Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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7.3 °C

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11.3 km/h

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1010.4 hPa

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 Wiadomości z astronet.pl

› Katalog Caldwella: C54
› Misje kosmiczne XX wieku: Program Discovery
› Powrót po serii porażek. Ostatni lot rakiety Alpha Block 1
› Do 20 marca zapisy do konkursu Łowcy Cząstek 2026
› Katalog Caldwella: C64
› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
› Niebo w marcu 2026 roku
› Artemis III nie wyląduje na Księżycu. NASA ogłasza duże zmiany
› Startrails, czyli najprostszy astrokrajobraz
› W Układzie Słonecznym: Granice Układu Słonecznego
RSS  Najnowsze prace na astro-ph:

› A simulation-based inference of the Milky Way merger history
› Phenomenology of an Open Effective Field Theory of Dark Energy
› Simulating AGN wind feedback with variable feedback efficiencies in idealised disc galaxies
› A Hot DOG Forged in FIRE: Nuclear and Starburst Spectral Decomposition of a Luminous Infrared Galaxy Simulation with a Resolved Dust Torus
› Fast Fourier Transform evaluation of the Fresnel integral for gravitational-wave lensing
› Probing Cosmology through Higher-Order CMB Lensing Statistics
› Microquasar remnants as reservoirs of PeV cosmic rays
› Reheating with Axion-SU(2) and Gravitational Chern-Simons Couplings
› Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS and Insights into the Neptunian desert around M dwarfs
› Robustness of Neural Networks for CMB Polarization Foreground Removal
› The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
› HaloFlow II: Robust Galaxy Halo Mass Inference with Domain Adaptation
› Gravitational self-lensing of Fast Radio Bursts in neutron star magnetospheres: II. Applications to strong repeaters and the CHIME population
› SPHEREx Wide-Field Infrared Spectral Mapping of Interstellar Ices and Polycyclic Aromatic Hydrocarbons
› Long-term monitoring of WASP-19 b: Signs of apsidal precession and molecular signatures
› Refinements to the Solar Polar Magnetic Flux: Implications from Inversion Methodologies
› Integral Field Spectroscopy of Collisional Ring Galaxies I: Stellar Populations Analysis
› Standard Perturbation Theory for Interacting Dark Sector cosmologies I: Breakdown of Einstein de Sitter kernels
› Relativistic astrospheres of gamma-ray binaries: modeling of non-thermal processes
› Bridging the Gap: Using Brown Dwarfs to Examine Silicate Clouds in Giant Exoplanet Atmospheres
› Exploring Beyond {\Lambda}CDM with the Weak Lensing Power Spectrum and Bispectrum
› Spatial and spectral constraints on resolved mass-loss of the massive Post-RSG star IRAS 17163-3907 and its Fried Egg Nebula
› Hot Jupiter - Cold Jupiter: A complex sibling relation
› Sound Speed Resonance in the Gravitational Wave Background as a probe for non-standard early universe cosmologies
› Galaxy fly-bys sustain bar-halo friction and bar slowdown in disk galaxies
› Spectral Dataset of Stripped-Envelope Supernovae from the Tsinghua Supernova Group
› Slowly Rotating Two-Fluid Neutron Stars: Coupled Frame-Dragging, Inertia Splitting, and Universal Relations
› Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope
› Beyond the Merger-Quasar-Quench Paradigm I: Mergers are neither necessary nor sufficient to quench central galaxies in IllustrisTNG
› The influence of plasma lensing magnification to the luminosity function of fast radio bursts
› Bolometric corrections of stellar oscillation mode amplitudes as observed by the PLATO mission. I. Planck-spectrum estimates
› Chemical Properties and Sagittarius-induced Dynamical Perturbations of the GD-1 Stream
› Spectroscopical Confirmation and Lens Modeling of a Complex Strong Lensing System Produced by a Close Galaxy Pair at $z_d=0.79$
› Halo abundance and clustering in cosmologies with massive and asymmetric neutrinos
› A Census of Active Galactic Nuclei Identified by the Mid-infrared [Ne v] Line at $\boldsymbol{z \leq 0.025}$
