Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› Uncertainty-Aware Solar Flare Regression
› The Cluster Evolutionary Reference Ensemble at Low-$z$ (CEREAL) Sample of Galaxy Clusters I: X-ray Morphological Properties and Demographics
› Thermalization of Neutrinos in a Neutron Star Merger Simulation
› Enhanced Neutrino Cooling from Parity-Doubled Nucleons in Neutron Star Cooling Simulations
› The Binary Populations of Stellar Streams are Set by Cluster Dynamics
› A differentiable and optimizable 3D model for interpretation of observed spectral data cubes
› Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
› BICEP/Keck XXI: Constraints on Early-Universe Parity Violation from Multipole-Dependent Birefringence
› Caught in the web: galaxy mergers along cosmic filaments
› On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints
› Study of UV line and continuum variabilities in the Broadline Seyfert 1 Galaxy ESO 141-G55
› Empirical signatures of velocity and density cascades in the Local Universe probed by CosmicFlows4 dataset
› A clean broad iron line in GS 1354--64 as seen by XRISM
› Estimating the completeness of the QUBRICS Survey with 3501 QSO redshifts from Gaia DR3 spectra
› Isotopic Evidence for a Cold and Distant Origin of the Interstellar Object 3I/ATLAS
› Imaging the disk-halo interface of NGC 891: a 2.7 kpc-thick molecular gas disk
› Different polarized components of the quasar 3C 286 revealed by FAST
› Effect of gravity-driven longitudinal flows in filaments on angular momentum transport to embedded cores
› Multi-wavelength ALMA Imaging of HD 34282: Dust-trapping Signatures of a Vortex Candidate
› Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation
› A Direct View of the Chemical Properties of Water from Another Planetary System: Water D/H in 3I/ATLAS
› Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission
› New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity
› Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC
› Supernovae interacting with Si and S-rich circumstellar matter from double white dwarf mergers
› Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor
› The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
› A Delayed Radio Flare Traces Kinetic Energy Injection in the SMBHB Candidate SDSS~J143016.05+230344.4
› Polarimetric Tomography Applied to Synthetic Multi-Spacecraft White-Light Images: Observing Coronal Mass Ejections in 3D
› Fuzzy Dark Matter and the Impact of Core-Halo Diversity on Its Particle Mass Constraints
› High nitrogen and carbon isotopic ratios in the interstellar comet 3I/ATLAS
› Understanding the formation and eruption of sigmoidal structure through data-driven modeling of magnetic evolution in solar active region 13500
› To What Extent Are Star Cluster Ages Encoded in Their Environments? Exploring the Spatial Distribution of Age-Related Information with PHANGS-HST Imaging and Convolutional Neural Networks
› Flip-flop states in X-ray binaries and changing-state AGN
› Broadband SETI: a New Strategy To Find Nearby Alien Civilizations
› A Reproducible Black Hole-Neutron Star Merger Gallery Example for the Einstein Toolkit
› Forecasting Catastrophe: Constraints on the Fomalhaut Main Belt Planetesimal Population from Observed Collisional Remnants
› Study of the cosmological tensions and DESI-DR2 in the framework of the Little Rip model
› Catching TeV emission from GRB 221009A and alike with LHAASO, LACT and SWGO
› New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences
› A jet formation model for astrophysical objects
› An Attempt to Search for Unintended Electromagnetic Radiation from Starlink Satellites with the 21 Centimeter Array: Methodology and RFI Characterization
› WD 1054-226 revisited: a stable transiting debris system
› Hydrogen photoionization in a magnetized medium: the rigid-wavefunction approach revisited
› Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets
› Inefficiency of chiral dynamos in protoneutron stars and the early universe
› Post-perihelion Coma Composition of the Interstellar Comet 3I/ATLAS from Optical Spectroscopy
› BlackGEM observations of compact pulsating stars: Mode identification for the DOV PG 1159--035 using multi-colour photometr
› Here Be SDRAGNs - Spiral Galaxies Hosting Large Double Radio Sources
› Discovery of a 36-minute long-period transient ASKAP J142431.2-612611
› Symmetry-Protected Momentum Exchange between Dark Matter and Dark Energy
› High-Energy Neutrino Emission in NGC1068 driven by Turbulent Magnetic Reconnection
› The Average Age Map of the Galactic Bulge
› Exploring the spin dependence on mass inclination and distance for the newly discovered black hole X-ray binary Swift J151857.0-572147
› Fine Structure and Formation Mechanism of a Sunspot Bipolar Light Bridge in NOAA AR 13663
› Structural Design and Performance Analysis of Laser Transmitting Telescope for Space Gravitational Wave Detection
› K-DRIFT Science Theme: New Theoretical Framework Using the Galaxy Replacement Technique for LSB studies
› Measuring the evolution of stellar bars with the host galaxy's spin
