Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Artemis II – Welcome Home. Podsumowanie misji
› Sławosz Uznański-Wiśniewski uhonorowany tytułem doktora honoris causa Szkoły Głównej Handlowej w Warszawie
› Scanway S.A. i Łukasiewicz – ILOT łączą siły
› Najsłynniejsze zdjęcia Ziemi z kosmosu
› Misje kosmiczne XX wieku: program Energia-Buran
› Relacja z Zimowych Warsztatów Naukowych 2026 w Opolu
› Rekord odległości ludzi od Ziemi. Artemis II wraca do domu
› Spotkaj ekspertkę: Efekty misji IGNIS – kosmiczna opaska zdrowia
› Film poklatkowy (timelapse) w astrofotografii
› Start misji Artemis II – od podstaw
RSS  Najnowsze prace na astro-ph:

› Consistent Treatment of Muons in Binary Neutron Star Mergers
› Could the high-mass black holes from gravitational-wave observations be explained by lensing?
› Deep Imaging Meets Motion: Complementing Stream Photometry Through Planetary Nebula Kinematics
› Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
› Combining spectroscopy and wavefront control at deep contrast with photonic lanterns
› Stream on: Evolution of stellar shells and streams - A case study
› The splash beneath the largest radio bubble in a cluster core
› Rapid-response 1.3 mm Observations of GRB 260127A with the Submillimeter Array
› The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations
› An Improved Fit for Linear Halo Bias at High Redshift
› The azimuthal structure of magnetically arrested disks during flux eruption events
› The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect
› A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation
› A Fast and Physically Grounded Ocean Model for GCMs: The Dynamical Slab Ocean Model of the Generic-PCM (rev. 3423)
› GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at $z = 2.34$
› Simulating the interplay between the snowline pebble flux and ongoing planet formation and migration
› Thermophysical Properties of Europa's Surface Constrained by Galileo Photopolarimeter-Radiometer Temperature Measurements
› Synchrotron-cooled plasma distribution in the outer magnetosphere of a neutron star
› FAIR Universe Weak Lensing ML Uncertainty Challenge: Handling Uncertainties and Distribution Shifts for Precision Cosmology
› The Last Galactic Firework: Timing the last significant merger with stars, globular clusters and $\omega$Centauri
› Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope
› Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe
› The GECKOS survey: Resolving the molecular and ionised gas in the galactic outflow of ESO~484-036
› Discovery of low-redshift analogues to "Little Red Dots" in DESI: A later evolutionary stage of compact LRDs?
› Misaligned circumbinary discs around unequal-mass eccentric binaries: alignment, morphology, and binary accretion variability
› Impact of Baseline, Cadence, and Host Contamination on AGN Variability Metrics: A Systematic Study with ZTF
› Disk-like galaxies at 4 < z < 7.7 : JWST/NIRCam morphologies revealed by denoising VAE-GCNN classification
› Upper bound of ejecta mass in a nova outburst
› Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements
› Closing the Observational Gap in Cosmic Dynamics: AI-Enabled Reconstruction of the Universe's Vorticity and Rotational Flow Morphology
› Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway
› A simple yet effective model of galaxy mergers
› Tracking ionization balance in intergalactic medium and its implications towards metallicity
› Systematic assessment of disk truncation in the black hole X-ray binary Swift J1727.8-1613 using NICER
› FAST and Dark: A catalogue of Dark Galaxy Candidates within 50 Mpc
› Influence of winds on shocked magnetized viscous accretion flows around rotating black holes
› NOMAI : A real-time photometric classifier for superluminous supernovae identification. A science module for the Fink broker
› Deeper analysis of Fermi-LAT unassociated 4FGL J2112.5-3043 for possible identification
› Euclid. Populating a dark universe with galaxies using SciPIC
› Numerical investigation of particle acceleration at interplanetary shocks: diffusive and superdiffusive scenarios
› Sky background accounting in spectral infrared observations of extended objects at the Caucasus Mountain Observatory of the SAI MSU
› Microscopic primordial black holes as macroscopic dark matter from large extra dimensions
› ALMA-IMF XXII. Role of core subfragmentation in the IMF origin: Hierarchical fragmentation cascade and CMF in W43-MM1
› Enhanced activity in close dual-AGN systems in the local Universe
› A simple relation: Neutron star magnetic field strength and spectral shape at low mass accretion rates
› Do galaxy mergers increase star formation and turbulence at cosmic noon?
› Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints
› A Generalized Algorithmic Framework for Detecting Faraday Rotation Measure Flares in Repeating Fast Radio Bursts
› The multi-planet system TOI-5624: four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
› Structure and Large-Scale Kinematics of Young Stellar Populations in the NGC 6357 and NGC 6334 Giant Molecular Cloud Complex
› Continuing to Advance European High Contrast Imaging Research and Development towards HWO and LIFE
› An FUor-like Outbursting Class I Protostar in NGC 7538
› Photometric Metallicities for 367,324 stars of Omega Centauri
› Localization and Confidence Region Estimation of Short GRBs with the COSI BGO Shield Using a HEALPix-Based Deep Learning Approach
› Las Cumbres Observatory Gravitational-Wave Follow-up in O3 and O4: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy
› Radiation doses during extreme solar energetic particle events
› Understanding the regulation of star formation within TNG100 galaxies on kpc-scales using machine learning I: Global versus local
› Stellar nucleosynthesis in the era of large surveys: s-process polluted binaries in GALAH DR4
› Photometry and physical characterization of near-Earth asteroid 2025 FA$_{22}$ from one apparition
› Tracing evolutionary pathways of bar-driven quenching in local Universe disc galaxies
› Nonperturbative stochastic inflation in perturbative dynamical background
› Age bimodality in pseudo-bulges of barred spiral galaxies: Bar-driven evolution across cosmic time
› Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra
› Cloudy with a chance of metals: Indications of CO$_2$ in the atmosphere of GJ 1214 b from high-resolution K-band spectroscopy
› A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
› Gravitational-wave lensing beyond rays: a disordered-system approach
› Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment
› Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries
› Quantum correction to the diffusion term in stochastic inflation from composite-operator matching in Soft de Sitter Effective Theory
› Emergent structure in the binary black hole mass distribution and implications for population-based cosmology
› Astrophysical bounds on the high-energy evolution of neutrino mixing
› Inflaton Regeneration via Scalar Couplings: Generic Models and the Higgs Portal
› Exploring non-equilibrium effects in sequential freeze-in
› Nonlinear backstepping with saturation for low-thrust station-keeping of libration point orbits
› Static Tidal Perturbations of Relativistic Stars: Corrected Center Expansion and Love Numbers-I
› Boson star-black hole binaries: initial data and head-on collisions
› Echoes of Global Cosmic Strings
› DESI Dark Secrets
› Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5
› Initial Characterization of Stellar Photometry of Roman images from the OpenUniverse Simulations
› From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
› Multidimensional Nebular-Phase Calculations of Dynamically-Driven Double-Degenerate Double-Detonation Models for Type Ia Supernovae
› A Systematic Search for Active Galactic Nucleus Flares in ZTF Data Release 23
› Using Symbolic Regression to Emulate the Radial Fourier Transform of the S\'ersic profile for Fast, Accurate and Differentiable Galaxy Profile Fitting
› Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger
› The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0
› Improving radial velocity precision with CARMENES-PLUS:An upgrade of the near-infrared spectrograph cooling system
› WaveDriver: a Laser Guide Star AO System for HWO
› Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman
› GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
› Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data
› Image reconstruction with the JWST Interferometer
› The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes
› High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4
› Nested Sampling for ARIMA Model Selection in Astronomical Time-Series Analysis
› Cosmic Duets I. High-spatial resolution spectroscopy of dual and lensed AGN with MUSE-NFM
› Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
› Constraining primordial non-Gaussianity from DESI DR1 quasars and Planck PR4 CMB Lensing
› New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
› Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration
› Polarimetry and albedo of the Near-Earth Asteroid 2025 FA22
› PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
› Spectral Hardening Revealed by Geometric De-boosting in the Masked Jet of PKS 2155$-$304
› CTAO Simulations for Potential PeVatron Candidates
› New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity
› Predictions of Stellar Occultations by Haumea and the Event of 4 May 2026
› Atmospheric Supply of Hydrogen Cyanide Is Not the Rate-limiting Step for Prebiotic Chemistry across Rocky Exoplanets
› Finding the elusive RR Lyrae companions via speckle imaging
› Holmberg IX: A Unique, Infant but Inactive Galaxy as Revealed via a Multiwavelength Approach
› Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates
› Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations
› Reionization Topology as a Probe of Self-Interacting Dark Matter
› Finite temperature effects on g-modes of inviscid neutron stars
› The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
› The DECam MAGIC Survey: Investigating the Jet Stellar Stream with Photometric Metallicities
› CHARA Interferometry and TESS Asteroseismology of the Core-Helium Burning Red Giant $\kappa$ Cyg
› CHILES XII: The H I evolution of Luminous Compact Blue Galaxies between 0
› Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
› A Salpeter-like filament linear density function across nearby molecular clouds
› Dark matter and modified gravity: Einstein clusters from a non-minimally coupled vector field
› WIMP/FIMP dark matter and primordial black holes with memory burden effect
› Asymmetric Cannibal Dark Matter: Constraints from Neutron Star
› Imperfect dark matter with higher derivatives
› Exact black holes and black branes with bumpy horizons supported by superfluid pions
› On the Cuspy Structure of Rotating Wormhole Shadows
› Towards a complete theory of thermal leptogenesis in the SM and MSSM

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