› Gaia GraL X.: The GraL catalogue of gravitationally lensed quasars Matched with \textit{Gaia} data, redshifts, and time delays
› Does supernova feedback regulate the star formation rate in dwarf galaxies?
› Scrutinizing the 2020 multiwavelength outburst of PKS 0903-57 through observations with H.E.S.S
› exoALMA XXI: The Morphology and Dynamics of Vertical Flows
› Hub Formation and Filament-Filament Collision: An Analytical Model
› ZTF J021804.16+071152.93: a dead cataclysmic variable and potential solution to the missing period bouncers
› WISDOM Project -- XXVIII. Molecular gas measurement of the supermassive black hole mass of the galaxy NGC 1387
› MAXI J1820+070: A rapidly spinning black hole with mild disk truncation in the soft state and a warm corona
› A low mass and radius neutron star candidate in XTE J1810-189?
› Tied-array beam flatfielding
› A near field guide to Roman's wide-area surveys
› Detection of a molecular hydrogen envelope around nova GK Persei
› Are supernovae driving turbulence in the solar neighborhood?
› Calibrating Galaxy Infall Times in Groups and Clusters with IllustrisTNG Simulations
› Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS
› exoALMA XXII: A Two-dimensional Atlas of Deviations from Keplerian Disks
› Towards the Two-Loop EFTofLSS in Galaxy Lensing Surveys
› A unified harmonic framework for dark siren cosmology
› Impact of stellar spots on the high-resolution transmission spectra of a giant planet around a Sun-like star
› IceCube Search for MeV Neutrinos from Mergers using Gravitational Wave Catalogs
› Three-band dark-siren cosmology with intermediate-mass black hole binaries: synergy of Taiji, LGWA, and Einstein Telescope
› exoALMA. XXIV. Formaldehyde Emission in Protoplanetary Disks of exoALMA Compared with Their Properties and Dynamical State
› Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms
› Modelling the expulsion of baryons from haloes from first principles: the role of feedback and of the cosmological constant
› Ridged Lagrangian Perturbation Theory (RLPT)
› The elusive cyclotron line in 4U 1901+03: hidden, yet present
› When Dark Energy Turns On: Constraints on a Critical Emergence Model
› Structural Parameters of the Globular Cluster M 15
› Euclid preparation. Simulated galaxy catalogues for non-standard cosmological models
› exoALMA XXIII. Estimating Disk and Planet Properties from Dust Morphologies with DBNets2.0
› exoALMA XX: Tomographic Detection of Embedded Planets in Protoplanetary Disks
› Connecting JWST Silicate Cloud Observations to Exoplanet Cloud Microphysics with Nimbus
› Ortho-Para Chemistry of H2CO in the Protoplanetary Disk TW Hya
› Clustering Astronomical Orbital Synthetic Data Using Advanced Feature Extraction and Dimensionality Reduction Techniques
› Euclid preparation. Far-infrared predictions for Euclid galaxy catalogues: cluster, protocluster, and field
› Optimising Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
› A Commensal Radio-Only Cosmic Ray Detector at the Owens Valley Radio Observatory Long Wavelength Array
› Negative Masses and Spatial Curvature: Alleviating Neutrino Mass Tensions in LambdaCDM and Extended Cosmologies
› Comparison of Cross-Correlation Methods for Line Intensity Mapping
› A 2% determination of $N_{\rm eff}$ from primordial element abundance, cosmic microwave background, and baryon acoustic oscillation measurements
› Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator
› Dark Matter, Baryon Number, and Cosmic-Ray Antinuclei
› All-electron dark matter-electron scattering with random-phase approximation dielectric screening and local field effects
› Traversable Wormholes induced by Thomas-Fermi energy density
› Weibel Instability in Collisionless Plasmas Across Astrophysical and Laboratory Shocks
› Not So Minimal Warm Inflation
› Design of a Dichroic Transmissive Huygens' Metasurface Unit-Cell Presenting Refraction Angle Duality
› A basic model for high energy cosmic ray interactions
