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:

› The Catastrophic Consequences of Agnosticism for Life Searches and a Possible Workaround
› Wave interference as the origin of the cyclic magnetorotational dynamo in accretion disks: insights from weakly nonlinear theory and local shearing box simulations
› Built to Rest: The Evolving Star-Forming Main Sequence Requires Episodic Quiescence or Late Assembly
› The SRG/eROSITA diffuse soft X-ray background II. spectra and morphology of the eROSITA bubbles in the western Galactic hemisphere
› Peering down the barrel with DESI DR2: 10 000+ inflows at $z$ < 0.6 reveal how galaxies accrete cold gas
› Are Nucleosynthetic Yields Universal? Interpreting the Multi-Elemental Abundances of Quiescent Galaxies over Cosmic Time Using Milky Way Stars
› Comparing Hemispheres: Anisotropy in the deceleration parameter $q_0$
› Post-Recombination Fluctuations from a Sequestered Dark Sector
› Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations
› The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) XI: Gas-dust interactions and radial offsets between micron and millimetre-sized grains
› Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
› Euclid preparation. Three-dimensional galaxy clustering in configuration space: Three-point correlation function estimation
› Resolving the Multiphase Outflow, Shock Signatures, and PAHs in the AGN-Starburst Composite ULIRG F10565+2448 with JWST MIRI/MRS
› Chromosphere of the quiet Sun -- II. Atmospheric response to small-scale magnetic flux emergence
› Uncovering the multi-scale structure of dust distribution in nearby galaxies
› On the cool nature of coronal nanojets
› Anisotropic non-Maxwellian velocity distributions in the solar transition region
› A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications
› Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST
› Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors
› ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
› Primordial Black Hole contribution to the stochastic background of Gravitational Waves
› Utilizing Dispersion Measure of Fast Radio Bursts to Probe the Intergalactic Medium Turbulence
› A Search for High Frequency Oscillations in TESS Cycle 7
› COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling
› Data-Constrained Modeling of Electron Transport and Asymmetric Precipitation in the 2011 August 4 Solar Flare
› StreakMind: AI detection and analysis of satellite streaks in astronomical images with automated database integration
› High-Redshift Gravitational Lens Discoveries in JWST NIRCam Using AnomalyMatch
› Mitigating effects of telescope jitter through differentiable forward-modeling
› \textit{Euclid} preparation. Baryon acoustic oscillations extraction techniques: comparison and optimisation
› Interpreting Galaxy Physical Properties Using Stellar Population Synthesis
› Identification and characterization of 15265 super-Nyquist frequencies in 1309 {\delta} Scuti stars from Kepler photometry
› Systematic underestimation of polarisation angle dispersion and its consequences for magnetic field strength estimates in star-forming regions
› The ESO SupJup Survey. X. A carbon isotope contrast in the young ROXs 12 system
› Unveiling hidden millihertz quasi-periodic oscillations in 1A 0535+262
› Searching For Fast Radio Transients And Radio Pulsars Using SPOTLIGHT
› The Cocoon from a Massive Star's Death: VLA Radio Polarization Study of Possible Historical Supernova Remnant G7.7$-$3.7
› Iterative Poisson Solvers for Self-gravity with the GPU Code Astaroth
› The Significant Role of Hydrogen in the Formation of Silicon Carbide in Evolved Stars
› Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves
› Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants
› Primordial high energy neutrinos
› The JWST early galaxy crisis resolved by a reionization degeneracy
› Not So Isolated: Green Pea Galaxies in Overdense Environments revealed by VLT/MUSE
› A public dataset of Ariel simulated observations for developing exoplanetary atmosphere data reduction pipelines
› The First Look of Gaia: Daily data quality and instrument health assessment with automated early warnings
› Modeling the UV-photon irradiation of CS$_2$-bearing ices in the laboratory with the pyRate gas-grain astrochemical code. New insights into the missing sulfur problem
› PALEOS: Multiphase Equations of State and Mass-Radius Relations for Exoplanet Interiors
› What is the Strouhal number of turbulence driven by supernovae?
