Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Drugi w historii lot komercyjnej rakiety z lądowaniem boostera!
› Misje Kosmiczne XX wieku: Atlantis
› Recenzja książki „Księżyc. Jak zmienił naszą planetę, przewodził ewolucji i stworzył nas takimi, jakimi jesteśmy”
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› W Układzie Słonecznym: Obłok Oorta
› Misje kosmiczne XX wieku: Challenger
› Galaktyczny kartograf – Teleskop Nancy Grace Roman
› Niebo w listopadzie 2025 roku
› Misje kosmiczne XX wieku: Discovery
› Japońska technologia powraca na ISS. Pierwsza misja nowej kapsuły zaopatrzeniowej HTV-X
RSS  Najnowsze prace na astro-ph:

› Towards Mitigating Systematics in Large-Scale Surveys via Few-Shot Optimal Transport-Based Feature Alignment
› Non-Parametric Reconstruction of the Hubble Parameter from the Fourth Gravitational Wave Transient Catalog and DESI Baryonic Acoustic Oscillations
› Hydrodynamic instabilities in long-term three-dimensional simulations of neutrino-driven supernovae of 13 red supergiant progenitors
› Rock vapour is opaque: implications for dynamics and observations of lava planets
› Not all cores are equal: Phase-space origins of dynamical friction, stalling and buoyancy
› LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
› KDP as a thermal blocking filter - Deep near IR observations with a warm narrow band filter
› Inflation without an Inflaton II: observational predictions
› On the coincidence between the close passage of HD7977 and the Pliocene-Pleistocene transition
› The Transition from Giant Planets to Brown Dwarfs beyond 1 au from the Stellar Metallicity Distribution
› ODIN: Characterizing the Three-dimensional Structure of Two Protocluster Complexes at $z = 3.1$
› Infrared Signatures of Dusty Tori Formed by MHD-Driven Outflows
› Modeling X-ray photon pile-up with a normalizing flow
› A new estimate of the zero-point shift of the Gaia DR3 parallaxes obtained from a comparison with VLBI measurements of masers and radio stars
› Disk mass predictions for binary neutron star mergers: limitations of proposed symbolic regression models
› The Atmospheric Response to Large Electron Beam Fluxes in Solar Flares III: Comprehensive Modeling of the Brightest Observed Near-Ultraviolet Continuum Source in an X9 Solar Flare
› PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies
› Through the Heliospheric Lens: Directional Deflection of High-Energy Cosmic-Ray Electrons and Positrons
› Euclid Quick Data Release (Q1): Identification of massive galaxy candidates at the end of the Epoch of Reionisation
› SourceREACH (Source REconstruction of Arcs behind Cluster Halos): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses
› Functionality of Ice Line Latitudinal EBM Tenacity (FILLET). Protocol Version 1.1
› Formation of Close Binaries through Massive Black Hole Perturbations and Chaotic Tides
› First Light And Reionisation Epoch Simulations (FLARES) XX: Comparing semi-analytic models at high-redshift
› He-star donor pathway for the hypervelocity star D6-2
› The Impact of Orbital Anisotropy Assumptions in Lensing-Dynamics Modeling
› Gravitational wave standard sirens from GWTC-3 combined with DESI DR2 and DESY5: A late-universe probe of the Hubble constant and dark energy
› Dual core system candidates: a sample of objects with large velocity offset between absorption and narrow emission lines
› 3D extinction maps of the Milky Way disc from Gaia GSP-Spec parameters
› Chemically primitive dwarf accretion reignites the inner disk assembly of Malin 1
› Doppler imaging combined with high-cadence photometry. I. Revisiting the surface of a pre-main-sequence flare star
› High-impact Scientific Software in Astronomy and its creators
› Metallicity Effects on Machine Learning Classification of Dusty Stellar Sources in the Magellanic Clouds
› Implications of Mini-EUSO measurements for a space-based observation of UHECRs
› Pre-Supernova Multiple Giant Eruptions in Massive Stars
› Clustering effects on the Dark Siren determination of $H_0$: A simulation study
› AstroMLab 5: Structured Summaries and Concept Extraction for 400,000 Astrophysics Papers
› QuaRT: A toolkit for the exploration of quantum methods for radiation transport
› Characterization of type Ibn SNe
› The X-$\gamma$ detector onboard the POEMMA-Balloon with Radio payload
› Examining Turbulence in Galactic Molecular Clouds - II: Continuity of Turbulence Cascading in a Portion of the Local Arm
› Made-to-Measure Outperforms Schwarzschild's Method
