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Obserwatorium Astronomiczne na Suhorze

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Najnowsze prace na astro-ph:
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Blackholistic 2026 meeting report ›
The Cosmological Hart-Tipler Conjecture ›
Relativistic Lightsail Propulsion Dynamics ›
The role of major mergers in triggering super-Eddington accretion ›
Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks ›
Studying the absorption signatures of H I Lyman-\alpha\ in the warm-hot circumgalactic medium with TNG50 ›
Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster ›
Ceci n'est pas une Couche de M\'elange: The Meaning of Resolved Turbulent Radiative Mixing ›
A multi-eigenbasis approach to covariance matrix denoising for cosmological inference ›
Mapping the nuclear environments of extreme coronal line emitting galaxies ›
The Origin of Da Scaling: Suppressed Cooling in Fast-Cooling Mixing Layers ›
Multifrequency Synthesis via CHIBI: Colorful Hierarchical Interferometric Bayesian Imaging ›
Predictive Rankings of the Probability for Temperate Terrestrial Worlds for the HWO ExEP Mission Star List ›
NSV 4031 is a gamma Doradus variable after all ›
Rotational Modulation and Long-Term Variability of Magnetic Fields in T-Tauri Stars with IGRINS ›
HST's Deep Blue: extremely deep UV imaging to reveal the contributors to reionization ›
Temporal Invariance Is an Illusion: Time-Dependent Influences of the Galactic Magnetic Field on UHECR Observations ›
Characterizing Transiting Exoplanet Atmospheres in the 2030s with the Hubble Space Telescope ›
Predictions for the X-ray polarisation modulation in Cygnus X-1 from reflection off the stellar companion and its wind ›
HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy ›
Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary ›
The Role of Source Geometry and Atmospheric Propagation in Global Bolide Infrasound Detectability ›
Preparing for the Early eVolution Explorer: Detecting the Primordial, Transiting Exoplanet Population ›
The Y Dwarf Companion to the White Dwarf WD 0806-66: Resolving the Discrepancy Between Atmospheric and Evolutionary Models ›
All-Sky Ultra-Narrowband Spectral Imaging with the OVRO-LWA: Technosignature Constraints and Axion-Like Particle Prospects ›
CO-dark molecular gas traced by HCO$^+$ in the diffuse interstellar medium ›
Hybrid Particle Gaussian Mixture (H-PGM) Solution for Cislunar Target Tracking ›
A Planetary Nebula from a 5.7 $M_{\odot}$ Progenitor in a 90 Myr M31 Star Cluster ›
A High-Likelihood Polar Interstellar Meteor Candidate ›
Fast-spinning massive black holes from slowly rotating low-metallicity stars: implications for GW231123 ›
A More Complex Than Expected Formation History of the Milky Way's Last Major Merger ›
Primordial Binary Stars, Mass segregation and Fractality Effects on the Early Evolution of Young Open Clusters ›
Detection of stratospheric HCN and tropospheric CO in Uranus and the implication for their sources ›
Late infall of molecular cloud material reshaped the outer Solar System ›
The GALAH Survey: Neutron-Capture Elemental Abundances for 350,000 Gaia-RVS Spectra and the Chemodynamics of Accreted Structures ›
Cosmography of the Sloan Basin of Attraction and Neighborhood ›
Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification ›
Blue Straggler Stars in Berkeley 18: A Multiwavelength Study of Their Physical Properties and Dynamical Evolution ›
Environmental Dependence of Star Formation and Galaxy Colors around Abell 2029 ›
NICER detection of a new candidate cyclotron line in the bursting X-ray pulsar GRO J1744-28 ›
Upper limits on exosatellites around $\beta$ Pictoris b ›
Long-term investigation of gamma Cas analogs ›
BBN constraints on primordial black holes with a continuous memory-burden crossover ›
ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement ›
The Extreme Rarity and Physical Properties of Low-redshift AGNs with Balmer Absorption ›
Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions ›
Recurrent Coronal Jets and QPPs: Periodic Reconnection and Localized Heating Across Quiet-Sun to Active Regions ›
A candidate cyclotron line at 1.89 keV in the ultraluminous X-ray source NGC 4861 X-2 ›
TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates ›
Galactic absorption measured by X-ray observations of clusters of galaxies at the low Galactic latitude ›
Granular mass perturbations on the pulsar - supermassive black hole system ›
Cooler Phases of the Circumgalactic Medium Are More Centrally Concentrated: Constraints from Multiphase Absorption Lines ›
Steep Redshift Evolution of the Ionizing Escape Fraction at $z = 5$--$12$: Empirical Constraints and Comparison with Simulations ›
Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis ›
The open cluster NGC 2509. Stellar rotation and main sequence turnoff extension from FLAMES spectroscopy ›
Rediscussion of eclipsing binaries. Paper 31. The slowly-pulsating B-star system CV Velorum in the PLATO southern field ›
A Model Selection Criterion for Multidimensional Gaussian Processes: Application to Radial Velocities ›
Dissipative Dark Energy can explain the DESI phantom crossing ›
$E_{\rm peak}$-$\alpha$ Correlation in Time Resolved GRB Spectra: A Bottom-Up Approach with Optically Thin Inverse Compton Scattering Model ›
Posterior sampling in the Age of Emulators ›
Bridging Roche Lobe Overflow and micro-TDEs: The Runaway Evolution of Eccentric Mass Transfer in Star-Black Hole Binaries ›
