Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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RSS  Najnowsze prace na astro-ph:

› Hydrodynamical simulations of helium-ignited binary white dwarf mergers
› Zooming in on the circumgalactic medium with GIBLE: Cloud-scale simulations with cosmological initial conditions
› Large-amplitude modulations and hours-timescale variability in the early X-ray light curve of a tidal disruption flare
› Worlds Next Door. III. Indirect Evidence for Enhanced Atmospheric Metallicity and/or the Presence of Water Clouds in the Nearest Jupiter-analog $\epsilon$ Eri b
› Gravitational waves from primordial black holes passing by neutron stars: observational prospects for the Galactic center
› Survival Analysis of Intermediate-Mass Black Holes in Dense Star Clusters
› The PLUTO Code on GPUs: Offloading Lagrangian Particle Methods
› The role of Bethe-Heitler pair production in reconnection-driven flares in M87*
› Starbursts hiding in the main sequence: a pathway toward quenching?
› Modeling individual nearby radio galaxies as ultra-high-energy cosmic-ray accelerators
› OmegaNeuron: Applying GravitySpy Similarity Methods to the Search for LIGO Glitch Witnesses
› nanoCMB: A minimal CMB power spectrum calculator in Python
› Transient X-ray Sources as Extremely Eccentric Mass-Transfer Binaries with Compact Companions
› ALMA High-J CO Spectroscopy of High-Redshift Galaxies. I. An Archive-based Catalog of CO Spectral Line Energy Distributions
› Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
› Evolution of Sink Pixels in ACS/WFC and Connection to Charge Transfer Efficiency
› Updates to the SBC Dark Rate Monitor
› Contemporaneous Optical and Near-Infrared Observations of the Interstellar Comet 3I/ATLAS Pre- and Post-Perihelion
› Can the dust eclipses in WR 104 provide constraints on the system's inclination?
› Superposition model for energy reconstruction and mass identification in cosmic ray spectra
› The Split Janus-faced Sun: Magnetic Rhythm and Duality in the Solar Cycle
› Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies
› Active Learning for Planet Habitability Classification under Extreme Class Imbalance
› The environmental dependence of mid-IR luminous dusty Supernovae
› Search for Gamma-ray emission from Abell 119 galaxy cluster using INTEGRAL/ISGRI, COMPTEL, and DAMPE data
› Tri-coupler geometries for achromatic nulling interferometry in the near infrared
› Acceleration of relativistic protons in a CME-perturbed solar wind
› X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon
› An investigation on the FWHM of absorption features of type Ia supernovae
› A NICER View of PSR J0030+0451: Updated Constraints from Six Years of NICER Observations
› Constraining the mass of the M31 ionized baryon Halo using CHIME/FRB Catalog 2
› Predicting Resolved Dust Attenuation from Local Galaxy Properties Using MaNGA
› New possible way to determine stellar wind terminal velocity from analysis of Lyman-$\alpha$ absorption spectra
› The capture of halo material by orbiting subhaloes
› Eigenmode initialisation of 2D (magneto)hydrodynamic simulations
› Magnetic Flux Tubes Illuminated by Pulsar Winds
› Timing and scintillation of a young Galactic halo pulsar
› Dark Acoustic Oscillations and the Hubble Tension
› Discovery of a runaway star likely ejected by a Type Iax Supernova
› Age and metallicity of the Milky Way's nuclear star cluster studied at 3 pc from Sagittarius A*
› Probing inflationary features with galaxy ultraviolet luminosity function observables
› Ruling out conventional photoionization models in the closest LINER M31 with CFHT/SITELLE observations
› Comparison of symbolic regression algorithms in Star/galaxy/quasar separation
› A Quality Framework for Testing Gravity with Wide Binaries: No Evidence for MOND
› A Unified Origin of Primordial Black Hole Dark Matter and Nanohertz Gravitational Waves
› Monitoring the magnetospheric accretion of the classical T Tauri star DO Tau with SPIRou
› The hydrodynamics of stratified ultra-relativistic outflows and the origin of GRB X-ray plateaus
› Multi-messenger emission derived from relativistic magnetized jet dynamics using a multi-zone framework
› Probing power spectrum enhancement at small scales with SKA
› Temporal Evolution of Sunspot Groups and Increase in the Open flux During Solar Maximum in Cycle 24