› The influence of AGN feedback on star formation in red spiral galaxies
› Spectral-Timing Evolution of a Black hole X-ray binary Swift J1727.8-1613: Linking Disk Reflection and Type-C QPO Frequency During the 2023 Outburst
› Detection of disk-jet co-precession in a tidal disruption event
› Mock Observations for the CSST Mission: Multi-Channel Imager--Instrument Simulation
› Mock Observations for the CSST Mission: Integral Field Spectrograph--Instrument Simulation
› The first AKRA mass map reconstruction from HSC Y1 data
› Unraveling eMSTO in NGC 2355: Stellar Rotation and Binaries
› The homogeneity scale in the Local Universe: model-independent estimate from S-PLUS DR4 blue galaxies
› Sub-millimeter galaxies in hierarchical models: revisiting the need for a top-heavy stellar initial mass function with Bayesian optimisation
› Simulations of structured upflows from plumes and their connection to the solar wind
› IdentYS: A Python-Based Tool for Identifying Young Stars in Star-Forming Regions
› The Chandra Strong Lens Sample: Measuring the Dynamical States and Relaxation Fraction of a Sample of 28 Strong Lensing Selected Galaxy Clusters
› Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
› From Images to Physics: Probabilistic Inference of Galaxy Parameters and Emission Lines via VAE & Normalizing Flows
› Observations of Five Southern-Hemisphere Cataclysmic Binary Stars
› On the Temporal Variability in the Magnetic Dichotomy of Late M Dwarf Stars
› Orbital Eccentricities Suggest a Gradual Transition from Giant Planets to Brown Dwarfs
› Modeling stellar convective transport with plumes : II. Transport Properties of Locally and Non-locally driven Convection
› Near-infrared [P II] and [Fe II] line mapping of Galactic supernova remnants
› SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material
› Orbit Elements from Kepler Solutions in Projective Coordinates
› Helical Magnetic Field in the Acceleration--Collimation Zone of the M87 Jet
› AGN feedback in merging galaxies with a SMUGGLE multiphase ISM
› Thermal infrared characterization of spatially unresolved resident space objects: Prospects from analytical two-component modeling
› Reheating and Inflationary dynamics driven by an inverse tangent potential
› The B[e] Phenomenon in Supergiants. A Result of Mass Transfer in Binaries, Mergers, or What?
› Topological Signatures of Heating and Dark Matter in the 21 cm Forest
› Wide-Field X-ray Polarimetry for High Energy Astronomical Transients: First results of the pathfinder CXPD Cubesat Mission
› Prospects for detecting periodic or sharp fast-time features in the supernova neutrino lightcurve with IceCube
› Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo
› Infrared photometry and CaT spectroscopy of the most metal-poor in-situ globular cluster VVV-CL001
› Spectral component imaging of solar X-ray flares
› Probing the Nature of Dark Matter Self-Interactions Through Observations of Massive Black Hole Mergers
› Natural gradient descent for improving variational inference based classification of radio galaxies
› The Spontaneous Genesis of Solar Prominence Structures Driven by Supergranulation in Three-Dimensional Simulations
› Vortex creep heating in neutron star cooling with direct Urca processes in heavy neutron stars
› TransFit-CSM: A Fast, Physically Consistent Framework for Interaction-Powered Transients
› Unveiling the nature of the Einstein Probe transient EP 241021a
› Multiple Components and Spectral Evolution of BL Lacertae as Revealed by Multiwavelength Variability and SED Modeling
› Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
› Stray Light Correction for the Helioseismic and Magnetic Imager
› Constraining the Neutral Hydrogen Fraction from SKA Simulated Observation using a Double-Gaussian Decomposition Technique
› Constraining r-process nucleosynthesis with multi-objective Galactic chemical evolution models
› An Unusual Velocity Field in a Sunspot Penumbra
› PDRs4All XX. Haute Couture: Spectral stitching of JWST MIRI-IFU cubes with matrix completion
› Cosmic Expansion Driven by Gravitational Particle Production: Toward a Complete Cosmological Scenario
› Learning Cosmology from Nearest Neighbour Statistics
› The PAH 3.4 micron feature as a tracer of shielding in the Orion Bar and NGC 6240
› Investigating magnetic activity cycles in solar-like oscillators using asteroseismic data from the K2 mission
› Magnetic fields in the close neighborhood of LDN 328 core
› Shaping the Mantle: The Role of Superheated Cores After Giant Impacts
