Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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RSS  Najnowsze prace na astro-ph:

› Planetary Exploration 3.0: A Roadmap for Software-Defined, Radically Adaptive Space Systems
› Interpretable Analytic Formulae for GWTC-4 Binary Black Hole Population Properties via Symbolic Regression
› Revisiting radio synchrotron diagnostics in star-forming galaxies
› Black hole mass, host galaxy mass, and dark matter halos: Testing the environmental connection
› Characterizing the GD-1 Stream with DESI DR2 Data: Thin Stream and Hot Cocoon
› Light, heavy, primordial: exploring the diversity of black hole seeding and growth mechanisms in the JWST era
› Chaotic migration of LISA Extreme Mass Ratio Inspirals in a turbulent accretion disk: effect on waveform de-phasing
› Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays
› Relativistic effects in k-essence
› DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Proto-clusters
› Gravity Echoes from Supermassive Black Hole Binaries
› Archival Multiband Gravitational-Wave Signals from Massive Black Hole Binary Mergers
› Cosmological Gravitational Waves from Ultralight Vector Dark Matter
› An Analytic Threshold for LESA-Driven Negative ELN Flux Directions in Core-Collapse Supernovae: Derivation and Population Census
› Constraining Dark Matter Density Profiles in UFDs with Wide Binaries: Forecast for the Chinese Space Station Survey Telescope
› Orbital evolution of highly eccentric bodies embedded in a ringed accretion disc
› Joint Estimation of Properties of the Lunar Subsurface and Galactic Foregrounds with LuSEE-Night
› Predicting the thermodynamics in the chromosphere from the translation of SDO data into the IRIS$^{2}$ inversion results using a visual transformer model
› Early metal-enriched baryon cycling before the midpoint of cosmic reionization
› Geometry, Not Calorimetry, Drives the Radio/Infrared/Gamma-Ray Correlation
› Turbulent infall onto class 0 disks as cause of CAI brief condensation episode in the solar system
› Bayesian Inference of Dense-Matter Equations of State from Small-Radius Compact Stars with Twin-Star Scenarios
› Filter Design for Estimating the Stellar Metallicity of Metal-poor Stars from Gaia XP Spectra
› A Synchronized Spin Model for Black-Hole Accretion Systems
› A New Pathway to Single Be Stars: Ejected Companions from Type Ia Supernovae
› Supermassive Black Hole Winds in X-rays: SUBWAYS IV. Tracing Radio Emission and Unveiling the Role of Winds
› Energy Loss of Newborn Magnetars by Schwinger Process
› Hill's level surfaces in the circular restricted three-body problem solved
› SFUMATO#: a GPU accelerated code for Self-Gravitational Radiation Hydrodynamics Simulation with Adaptive Mesh Refinement
› Investigation of White-light Emission in Compact Flares
› BV photometry of the ultracompact binary star GP Com
› X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
› One's loss is (not) another's gain: Isotropic re-emission destabilizes mass transfer from radiative donor stars
› Impact of the Infrared Cutoff on Structure Formation in Tsallis Holographic Dark Energy
› Signatures of Very Massive Stars in the Epoch of Reionization
› XRISM High-Resolution X-ray Spectroscopy of Cygnus X-1 -- highly ionized Iron absorption structures
› SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at $z=9.3$
› Cosmological discrete self-similarity in primordial black hole formation
› XRISM High-Resolution X-ray Spectroscopy of Cygnus X-1 -- Orbital and Short-Term Variability of Iron Absorption
› Diffraction in the ASPIICS coronagraph: observations and modeling
› VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr
› Multi-wavelength study of EP250416a / GRB 250416C: An Optically Dark Long GRB with a Late Jet Break
› Aspects of gravitational clustering and structure formation in the Universe
› Tracking Magnetic Topological Change in a Time-Dependent Coronal Model
› An Old, Low-mass, Metal-poor Hypervelocity Star Candidate Consistent with a Galactic Center Origin
› Modeling of the magnetic stellar wind braking of the ssrAp 33 Lib (HD137949)
› Impact of Primordial Black Hole population on 21 cm observables at high redshift
› Saturation Mechanisms in the Interacting Dark Sector
› Delving into the depths of NGC 3783 with XRISM: V. Broad-band modeling of ionized outflows
› Massive star formation at the Galactic crossroads: Insights from G358.69+0.03 in the Galactic center
› Correlation between active regions' spectra at high radio frequencies and solar flare occurrences
› Gauging the Impact of Cosmic Ray Feedback on the Stellar Initial Mass Function
› Magnetar Engines in Broad-lined Type Ic Supernovae and a Unified Picture for Magnetar-powered Stripped-envelope Supernovae
› Informative Priors on Primordial Non-Gaussianity Bias $b_{\phi}$ From Galaxy Formation
› MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?
