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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Astronomia w Krakowie
Zdjecie: The International Space Station and a halo around the Moon
The International Space Station and a halo around the Moon
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 Wiadomości z astronet.pl

› Pixinsight cz.VI – Łączenie zdjęć monochromatycznych w kolorowy obraz
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› Katalog Caldwella: C98
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› Podsumowanie roku 2025 w astronomii i astronautyce
› Katalog Caldwella: C19
RSS  Najnowsze prace na astro-ph:

› Emergent Complexity in Nuclear Reaction Networks: A Study of Stellar Nucleosynthesis through Chemical Organization Theory
› Exoplanet characterization with NASA's Habitable Worlds Observatory
› Transiting exoplanets as the immediate future for population-level atmospheric science
› Characterizing turbulence in galaxy clusters: defining turbulent energies and assessing multi-scale versus fixed-scale filters
› Formation of massive multiple-star systems: early migration and mergers
› Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks
› GA-NIFS: high prevalence of dusty and metal-enriched outflows in massive and luminous star-forming galaxies at $z\sim3-9$
› Cosmological back-reaction of baryons on dark matter in the CAMELS simulations
› Ultraviolet observations of atmospheric escape in exoplanets with the Habitable Worlds Observatory
› Spectral Signatures of Spinning Dust from Grain Ensembles in Diverse Environments: A Combined Theoretical and Observational Study
› The Energy-Duration Relationship in Astrophysical Self-Organized Criticality Systems
› VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion
› CAMELS Environments: The Impact of Local Neighbours on Galaxy Evolution across the SIMBA, IllustrisTNG, ASTRID, and Swift-EAGLE Simulations
› Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
› The Role of Interferometric Phase in Measuring Black Hole Photon Rings
› Incorporating Wavefront Error, Wavefront Sensing and Control, and Sensitivities into Exposure Time Calculations for Future Space Missions with the Error Budget Software (EBS)
› Collision between molecular clouds IV: The role of feedback and magnetic field in head on collisions
› Exploring the internal structure of a neutron star and the associated magnetic fields aided by the mass-radius relationship
› NASA Decadal Astrobiology Research and Exploration Strategy (NASA-DARES 2025) White Paper -- Habitable Worlds Observatory Living Worlds Science Cases: Research Gaps and Needs
› Generalized Bondi Accretion Flow with and without Outflow
› Radio Signatures of Cosmic-Ray Particle Showers in Deep In-Ice Antennas
› In-ice Radio Signatures of Cosmic Ray Particle Cascades
› Radio Morphing: Fast computation of inclined air shower radio emission
› Simulations of Electron Beam Interactions in Brown Dwarf Atmospheres
› Brahe: A Modern Astrodynamics Library for Research and Engineering Applications
› Ruling Out Compact Jets as the Dominant Source of Radio Emission in Radio-quiet, High Eddington-ratio Active Galactic Nuclei
› High-order expansions of multi-revolution elliptic Halo orbits in the elliptic restricted three-body problem
› A binary merger product as the direct progenitor of a Type II-P supernova
› AstroSat UV Deep Field IV. An Extended UV disk around a massive spiral galaxy at z=0.67
› Constraining Inflation Models with Spinning Voids
› Impact of a negative cosmological constant on the reconstruction of dark energy in light of DESI BAO data
› Evaluating the efficacy of a data cube treatment procedure for kinematic analyses: application to NGC 3115 and NGC 4699
› SPHEREx Re-Observation of Interstellar Object 3I/ATLAS in December 2025: Detection of Increased Post-Perihelion Activity, Refractory Coma Dust, and New Coma Gas Species
› Joint Optical-HI mock catalogs and prospects for upcoming HI surveys
› Computing Natural Magnitudes in the Photometric Systems of Astronomical Plates using Gaia DR3 SEDs
› Turbulent Properties of Interplanetary Coronal Mass Ejections Observed by Solar Orbiter in the Inner Heliosphere
› The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies-VIII. A Census of Long-Period Variable Stars across the Andromeda Dwarf Satellite System
› Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated
› Rings around irregular bodies. II. Numerical simulations of the 1/3 spin-orbit resonance confinement and applications to Chariklo
› Magnetic winds in resistive compact binary discs
› The Structure of Poloidal Fields Embedded in Thin Disks
› A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements
› Magma Ocean Waves and Thermal Variability on Lava Worlds
› On the 3D time evolution of the dust size distribution in protostellar envelopes
› More power on large scales
› The Hierarchical Structure of the Open Cluster NGC 752
› The Potential Impact of Neuromorphic Computing on Radio Telescope Observatories
› Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements
› Limit cycles and the climate history of Mars
› First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars
› A Study Revealing Physical Attributes of Supernova Remnant in G321.3-3.9
› Does the radio-active phase of XTE~J1810$-$197 recur following the same evolutionary pattern?
