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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RSS  Najnowsze prace na astro-ph:

› Spatially Resolved AGN Ionization and Star Formation at Cosmic Noon with JWST/JEMS
› Geomagnetic Storm Impacts On The Ionosphere Over T\"urkiye During Solar Cycle 25: Focusing On The May 2024 Storm
› Probabilistic neural network approach to determining parameters of eclipsing binaries
› Constraints on the Galactic Chemical Evolution of $^3\rm{He}$
› Tree-ring structure of Galactic bar resonance in N-body simulations
› Low-mass Active Galaxies in the SAMI Galaxy Survey with Spatially-resolved Spectroscopy
› Euclid preparation. Non-Gaussianity of 2-pt statistics likelihood: Parameter inference with a non-Gaussian likelihood in Fourier and configuration space
› Three Thousand Motion-Confirmed L and T Dwarf Candidates from the Backyard Worlds:~Planet 9 Citizen Science Project
› Calibrating Photometric Mid-Infrared Star Formation Rates for JWST
› Analysing Turbulent Energy Cascade in a Coronal Mass Ejection using Empirical Mode Decomposition
› The unusually red delay spectrum of the low-mass black hole AGN NGC\,4051 as revealed by intensive continuum reverberation mapping with the Las Cumbres Observatory
› Low-mass failed supernovae and the $10\,M_{\odot}$ peak in the merging black hole mass distribution
› Galaxy formation in the first billion years
› The Cosmic Web in the DESI Early Data Release: A Probabilistic Environment Catalog
› Insights from GRBs for optical follow-up of gravitational wave counterparts
› Impacts of Voids, Line of Sight Interactions, and Local Emission Environment on Detectability of Gamma-Ray AGN
› The velocity field of our Milky Way outer stellar halo based on DESI DR2
› The Galactic Halo Rotation by Weyl Incorporated Gravity
› Unusually Hot Interiors Could Reconcile the Missing Methane Problem for Warm-to-Hot Exoplanets with Hydrogen Atmospheres
› Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters
› Cosmological Constraints on the Generalized Uncertainty Principle from Redshift-Space Distortions
› Estimates of the Dynamic Characteristics of Binary Systems for Traversable Wormholes Search
› Diverse lifestyles of bar-like galaxies and their coevolution with the brightest galaxy in the most massive cluster of TNG50
› Spectroscopic Case Studies of Four Long-duration Transition-region Explosive Events
› Heating of a plasma sheet in nonequilibrium ionization with nonthermal electrons
› SN2024abfl: A Low-Luminosity Type IIP Supernova at the Low-Mass End of Core Collapse
› The impact of the eROSITA bubbles on Galactic cosmic-ray transport
› The Real and Pseudo Dispersion Measures of FRB~20220912A
› Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing
› Asteroseismic Diagnostics for Red Giants with Kepler: Measuring epsilon and Small Frequency Separations in 16,000 Stars
› CORSIKA 8: A General Framework for Particle Cascade Simulations
› Spectropolarimetry of the changing-look active galactic nucleus NGC 1566 and its potential link to supermassive black hole binaries
› Gaussian Process Inference of Stochastic Magneto-Active Dynamics and Viscosity in Swift J1727.8-1613
› Geant4-IcyMoons: Simulating Electron Interaction Physics in Irradiated Astrophysical Ices
› No evidence for dynamical dark energy from the Combo correlation of GRBs
› Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog
› SDSS J153231.80+420342.7: a triple black hole candidate with a close binary black hole
› Non-minimally coupled quintessence with sign-switching interaction
› Consistency relations of amplitude and phase fluctuations of gravitational waves magnified by strong gravitational lensing
› A research roadmap for assessing the feasibility of warming Mars
› GECAM discovery of a peculiar magnetar X-ray burst (MXB 221120) from SGR J1935+2154 associated with a fast radio burst
› Revealing the neutrino mass through persistent homology of the cosmic web
› Magneto-Active Environments in Pulsar Binaries with the MeerKAT Telescope: I. Pulsar sample and their basic properties
› Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI
› Possible Reforms of the Tibetan Lunisolar Calendar
› Plummer Dark Matter Black Hole with Topological Defects: Shadow, Greybody Factors, Quasinormal Modes, and Thermodynamics
› A framework for creating galaxy models in the geometry of the conservation group with dark matter halos and flat rotation curves
› Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\gamma$-ray Sky
› Influence of tides and self-gravity on Ultra-Light Dark Matter Bounds from Dwarf Galaxies
› Is Gravity Always Enough to Yield a Classical Universe?