› An RXTE Search for the Sterile Neutrino Decay in Galaxy Clusters
› Broad-band High-Energy Resolution Hard X-ray Spectroscopy using Transition Edge Sensors at SPring-8
› Toward Inferring the Surface Fluxes of Biosignature Gases on Rocky Exoplanets from Telescope Spectra
› Mitigating Systematic Errors in Parameter Estimation of Binary Black Hole Mergers in O1-O3 LIGO-Virgo Data
› Testing solitonic boson star interpretations of Sagittarius A* with near-infrared flare astrometry
› The Dyson Minds 2025 Workshop: SETI around Black Holes
› The impact of hydrogen atom tunneling on aromatic chemistry in TMC-1
› First measurement of wind line formation regions in an early O-type star
› Spectral Kernel Dynamics for Planetary Surface Graphs: Distinction Dynamics and Topological Conservation
› Cracking Gravitational Wave Multiple Ringdown Modes in Space
› Radial adiabatic perturbations of stellar compact objects
› Turbulence Mode Decomposition and Anisotropy in Magnetically Dominated Collisionless Plasmas
› Chaos Gated Tunneling Drives Molecular Reactivity in Astrophysical Environments
› Multimessenger probes of Axions from Compact Objects
› Ultra High Energy Cosmic Rays from the Local Void
› Neutron Portal and Dark Matter-Baryon Coincidence: from UV Completion to Phenomenology
› Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit
› Relativistic frequency shifts in gravitational waves from axion clouds
› Phase transition structure of scalarized neutron stars: the effect of rotation and linear coupling
› Collisionless Phase Mixing Mimics Diffusive Transport in Radiation Belt Observations
› Exploring the statistical anisotropy of primordial curvature perturbations with pulsar timing arrays
› Constraining dark matter self-interaction from kinetic heating in neutron stars
› Quantum-information diagnostics of cosmological perturbations with nontrivial sound speed in inflation
› Accelerating scaling solutions from dark matter particle creation
› Cosmological Analysis with Calibrated Neural Quantile Estimation and Approximate Simulators
› Relationship between the $\gamma-$ray variability and the pc-scale jet in the blazar 3C 454.3
› Scalar-induced gravitational waves with non-Gaussianity up to all orders
› Effects of density stratification on Rossby waves in deep atmospheres
› Artificial Precision Polarization Array: Sensitivity for the axion-like dark matter with clock satellites
› Combining CMB datasets with consistent foreground modelling
› Observations of [O I] emission in Comets C/2014 Q2 (Lovejoy) and C/2007 N3 (Lulin): Possible Influence of Solar Activity on Oxygen Line Ratios
› Galaxy evolution in the post-merger regime. IV -- The long-term effect of mergers on galactic stellar mass growth and distribution
› Searching for EeV photons with Telescope Array Surface Detector and neural networks
› The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios
› Multi-Tracer Cross-Correlations of the Unresolved $\gamma$-Ray Sky
› Fading Echoes of Interaction: Probing Centuries of Preexplosion Mass-Loss in Four Type IIn Supernovae
› SED and Galactic kinematic diagnostics for dormant BH/NS binary candidates
› Subaru High-$z$ Exploration of Low-Luminosity Quasars (SHELLQs). XXV. Large-scale environments of low-luminosity quasars at $z\sim6$ traced by Ly$\alpha$ emitters
› Solar active region scaling laws revisited
› The diverse nature of spiral arms in the Auriga Superstars cosmological hydrodynamic simulations
› Stellar microlensing surveys as a probe of Primordial Black Holes: status and prospects
› Multiple protostellar outflows from a single protostar with a misaligned disk
› Active Learning for Planet Habitability Classification under Extreme Class Imbalance
› Exploring Beyond {\Lambda}CDM with the Weak Lensing Power Spectrum and Bispectrum
› The RRATalog: a Galactic census of rotating radio transients
› Multi-scale Gas Structure and Dynamics in an Extragalactic Central Molecular Zone
› Three-dimensional transport-induced chemistry on temperate sub-Neptune K2-18b, Part II: the combined effects of atmospheric dynamics and chemical reactions
› Consistent Treatment of Muons in Binary Neutron Star Mergers
› Ice as a Photochemical Shield: Adsorption Energetics and Spectroscopic Modulation of Interstellar Thiocyanates HCSCN and HCSCCH in TMC-1
› Cosmological constraints from the small scale clustering of Emission Line Galaxies
› Detections of nearly bias-free core shifts with 5-30 $\mu$as precisions at 8-43 GHz in BL Lacertae
› Deep VLBI constraints on compact radio cores in four ultraluminous X-ray sources
› Chiral Gravitational Wave Background from Audible Axion via Nieh-Yan Term
› Relic gravitational waves from primordial gravitational collapses
› Inflaton perturbations through an Ultra-Slow Roll transition and Hamilton-Jacobi attractors
› Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter
› Neutron star evolution with the Bemfica-Disconzi-Noronha-Kovtun viscous hydrodynamics framework
› Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter
› Stationary Stars Are Axisymmetric in Higher Curvature Gravity
› $\ell$-Boson stars in anti-de Sitter spacetime
› Spec-o3: A Tool-Augmented Vision-Language Agent for Rare Celestial Object Candidate Vetting via Automated Spectral Inspection
› Induced-Gravity Higgs Inflation in Palatini Supergravity Confronts ACT DR6

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