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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Temperatura
7.6 °C

Wilgotność
 44%

Wiatr
12.9 km/h

Ciśnienie
1023.6 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

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› Tam, gdzie SPACE spotyka DEFENCE. SpaceShield Summit 2026 – ostatnie wolne miejsca!
› Misje kosmiczne XX wieku: program Sojuz
› Pixinsight cz. VII – XTerminatory
› Stany Zjednoczone odtajniły informacje o programie satelitów szpiegowskich JUMPSEAT
RSS  Najnowsze prace na astro-ph:

› UK White Paper on Magnetohydrodynamic (MHD) seismology of solar and heliospheric plasmas
› ENhanced Galactic Atmospheres With Arepo: Resolving the CGM at 200 pc with the ENGAWA Simulations
› The TESS All-Sky Rotation Survey: Periods for 944,056 Stars Within 500 pc
› Predictions of Imminent Earth Impactors Discovered by LSST
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion
› The Extremely Large Telescope Interferometer
› Solar Irradiance Reconstruction over the Telescopic Era Using a Revised Photospheric Magnetic Field Model
› Consistent Gas-Phase Temperatures and Metallicities from UV and Optical Nebular Emission: A Reliable Foundation from z=0 to Cosmic Dawn
› X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates
› Weighing gas-rich starless halos: dark matter parameters inference from their gas distributions
› Vertical Structure of Protoplanetary Disks in Scattered Light: A large sample analysis
› Exocomets of $\beta$ Pictoris II: Two dynamical families of exocomets simulated with REBOUND
› Long-Integration Magnetar Burst Observatory (LIMBO): Instrument Summary and Early FRB Rate Constraints
› The case of NGC 5824, a cluster possibly embedded in a dark matter halo
› Thermal Electrons in an Ultra-Relativistic Shock Shape the Optical Afterglow of GRB 250702F
› A cationic carrier for diffuse interstellar band at 862.1 nm: Evidence from the skin effect in nearby diffuse-to-translucent clouds
› Active regions and the large-scale magnetic field of solar cycle 24
› A search for optical counterparts in quiescent black hole X-ray transients
› SuperSNEC: Fast and Accurate Light Curve Production for Large Hydrodynamic Model Grids Using Adaptive Gridding
› Determination of the Height-Temperature Profile Above a Solar Active Region from Multi-Frequency Radio Observations
› Photodynamical modeling of TOI-4504 reveals its deeply resonant state and similarity to GJ 876
› Fingerprints of Individual Supermassive Black Hole Binaries in Pulsar Timing Arrays
› Case study of a national-level academic conference organised in hybrid mode at low cost
› Multiwavelength quasi-periodic variability of the blazar Ton 599
› An updated model for the Perseus Spiral Arm from Trigonometric Parallax and 3D kinematic distances of distant young stars
› Confirmation and Refutation of Lyman Continuum Leakers at $z\sim3$ with JWST NIRSpec/IFU
› CTAO Simulations for Potential PeVatron Candidates
› Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
› Extremely Metal-Poor Galaxies in DESI DR1: Connections to Galaxies in the Early Universe
› SwinYNet: A Transformer-based Multi-Task Model for Accurate and Efficient FRB Search
› The MeerKAT 1.3 GHz survey of the Large Magellanic Cloud: Point Source Catalogue
› Indications of electron-to-proton mass ratio variations in the Galaxy. III. 0.6mm methanol lines toward SgrB2(N) and Orion-KL
› Investigating the Circumnuclear Medium of Tidal Disruption Events with Radio Observations
› X-Ray Intraday Variability of the Blazar OJ 287 Observed with XMM-Newton
› Variability Study and Searching for QPOs with day-like periods in the blazar S5 0716+714 with TESS
› Accretion dynamics and coronal geometry in Mrk 530: Insights from 24 years of X-ray monitoring
› Untangling dust emission and CIB anisotropies with the Scattering Transform Statistics
› Detection of quasi-periodic oscillations in the 37 GHz radio light curve of the blazar Ton 599 during 1990-2020
› Global Abiotic Sulfur Cycling on Earth-like Terrestrial Planets
› Search for Periodic Radio Signals from Double Neutron Star System Companions Using the Fast Folding Algorithm
› Size measurements and characterization of the astrophysical properties of multiple-component radio-AGNs in the ROGUE I catalog
› Mid-infrared Variability-based AGN Selection using the Multi-epoch Photometric Data from WISE
› Fundamental properties of protoplanetary discs determined from simultaneous fits to thermal dust images and spectral energy distributions
› The contribution to Galactic Centre {\gamma}-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations
› Star-based Navigation in the Outer Solar System
› The trigonometric parallax of IRAS 23385+6053 and physical properties of molecular clouds based on the VLBI astrometry
› Polarized quasi-periodic oscillations reveal kink instability in magnetized jets of black holes
› Motional induction in Ganymede's ocean
› Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores
› Enhancing Gravitational Lens Study with Deep Learning: A Study on Effects of Dropout Regularization
› Disentangling the Galactic binary zoo: Machine learning classification of stellar remnant binaries in LISA data
› Searching for outbursts from Symbiotic Binaries in GOTO and ATLAS data
› Generation of Imaging Air Cherenkov Telescope images using Diffusion Models
› Survival of ultraheavy nuclei in astrophysical sources: applications to protomagnetar outflows
› WIMP Dark Matter Searches in Reticulum II Using MeerKAT
› Molecular Clouds Resolved at the Onset of Cosmic Noon
› The Collective Voice of Ly$\alpha$ Emitters: Insights from JWST Stacked Spectroscopy
› Ly{\alpha} Nebulae in HETDEX: The Largest Statistical Census Bridging Ly{\alpha} Halos and Blobs across Cosmic Noon