› Identifying Red Supergiants in the Local Group Using JWST Photometry. I. NGC 6822, Sextans A, NGC 300, WLM, and IC 1613
› Pre-Virialized Assembly at Cosmic Dawn: The Dynamics and Extreme Ionization of Compact Group CGG-z7 at $z\sim7.04$
› Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance
› s-process nucleosynthesis in low-mass AGB stars by the $^{13}$C($\alpha$,n)$^{16}$O neutron source
› One Hundred Years of Venus Polarimetry: PICSARR Observations of the Phase Curves
› Hydrocarbon complexity and photochemical shielding of prebiotic feedstock molecules in exoplanet atmospheres
› A probable inside-out dwarf nova outburst from the period bouncer candidate ASASSN-25dc
› Disc accretion onto a binary black hole in a hierarchical triple system as an origin of the most luminous hyper-soft sources
› Compression-Driven Kinetic Instabilities in Magnetically Arrested Disks
› A reaction-diffusion model for describing the ring/gap structure in disks surrounding individual young stars
› Homogenization of the Stetson Photometry with the BEST Database
› Double White Dwarf Mergers as Progenitors of Long-Period Transients
› Robust ellipticity measurements of 29 Galactic globular clusters
› How interacting winds shape the mechanical feedback of massive star clusters over millions of years
› Extreme mass loss during common envelope evolution: the origin of the double low-mass white dwarf system J2102--4145
› Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
› Non-common path aberration compensation and a dark hole loop with a pyramid adaptive optics system: Application to SAXO+
› ML in Astrophysical Turbulence I: Predicting Prestellar Cores in Magnetized Molecular Clouds using eXtreme Gradient Boosting
› Nonlinear evolution of unstable solar inertial modes: The case of viscous modes on a differentially rotating sphere
› Gas chemistry in the dust depleted inner regions of protoplanetary disks. I. Near-IR spectra and overtones
› Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactions
› LeMMINGs VII: 5 GHz, 50 mas e-MERLIN observations of a statistically complete sample of nearby AGN
› Systematic selection of surrogate models for nonequilibrium chemistry
› Evolution and formation of ultramassive white dwarf stars: The case for a 9Msun progenitor
› A GPU-Accelerated Transient Detection Pipeline for DECam Time-Domain Surveys
› An Alternate Pathway for H$_2$ Formation in the Early Universe: A physical process to account for the presence and coevolution of the luminous galaxies and supermassive black holes at the high redshifts
› Multimessenger Characterization of High-Energy Neutrino Emission from the Brightest Neutrino-Active Galactic Nuclei
› Very High Energy Gamma Rays from Ultra Fast Outflows
› Fundamental Limits of Quantum Sensors for Gravitational Wave Detection
› Spectral sirens cosmology from binary black holes populations with sharper mass features
› Low-Energy and Low-Thrust Exploration Tour of Saturnian Moons with Full Lunar Surface Coverage
› Shadows and Polarization Images of a Four-dimensional Gauss-Bonnet Black Hole Irradiated by a Thick Accretion Disk
› Gravitational waves from warm inflation in the weak dissipative regime
› MMS Observations of Kinetic Alfv\'en Wave Turbulence and Steep Kinetic-Range Spectra in the Outer Plasma Sheet Boundary Layer
› Local Origin of Hidden Symmetry in Rotating Spacetimes
› Spatiotemporal Properties of Compressible Magnetohydrodynamic Turbulence from Space Plasma
› A Deep Learning Framework for Amplitude Generation of Generic EMRIs
› Black Hole Mergers as the Fastest Photon Ring Scramblers
› Flash from the Past: New Gamma-Ray Constraints on Light CP-even Scalar from SN1987A
› A Remarkably Accurate Predictor of Sunspot Cycle Amplitude
› Quasi-steady emission from repeating fast radio bursts can be explained by magnetar wind nebulae
› Revisiting the Chern-Simons interaction during inflation with a non-canonical pseudo-scalar
› Chasing the light: Shadowing, collimation, and the super-Eddington growth of infant black holes in JWST broad-line AGNs
› Dynamical reconstruction of SPARC galactic halos within self-interacting fuzzy dark matter
› The cosmological Mass Varying Neutrino model in the late universe
› Principal Components for Model-Agnostic Modified Gravity with 3x2pt
› A machine-learning photometric classifier for massive stars in nearby galaxies II. The catalog
› Symmetry in Fundamental Parameters of Galaxies on the Star-forming Main Sequence
› Probing neutral outflows in z ~ 2 galaxies using JWST observations of Ca II H and K absorption lines
› Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter
› Empirical Calibration of Na I D and Other Absorption Lines as Tracers of High-Redshift Neutral Outflows
› The JWST Spectroscopic Properties of Galaxies at $z=9-14$
› A Method for Testing Diffusive Shock Acceleration and Diffusion Propagation of 1-100 TeV Cosmic Electron with Multi-wavelength Observation of Geminga Halo and Pulsar Wind Nebula
› Imprints of gravitational-wave polarizations on projected tidal tensor in three dimensions
