Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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Astronomia w Krakowie
Zdjecie: The International Space Station and a halo around the Moon
The International Space Station and a halo around the Moon
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 Wiadomości z astronet.pl

› Co marsjańskie trzęsienia ziemi mówią o jego historii
› Katalog Caldwella: C75
› Silne dowody na atmosferę na skalistej egzoplanecie
› Przełomowe odkrycie! Pierwsza planeta swobodna odkryta i ,,zważona” przez polskich naukowców
› Rozsiewanie nasion za pomocą satelity – projekt Greenstar
› Katalog Caldwella: C98
› Niebo w styczniu 2026 roku
› Podsumowanie roku 2025 w astronomii i astronautyce
› Katalog Caldwella: C19
› Misje kosmiczne XX wieku: Program Landsat
RSS  Najnowsze prace na astro-ph:

› Predictability of bursts of a recurrent nova using topological data analysis and machine learning
› Exactly solved model of a one dimensional self gravitating system
› Experiments in binary evolution
› Validation of Satellite Lifetime Predictions at Leonid Space
› Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
› Magnetic reconnection with a 0.1 rate: Effective resistivity in general relativistic magnetohydrodynamics
› Neutrino flavor instabilities in neutron star mergers with moment transport: slow, fast, and collisional modes
› Exposure-averaged Gaussian Processes for Combining Overlapping Datasets
› Electron temperature relations and the direct N, O, Ne, S and Ar abundances of 49959 star-forming galaxies in DESI Data Release 2
› A possible challenge for Cold and Warm Dark Matter
› On the exceptionality of exceptional gravitational-wave events
› Hunting for the First Explosions at the High-Redshift Frontier
› The Maximum Gravity Model for partial Tidal Disruption Events: Mass Loss, Peak Fallback Rate and Dependence on Stellar Properties
› Towards a global model for planet formation in layered MHD wind-driven discs: A population synthesis approach to investigate the impact of low viscosity and accretion layer thickness
› Cosmic Chance Superpositions: Largest Catalog of Quasar-Galaxy Pairs at a Projected Separation of $D \lesssim 20$ kpc
› Resolving the Fe K$\alpha$ Doublet of the Galactic Center Molecular Cloud G0.11-0.11 with XRISM
› CHANG-ES XXXVI. Effects of spectral aging on radio scale heights
› Models and Observational Predictions of Dust Traps in Protoplanetary Discs
› Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN
› The intermediate neutron capture process. VI. Proton ingestion and i-process in rotating magnetic asymptotic giant branch stars
› Dynamical Origins of Azimuthal Metallicity Variations in the Galactic Disk: Insights from Kinematic Ridges with Gaia
› Gas rotation and turbulence in the galaxy cluster Abell 2029
› Dynamically consistent analysis of Galactic WN4b stars
› Star Formation in Galaxy Collisions: Dependence on Impact Velocity and Gas Mass of Galaxies in GADGET-4 Simulations
› The origin of strong $\alpha$-element bimodalities in FIRE simulations of Milky Way-mass galaxies
› Scalable Gaussian Processes for Integrated and Overlapping Measurements Via Augmented State Space Models
› Catching 3I/ATLAS Using a Solar Oberth
› Composite Bulges - V. Detecting signatures of gas inflows in IFU data: The MUSE view of ionised gas kinematics in nearby galaxies
› Tracing Pebble Drift History in Two Protoplanetary Disks with CO Enhancement
› Dearth of Photosynthetically Active Radiation Suggests No Complex Life on Late M-Star Exoplanets
› Using 23 Years of ACS/SBC Data to Understand Backgrounds: Significant Reductions in Expected Background Levels
› The Lazuli Space Observatory: Architecture & Capabilities
› Optomechanical platform for high-frequency gravitational wave and vector dark matter detection
› COUGS-DESI: A Catalog of Unusual Galaxies with Polar Structures in the DESI Legacy Imaging Surveys
› Isotopic Ratios in the Disk of HD 163296
› Meteor observations as a tool to constrain cosmogonic models of the Solar System
› Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations
› Where does the simplified Stellar Contamination Model fail in Exoplanet Transmission Spectroscopy?
