Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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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:

› Observing the Peculiar Acceleration of our Solar System with Quasar Proper Motions
› Reconciling GW170817 and GW190814 with a Nonmonotonic Sound-Speed Equation of State
› The EPS Research Astro-RAG Platform: A Unified Open-Science Infrastructure for Cross-Epoch Astrophysical Kinematic Analysis, LLM-Assisted Research Workflows, and Educational Outreach
› Experiments on Settling of Granular and Cohesive Material in Low Gravity
› RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9
› Choosing the right MCMC sampler: a systematic benchmark of gradient-free methods
› A Rapid Evolution in the Observed Mbh/M* Relation at z > 3 Revealed via Spectro-photometric SED-Modeling
› Parameter resolution of near-Earth asteroids using LISA
› High-ionization coronal lines trace quasar-like activity in recently quenched galaxies at high redshift
› The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening
› A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones
› JWST Predictions for $z > 10$ Galaxies from the Renaissance Simulations -- I: Photometry and Sizes
› Euclid preparation. Probing galaxy evolution within cosmic voids in Euclid-like simulations
› Simultaneous modeling of FeII emission in the optical and near-infrared in a prototypical Narrow-Line Seyfert 1 galaxy
› Multi-Scale Magnetic Field Observations Reveal how Colliding Flows Trigger Star Formation
› Transformer-Based Source Detection and Morphological Classification in LOFAR Deep-Field Continuum Images
› The JADES Mass-Metallicity and Fundamental Metallicity Relations at $z\gtrsim2$ Using New High-Redshift Metallicity Calibrations
› Automated void identification by Blendmask: from hierarchical molecular gas to hierarchical voids in NGC 628
› Magnetic Eruption and Nucleosynthesis in GR{\nu}MHD Simulations of Spinning Neutron Star Mergers
› Gratis Mitigation of Polarization Aberration Effects in Coronagraphic Dark Holes
› Mapping the Universe as a Bianchi I cosmology with Gaia data
› Tracing the dynamical states and mass accretion histories of galaxy clusters in IllustrisTNG
› Statistical imprints of wave-like dark matter on multiply-imaged galaxies in strong cluster lenses from JWST
› Weak-CN Stars Are Ordinary Cool Red Supergiants
› Characterising and mitigating Bluetooth and WiFi radio frequency interference at the Parkes Observatory
› An extended catalogue of Herbig-Haro objects
› Coupling dynamical accretion and chemical differentiation: a unified framework for Earth-Mars diversity
› Detection of CO, H$_2$O, and OH in WASP-18b with JWST/NIRISS using Direct-Extracted Spectra and Cross-Correlation
› Interstellar Scintillation of Three Nearby Pulsars with FAST
› Matter influence on large-scale scalar dynamics
› (The) Wiggles going non-linear
› The Galactic Squeeze: How Aggregate and Highly Dynamical Environments Shape Star Formation in the Local Universe
› The MeerKAT Thousand-Pulsar Polarisation Array II: Searches for Ultralight Axion-Like Dark Matter
› Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- II. The role of AGN feedback and environment on their emergence
› Chemical paradox in a binary system: Exploring metal enrichment in HD 81809B
› Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots
› Oxidation Constraints on Terrestrial Planet Formation from a Ring
› Extreme Transients in Gamma Rays
› Metamorphoses of carbon and oxygen in protoplanetary discs: how chemistry and radial drift transform inner disc C/O ratios
› High-redshift GRB 140304A at z = 5.282 with flaring activity: A multi-wavelength study
› Neutron Star Equation of State via Physics Informed Neural Network
› Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
› An Automated Photometric Pipeline for the 80cm Xizang University Telescope
› Time-reversed stochastic inflation in the quantum well
› Gravothermal Collapse: Robust Against Baryonic Feedback
› Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays
› Refining the Gaia DR3 Parallax Zero-point: A Hybrid Approach Combining Global Parametric Correction with Local Refinement
› MAUVE-MUSE: When Metallicity Follows or Fights Star Formation -- A Mass-Dependent Inversion in Virgo Galaxies
› COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $\mu$m Since $z=3$
› Enhancing Galaxy Classification with U-Net Variational Autoencoders. III. Disk-like Galaxy Identification in JWST Samples of up to redshift 4
› Dynamics of tidal tails of open clusters: I. effects of bar, spiral arms and giant molecular clouds
› Frequency-time-resolved Imaging Spectroscopy of Fine Structures in a Solar Radio Noise Storm