› The Migdal effect in Semiconductors for the Effective Field Theory of Dark Matter Direct Detection
› Axion search with telescope for radio astronomy (ASTRA): forecast for observations between 0.5 and 4~GHz
› Challenging the Weak Cosmic Censorship with Phantom Fields
› Disentangling the anisotropic radio sky: Fisher forecasts for 21cm arrays
› BICEP/Keck XIX: Extremely Thin Composite Polymer Vacuum Windows for BICEP and Other High Throughput Millimeter Wave Telescopes
› Toward a Distributed Radio Telescope Using Global IoT Networks: Calibration Methods and Feasibility Analysis
› Continuous Design and Reprogramming of Totimorphic Structures for Space Applications
› Estimating the Lensing Probability for Binary Black Hole Mergers in AGN disk by Using Mismatch Threshold
› Implementation of CR Energy SPectrum (CRESP) algorithm in PIERNIK MHD code. II. Propagation of Primary and Secondary nuclei in a magneto-hydrodynamical environment
› Exploring future synergies for large-scale structure between gravitational waves and radio sources
› Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
› Revealing tensions in neutron star observations with pressure anisotropy
› Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach
› Diversity and Evolution of Dust Attenuation Curves from Redshift z ~ 1 to 9
› Optimized HDBSCAN clustering for reconstructing the merger history of the Milky Way: applications and limitations
› DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
› Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
› The causal structure of galactic astrophysics
› Elusive Plunges and Heavy Intermediate-mass-ratio Inspirals from Single and Binary Supermassive Black Holes
› Saving Doomed Planets: Mass Loss and Angular Momentum Return Boost Hot Jupiter Survival Rates
› Solving the cooling flow problem with combined jet-wind AGN feedback
› Finding the boundary: Using galaxy membership to inform galaxy cluster extent through machine learning
› Gas excitation of post-starburst galaxies at 0.6 < z < 1.3
› Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension
› Optical and cm follow-ups of the Changing-Look event in Mkn 590
› Enhancing evidence estimation through informed probability density approximation
› Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
› Primordial Black Holes as Seeds for Extremely Overmassive AGN Observed by JWST
› An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4
› Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots
› Unveiling the spectral morphological division of fast radio bursts with CHIME/FRB Catalog 2
› A positive period derivative in the quasi-periodic eruptions of ZTF19acnskyy
› A Catalogue of Orbital Periods of Cataclysmic Variables and Candidates from TESS Observations
› Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate
› Martian concretion sizes predicted from two independently constrained inputs: atmospheric dust grain size and obliquity-forced wetting duration
› FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology
› Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion
› SN 2023axu: A Type IIP Supernova Interacted with a Low-Density Stellar Wind
› Solar neutrino physics
› A Traveling-Wave Parametric Amplifier and Converter
› Multifield theories invariant under transverse diffeomorphisms: The mixed regime case
› Cosmic Axion Background Detection Using Resonant Cavity Arrays
› A dynamical systems perspective on the thermodynamics of late-time cosmology
› Efficient Reconstruction of Matched-Filter Signal-to-Noise Ratio Time Series from Nearby Templates for Compact Binary Coalescences Searches
› Natural inflation in Palatini $F(R)$
› Small-scale turbulent dynamo for low-Prandtl number fluid: comparison of the theory with results of numerical simulations
› Simulating first-order phase transition during inflation
› Accelerating Black Hole Image Generation via Latent Space Diffusion Models
› Detectability Scaling Laws for Environmental Phase Modulation in Gravitational-Wave Signals

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