› E-XQR-30: Evidence for an Increase in the Ionization State of Metal Absorbers from z~6 to z~2
› Quantifying the Contamination of TESS Ecliptic-Plane Light Curves by Minor Planets
› SN 2024abfl: A Flat-Plateau, Low-Luminosity Type IIP Supernova with Early CSM Interaction
› TOI-4495: A Pair of Aligned, Near-Resonant Sub-Neptunes that Likely Experienced Overstable Migration
› The Origin of Spin-Alignment of Dark Matter Subhalos
› The Study of a Cosmic Ray Candidate Detected by the Askaryan Radio Array
› A Tale of Two Dust Disks in Our Milky
› Super-Orbital Variations in Magnetar Rotation Measure Arising from the Precession of Companion Star: Implications for FRB 20220529
› A Galactic Supernova Remnant Candidate at l =25.8, b=+0.2 Revealed by Near-Infrared Imaging and Spectroscopy
› Finite Plasma Beta Three-dimensional Magnetic Field Extrapolation Based on MHD Relaxation Method
› SpaceWire-based Data Acquisition Network for the Solar Flare Sounding Rocket Experiment FOXSI-4 and FOXSI-5
› Indications of a Late-Time Transition to a Strongly Interacting Dark Sector
› A New Collision Avoidance Fiber Assignment Algorithm for Robotic Fiber Positioners in Multi-Object Spectroscopy
› Transient Large-Scale Anisotropy in TeV Cosmic Rays due to an Interplanetary Coronal Mass Ejection
› Beyond Sgr A* and M87*: Sub-Microarcsecond Black Hole Shadow Detection via Lunar-based Extremely Long Baseline Interferometry
› Nonlinear Weak Lensing reconstruction for Galaxy Clusters
› Studying the surface effect in Procyon A as an F-type star
› Investigating the Anisotropy of Dispersion Measure Contribution from the Galactic Halo by Using Fast Radio Bursts
› BEACON: JWST NIRCam Pure-parallel Imaging Survey. II. Physical Properties of $z=7-14$ Galaxies
› GATOS XI : Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI
› Measuring the homogeneity scale using the peculiar velocity field
› Probing ionized bubbles around luminous sources during reionization with SKA 21-cm observations
› Asteroseismology of solar-like oscillators: emulating individual mode frequencies with a branching neural network
› Discovery of an Extremely Luminous Type II Cepheid in the Andromeda Giant Stellar Stream: Evidence for a Hierarchical Triple with an Inner Binary Merger
› Polarization of the CMB in the Standard Model Extension
› Mean opacity tables for probing the interior and atmosphere of giant planets
› Bounce Inflation with Dynamical Dark Energy in Light of DESI DR2
› The winds of OBA hypergiants and luminous blue variables: Dynamically-consistent atmosphere models reveal multiple wind regimes
› A Long Tidal Feature Extending from a Low-Redshift Galaxy Revealed in Rubin Data Preview 1 Imaging
› Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
› Large-scale radio bubbles around the black hole transient V4641 Sgr
› Helioseismic Evidence That the Solar Dynamo Originates near the Tachocline
› The Squeezed Bispectrum from CHIME HI Emission and Planck CMB Lensing: Current Sensitivity and Forecasts
› Heavy Black-Holes Also Matter in Standard Siren Cosmology
› Spectral Properties and Energy Injection in Mercury's Magnetotail Current Sheet
› Primordial Black Hole Formation in $f(R)=R+\alpha R^2$ Gravity: Perturbative and Non-Perturbative Analysis
› Resonances in b-EMRIs: playing the black hole piano
› Orchestral AI: A Framework for Agent Orchestration
› Utilizing anticoincidence veto in a search for gravitational-wave transients
› A Universal Upper Bound on the Pressure-to-Energy Density Ratio in Neutron Stars
› Inflation in Extra-Dimensions with one or two branes
› Standard Model Higgs Peaks: a Note on the Vacuum Instability during Inflation
› Extended Very-High-Energy Gamma-Ray Emission Surrounding PSR J0622 + 3749 Observed by LHAASO-KM2A