› Mind the Companion : Demographics of Transiting S-type Exoplanets
› Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars
› Reconciling the Fundamental Plane of Early-Type Galaxies with hydrodynamical simulations: The case of IllustrisTNG100-1
› Expanding the Population of Short Gamma-Ray Transients with a Coherent Fermi/GBM Search. A 13-year catalog of short GRBs
› Insights on the Gamma-Ray Bursts variability in their cosmological rest frame
› Gravitational Waves from hybrid defects as probe of Flavor symmetry breaking: Machine-Learning Approach
› Dark Energy Stars in Finch-Skea Spacetime with a Schwarzschild-(Anti)-de Sitter Exterior
› Toward a Phenomenologically Acceptable Quantum Cyclic Universe
› Axions Create Singularities on Extremal Horizons
› Millicharged Particle Constraints from Asymptotic Giant Branch Stars
› Exact Mass Conservation in Binary Neutron Star Merger Simulations
› Effects of the Symmetry energy slope on the exotic content of the neutron stars
› Advancing Heliophysics and Space Weather Modeling through Open Science
› Predictive tracking of radar aurora reveals 500+ mV/m electric-field bursts during the May 2024 G5 storm
› Neutrino helicity oscillations in astrophysical environments: a many-body approach
› Orbital Networks in the Three-Body Problem
› The Escape Velocity Profile of the Milky Way from Gaia DR3
› On the effective spin-mass ratio relation of binary black hole mergers that evolved in isolation
› Vortex driven Schwinger pair creation in the magnetosphere of SgrA*
› Euclid Quick Data Release (Q1). The role of cosmic connectivity in shaping galaxy clusters
› Evolving Dark Sector and the Dark Dimension Scenario
› Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
› Cosmological constraints on Galileon dark energy with broken shift symmetry
› Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves
› A JWST Transit of a Jupiter Analog: II. A Search for Exomoons
› In-depth analysis of the clustering of dark matter particles around primordial black holes. Part II. Analytical prescriptions for spikes
› The heartbeat of stellar halos: Insights from the stellar halo mass-metallicity relation
› Non-Equilibrium Thermodynamics of Black-Hole Coronae: QPOs, Turbulence, and Jets
› Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations
› Leptonic and hadronic models of high-energy nebula around V4641 Sgr
› Unveiling the population of massive quenched galaxies at $z\ge2$ in the COLIBRE simulations -- I. Galaxy demographics
› Super-resolution wavefront reconstruction in adaptive-optics with pyramid sensors
› The influence of magnetic fields in Cloud-Cloud Collisions
› The Keck/DEIMOS Stellar Archive: I. Uniform Velocities and Metallicities for 78 Milky Way Dwarf Galaxies and Globular Clusters
› Bulk and turbulent gas motions in the interacting galaxy cluster Abell 3395 South observed with XRISM
› The Galaxy Stellar Mass-SFR-Size Relation in EAGLE, TNG100, and Observations
› Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC
› A Non-parametric Method for the Inference of Halo Occupation Distributions
› Time-domain Radio-loudness of Active Galactic Nuclei: Intermittency, Memory, and Jet Escape
› First constraints on point-like astrophysical sources using Baikal-GVD muon neutrino events
› A Wide and Deep Exploration of Radio-detected Active Galactic Nuclei with Subaru HSC (WERGS). XII. Final Optical Identification of VLASS Radio Sources from the Subaru/HSC-SSP Wide Survey Over 1200 deg$^2$
› Replacing Gaussian Processes with Neural Networks in Pulsar Timing Array Inference of the Gravitational-Wave Background
› The Illusory Precision of TTV Masses: Hidden Solutions Behind Kepler-9's Tight Mass Ratio
› Large or bright satellite constellations: Effects on observations, including on the background sky brightness
› Eccentricities of millisecond pulsars with intermediate-mass progenitors
› QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole
› Maximum Lifetime of the Vegetative Biosphere
› The role of the Hubble Space Telescope in advancing our understanding of atmospheric escape in exoplanets
› FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays
› First head-to-head comparison of agentic AI applied to the analysis of simulated data of the Einstein Telescope
› A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages
› Enhanced All-Distance Equi-Zenith Angle Method for Cosmic-Ray Anisotropy Measurement
› Strong Constraints on Dark Photon and Scalar Dark Matter Decay from INTEGRAL and AMS-02 data
› Massive hybrid stars within the extended three-flavor quark-meson diquark model

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