› The stellar initial mass function of nearby young moving groups
› Broad line regions behind haze: Intrinsic shape of Br$\gamma$ line and its origin in a type-1 Seyfert galaxy
› The magnetic helicity driven solar-type dynamo
› What can be learnt from UHECR anisotropies observations Paper III: Update with new data and Galactic magnetic fields models
› Photometric Redshift Estimation Using Scaled Ensemble Learning
› WISE/CatWISE Constraints on Dysonian Waste-Heat Technosignatures in Nearby Galaxies
› Emulator-Based Inference of Cosmological Subgrid Models
› Multi-wavelength properties of changing-state active galactic nuclei: I. the evolution of soft excess and X-ray continuum
› New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
› Direct detection of the non-thermal X-ray emission from the Arches star cluster
› Strong Evidence for Dark Sector Interactions
› Expanding the C$_3$H$_6$O$_2$ Isomeric Interstellar Inventory: Discovery of Lactaldehyde and Methoxyacetaldehyde in G+0.693-0.027
› Possible evidence for a pair-instability supernova nature of ultra-early JWST sources
› Temporal variability of polarization in blazars
› Asymmetric distribution of Fe-peak elements in Cassiopeia A revealed by XRISM
› The converging gas flow around the infrared dark cloud G28.3
› Characterization of two new transiting sub-Neptunes and a terrestrial planet around M-dwarf hosts
› A free-fall-based switching criterion for P^3 T N-body methods in collisional stellar systems
› Advanced computing for reproducibility of astronomy Big Data Science, with a showcase of AMIGA and the SKA Science prototype
› A Study of Two Type IIb Supernovae: SNe 2008aq and 2019gaf
› Functionalization of Benzene Ices by Atomic Oxygen
› Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline
› Instantaneous thermally-driven erosion can explain dearth of dark near-Sun asteroids
› A Guided Unconditional Diffusion Model to Synthesize and Inpaint Radio Galaxies from FIRST, MGCLS and Radio Zoo
› Modified Gravity and the Origin of the Excess Radio Galaxy Number-Count Dipole
› The combined X-ray and $\gamma$-ray modeling of millisecond pulsars PSR J0030+0451 in the dissipative magnetospheres
› High-resolution simulations of non-thermal emission from LS 5039
› Revealing the diversity of Type IIn supernova progenitors through their environments
› CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
› Isochrone Fitting of Galactic Globular Clusters -- VII. NGC\,1904 (M79), NGC\,4372, and revision of NGC\,288, NGC\,362, NGC\,5904 (M5), NGC\,6205 (M13), and NGC\,6218 (M12)
› Uniform models of neutron and quark (strange) stars in General Relativity
› Cosmic rays, gamma rays and neutrinos from discrete black hole X-ray binary ejecta
› Timing Gamma-ray Pulsars using Gibbs Sampling
› Deep Search for Joint Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of LIGO and Virgo
› Galaxy Mergers in UNIONS -- II: Predicting Timescales in the Post-Merger Regime
› Impact of Nuclear Reaction Rates on Calcium Production in Population III Stars: A Global Analysis
› A Unified Charge-Dependent Modulation Model for AMS-02 Proton and Antiproton Fluxes during Solar Minimum
› CHEX-MATE: Relationship between X-ray and millimetre inferences of galaxy cluster temperature profiles
› Tachyonic gravitational dark matter production after inflation
› Brightest GRB flare observed in GRB 221009A: bridge the last gap between flare and prompt emission in GRB
› Brightness Characterization and Modeling for Amazon Leo Satellites
› Induced gravitational waves - beyond linear cosmological perturbation theory
› A COLIBRI Photometric Study of SN 2025bvm: A Normal, Slowly Declining Type Ia Supernova
