Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Nowe dowody dotyczące atmosfer w układzie TRAPPIST-1
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RSS  Najnowsze prace na astro-ph:

› Characterisation of all known multiple stellar systems within 10 pc
› Shaping the future of Global Interferometric Arrays: Imaging Strong Gravity and Magnetic Fields
› Galactic Amnesia: The Information Washout of the Milky Way Merger History
› The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
› The galaxy-halo connection and the dynamical evolution of a giant disc in a massive node of the Cosmic Web at z~3
› TOI-159 b: an eccentric hot-Jupiter planet around a young, pulsating $\gamma$ Doradus star
› On the spin dependence of the emergent gravity phenomena as observed in axially symmetric black hole accretion with spatially varying adiabatic index
› Overview of the New Hubble Spectroscopic Legacy Archive
› Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444
› Matter Clustering in Astrid: Reduced Baryonic Suppression from Realistic Black Hole Dynamics
› Multiwavelength Characterization of a New Magnetic Cataclysmic Variable 2CXO J050740.7-091337
› Impact of Climate States and Seasons on Future Exo-Earth Observations
› Taming Additive Systematics via Redshift-Bin-Optimized Star-Galaxy Separation
› Modeling Flare Continuum Emission Observed by Hinode/EIS: Instrument Calibration and Element Composition Results
› Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos
› Ensemble modeling of Coronal Mass Ejection dynamics and forecasts at 1 AU with a semi-analytic flux-rope model
› Neutrino Flavor Transformation in Collapsing Supermassive Objects
› Modeling Volcanic Plume Heights Across Exoplanet Atmospheres: Insights from TRAPPIST-1
› A CNN--Transformer Denoiser for low-$S/N$ Galaxy Spectra: Stellar Population Recovery in Synthetic Tests
› Nonlinear steepening of a fast magnetoacoustic wave in the vicinity of a coronal magnetic null point
› Beyond the $\alpha$ model: scaling the wind-driven accretion rate in protoplanetary disks using systematic non-ideal magnetohydrodynamical simulations
› Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations
› Investigating the Effects of Bars on Star Formation and Nuclear Activity of Galaxies Using DESI Survey Data
› HD3191, the high-mass X-ray binary that wasn't there
› The magnetic fields in Be stars are stronger than previously suggested
› Mitigating stellar radial velocity jitter using orthogonal activity indices and a time-aware neural network
› Spectroscopic Disentangling Revealed the Tertiary Component in the Multiple System EM Boo
› Spectro-Polarimetric Observations of TeV Sources (SPOTS): First results
› Dynamics and Radiative Signatures of Accretion Flows onto a Kerr-like Wormhole
› Revealing the cold skeleton of the Magellanic Clouds and the Magellanic Bridge with ASKAP
› A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling
› The MeerKAT Massive Distant Clusters Survey: a search for diffuse radio emission in 30 massive SZ-selected clusters at $z > 1$
› Compact, AGN-hosting Dwarf Galaxies with "Little Red Dots"-like SEDs in the Local Universe
› Theoretical Constraints on Neutron Star Superfluidity from Her X-1 Precession
› Activity and composition of periodic comets 67P/Churyumov-Gerasimenko and 103P/Hartley 2 at two different perihelion passages
› Confirmation of Binary Clustering in Gamma-Ray Bursts through an Integrated $p$-value from Multiple Nonparametric Tests of Hypotheses
› Redshift Evolution of the Ratio of Supermassive Black Hole Mass to Stellar Mass
› Statistical evidence for massive black hole recoils in active galactic nuclei
› Accessible does not mean exploitable: HiPERCAM reveals the ultra-fast rotation of 2022 OB$_5$
› The Next-Generation 21CMA Telescope: Design, Commissioning, and Instrumental Effects in an SKA-LFAA-Like System
› Exact solutions, trajectories and radiation patterns in the classical relativistic St\"{o}rmer problem
› Contribution of interstellar objects to local dark matter density
› Connecting the long-term variability behaviour of active galactic nuclei to their central engines
› Primordial black holes from inflation: on the decoupling between large and small scales
› AGILE detection of transient {\gamma}-ray emission from the region of the supergiant fast X-ray transient source IGR J17354-3255
› Earth and Mars interior structures set by re-melting of the first solid mantle
› Bayesian parameter estimation for the Core-bounce phase of Rapidly Rotating Core-Collapse Supernovae in real interferometric data
› Efficient estimators for power spectrum and bispectrum multipole measurements
› Exploration of the inner region of the system HD 142527
› Sensitivity of the Cherenkov Telescope Array Observatory to Gamma-Ray Signals in Dwarf Irregular Galaxies
› Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors
› Near-infrared diagnostic diagrams of the gas ionization sources in nearby galaxies: a JWST NIRSpec view
› Horizontal transport as a source of disequilibrium chemistry on the nightside of a hot exoplanet
› Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants
› Capturing statistical isotropy violation with rotational averages
› The one and the only: the pulsar - white dwarf system in NGC 6749
› First Detection of Extensive Air Showers Using a Small-Aperture Fluorescence Telescope
› The NUV transit of XO-3 b
› Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses
› A formation pathway for giant planets in S-type discs of {\gamma}-Cephei-like compact binaries
› Turbulent damping of fast tidal oscillations by three-dimensional Rayleigh-B\'enard convection with a radiating free surface
› Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges
› Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter
› Are PTA measurements sensitive to gravitational wave non-Gaussianities?