› Velocity dispersion of Solar Energetic Particles in turbulent heliosphere
› Efficient Numerical Evaluation of a Two-Loop Contribution to the Dark-Matter Trispectrum
› Formation of mega-parsec giant radio sources from hosts residing in dark matter halos of different masses and with normal hot baryonic gas fractions
› MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z \sim 2.5$
› Angular momentum drives proton-rich nucleosynthesis in hyperaccreting neutron stars in common envelopes
› Unbiased Bayesian Inference of Peculiar Motions of Galaxies from Type Ia Supernovae Observations
› WALLABY pilot survey: Blinded by the light -- discovery of a fourth member in the ESO 179-013 system
› Discovery and Timing of the First Millisecond Pulsar in NGC 6316
› The Baryonic Mass-Halo Mass Relation of Extragalactic Systems
› Galaxy UV Legacy Project: Survey Description and First Insights Into NGC 4449 Recent History of Star Formation
› Constraining turbulent solar flare acceleration regions by connecting kinetic modeling and X-ray observations
› Comment on: "Third-order corrections to the slow-roll expansion: Calculation and constraints with Planck, ACT, SPT, and BICEP/Keck [2025 PDU 47 101813]"
› Kinematically Coherent Multiphase Galactic Winds in Star-Forming Galaxies Revealed by Unified Radiative Transfer Modeling of UV Emission and Absorption Lines
› Data-Driven Trends and Subpopulations in the Gravitational Wave Binary Black Hole Merger Population with UMAP
› The Prevalence of Turbulence-Regulated Multiphase Galactic Winds in Star-Forming Galaxies
› Environmental Measurements in the Sedrun Access Shaft to the Gotthard Base Tunnel -- a Promising Site for a Long-Baseline Atom Interferometer
› On the Value of Tokeniser Pretraining in Physics Foundation Models
› The continuum spectrum of nonrelativistic multi-frequency Proca stars
› Pathologies of dimension-zero scalar fields
› Searching for precessing binary systems with mode-by-mode filtering and marginalization
› Black Hole Vision: An Interactive iOS Application for Visualizing Black Holes
› Accelerated Time-domain Analysis for Gravitational Wave Astronomy
› Inverse-mapped density-dependent relativistic mean-field inference of the neutron-star equation of state with multi-messenger constraints
› Latin American HECAP Physics Briefing Book 2025
› Revisiting unitarity of single scalar field with non-minimal coupling
› Implications for Type Ia Supernova Nucleosynthesis from an Experimentally Constrained $^{16}$O$(p,\alpha)^{13}$N Reaction Rate
› A High Efficiency Superconducting On-chip Filterbank with Directional Filters for Integral Field Units in the Sub-millimeter Regime
› The 2024 BBN baryon abundance update
› Scales of Stability and Turbulence in the Molecular ISM
› Dust Evolution in Simulated Multiphase Galactic Outflows
› Forward vs Backward: Improving BAO Constraints with Field-Level Inference
› Evidence for Hydrostatic Equilibrium in the Extragalactic Molecular Clouds of M31
› Large Language Models -- the Future of Fundamental Physics?
› DESI DR2 reference mocks: clustering results from Uchuu-BGS and LRG
› PyBird-JAX: Accelerated inference in large-scale structure with model-independent emulation of one-loop galaxy power spectra
› Search for Signatures of Dark Matter Annihilation in the Galactic Center with HAWC
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: II. Super-Eddington Accretion
› Parity in Composite-Field Galaxy Correlators
› Effect of temperature on the structure of porous dust aggregates formed by coagulation
› Supernovae Exploding within Dense Extended Material: Early Emission Regimes and Degeneracies in Parameter Inference from Observations
› Excursion Set Approach to Primordial Black Holes: Cloud-in-Cloud and Mass Function Revisited
› Probing Primordial black holes with the distortion of Stochastic Gravitational Wave Background
› Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443
› A Large-Area Optical Time Projection Chamber for Hard X-ray Polarimetry with Directional Imaging of Low-Energy Electron Recoils
› Exoplanets synchronization in the habitable zone: Learning from Venus' retrograde rotation
› Bimetric MOND as a framework for variable-$G$ theories -- local systems and cosmology
› The maximum offsets of binary neutron star mergers from host galaxies
› Central flashes during stellar occultations. Effects of diffraction, interferences, and stellar diameter
› Star formation outside galaxies undergoing gravitational and hydrodynamic interactions: Dust attenuation and the star formation rate
› Quantifying the C/O Ratio in the Planet-forming Environments around Very Low Mass stars
› Formation of dust clumps in the torus of active galactic nuclei
› The hydrodynamics of stratified ultra-relativistic outflows and the origin of GRB X-ray plateaus
› A New Method for Identifying Contaminating Sources and Locating Target Sources through the Cross-Arm Features of Micro Pore Optics
› GASTON-GP: Source catalogue and millimetre variability of massive protostellar objects
› Multimessenger Astronomy Beyond the Standard Model: New Window from Quantum Sensors
› A mock data challenge for next-generation detectors
› High-frequency gravitational waves from first-order phase transitions
› Scrutinizing Fermionic Dark Matter in Scotogenic Model with Low Reheating Temperature
› Rotating neutron stars within the macroscopic effective-surface approximation
› The trichotomy of primordial black holes initial conditions
› Unified Origin of Dirac Neutrino and Asymmetric Dark Matter Masses via a Dirac-Type Leptogenesis
› Mass-to-Horizon Entropic Cosmology: A Unified Thermodynamic Pathway to Cosmic Acceleration
› Limits on the mass of compact objects in Ho\v{r}ava-Lifshitz gravity
› An upper limit on cosmological chiral gravitational wave background

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