› Thermal activation rate of dilute axion stars close to the maximum mass
› VERSUS: An excursion-set-inspired void-finder for the Stage-IV era
› New constraints on primordial non-Gaussianity from large-scale cross-correlations of CMB lensing and the cosmic infrared background
› Unifying Transport Models of Thermohaline Convection in Stars
› IRIS NUV diagnostics for Ellerman bombs: spectral properties, thermodynamics, and formation height
› Multipole Functions for Image Analysis II: Equal Area Weighting and Application to Supernova Remnant Images
› The Keplerian disk, envelope, and streamers surrounding an early O-type protostar in the Sagittarius C cloud of the Central Molecular Zone
› Microlensing time-scales and flux magnification probabilities of a sample of 204 lensed quasars
› On the slope of the power spectrum of the density field in isothermal supersonic compressible turbulence
› The Range of Cumulative XUV Flux on GJ 1132 b
› Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers
› The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
› Synergistic Effects of Ocean Salinity and Planetary Obliquity Enhance Habitability of Cold Exo-Earths
› PySME v1.0: improved modelling of stellar spectra for survey-scale applications
› The Computed Microwave Spectrum of the Protonated Fullerene C60H+
› A Multi-parameter Fuzzy Set Framework for Classifying Red, Blue, and Green Valley Galaxies
› Orbital Nodal Phase as a Pipeline Invariant in Black Hole Timing
› Metastable strings at PTAs: classical stability analysis
› Searching for UFOs from the early universe: direct detection prospects for relativistically decoupling dark matter
› Can wormholes have vanishing Love numbers?
› On The Nonthermal Power Laws In Magnetized Turbulent Plasmas
› Constraining Tsallis Corrections to Photon Reheating from Electron-Positron Annihilation
› Non-radial pulsations of gravitationally coupled two-fluid neutron stars in general relativity
› Self-Interaction Bounds on Ultralight Dark Matter Couplings to Matter
› Resonances as signatures of scalar clouds in eccentric extreme-mass-ratio inspirals
› Minimum lifetime of a black hole
› Methodological refinement of the submillimeter galaxy cross-correlation function measurements and their uncertainty estimation
› Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites
› The NANOGrav 15-Year Data Set: A Case Study for Simplified Dispersion Measure Modeling for PSR J1455-3330 and the Impact on Gravitational Wave Sensitivity
› NASA Exoplanet Exploration Program (ExEP) Science Gap List
› Artificial Broadcasts as Galactic Populations: III. Constraints on Radio Broadcasts from the Cosmic Population of Inhabited Galaxies
› Placing the Near-Earth Object Impact Probability in Context
› Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid
› JWST's first view of the most vigorously star-forming cloud in the Galactic center -- Sagittarius B2
› Probing the limits of cosmological information from the Lyman-$\alpha$ forest 2-point correlation functions
› Detection of supernova magnitude fluctuations induced by large-scale structure
› Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. I. Hydrodynamics
› Formation of Close Binaries through Massive Black Hole Perturbations and Chaotic Tides
› Squeezed Limit non-Gaussianity Estimation with Cosmic Shear
› Comparing cosmic shear nulling methods for Stage-IV surveys
› Magnetic field spreading from stellar and galactic dynamos into the exterior
› Characterization of telecentric dual-etalon Fabry-P\'erot systems from observational data. Properties of the CRISP2 instrument at the Swedish 1-m Solar Telescope
› Detection of Lensed Gravitational Waves in the Millihertz Band Using Frequency-Domain Lensing Feature Extraction Network
› Orbital Stability of Closely-Spaced Four-planet Systems
› Shadows of Giants: Constraints on Stupendously Large Black Holes from Negative Sources against the Cosmic Microwave Background
› Universality in spacetime $\omega$ modes of quarkyonic stars
› Planetary Desert around Compact Binaries: Dynamical Instability Triggered by Resonance-Induced Eccentricity Excitation
› ULTIMATE deblending I. A 50-band UV-to-MIR photometric catalog combining space- and ground-based data in the JWST/PRIMER survey
› Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores
› Cosmological simulation of a radio synchrotron bridge between pre-merging galaxy clusters
› The diffuse gamma-ray sky of a Milky Way analogue: Local diversity and global constraints
› Variable ADAF disk as the origin of Changing-Look AGN
› Magnetic geometry of M dwarfs in the southern PLATO field
› Scale-dependent surface and volume density properties of filaments in molecular clouds
› Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO
› Differentiable Forward Modeling for Efficient and Accurate Shear Inference
› Microlensing of fast and slow compact objects
› Six New Variable Stars Discovered from Ground-Based Photometry and Characterized with TESS Data
› A common four-beam geometry reveals altitude-stratified GeV pulses in canonical young pulsars
› Deep Learning galaxy cluster's structural parameters from Weak Lensing observations
› Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
› Pulsar timing array analysis in a Legendre polynomial basis
› Strongly Coupled Sectors in Inflation: Gapped Theories of Unparticles
› Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
› Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr

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