Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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Astronomia w Krakowie
Zdjecie: Zdjęcie mgławicy w Orionie (M42) zrobione z Suhory
Zdjęcie mgławicy w Orionie (M42) zrobione z Suhory
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 Wiadomości z astronet.pl

› Kosmiczny przegląd miesiąca AstroNETu – maj 2026 roku
› Niebo w czerwcu 2026 roku
› Wybuch New Glenna podczas testu – Blue Origin apeluje o zbieranie szczątek
› Dalekie ekspozycje w astrokrajobrazie
› NASA przedstawiła szczegóły planów bazy księżycowej – w tym 3 nowe misje
› Creotech udostępnił strategię rozwoju na nadchodzące lata
› Starship IFT-12 poleciał: czy to krok SpaceX w stronę Księżyca?
› Masywne gromady gwiazd szybciej rozpraszają otaczające je obłoki gazowe
› Co w piszczy w Polskiej branży kosmicznej? Czyli XVIII Europejski Kongres Gospodarczy
› Łazik Curiosity odkrył na Marsie związki organiczne dotychczas tam niezidentyfikowane
RSS  Najnowsze prace na astro-ph:

› Astronomical Advantages of a Boost Mission to Facilitate HST Science into the 2030s: Imaging the Circumgalactic Medium of Galaxies
› Eigenvalue formulation of Stochastic Inflation and application to large perturbation generating inflationary features
› Magnesium Silicate Clouds in the Atmosphere of HD 209458b from a Rule-Based Tree-Structured Data Reduction
› Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages
› JWST Reveals Large Reservoirs of Dust and Ongoing Circumstellar Interaction in SN Ibn/Icn 2023xgo over a Year Post-Explosion
› On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm
› Subarcsecond Multi-line Observations of NH$_3$ with VLA toward the Class 0 Source IRAS 16293-2422
› Far-infrared synchrotron properties of the inner lobes of the radio galaxy Centaurus A revealed with the Herschel observatory
› Hubble Science in the 2030s White Paper: High-Contrast Optical and UV Spectroscopy with HST/STIS
› Prospects of resolving and localising individual supermassive black hole binaries with pulsar timing arrays: the host ranking challenge
› 21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables
› It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system
› Comparative properties of X-Ray Flashes and Gamma-Ray Bursts from BeppoSAX observations of Fast X-ray Transients
› BBH-Genesis: Disentangling Binary Black Hole Formation Channels with GWTC-4
› The Delta Resonance in the Neutrino Sky
› OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots
› Constraining Extragalactic Proper Motion with Gaia Astrometry
› Halo stars harbour few wide ultracool companions
› Building a Global Astrotourism Community of Practice Through Astronomy for Development
› Hard X-ray Sources in Fermi UFOs
› Spectroscopic characterization of Young Stellar Populations and their Feedback in NGC 5253
› The sound of dynamical dark energy and modified gravity
› Vision-Language Model Ensembles Achieve Human-Expert Accuracy for Galaxy Merger Classification
› Narrowing the solar surface flux transport parameter space through nonlinear feedbacks
› Jets and Superrotation in Deep and Shallow Planetary Atmospheres
› Some Thoughts on the Future of Technosignature Searches: Constraining the Fermi Paradox
› Non-linear Dynamical Stability of Magnetic Polytropes
› Suppression of boosted relic neutrinos by photon backgrounds during ultra-high-energy cosmic ray propagation
› Decaying Dark Matter as a Possible Solution for Cosmological Tensions
› Interacting dark energy constraints from Fermi GRBs and Pantheon+ SNe Ia with full GRB covariance
› Testing the cosmological principle with quasars