› A Compact Radio Ring with a Diffuse Envelope in LOFAR: Odd Radio Circle or Distinct Phenomenon?
› Non-conservation and time non-locality of biased tracers
› Segmenting proto-halos with vision transformers
› High-Power AM-CW Lunar Laser Ranging as a $\mu$Hz SGWB Detector
› Proton-Proton to Antinucleon Cross Sections for Cosmic Ray Applications
› Emergent gravity from nonlinear perturbation of spherical accretion with variable adiabatic index
› Three dimensional, spherically polarized magnetic fields
› Transport of electrons in tangled magnetic fields
› Landscape of Spontaneous CP Violation
› New Exponential and Polynomial $\xi$-attractors
› Charged current neutrino processes in hot nuclear matter with a recent Skyrme parametrization constrained by microscopic calculations
› Singlet-doublet dark matter induced radiative neutrino mass and TeV scale leptogenesis
› Phase Transitions and Gravitational Waves
› Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods
› Probing Low-Luminosity Gamma-Ray Emission from SNR G296.5+10.0 and CCO 1E 1207.4-5209 with CTAO
› Discovery and Timing of 49 Pulsars from the Arecibo 327-MHz Drift Survey
› Mass-dependent chemical enrichment sequences of SDSS star-forming galaxies out to z~0.3 revealed by direct O & Ar abundances
› An Alternative Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole
› The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at $z > 1$
› New Insights into Dark Energy from DESI DR2 with CMB and SNIa
› Wavefront super-resolution for Adaptive Optics systems on ground-based telescopes
› Future Parameter Constraints from Weak Lensing CMB and Galaxy Lensing Power- and Bispectra
› Generative AI for image reconstruction in Intensity Interferometry: a first attempt
› Primordial Black Holes Evaporating before Big Bang Nucleosynthesis
› Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
› Exploring the impact of AGN feedback model variations on the Lyman-$\alpha$ Forest Flux Power Spectrum
› Euclid preparation. XCVIII. Cosmology Likelihood for Observables in Euclid (CLOE). 5: Extensions beyond the standard modelling of theoretical probes and systematic effects
› Euclid preparation. XCVI. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and Forecasts
› Deep Learning in Astrophysics
› Egent: An Autonomous Agent for Equivalent Width Measurement
› EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction
› Eccentric Disks from Gaseous Rings around Equal-Mass, Circular Binaries
› Non-thermal particle acceleration in multi-species kinetic plasmas: universal power-law distribution functions and temperature inversion in the solar corona
› WISE/CatWISE Constraints on Dysonian Waste-Heat Technosignatures in Nearby Galaxies
› MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
› The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products
› Photometric Redshift PDFs via Neural Network Classification for DESI Legacy Imaging Surveys and Pan-STARRS
› The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A
› Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
› The multi-wavelength vertical structure of the archetypal $\beta$ Pictoris debris disk
› The emerging timescale of young star clusters regulated by cluster stellar mass
› The counterjet dominates the production of PeV photons from Cyg X-3
› The PLATO field selection process III. Selection of the Prime Sample for the LOPS2 field
› Neutron star atmospheres composed of fusion ashes
› Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS
› Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the far-Infrared in the Era of Next-Generation Radio Telescopes
› A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XXI. Statistical properties of individual HII regions in perturbed galaxies
› Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas
› Data-Constrained Modeling of Electron Transport and Asymmetric Precipitation in the 2011 August 4 Solar Flare
› Searching For Fast Radio Transients And Radio Pulsars Using SPOTLIGHT
› Curvature Perturbations from First-Order Phase Transitions: Implications to Black Holes and Gravitational Waves
› Does thermal leptogenesis in a canonical seesaw rely on initial memory?
› INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_{i}-L_{j}$ Vectors
› Constraints on the extreme mass-ratio inspiral population from LISA data
› Development and Testing of a Modular Large-Area Cosmic Ray Telescope Using Scintillator-Fiber Hybrid Design for Millimeter-Level Muon Tracking
› Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123
› The relativistic restricted three-body problem: geometry and motion around tidally perturbed black holes
› Photons x Force: Differentiable Radiation Pressure Modeling

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