› Core Scouring Dynamics and Gravitational Wave Consequences: Constraints on Supermassive Black Hole Binary Hardening
› Popcorn in the sky: Identifying primordial black holes in the gravitational-wave background
› Euclid preparation. Testing analytic models of galaxy intrinsic alignments in the Euclid Flagship simulation
› Euclid preparation. Calibrated intrinsic galaxy alignments in the Euclid Flagship simulation
› Testing subhalo abundance matching with galaxy kinematics
› Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE
› Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequencies
› Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISE
› Axion misalignment as a synchronization phenomenon
› First Multi-Constellation Observations of Navigation Satellite Signals in the Lunar Domain by Post-Processing L1/L5 IQ Snapshots
› Temperature-Dependent CPT Violation: Constraints from Big Bang Nucleosynthesis
› Cosmological Dynamics on a Novel $f(Q)$ Gravity Model with Recent DESI DR2 Observation
› Spec-o3: A Tool-Augmented Vision-Language Agent for Rare Celestial Object Candidate Vetting via Automated Spectral Inspection
› Mati\`ere noire et (ou) gravitation modifi\'ee : une approche historique et \'epist\'emologique
› Kerr-Newman-de Sitter black holes in $f(R)$ gravity with constant curvature: horizon structure and extremality
› Limits of vacuum-template subtraction for LISA massive black hole binary sources in realistic environments
› Numerical Study of Polytropes with n=1 and Differential Rotation
› Strong Einstein-Hilbert Gravity Inflation and ACT Phenomenology
› Viable f(R) Scenarios Unifying Inflation with Realistic Dynamical Dark Energy
› IndIGO-D: Probing Compact Binary Coalescences in the Decihertz GW Band
› Oscillatory Freeze from Inertial Holographic Dark Energy
› Chiroptical effect induced by gravitational waves
› Bringing Computation to the data: Interoperable serverless function execution for astrophysical data analysis in the SRCNet
› Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility
› Landau damping of disturbances in nearly inviscid inflectional shear flows
› Multi-Physics Bayesian Analysis of Neutron Star Crust Using Relativistic Mean-Field Model
› Learning the relations between neutron star and nuclear matter properties with symbolic regression
› Rotation-dependent $I$-Love-$Q$-$\delta M$ relations in perturbation theory
› Systematic Biases in Gravitational-Wave Parameter Estimation from Neglecting Orbital Eccentricity in Space-Based Detectors
› Exploring Lorentz Invariance Violation from Ultra-high-energy Gamma Rays Observed by LHAASO
› Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations
› Exploring the interplay between star formation efficiency and dust in regulating the UV luminosity of early systems in the JWST and ALMA era
› A model of the heliocentric dust ring on Venus orbit
› Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT
› The PAU Survey: Measuring intrinsic galaxy alignments in deep wide fields as a function of colour, luminosity, stellar mass and redshift
› PEARLS: 21 Transients Found in the Three-Epoch NIRCam Observations in the Continuous Viewing Zone of the James Webb Space Telescope
› JWST Reveals a Candidate Jellyfish Galaxy at z=1.156
› Bayesian constraints on quark stars from multi-messenger observations
› Angular correlation functions of bright Lyman-break galaxies at $\mathbf{3 \lesssim z \lesssim 5}$
› Confronting Mukhanov Parametrization of Inflationary Equation-of-State with ACT-DR6
› MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
› Little Red Dots and their Progenitors from Direct Collapse Black Holes
› What determines the $\gamma$-ray luminosities of classical novae?
