a follow-up case study for continuous gravitational-wave candidates ›
Gravitational radiation from binary systems with time varying masses ›
Probing Memory-Burdened Primordial Black Holes with High-Energy Neutrinos ›
On the nonlinear instability of nonrotating Stars ›
Estimating Uncertainty in Galaxy Morphology Classification ›
Horizon-Dependent Tube MPC for Spacecraft Rendezvous on Elliptical Orbits with Conditional Robust Constraint Satisfaction ›
Hadron-quark phase transitions along proto-neutron-star evolution ›
Correlated parity violation in gravity and electromagnetism from five-dimensional spacetime ›
High-order fully discrete multi-entropy-stable and bound-preserving schemes for relativistic Euler equations ›
Observational constraints on fractional holographic dark energy in the light of DESI DR2 ›
A Gaussian Process framework for constraining the nuclear equation of state from microscopic calculations with correlated uncertainties ›
Adiabatic Perturbations in GW170817-Compatible Einstein-Gauss-Bonnet Inflation ›
Thermal Origin of Black Hole Quasinormal Modes ›
Probing ultralight bosons with LISA observations of spinning black hole mergers and follow-up searches of merger remnants ›
SN 2018bsz: significant dust formation in a nearby superluminous supernova ›
DESI Dark Secrets ›
Constant-Roll Inflation ›
Assessing the Power-Law Emissivity Assumption in X-ray Reflection Spectroscopy: A Simulation-Based Evaluation of Different Coronal Geometries ›
Measuring the Temperature of Extremely Hot Shock-Heated Gas in the Major Merger MACS J0717.5+3745 With Relativistic Corrections to the Sunyaev-Zel'dovich Effect ›
Evolution of accretion disc-corona in the TDE Candidate AT 2019avd ›
Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra ›
A JWST/NIRSpec Integral Field Unit Survey of Luminous Quasars at z ~ 5-6 (Q-IFU): Rest-frame Optical Nuclear Properties and Extended Nebulae ›
Absorption effects in the expanding Universe: spectral transmittance functions of the intergalactic medium for distant sources ›
Deep Investigation of Neutral Gas Origins (DINGO): Options for robust Deep Spectral Line Imaging in the SKA-Era ›
Transit Timing of the White Dwarf-cold Jupiter System WD 1856+534 ›
The velocity coherence scale: a novel probe of cosmic homogeneity and a potential standard ruler ›
Detection of a puzzling dual-superorbital hard X-ray modulation in the X-ray binary GX 301-2 ›
Balancing Variety and Sample Size: Optimal Parameter Sampling for Ariel Target Selection ›
A Variable-Slope Smooth-$k$ Filter for Modeling Halo Abundances with Damped and Oscillatory Power Spectra ›
Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework ›
A simple model for extracting astrophysics from black hole images ›
Timescale-dependent Optical Variability of Turn-on Changing-look Active Galactic Nuclei ›
Identifying AGNs from X-ray detections-I: Metallicity calibrations in AGNs with X-ray luminosity as the primary input parameter ›
Near-Infrared and Optical Observations of SN 2024rbc: The First Early Detection of CO and Dust in a Type Ib Supernova ›
Estimates of the Dynamic Characteristics of Binary Systems for Traversable Wormholes Search ›
Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies ›
A GLIMPSE of the 99%: a census of the faintest galaxies during the epoch of reionization and its implications for galaxy formation models ›
A sound-horizon-free measurement of the Hubble constant from DESI DR2 baryon acoustic oscillations using artificial neural networks ›
Unifying Transport Models of Thermohaline Convection in Stars ›
Matter Clustering in Astrid: Reduced Baryonic Suppression from Realistic Black Hole Dynamics ›
Vacuum polarization and cyclotron resonance effects on radiative transfer and plasma deceleration in subcritical X-ray pulsars ›
Eclipses of Nearby Millimeter-Bright Galactic Nuclei by Stars in Nuclear Star Clusters ›
The first IXPE view of the eclipsing ADC source 4U 1822-37 ›
Suppression of Radiative Cooling in Galaxy Cluster Cores by the Combination of AGN Heating and Sloshing ›
ODIN: Rest-frame Optical Morphologies and Star Formation Activity of Ly{\alpha} Emitters at z=2.4, 3.1, and 4.5 ›
Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots ›
LAMOST J010103.13+275449.6: A New Binary Exhibiting a Switch in Photometric Period from 1.7216\,d to 0.8444\,d ›
Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots ›
Grain alignment and dust evolution physics with polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra ›
TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS ›
Discovery of a gravitational arc candidate at photometric redshift 1.4 in MACS J0308.9+2645 from a catalogue-based search of JWST imaging ›
A Periodically Interacting Dark Sector: Signatures and Constraints from CMB and Cosmic Expansion Data ›
Recovering Electron-Distribution Information from the Quiet-Sun Temperature Discrepancy ›
A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations ›
Investigating the differential limb coupling effect for diffraction-limited spectrographs with PARVI ›
MiraSOL: a DMD-based spectrograph for resolved solar spectroscopy ›
A broad exploration of climate and observability of close-in rocky exoplanets: applications to Ross 128 b ›
A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction ›
HST imaging, pipeline modeling, and time-delay predictions of 2 triply-imaged and 15 quadruply-imaged lensed quasars ›
NeuralDMD: Interpretable Neural Representation of Dynamics from Sparse and Noisy Measurements ›
Backreaction of Halilsoy and Chandrasekhar waves ›
Electroweak Baryogenesis with BARYONET: a self-contained review of the WKB approach ›
Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run ›
Deep-Learning Denoising of Radio Signals for Ultra-High-Energy Cosmic-Ray Detection ›
All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects ›
Interior geometry of black holes as a probe of first-order phase transition ›
Localized Steps toward ACT-Favored Inflation ›
Cosmological collider signals of modular spontaneous CP breaking ›
The Quantum Noise Fraction and the addressable fraction in High-Frequency Gravitational Wave Detection ›
Pole structure of the Kerr Green's function ›
Non-Dynamic Alignment in Magnetohydrodynamic Turbulence ›
Counterintuitive Magnetic Connectivity and Energetic Particle Flux Differences among Nearby Spacecraft During the 2023 February 24 Solar Energetic Particle Event ›
Modeling the response of the marine carbon cycle to extreme CO$_2$ injection events ›
Earth as a transducer for ultralight bosonic dark-matter detection ›
Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity ›
Evading Cauchy horizon excision in scalarized regular black holes ↓↑