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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Księżyc

 Wiadomości z astronet.pl

› Misje Kosmiczne XX wieku: Atlantis
› Recenzja książki „Księżyc. Jak zmienił naszą planetę, przewodził ewolucji i stworzył nas takimi, jakimi jesteśmy”
› Insekty przyszłością diety astronautów?
› W Układzie Słonecznym: Obłok Oorta
› Misje kosmiczne XX wieku: Challenger
› Galaktyczny kartograf – Teleskop Nancy Grace Roman
› Niebo w listopadzie 2025 roku
› Misje kosmiczne XX wieku: Discovery
› Japońska technologia powraca na ISS. Pierwsza misja nowej kapsuły zaopatrzeniowej HTV-X
› Medale dla Polski na IV Międzynarodowej Olimpiadzie z Astronomii i Astrofizyki Juniorów
RSS  Najnowsze prace na astro-ph:

› Is a 1D perturbative method sufficient for asteroseismic modelling of $\beta$ Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
› Think inside the box: cosmic variance and large-scale conformity of high-redshift massive galaxies in the FLAMINGO simulations
› Changing-Look AGN Powered By Disk Tearing
› A Submillimeter Survey of CS Excitation in Protoplanetary Disks: Evidence of X-ray-Driven Sulfur Chemistry
› Dark Photons in the Radio Sky: I. Resonant Conversions in Halos
› Prebiotic Chemistry Insights for Dragonfly: Thermodynamics of Amino Acid Synthesis in Selk Crater on Titan
› Dark Photons in the Radio Sky: II. Resonant Conversions in the Intergalactic Medium
› The SEEDZ Simulations: Methodology and First Results on Massive Black Hole Seeding and Early Galaxy Growth
› Chandra and HST Observations of Radio-Selected (Wandering) Massive Black Hole Candidates in Dwarf Galaxies
› statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys
› Fractional Dynamics in Galactic Nuclei: Non-Local Transport, Transient Phenomena and the Nullification of the Schwarzschild Barrier
› The origin of scatter in the X-ray luminosity - halo mass relation of galaxy clusters
› Analysis of the TAIGA-HiSCORE Data Using the Latent Space of Autoencoders
› Measuring the Dark Matter Self-Interaction Cross-Section with Deep Compact Clustering for Robust Machine Learning Inference
› glitterin: Towards Replacing the Role of Lorenz-Mie Theory in Astronomy Using Neural Networks Trained on Light Scattering of Irregularly Shaped Grains
› Planetary architectures under the influence of a stellar binary
› Analyzing Exoplanet Transits Observed with the WFC3/UVIS G280 Grism
› Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos
› Simulated Real-Time Testing of the Prototype Implementation of the SOFIE Model: The 2025 Space Weather Prediction Testbed Exercise
› Type Ia supernova feedback effects on globular clusters of different masses
› PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-Resolution Phased-Resolved Spectroscopy of The Ultra Hot Jupiter KELT-20 b
› Towards model-free stellar chemical abundances. Potential applications in the search for chemically peculiar stars in large spectroscopic surveys
› Seasonal and Diurnal Variability of Atmospheric Pressure in Jezero Crater, Mars, from MEDA Measurements on the Perseverance Rover
› Searching for Long-Period Radio Transients in ASKAP EMU Data with 10-Second Imaging
› Simulating the Diffuse Neutrino Emission from the Milky Way with GALPROP
› Modeling the Contact Surfaces Formed by Pebble Collisions: Application to Formation of Comet 67P/Churyumov--Gerasimenko
› A precessing magnetic jet as the engine of GRB 250702B
› GalaxyClusters from the DESILegacy ImagingSurveys. III.Star-forming Fraction of Brightest Cluster Galaxies
› Mock Observations for the CSST Mission: CPI-C -- Targets for High Contrast Imaging
› Topmetal-L: A Low Noise Charge-Sensitive Pixel Sensor for POLAR2/LPD
› fiDrizzle-MU: A Fast Iterative Drizzle with Multiplicative Updates
› findAbar: how astronomers may perceive the bar in galaxies differently
› JWST View of the Supernebula in NGC 5253. I. Overview and Continuum Features
› View of the Supernebula in NGC 5253. II. Nebular Lines
› Slow neutrinos: non-linearity and momentum-space emulation
› New ASKAP radio-continuum surveys of the Small Magellanic Cloud
› Where Galaxies Point: First Measurement of the Large-Scale Axial Intrinsic Alignment
› Composite Dissipation in Warm Inflation: Implications for the Primordial Power Spectrum
› Impact of selection criteria on the structural parameters of the Galactic thin and thick discs
› Fast Rotating Blue Straggler Stars in the globular cluster NGC 1851
› Synchrotron radiation from NGC 470 HLX1 - a hidden hyperluminous accreting neutron star?