› Calibrating Self-Weighted Shear Estimation via Field Distortion
› Non-detection of HC(S)SH: Estimating Upper Limits and Constraining Chemistry
› Prospects for Astrobiology and Technosignature Searches with the Vera C. Rubin Observatory Legacy Survey of Space and Time
› The Mass, Orbit and Location of Planet Nine Derived from Classical Astrophysics
› Ca-bearing cyanopolyynes in IRC+10216
› The Radio--X-ray Correlation of High-Redshift AGN: A Numerical Study of Inverse-Compton Scattering of the CMB Photons in Relativistic Jets
› Bayesian estimation of spectral parameters of the 6.7-GHz methanol maser G339.884-1.259 from GRAO observations
› The Pan-Pacific Planet Search -- IX. A menagerie of companions orbiting evolved stars
› TeV gamma-ray spectral spikes produced by magnetic reconnection in blazar jets: the case of the 2014 high state of Markarian 501
› Generative Diffusion Priors for 3D Mapping of the Dark Universe
› High-Synchrotron-Peaked BL Lacs as Multi-Messenger Sources: Connecting Ultra-High-Energy Cosmic Rays and Neutrinos
› The cosmic ray ionization rate from H3+ observations can be overestimated due to neglect of time-dependent chemistry
› Photochemical CS$_2$ Gas Detected on a 20-Myr-old Exoplanet
› Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes
› Enhancing the Angular Resolution of Large Array of imaging atmospheric Cherenkov Telescope (LACT) at Ultra-High Energies
› Hunting for Compact Object Binaries from eRASS1 Optical Counterparts through ZTF Time-domain Photometry and Multi-wavelength Census
› Photon Escape from Slab Thomson Media: A Scattering-order-resolved Recursive Formalism for Comptonization Applications
› The First Glimpse of Water Ice Absorption Map in the Milky Way
› Deep Optical Follow-up Observations to IceCube Cosmic Neutrinos: a case for IC230724A with Subaru/HSC and prospects with Rubin/LSST
› Is the Dark Comet 1998 KY$_{26}$ the Spacecraft Phobos 1?
› PSF-like Alpha-Particle Events in LSST Images
› Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment
› A short review on Quintom dark energy theory
› Assessment of the Mass Loss and Radius Change of 3I/ATLAS Based on Observed Production Rates
› Multiwavelength study of the Carina--Sagittarius Arm. I.Astrometric and photometric search for new open clusters in the 320$^ \circ $ $\le$ l $\le$ 325$^ \circ $ region
› The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters?
› Optimal Transport Reconstruction of Biased Tracers in Primordial Non-Gaussian Fields
› JAXtronomy: A JAX port of lenstronomy
› Morphology of Optical Changing-Look AGN-host Galaxies: Evidence for an Important Role of Mergers
› Primordial black holes spin from cosmological first-order phase transitions
› Study of Massive OBA Stars with X-ray Emission
› Signatures of Accreting Black Holes in Line Intensity Mapping
› Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262
› The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised
› Magneto-Gravitational Regulated Streamer Accretion onto a Class 0 Protostellar System
› Large ephemeral regions and their tilt angles
› Design and development of Fabry-Perot based wavelength calibration system for PARAS-2 spectrograph
› Reconnection-Driven Injection and Stochastic Reacceleration during Cosmological Magnetogenesis
› A new Chandra look at the globular cluster NGC 6540 and its peculiar X-ray flaring source
› A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105
› Possible High-Energy Neutrino Emission from Dark Matter Annihilation in the Disrupting Dwarf Galaxy Bo\"{o}tes~III
› Fast radio bursts, magnetars and earthquakes: their "family feud"?