› COCONUT: A coronal model with an energy decomposition strategy
› Accelerated calibration of semi-analytic galaxy formation models
› Needlets and foreground removal for SKAO hydrogen intensity maps
› $\texttt{Jipole}$: A Differentiable $\texttt{ipole}$-based Code for Radiative Transfer in Curved Spacetimes
› A Pristine Star-Forming Complex at z=4.19
› Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts
› Measuring the Central Dark Mass in NGC 4258 with JWST/NIRSpec Stellar Kinematics
› SymBoltz.jl: a symbolic-numeric, approximation-free and differentiable linear Einstein-Boltzmann solver
› Modeling gravitational wave sources in the MillenniumTNG simulations
› New ultralight scalar particles and the mass-radius relation of white dwarfs -- the important role of Sirius B
› MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars
› Born to be recycled: a comprehensive population synthesis of the Galactic millisecond pulsars
› Implications of Joint Spectral Analysis of Gamma-Ray Bursts detected by Fermi Large Area Telescope and Gamma-ray Burst Monitor on Phenomenological Correlations
› Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots
› Stellar Wind-Blown Bubbles as Environments for Late-Time Rebrightening of Gamma-Ray Burst Afterglows
› Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
› First Cosmological Constraints from the Joint Analysis of Galaxy Clustering and the Kinetic Sunyaev-Zel'dovich Effect
› Machine-Learning Estimation of Energy Fractions in MHD Turbulence Modes
› SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material
› The HITRAN2024 methane update
› JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS
› Large Language Models for Limited Noisy Data: A Gravitational Wave Identification Study
› The Narrow Emission Lines of Seyfert 1 Galaxies: Comparisons with a Large SDSS Sample
› ExoMol line lists -- LXIII: ExoMol line lists for 12 isotopologues of CO$_2$
› Ultralight Dark Matter Constraints from NanoHertz Gravitational Waves
› First reverberation mapping of a Bowen fluorescence line
› Einstein Probe Discovery of an X-ray Flare from K-type Star PM J23221-0301
› Pre-supernova O-C shell mergers could produce more $^{44}\mathrm{Ti}$ than the explosion
› Multiband Gravitational Wave Detection Prospects for M31 UCXB-1 System in Low and Middle Frequency Band
› Particle production and Higgs reheating
› A global view of post-interaction white dwarf-main sequence binaries
› Vetting and False Positive Analysis of TOI 864.01: Evidence for a Likely Hierarchical Eclipsing Binary Masked by Dilution
› A Long Tidal Feature Extending from a Low-Redshift Galaxy Revealed in Rubin Data Preview 1 Imaging
› Energetic particles accelerated via turbulent magnetic reconnection in protoplanetary discs - I. Ionisation rates
› Hidden pattern of self-invariant cosmic expansion: Empirical evidence from Hubble diagram of supernovae
› Corrections to the Black hole entropy from a Bose Einstein condensate: a semi-classical phenomenological approach
› Supernova constraints on lepton flavor violating ALPs
› Sound waves from primordial black hole formations
› Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
› Dark Matter in X-rays: Revised XMM-Newton Limits and New Constraints from eROSITA
› Diffuse astrophysical neutrinos from dark matter around blazars
› Stability of Thin Shell and Wormhole Configurations: Schwarzschild, Schwarzschild -- (Anti-) de Sitter, and FLRW Spacetimes
› Quasi-Normal Modes and Nonlinear Electrodynamics in Black Hole Phase Transitions
› Color-superconducting quarkyonic matter
› Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
› Infrared Quantum Electrodynamics and the Rayleigh-Jeans Physics
› Cavity Multimodes as an Array for High-Frequency Gravitational Waves
› Machine learning for radiative hydrodynamics in astrophysics

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