› Analysis of the magnetic fields in massive young stellar objects with masers
› Estimating accretion times of halo substructures in the Milky Way
› Probing AGN Disks Density Profiles through Gravitational Wave Observations
› Systematic Analysis of Changing-look AGN Variability Using ZTF Light Curves
› Fundamentals of interior modelling and challenges in the interpretation of observed rocky exoplanets
› True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets
› A Dynamical Scalar Field Model for Dark Energy: Addressing the Hubble Tension and Cosmic Evolution
› Curious Case of CGRaBS J0211+1051: Observational Evidence of Lepto-Hadronic Origin of High-Energy Emission?
› Alfven Waves in Partially Ionised Solar Steady-State Plasmas
› Using the Cherenkov Telescope onboard EUSO-SPB2 for Target of Opportunity searches of very high energy neutrino sources
› A predictive framework for realistic star planet radio emission in compact systems
› Ginnungagap -- a massively parallel cosmological initial conditions generator
› Extending the Frontier of Spatially-Resolved Supermassive Black Hole Mass Measurements to at $1\lesssim z\lesssim2$: Simulations with ELT/MICADO High-Resolution Mass Models and HARMONI Integral-Field Stellar Kinematics
› How much can we learn from resolved stellar kinematics of galactic haloes using action-based dynamical models?
› A scalable and accurate framework for self-calibrating null depth retrieval using neural posterior estimation
› Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\lesssim$100 parsec in nearby star-forming galaxies from PHANGS
› Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations
› Collisional and magnetic effects on the polarization of the solar oxygen infrared triplet
› Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
› Les Trente Glorieuses: 29 years of helioseismic observations with the Luminosity Oscillations Imager
› Bayesian model comparison and validation with Gaussian Process Regression for interferometric 21-cm signal recovery
› Shapiro Delay Measurements from Fifteen Years of PSR J1231$-$1411 Radio Observations
› VELOCE III. Reconstructing Radial Velocity Curves of Classical Cepheids
› Constraining the nature of the most extreme Galactic particle accelerator. H.E.S.S. observations of the microquasar V4641 Sgr
› Carbox: an end-to-end differentiable astrochemical simulation framework
› UHECRs Propagation and their Multimessengers: Upper limits and the Impact of the Extragalactic Magnetic Field
› Co-evolution of baryons and dark matter halos of LYRA dwarf galaxies
› The relationship between warm and hot gas-phase metallicity in massive elliptical galaxies and the influence of AGN feedback
› The Local Group L-band Survey: Probing Cold Atomic Gas in IC10 with Neutral Hydrogen Absorption
› A new multiprobe analysis of modified gravity and evolving dark energy
› Dark Matter from Holography
› The Atacama Cosmology Telescope. CMB Lensing from Daytime Data: A First Demonstration
› A Bayesian Perspective on Evidence for Evolving Dark Energy
› Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum
› Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
› Analytical approximations for curved primordial tensor spectra
› Revisiting the maximum mass limit of strange stars in quadratic curvature-matter coupled gravity
› The Non-thermal Energy Window for Laser-Driven Nuclear Reactions
› Evading the BBN bound with a soft stiff period
› Cosmological Limits on Strong Dark Forces
› $L_\mu-L_\tau$ gauge bosons in beam dumps and supernovae
› Ultralight Dark Matter from the Edge of Field Space
› Freezing-in the Axiverse
› Dark matter by design: $Q$-balls, neural networks and galaxy rotation curves
› Photon counting readout for detection and inference of gravitational waves from neutron star merger remnants
› Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
› Searching for screened scalar forces with long-baseline atom interferometers
› Mitigating numerical dissipation in simulations of subsonic turbulent flows
› CORONA-Fields: Leveraging Foundation Models for Classification of Solar Wind Phenomena
› Rediscovering the Lunar Equation of the Centre with AI Feynman via Embedded Physical Biases