› Discovery of the Ultra-high energy gamma-ray source LHAASO J2108+5157
› Discovery of a new $\gamma$-ray source LHAASO J0341+5258 with emission up to 200TeV
› Constraints on heavy decaying dark matter from 570 days of LHAASO observations
› An Ultrahigh-energy $\gamma$-ray Bubble Powered by a Super PeVatron
› Evidence for particle acceleration approaching PeV energies in the W51 complex
› Deep view of Composite SNR CTA1 with LHAASO in $\gamma$-rays up to 300 TeV
› An Enigmatic PeVatron in an Area around HII Region G35.6$-$0.5
› Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization
› Constraining the Cosmic-ray Energy Based on Observations of Nearby Galaxy Clusters by LHAASO
› Unifying Circumstellar Environment in Broad-Lined Type Ic Radio Supernovae Towards Off-axis Gamma-Ray Burst Exploration
› Water ice in the debris disk around HD 181327
› Going beyond $S_8$: fast inference of the matter power spectrum from weak-lensing surveys
› Constraining the Stellar-to-Halo Mass Relation with Galaxy Clustering and Weak Lensing from DES Year 3 Data
› Helium Atmospheres May Hide in Current Exoplanet Analysis Frameworks
› Effective Theories of Redshift-Space Galaxy Peculiar Velocities
› Cosmological Constraints on $f(T,B)$ Gravity from Observations of Early and Late Universe
› Supermassive black hole growth from stellar binary encounters
› A census of quiescent galaxies across $0.5 < z < 8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
› Forecasts of constraining isotropic cosmic birefringence on AliCPT-1
› The Advanced X-ray Imaging Satellite (AXIS) Community Science Book
› LHAASO Detection of Ultra-High-Energy Gamma-Ray Emission toward the Giant Molecular Clouds
› Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles
› Starlight-driven flared-staircase geometry in radiation hydrodynamic models of protoplanetary disks
› Delayed Wind Onset in Pa 30, the Remnant of Type Iax SN 1181
› Excitation of Inertial Modes in 3D Simulations of Rotating Convection in Planets and Stars
› Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5
› Spaceflight KID Readout Electronics for PRIMA
› Squared-field cross-correlation between kinetic Sunyaev-Zel'dovich effect and 21-cm intensity mapping
› A high-dynamic-range view of the growth of structure and the warm/hot Universe
› Cygnus X-3: A variable petaelectronvolt gamma-ray source
› Energy-Dependent Shifts of Medium-Scale Anisotropies in Very-High-Energy Cosmic Rays Observed by LHAASO-KM2A
› The Milky Way Bulge Extra-Tidal Star Survey: NGC 6569
› Turbulence-Driven Corrugation of Collisionless Fast-Magnetosonic Shocks
› Decoding Cygnus X-2: The Critical Role of Reflection in IXPE Data
› Inferring physical parameters of solar filaments from simultaneous longitudinal and transverse oscillations
› The Betelgeuse Enigma: The Betelbuddy Hypothesis
› Monitoring the daily variation of Sun-Earth magnetic fields using galactic cosmic rays
› Measurement of attenuation length of the muon content in extensive air showers from 0.3 to 30 PeV with LHAASO
› Dipole Polarizability of Finite Nuclei as a Probe of Neutron Stars
› How to obtain slow roll inflation driven by non-linear electrodynamics
› Physics beyond the Standard Model with the DSA-2000
› Freeze-in production of scalaron dark matter in $f(R)$ gravity
› Implications of DESI for Dark Matter & Cosmic Birefringence
› Classification of $f(R)$ Theories Of Inflation And The Uniqueness of Starobinsky Model
› Beyond $\rho^{2/3}$ Scaling: Microscopic Origins and Multimessengers of High-Density Nuclear Symmetry Energy
› Observable Signatures of a Quarkyonic Phase in Neutron Stars
› On the Bondi accretion of a self-interacting complex scalar field
› Graviton-Photon Mixing by a Kerr-Newman Black Hole with Worldline EFT

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