› High-Frequency Gravitational Wave Constraints from Graviton-Photon Conversion in the M87 Galaxy
› Supermassive Primordial Black Holes from a Catalyzed Dark Phase Transition for Little Red Dots
› Bipartite Solution to the Lithium Problem
› Vacuum bubbles from cosmic ripples
› Nonperturbative suppression of beyond-General-Relativity effects in quadratic gravity
› High-power Test and System Integration of Direct RF Sampling Based LLRF Control and Monitoring System for S-Band Accelerating Structures
› Small-Scale Dynamo for Full Spectrum of Hydrodynamic Turbulence in Kazantsev Model
› Interior geometry of black holes as a probe of first-order phase transition
› The Axion Helical Misalignment Mechanism
› Triggering physical plasmoids in forming current sheets: conditions and diagnostics
› Localized Steps toward ACT-Favored Inflation
› AstroConcepts: A Large-Scale Multi-Label Classification Corpus for Astrophysics
› X-ray Response of the Fully-Depleted, p-Channel SiSeRO-CCD
› Detection of Gamma-ray Halos around Nearby Late-type Galaxies
› Halo Spin Depends on The Distance to Cosmic Filament
› Conservative limits on primordial black holes from the LIGO-Virgo-KAGRA observations
› Interstellar dust production, destruction and effects of dust depletion in galaxies
› Alleviating the Hubble tension with Torsion Condensation (TorC)
› Rotating Neutron Stars with Dark Matter Halos
› Revealing Unresolved White Dwarf-Main Sequence Binaries using Gaia DR3 and GALEX I. A Volume limited study of 100 pc
› A nearly pristine star from the Large Magellanic Cloud
› Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint
› A GLIMPSE into the very faint-end of the H$\beta$+[OIII]$\lambda\lambda$4960,5008 luminosity function at z=7-9 behind Abell S1063
› Galaxy Underdensities Host the Clearest IGM Ly$\alpha$ Transmission and Indicate Anisotropic Reionization
› Thermal Deformations in Super-Eddington Magnetized Neutron Stars: Implications for Continuous Gravitational-Wave Detectability
› BlazEr1: The eROSITA Blazar Catalog. Blazars and Blazar Candidates in the First eROSITA Survey
› Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning
› Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region
› unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis
› Rotational Light-Curve Recovery & Predictions of the LSST Yield of Hildas
› SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars
› The GLASS-JWST Early Release Science Program. V. H$\alpha$ luminosity functions at $z\sim1.3$ and $z\sim2.0$
› Ring Asymmetry and Spin in M87*
› Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations
› A Closer Look at the Dynamical State of the High-redshift Galaxy Cluster SPT-CL J2215-3537
› Sunspot simulations with MURaM -- I. Parameter study using potential field initial conditions
› The approximate gravitational lensing multiple plane mass sheet degeneracy
› Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE Observations
› Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
› Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows
› A Bayesian Method for Air-Shower Reconstruction using Information Field Theory
› Small-Scale and Transient EUV Kernels in Solar Flare Ribbons
› Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages
› A bending in the size-mass relation of star-forming galaxies across $0.5 < z < 6.0$ at a critical stellar mass of $10^{10}M_\odot$ revealed by JWST
› Primordial Non-Gaussianity and the Field-Level Cramer-Rao Bound
› Dynamics and stability of magnetized AGN-blown bubbles in clusters of galaxies
› Universality of Halo Shape and its Morphological Evolution across Cosmic Time
› A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7
› Formation and disruption of wide binaries in star clusters revealed by N-body simulations
› The radial component of the local Galactic magnetic field in 3D
› Impostor Among $\nu$s: Dark Radiation Masquerading as Self-Interacting Neutrinos
› Exploration of vertical self-resonant bifurcations from Distant Retrograde Orbits (DROs) in the Earth-Moon Circular Restricted Three-Body Problem (CR3BP)
› String Corrected Scalar Field Inflation Compatible with the ACT Data
› Demagnifying gravitational lenses as probes of dark matter structures and nonminimal couplings to gravity
› Plotting correlated data
› Sculpting of Martian brain terrain reveals the drying of ancient Mars
› What does it take to have $N_{\rm eff} < 3$ at CMB times?
› Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run

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