Obserwatorium Astronomiczne na Suhorze Strona główna
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RSS  Najnowsze prace na astro-ph:

› Multi-mission Observations of GS 1354-64 during the 2025-26 Outburst: First Results
› Astronomy Open Science Competence Centre in Europe
› SPHEREx confirms predictions for artificial satellite trail pollution in Low Earth Orbit
› BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso-scale: Morphology and thermodynamics
› BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Morphology and thermodynamics
› BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Variability and kinematics
› BlackHoleWeather -- Chaotic cold accretion across the meso-scale: Morphology and thermodynamics
› BlackHoleWeather -- Spin-coupled chaotic cold accretion across the meso scale: Variability and kinematics
› Reconstructing the Globular Cluster Initial Mass Function from Present-Day Globular Cluster Systems
› The strength of Type-C quasi-periodic oscillations in black hole X-ray binaries correlates with the jet inclination
› BlackHoleWeather -- Jet-regulated chaotic cold accretion across the meso scale: Variability and kinematics
› DebrisWatch II: Digging deeper for geosynchronous debris
› TRINITY: A coupled model of winds, radiation, and photoionised gas in molecular clouds. I. Methods and validation
› The Ellis and Baldwin test of the Cosmic Dipole: Exploring the impact of multiple flux density cuts
› Probabilistic Data-Driven Modelling of Astrophysical Transients: The Neural Process Family for Ultrafast and Class-Agnostic Light Curve Reconstruction with NightLANP
› VROOM-SBI: A Fast Simulation-Based Bayesian Inference Methodology for QU-Fitting
› MAGAZ3NE: Spatially Resolved Ages and Chemical Abundances of Ultra-Massive Quiescent Galaxies at z $\sim$ 3.5 using JWST/NIRSpec IFU
› A Semi-Supervised Variational Autoencoder for Generating Neutron Star Equations of State
› Hydrodynamic Response of Mildly Evolved Common Envelope Donors in Luminous Red Novae
› Reading between the rings: observed dust ring properties as probes of planet masses
› The Celestial Reference Frame at K Band: The CRF-K-2025 Catalog
› Bar-driven gas redistribution suppresses star formation in spiral galaxies: Evidence from dust lanes in NGC 3351
› A Probabilistic Calibration Procedure for the CORSAIR Polarimeter
› The dynamical structure of the Earth co-orbital region and implications for the near-Earth asteroid population
› The Ultraviolet View of Star and Planet Formation: Disks, Accretion, and Outflows with the Hubble Space Telescope into the 2030s
› Study of the 1/f spectrum using virtual spacecraft sampling in MHD turbulence
› Can COSI detect $\gamma$-ray lines from rare isotopes produced in the astrophysical intermediate neutron-capture process?
› Comparing explodability predictions from a parameter-optimized semi-analytic model with structure-based progenitor criteria
› Double Dots: Compact Pairs Mark Little Red Dots and High-Redshift Broad-line AGNs
› Transient axion streams from disrupted miniclusters
› Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66
› Detection of a large-scale organized 2 kG order magnetic field in the Herbig Ae star HD179218
› Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the $52^{\circ}
› cBHBd: A fast code for the evolution of tidally limited star clusters and their binary black hole mergers
› Hybrid neural denoising for resource-efficient near- and sub-threshold radio triggering of extensive air showers
› FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays
› Mass and radius measurements of the neutron star 47~Tuc X7 -- A new bias-free method
› Noise Suppression and Radio Frequency Interference Rejection for Self-Triggered Radio Detectors of Extensive Air Showers
› Spectroscopic metallicities and first {\alpha}-element abundances of RR Lyrae stars in Baade's Window
› Isochrone Fitting of Galactic Globular Clusters -- VIII. Homogeneous estimates of parameters for 27 clusters
› Unsupervised Morphological Characterization of Gravitational-Wave Glitches in LIGO O4a Using Frozen DINOv2 Features
› GINKAKU: Scalable Cosmological Structure Formation Simulation Code and Post-processing Pipeline
› Dark Quest II: A Wide-Coverage Neural Network Emulator of the Nonlinear Matter Power Spectrum Across Extended Cosmologies
› Comparing telluric removal methods in their capability to recover injected exoplanet atmosphere signals with high resolution emission spectroscopy
› Triaxial shapes and densities of G!k\'un||'h\`omd\'im\`a, Haumea, and Varda from stellar occultations
› Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering
› Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks
› Testing cosmic anisotropy with the Combo correlation of gamma-ray bursts
› Magnetic Configuration Imprints on Quasi-Periodic Variability in GRMHD Simulations of Thin Accretion Disks
› A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$\lambda$ Trends in Three Gas-Giant Mass Regimes
› MIGHTEE-HI: HI catalogue of 293 sources for the COSMOS field and comparative study of 3-dimensional source finding methods
› Hidden worlds: a non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163
› Cluster-centric trends in bar size and pattern speed: the case of Abell 2199
› The unique ability of the Hubble Space Telescope to characterize young exoplanet environments
› Evolution of the dusty nova QY Mus from eruption to quiescence
› The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
› Entropic backreaction from cosmic structure formation: a thermodynamic approach to the late-time cosmological tensions
› Whispers of Supergravity in Gravitational Wave Backgrounds: Determining the Gravitino Mass from Cosmic Thermal History