› The bulk metal content of WASP-80 b from joint interior-atmosphere retrievals: Breaking degeneracies and exploring biases with panchromatic spectra
› High Resolution Observations of CO(3-2) in Haro 2: Cool Molecular Outflows of a Ly$\alpha$ Emitter
› A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy
› High-Precision Multi-Period Analysis of the Ellipsoidal Variable Candidate TIC~470127886 from TESS Photometry
› Statistical analysis of eclipsing binaries with monotonic orbital-period variations: A-type W UMa contact systems
› Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet
› Sense and Sensitivity - I. Uncertainty analysis of the gas-phase chemistry in AGB outflows
› JWST observes the assembly of a massive galaxy at z~4
› High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4
› A model-independent assessment of the late-time dark energy density evolution
› Investigating the Dark Energy Constraint from Strongly Lensed AGN at LSST-Scale
› The hard ultraluminous state of NGC 5055 ULX X-1
› The physical properties of post-mass-transfer binaries
› The Scatter of the Many Outweighs the Scatter of the Few: Systematic Error Asymmetry in Steeply-Falling Mass Functions for High-Redshift JWST Galaxies
› Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs
› On Bayesian inference considerations and other issues concerning Drake's equation of Astrosociobiology
› Kerr-Bertotti-Robinson Black Holes Surrounded by a Cloud of Strings
› Relativistic Maxwell-Bloch Equations with Applications to Astrophysics
› Testing general relativity with amplitudes of subdominant gravitational-wave modes
› Symmetric Bimetric Cosmology: A Minimal Extension of {\Lambda}CDM
› Upper Bound on the Cosmic Baryon Chemical Potential from Lepton-Flavor Asymmetry
› Spin precession effects in the phasing formula of eccentric compact binary inspirals till the second post-Newtonian order
› The Engineering and Programming Methods Used in Manufacture of Astrolabes and Errors Resulting
› Quintessence: Quadratic potentials
› From the Virgo interferometer calibration to the bias and uncertainty of the h(t) detector strain during the O4 run
› Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
› Thermal Quarkyonic Matter and Its Implications for Neutron Star Structure
› The Great January Comet of 1910 (C/1910 A1): A Key Opportunity Missed by New Zealand Astronomers
› Efficient Reconstruction of Matched-Filter SNR Time Series from Nearby Templates
› Chiral Magnetic Effect induced Spectator Process for Leptogenesis
› Towards an anomaly detection pipeline for gravitational waves at the Einstein Telescope
› Sub-Solar Mass Intermediate Mass Ratio Inspirals: Waveform Systematics and Detection Prospects with Gravitational Waves
› The Birth of Gravitational Particle Creation: the Enduring Legacy of Leonard Parker's 1966 Thesis
› Bimodular Gravity: Unimodularising Bimetric Scalar-Tensor Gravity
› Variable-temperature attenuator calibration method for on-wafer microwave noise characterization of low-noise amplifiers
› Gravitational--Electromagnetic Coupling on Kerr Spacetime
› In-orbit background and sky survey simulation study of POLAR-2/LPD
› Redshift Drift fluctuations from N-body simulations
› Discovering High-$z$ BL Lacs Using Swift/UVOT and SARA Observations with the Dropout Technique
› 3D Modeling of Moist Convective Inhibition in Idealized Sub-Neptune Atmospheres
› Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems
› The 3D pulsar magnetosphere with machine learning: first results
› Water-rich sub-Neptunes and rocky super Earths around different Stars: Radii shaped by Volatile Partitioning, Formation, and Evolution
› Constraints on the $z\sim6-13$ intergalactic medium from JWST spectroscopy of Lyman-alpha damping wings in galaxies
› The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
› Complementary signatures of $\alpha-$attractor inflation in CMB and cosmic string Gravitational Waves
› A Bayesian estimator for peculiar velocity correction in cosmological inference from supernovae data
› The role of triple evolution in the formation of LISA double white dwarfs
› The role of turbulence in setting the phase of the ISM and implications for the star formation rate
› Precision cross-sections for advancing cosmic-ray physics and other applications: a comprehensive programme for the next decade
› A Multi-Site Study of Radio Environment for Cosmology Experiments
› A possible correction of the Saha curve for non-equilibrium states