› A New Window into the Baryon Cycle at Cosmic Noon with Line Intensity Mapping: Forecasts for auto- and cross-correlations in [CII]-158$\mu$m, HI 21 cm, CO$_{J+1\rightarrow J}$, and H$\alpha$ galaxies
› Weak lensing higher-order statistics to disentangle modified gravity and massive neutrinos
› Filling the Gap in Cluster Evolution: JWST's Glimpse into a Young, Star-Forming Cluster at Cosmic Noon
› Few Made It Out: A Multi-Messenger Study of an In Situ Solar Energetic Electron Event Driven by a Solar Jet
› Linear Polarization Variations and Circular Polarization are Common Among Airless Bodies
› Forecasting the cross correlation of Terahertz Intensity Mapper [CII] line intensity maps with Euclid galaxies
› Discovery of a nearby radio relic in the low-mass, merging cluster Abell 4067
› Single Parameter Model for Galaxy Rotation Curves
› Weak emission line quasar SDSS J101353.45+492758.1 I. Continuum fitting
› First spectroscopic identification of the main sequence in Westerlund 1
› Principal Component Analysis for ACS/WFC Superbias Temporal Variation
› In-flight calibration of RADEM, the JUICE mission radiation monitor
› The First Four Ground-Level Enhancements in the 1940s: Investigation, Digitisation, and Analysis of Forgotten Data
› Direct VLBI Detection of Interstellar Turbulence Imprint on a Quasar: TXS 2005+403
› Black hole scalar sirens in the Milky Way
› Universality of the Blandford-Znajek emission in stationary and axisymmetric spacetimes
› Polarisation Singularities of Gravitational Waves
› Monte Carlo Simulations of Secondary Cosmic-Ray Variations in Atmospheric Electric Fields : Implications for Long Duration Electron and Gamma-ray Emissions from Thunderclouds
› Photon rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
› Transition of Magnetic Reconnection Regimes in Partially Ionized Plasmas
› High-Precision Mass Measurements of Proton-Rich Rh, Pd, Cd isotopes in the vicinity of 100Sn and Impact on X-Ray Burst and Supernova Nucleosynthesis
› Impact of non-standard neutrino-electron interactions on Big Bang Nucleosynthesis
› The Shape of Eccentricity: Rapid Classification of Eccentric Binaries with the Wavelet Scattering Transform
› Shaping the Digital Future of ErUM Research: Sustainability & Ethics
› Fermion Mass Hierarchy and a High Quality Axion From Gauged U(1) Flavor Symmetry
› Data-driven core collapse supernova multilateration with first neutrino events
› Extensive analysis of reconstruction algorithms for DESI 2024 baryon acoustic oscillations
› Performance Analysis of Digital Flux-locked Loop Circuit with Different SQUID $V$-$\phi$ Transfer Curves for TES Readout System
› Assessing the Robustness of the CPL Parametrization to Basis and Prior Variations: Insights from DESI DR2 BAO Data
› TDCOSMO XXIV. First spatially resolved kinematics of the lens galaxy obtained using JWST-NIRSpec to improve time-delay cosmography
› A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
› Challenges to the Two-Infall Scenario by Large Stellar Age Catalogs
› CCAT: Mod-Cam Readout Overview and Flexible Stripline Performance
› Dynamics and Observational Signatures of Core-Collapse Supernovae with Central Engines: Hydrodynamics Simulations with Monte Carlo Post-Processing
› StarStream on Gaia: Stream discovery and mass loss rate of globular clusters
› Velocity dispersion profiles of dwarf spheroidal galaxies with self-interacting ultralight dark matter
› Introducing RAFIKI: Refining AGN Feedback in Kinetic Implementations
› A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
› Shapiro Delay Measurements from Fifteen Years of PSR J1231$-$1411 Radio Observations
› On the impact of the supernova subsamples in reducing the Hubble tension
› The Milky Way stellar halo is twisted and doubly broken: insights from DESI DR2 Milky Way Survey observation
› Exploring the ultra-faint dwarf Bootes I using JWST and HST: Metallicity distribution and binaries
› AMKID -- a large KID-based camera at the APEX telescope
› High mass accretion rates onto evolved stripped-envelope massive stars by jet-induced mass removal
› The maximum mass ratio of hierarchical binary black hole mergers may cause the $q$-$\chi_{\rm eff}$ correlation
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› Algorithm to extract direction in 2D discrete distributions and a continuous Frobenius norm
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