› Fewer simulations, sharper covariances: Reducing mock covariance noise with Zeldovich approximation control variates
› Non-conservation and time non-locality of biased tracers
› Analytical Fluxes from Generic Schwarzschild Geodesics
› Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE
› GenSBI: Generative Methods for Simulation-Based Inference in JAX
› On the Validity of the Effective Theory of (Multi-)Field Inflation
› Neutrino-antineutrino superfluidity
› Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves
› From WIMP to FIMP during reheating: collider vs non-collider probes for p-wave annihilation
› Reconstructing ACT-compatible and GW170817-compatible Einstein-Gauss-Bonnet Inflation from the Observational Indices
› Dynamical Resolution of the Cosmic Coincidence Problem in Non-Interacting Holographic Dark Energy via Einstein-Cartan Torsion
› Fermionic Bubble Loop in Cosmological Collider Revisited: Exact signals from spectral and Mellin-Barnes methods
› Using the Pericentre Precession of LAGEOS II to Constrain Quadratically Coupled Ultralight Dark Matter
› Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess in $\mathrm{U}(1)_{L_\mu-L_\tau}$ model
› First-Order Perturbations of Covariant Maxwell Equations in Gravitational Waves
› Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM
› Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars
› Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference
› Inflation with vector fields revisited: non-Gaussianities
› Three-dimensional orbital-free density functional theory description of nuclear pasta in the inner crust of neutron stars
› Detecting Gravitational Wave Bursts From Stellar-Mass Binaries in the Milli-hertz Band
› Stochastic Gravitational Wave Background from Highly-Eccentric Stellar-Mass Binaries in the Milli-hertz Band
› Formation of neutron stars via accretion-induced collapse and core-merger-induced collapse inside planetary nebulae from white dwarf binaries
› Extracting Astrophysical Information of Highly-Eccentric Binaries in the Millihertz Gravitational Wave Band
› We Must Preserve Hubble given its Unique Complementarity to Webb, Roman, and Euclid
› Euclid: Photometric redshift calibration with the clustering redshifts technique
› Turbulence in Primordial Dark Matter Halos and Its Impact on the First Star Formation
› The Low-mass Dwarf Host Galaxy of Nonrepeating FRB 20230708A
› Interpreting the Hubble tension with a cascade decaying dark matter sector
› Constraints on DBI dark energy with chameleon mechanism
› Prototyping of 6.2-mm-Pitch Fiber Positioner Modules for Stage-V Telescope Instrumentation
› Influence of Dark Matter on Hybrid and Twin Stars
› Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE
› How precisely can we measure the ages of subgiant and giant stars?
› Numerical Studies on the Radio Afterglows in TDE: Forward Shock
› RGC: a radio AGN classifier based on deep learning. I. A semi-supervised multiclass model for VLA images
› Implication of multiple source populations of Galactic cosmic rays from proton and helium spectra
› Forecasting Constraint on Primordial Black Hole Properties with the CSST $3\times2$pt Analysis
› GASTRO library II: Exploring Chemical Bimodalities in Disk Galaxies with GSE-like Mergers and Massive Star-forming Clumps
› The quenched fraction of satellites around simulated Milky Way-mass galaxies
› A Convolutional Neural Network for the Recovery of Transfer Functions From Velocity-Resolved Reverberation Mapping Data
› Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering
› Evolution of Cosmic Voids: Structure, Galaxies, and Dynamics
› Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
› BLUEPRINT: Blue-dominant Lyman-alpha (Ly$\alpha$) emission as evidence of gas inflow in ultra-low-mass galaxies at z = 3
› Self-Limited Accretion onto Embedded Binaries in a Uniform Medium
› Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLAS
› Andromeda XXXVI: discovery of a new ultra-faint dwarf galaxy towards M31
› Imaging magnetically driven astrospheres: a forward modelling approach
› A Generalized Algorithmic Framework for Detecting Faraday Rotation Measure Flares in Repeating Fast Radio Bursts
› Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data
› Quantifying the Reconstructability of Astrophysical Methods with Large Language Models and Information Theory: A Case Study in Spectral Reconstruction
› Impact of stellar population models on the estimated physical properties of galaxies
› The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
› Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era
› Probing the faint end of simulated galaxy counts at z>3
› Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact
› Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
› Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena
› The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization
› Universe in a black hole in Einstein$-$Cartan gravity
› GRTresna: An open-source code to solve the initial data constraints in numerical relativity
› Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies
› Probing Quadratically Coupled Ultralight Dark Matter with Pulsar Timing Arrays
› Impact of conversion-driven processes on singlet-doublet Majorana dark matter relic
› Exploring New Propagation Scales With Galactic Neutrinos
› Search for Annual Modulation in Combined ANAIS 112 and COSINE 100 Data using Bayesian Model Comparison
› Terrestrial Test of Shapiro Time Delay: Forth test of Einstein General Theory of Relativity
› Part I: Low Energy Galactic Neutrinos
› Early-universe constraints on the electron mass
› May Negative Mass Objects exist in the sky?
› On The Nonthermal Power Laws In Magnetized Turbulent Plasmas

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