› A weak Ly$\alpha$ halo for an extremely bright Little Red Dot: Indications of enshrouded SMBH growth
› Displacement of ultra-high-energy cosmic ray source images by the intergalactic magnetic field: the cases of Cen A and M83
› Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
› TasVisAn and InsPy -- Python Packages for Triple-Axis Spectrometer Data Visualization, Analysis, Instrument Resolution Calculation, and Convolution
› The fate of Quasi-Exponential inflation in the light of ACT-DR6
› Reconstructing dark energy with model independent methods after DESI DR2 BAO
› Asteroids fail to retain cometary impact signatures
› Ruling Out Dark Energy Model induced by de-Sitter Regions of Non-Singular Black Holes with Planck2018, DESI BAO, and Union3 Supernovae
› The Distribution of Atomic Hydrogen in the Host Galaxies of FRBs
› Estimating cluster masses: a comparative study between machine learning and maximum likelihood
› 2D End-to-End Modeling of Kilonovae from Binary Neutron Star Merger Remnants
› A Turbulent Framework for Star Formation in High-Redshift Galaxies
› Radio Observations of a Candidate Redback Millisecond Pulsar: 1FGL J0523.5-2529
› The Dark Energy Camera All Data Everywhere cosmic shear project V: Constraints on cosmology and astrophysics from 270 million galaxies across 13,000 deg$^2$ of the sky
› Universal Structure of Turbulent Radiative Mixing Layers
› MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z${\sim}$2
› No evidence for local $H_0$ anisotropy from Tully--Fisher or supernova distances
› Bayesian Framework for the E1 and E2 Astrophysical Factors at 300 keV from Subthreshold and Ground-State Asymptotic Normalization Coefficients
› Detailed theoretical modelling of the kinetic Sunyaev-Zel'dovich stacking power spectrum
› Formation of Multiple Dynamical Classes in the Kuiper Belt via Disk Dissipation
› New Evidence for Extragalactic Einstein Probe Transients associated with Long Gamma-ray Bursts
› Exploring the connection between compact object mergers and fast X-ray transients: The cases of LXT 240402A & EP250207b
› Energetics of star-planet magnetic interactions: Novel insights from 3D modelling
› Towards a unified hadron-quark equation of state for neutron stars within the relativistic mean-field model
› Mock Observations for the CSST Mission: Main Surveys-the Slitless Spectroscopy Simulation
› JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios
› The Deepest GLIMPSE of a Dense Gas Cocoon Enshrouding a Little Red Dot
› Effect of molecular hydrogen self-shielding modeling on early Reionization Era galaxies in radiative hydrodynamic cosmological simulations
› Stellar Populations with MaNGA: Iron Kink and Nitrogen Fuzz
› Probing Time-Dependent Physics with Phase-Folding CMB Maps
› JWST View of the Supernebula in NGC 5253. II. Nebular Lines
› Ginnungagap -- a massively parallel cosmological initial conditions generator
› A new multiprobe analysis of modified gravity and evolving dark energy
› Hydrogen-line profiles from accreting gas giants and their CPDs
› A 34.6-day transiting sub-Neptune in the TOI-1422 planetary system
› Tests of General Relativity with GWTC-3
› The need for a nonlocal expansion in general relativity
› Complementarity between Cosmic String Gravitational Waves and long-lived particle searches in a laboratory
› Dynamical Solution to the Eta Problem in Spectator Field Models
› Non-interacting holographic dark energy with Torsion via Hubble Radius
› Korteweg-de Vries Integrals for Modified Black Hole Potentials: Instabilities and other Questions
› Quintessential Inflation in Palatini $F(R,X)$ gravity
› Black hole quasinormal mode resonances
› Insights on the Cosmic Origin of Matter from Proton Stability
› MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
› The Fast and the Frame-Dragging: Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly-spinning black holes
› High-Precision Relativistic Time Scales for Cislunar Navigation
› Automated Algorithmic Discovery for Scientific Computing through LLM-Guided Evolutionary Search: A Case Study in Gravitational-Wave Detection
› Modified Black Hole Potentials and Their Korteweg-de Vries Integrals: Instabilities and Beyond
› Is the $\Lambda$CDM Model in Crisis?
› Importance of being nonminimally coupled: Scalar Hawking radiation from regular black holes
› Conserved Quantities in Expanding G\"odel Cosmology
› Imaging and polarization patterns of various thick disks around Kerr-MOG black holes

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