› Trapped and Unstable: Axion-like particle fragmentation at finite temperature
› Confronting dark energy in Harada's Conformal Killing Gravity with observational data
› Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath
› Probing thermal leptogenesis and dark matter through primordial gravitational waves from a supercooled universe
› Bubble Friction in Symmetry-Restoring Transitions
› Generating optimal Gravitational-Wave template banks with metric-preserving autoencoders
› A Fast Earth-scattering Formalism for Light Dark Matter with Dark Photon Mediators
› Dark Matter and Baryon Asymmetry from Monopole-Axion Interactions
› Challenging the AGN scenario for JWST/NIRSpec LRD and non-LRD broad H$\alpha$ emitters in light of non-detection of NIRCam photometric variability and X-ray
› Extracting the Temperature Analytically In Hydrodynamics Simulations with Gas and Radiation Pressure
› Evidence for a hot galactic halo around the Andromeda Galaxy using fast radio bursts along two sightlines
› MOA-2010-BLG-328: Keck and HST Expose the Limits of Occams Razor in Microlensing
› Perturbation Theory in the Minimally Extended Varying Speed of Light (meVSL) Model
› The Host Galaxies of Fast Radio Bursts Track a Combination of Stellar Mass and Star Formation, Similar to Type Ia Supernovae
› Spectroscopic r-Process Abundance Retrieval for Kilonovae III: Linking Spectral and Light Curve Modeling of the GW170817 Kilonova
› Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
› The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters
› Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer
› ASASSN-24fw: Candidate circumplanetary disk occultation of a main-sequence star
› Neural-Network Chemical Emulator for First-Star Formation: Robust Iterative Predictions over a Wide Density Range
› Studying the black widow pulsars PSR J0312$-$0921 and PSR J1627$+$3219 in the optical and X-rays
› Relativistic Dissipative Magnetohydrodynamics for accretion disks
› Can "premature collapse" form black holes in the upper and lower mass gaps?
› Beyond No Tension: JWST z > 10 Galaxies Push Simulations to the Limit
› The Physics of Cometary Anti-tails as Observed in 3I/ATLAS
› Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe
› Enhancing the development of Cherenkov Telescope Array control software with Large Language Models
› Magnetic Field-Line Curvature and Its Role in Particle Acceleration by Magnetically Dominated Turbulence
› Direct multi-model dark-matter search with gravitational-wave interferometers using data from the first part of the fourth LIGO-Virgo-KAGRA observing run
› The effect of mass and morphology on the mass assembly of galaxies
› Exploring the spectral characteristics of the periodic burster 4U 1323-62: Type-I X-ray burst and persistent emission
› The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration
› J-PLUS Reconstructing the Milky Way Disc's star formation history with twelve-filter photometry
› Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation
› Mock Observations for the CSST Mission: HSTDM--Synthetic Data Generation
› Adsorption of volatiles on dust grains in protoplanetary disks
› From M100 to NGC 7331: A Multiband Study and Physical Parameters in Nearby Galaxies
› Tests of General Relativity with GWTC-3
› Numerical gravitational backreaction on cosmic string loops from simulation
› Detectability of Massive Boson Stars using Gravitational Waves from Fundamental Oscillations
› Finite-temperature bubble nucleation with shifting scale hierarchies
› Loops in inflation with strongly non-geodesic motion
› Broadband Optical Modulation and Control at Millikelvin Temperatures
› Linking the KM3-230213A Neutrino Event to Dark Matter Decay and Gravitational Wave signals
› How gravitational waves change photon orbital angular momentum quantum states
› $g$-mode oscillations of dark matter admixed neutron stars
› Alexei Starobinsky and Modern Cosmology
› Is the $\Lambda$CDM Model in Crisis?
› Extracting Properties of Dark Dense Environments around Black Holes from Gravitational Waves

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