› Ly$\alpha$ visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z $\sim$ 7
› The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
› Dynamical Evolution of Quasi-Hierarchical Triples
› Prospective constraints on dark energy from nanohertz individual gravitational wave sources
› X-ray Transmission Through Photoionized Gas with Moderate Thomson Optical Depth
› Nonlinear Independent Component Analysis Scheme and its application to gravitational wave data analysis
› A Differentiable Surrogate Model for the Generation of Radio Pulses from In-Ice Neutrino Interactions
› Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
› The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
› GroundBIRD Telescope: Systematics Modelization of MKID Arrays Response
› Mapping CO Ice in a Star-Forming Filament in the 3 kpc Arm with JWST
› CHRONOS: Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter
› Constraining the strangeness enhancement scenario of the UHECR muon puzzle with LHC experiments
› The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region
› Clustering analysis of medium-band selected high-redshift galaxies
› The anisotropic expansion rate of the local Universe and its covariant cosmographic interpretation
› Covariant cosmography in the presence of local structures: comparing exact solutions and perturbation theory
› The First Dedicated Survey of Atmospheric Escape from Planets Orbiting F Stars
› Intrinsic alignment of disks and ellipticals across hydrodynamical simulations
› A 3D Chemodynamical Census of Inner-Galaxy Metal-poor Giants to [Fe/H]~-3.5
› The Cosmic Baryon Cycle in IllustrisTNG: flows of mass, energy, and metals
› Solar photospheric velocities measured in space: a comparison between SO/PHI-HRT and SDO/HMI
› A Comparison of Galacticus and COZMIC WDM Subhalo Populations
› Nominal thresholds for good astrometric fits, and prospects for binary detectability, for the full extended Gaia mission
› The Challenge in Illuminating the Invisible: Constraining LyC Escape with Bayesian Modelling and Symbolic Regression
› Grand Unification Higgs-$\mathcal{R}^2$ Inflation: Complementarity between Proton Decay and CMB Observables
› Testing the cosmological Euler equation: viscosity, equivalence principle, and gravity beyond general relativity
› Type Iax supernovae as a source of iron-rich silicate dust
› Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon
› Astrometric view of companions in the inner dust cavities of protoplanetary disks
› Polarimetric and spectropolarimetric observations with FoReRo2: Instrument overview and standard star monitoring
› The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
› Discovering gravitational waveform distortions from lensing: a deep dive into GW231123
› Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution
› SN 2024abvb: A Type Icn Supernova in the Outskirts of its Host Galaxy
› Mathematical Anatomy of Neutrino Decoherence in Red Turbulence: A Fractional Calculus Approach
› Euclid preparation. Galaxy power spectrum modelling in redshift space
› Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
› Statistical Validation and Photometric Characterization of the Hot Jupiter Candidate TOI 7475.01
› Euclid preparation. Impact of galaxy intrinsic alignment modelling choices on Euclid 3x2pt cosmology
› Certified Uncertainty for Surrogate Models of Neutron Star Equations of State via Mondrian Conformal Prediction
› New axion bounds derived from the 100-parsec Gaia DR3 white dwarf luminosity function
› Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
› Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate
› Simultaneous Misalignment and Mode Mismatch Sensing in Optical Cavities Using Intensity-Only Measurements
› Explainable classification of astronomical uncertain time series
› Simultaneously search for multi-target Galactic binary gravitational waves
› General form for Pseudo-Newtonian Potentials, imitating Schwarzschild geodesics
› Incorporating curved geometry in cosmological simulations
› Cosmological Perturbation in New General Relativity: Propagating mode from the violation of local Lorentz invariance
› Novel very-high-frequency quasi-periodic oscillations of compact, non-singular objects
› Scattering of non-relativistic finite-size particles and puffy dark matter direct detection
› Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
› Enhancing low energy reconstruction and classification in KM3NeT/ORCA with transformers
› Apparent Phantom Crossing in Gauss-Bonnet Gravity
› Gravitational Noether-Ward identities for scalar field
› Kerr-Newman-de Sitter black holes in $f(R)$ gravity with constant curvature: horizon structure and extremality
› Limits of vacuum-template subtraction for LISA massive black hole binary sources in realistic environments
› New solution to the hyperon puzzle of neutron stars: Quantum many-body effects
› Kinetic Route to Helicity-Constrained Decay
› Using thermodynamics to learn gravitational wave physics
› Modified Teukolsky formalism: Null testing and numerical benchmarking

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