An update to Allocating Time on Scientific Platforms in Outer Space using five cycles of JWST General Observer programs ›
Full-Disk Spectroscopy of the Solar Corona Across a Solar Cycle with Hinode/EIS ›
Deep Learning with Magnetic Parameter Constraints for Short-Term Prediction of Solar Active Region Vector Magnetic Fields ›
Neutrino mass constraints in interacting dark energy models after DESI DR2 ›
A Measurement of the Thermal and Ionization State of the IGM at $z < 0.5$ ›
Transport of water in a Transient, Impact-Generated Atmosphere on Mercury ›
An 800-Million-Year-Old Impact Shower on the Terrestrial Planets from the Breakup of the Eulalia Parent Body ›
Full Nonlinear Velocity Reconstruction With Transformer and Ensemble Tree Machine Learning ›
First Constraints on the Ellipticities of Self-Interacting Fermionic Dark Matter Admixed Neutron Stars from Continuous Gravitational-Wave Searches ›
Observational signatures of thermonuclear electron-capture supernovae -- Ne II line strengthening and color evolution as traces of the explosion mechanism ›
The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Formaldehyde (H$_2$CO) emission and its links to disk properties ›
CMB Bounds on Primordial Black Holes via Radiation Capture ›
New Measurements of Distances to Galaxies in the NGC 1052 Field with the Hubble and James Webb Space Telescopes: Testing the Bullet-Dwarf Origin of the Trail ›
Early Multiwavelength Observations of AT 2026fgk: The Luminous Afterglow to Sub-luminous GRB 260310A, Identified Independently of a Gamma-ray Trigger ›
Three Extremely Metal-Poor stars: discovery of a new CEMP-no star ›
SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk ›
Compressed \emph{Gaussian} likelihood for the \textit{Planck} low-$\ell$ data ›
Towards Exascale Computing for Astrophysical Simulation Leveraging the Leonardo EuroHPC System ›
A Common Antimatter Response in AMS-02 Positrons and Antiprotons ›
Shape of U: Measuring the Curvature of the Universe with Gravitational Waves ›
Radiation-induced electron spin polarization in ultrarelativistic kinetic turbulence ›
Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries ›
Constraining Cosmological Parameters From Statistical Superluminal Effects Without a Distance Ladder ›
The geometry of lunar gravitational wave detection ›
Integrability of cosmological $R^2$ gravity models with radiation ›
Identifying Gems from Roman RAPIDly ›
Mapping the star formation peak with LIGO A# and Next-Generation detectors ›
Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometers ›
CosmoUiT: A Vision Transformer-UNet Hybrid for Fast and Accurate Emulation of 21-cm Maps from the Epoch of Reionization ›
The superclustering of hot gas: cosmological sensitivity in the Websky simulations ›
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff ›
Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning ›
Hot accretion onto spiral galaxies: the origin of extended and warped HI discs ›
Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters ›
Photon (Non)Conservation in the Reduced Speed of Light Approximation and How to (Almost) Fix It ›
Trapped fireshell (halo) of photons and pairs around black-hole horizon: source for ultra-high-energy particles ›
Improvements to the NSO Farside Mapping Pipeline: Noise Reduction Updates ›
NICER Perspective on TeV Blazar Mrk~421: X-ray Variability and Particle Acceleration ›
Cosmic Strings Gravitational Wave Probe of Leptogenesis: Thermal, Non-thermal, Near-resonant and Flavourful ›
Uniform models of neutron and quark (strange) stars in General Relativity ›
Quantifying Symmetry: Transformation Information for Planetary Nebulae and Supernova Remnants ›
Rotational enhancement and stability of protoquark stars during thermal evolution ›
TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy ›
TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter ›
Bounds on Lorentz invariance violation from muon fluctuations at the Pierre Auger Observatory ›
Scaling solutions in three-form cosmology ›
Imprints of primordial magnetic fields in gravitational collapse during early structure formation ›
Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor ›
UNIONS-3500 Weak Lensing: II. B-mode validation for cosmic shear ›
Modeling Volcanic Plume Heights Across Exoplanet Atmospheres: Insights from TRAPPIST-1 ›
Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges ›
XRISM detection of the 6.4 keV Fe K$\alpha$ line in the radio galaxy Cygnus A ›
Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study ›
Determining the incidence rate of magnetic $\delta$ Scuti candidates with CoRoT ›
Ca-bearing cyanopolyynes in IRC+10216 ›
Optimal Transport Reconstruction of Biased Tracers in Primordial Non-Gaussian Fields ›
Cosmological Cutting Rules ›
Modeling transport in weakly collisional plasmas using thermodynamic forcing ›
Black-hole hair from vector dark matter accretion ›
When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors ›
Inferring the stochastic gravitational-wave background from eccentric stellar-mass binary black holes with spaceborne detectors ›
Dark Matter and Baryon Asymmetry from Monopole-Axion Interactions ›
Improved cosmological constraints on axion-lepton interactions ›
Inflationary assessment of $F(\mathcal{R},\tilde{\mathcal{R}})$ Einstein-Cartan models ›
Observable Gravitational Wave Strain at Second Order ›
Gravitational waves from seesaw assisted collapsing domain walls ›
Low Energy Neutrinos in Milky Way and Cloud-9 ›
Toward universal coalescence models for antideuteron production ›
Kinky vortons in the 2HDM ↓↑