› LAMOST J010103.13+275449.6: A New Binary with a Gradually Halving Photometric Variability Period
› Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots
› Distribution and Evolution of the Debris Cloud from the Fragmentation of Intelsat 33E
› Visualizing the Magnetic Structure in Interplanetary Coronal Mass Ejections with ATHARV
› CSST large-scale structure analysis pipeline: IV. Cosmic Voids Identified from Galaxy Group Samples as Probes of the Large-scale Structure
› Accurate inner stellar density slopes from projected surface densities in galaxies
› Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity
› Polarized lines of the second solar spectrum (SrI, SrII, CaI, BaII) observed at the Pic du Midi Turret Dome spectropolarimeter with the slit orthogonal to the limb
› Locating the Production Sites of High-Energy Neutrinos in Blazar Jets
› A study of the Physical Properties and Star Formation Activity of a Large Sample of Molecular Clouds: I Distances
› Revealing the high redshift host galaxy of the short GRB 061201 with JWST
› Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts
› Escape of Water- and Metal-enriched Atmospheres from compact Hot mini-Neptunes with CHAIN
› Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference
› AstroSkyFlow: an astronomical sky image flow simulator for time domain survey validation and machine learning
› The magnetic field of the Milky Way: an observational perspective
› Statistical properties of type-II bursts in Rapid Burster observed with Insight-HXMT
› The light curve of T Cephei: humps, long-term changes and recent phenomena
› The First Detection of Sub-Populations in the Delay-Time Distribution of Binary Black Holes in GWTC-4 of LIGO-Virgo-KAGRA
› Solar vortex detection methods in MHD simulations: impact of magnetic field and spatial resolution
› Revisiting ram pressure stripping in Wolf-Lundmark-Melotte: No evidence for stripped HI with LGLBS
› Modeling the Thermal Low-Frequency Radio Sun with Ray Tracing
› Regression on Regression: Mapping Data-Driven Binary Black Hole Merger Rate Fits to Progenitor Histories
› Size limits on tidal debris around white dwarfs: the km-size barrier
› Orbit Refinement of WASP-18 b and Evidence Against the Existence of WASP-18 c
› Evaluating Cepheid Metallicity Effect Determinations via IC1613 and Gaia-independent Parallaxes
› On the Relationship between Solar Spicules and Propagating Coronal Disturbances: The Role of Shocks
› JWST's Little Red Dots as collapsed Supermassive Dark Stars
› Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter
› Searching for a waveform-agnostic gravitational wave signal in pulsar timing arrays
› Linear causality and stability constraints on relativistic second-order magnetohydrodynamics
› Coupled nuclear and leptonic longitudinal collective modes in neutron star matter : a covariant Vlasov approach
› A quarkyonic matter model
› Self-gravitating quantum stars with a globally relevant Bohm potential
› The Heuristic Approach to General Relativity in the Laplace-Beltrami Formalism
› Improving the resolution of double white dwarf systems with spaceborne gravitational wave observatories using a robust astrophysical prior
› He-CF4-CH4 ternary mixtures as target gas for the CYGNO directional dark matter experiment
› Gravitational-wave astronomy with a space-based optical clock network
› Pitching Cosmic Curveballs: Environmental Effects on Extreme-Mass-Ratio Inspirals with Spinning Secondaries
› Ellis-Bronnikov Wormhole Shadows with Spherically Symmetric Accretion Flow
› Tachyonic particle production: quantum 2PI formalism with momentum exchanging collisions
› COSMOS: A numerical relativity code specialized for PBH formation
› Counterintuitive Magnetic Connectivity and Energetic Particle Flux Differences among Nearby Spacecraft During the 2023 February 24 Solar Energetic Particle Event
› Dyonic Quark Stars in Quasi-Topological Electromagnetism
› On the Role of Chapman's Hydrostatic Solar Wind Mechanism in Parker's Hydrodynamic Solar Wind Model
› Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: forecasts for next-generation interferometers and the Euclid survey
› Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR). II. The inital mass function
› From Voids to Clusters: Mergers and Evolutionary Pathways of Star-Forming and Quenched Low-Mass Galaxies
› Testing Cosmic Distance Duality Relation and Transparency with DESI DR2
› Reconstructing Barrow Holographic Dark Energy in $f(Q,T)$ Gravity and Cosmic Constraint
› Analytical transit light curves for arbitrary power-law limb darkening: a unified framework
› Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
› Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$
› The Atacama Cosmology Telescope: Release of A databaSe of millimeTeR ObservatioNs of Asteroids Using acT (ASTRONAUT)
› The Nature of Post-Starburst Galaxies: Real Deal or Masquerading Impostors?
› Holographic dark energy in a coasting cosmology
› BlackTHUNDER: Evidence of three massive black holes in a z~5 galaxy
› halox: Dark matter halo properties and large-scale structure calculations using JAX
› 3D B-fieLds in the InterStellar medium and Star-forming regions (3D-BLISS): I. Using Starlight Polarization in the Massive IRDC Filament G11.11-0.12
› Confirming the uniformity of the Hubble flow with Pantheon+ Supernovae
› Accelerated inference of microlensed gravitational waves with machine learning
› The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes
› Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy
› Resolving the (Debate About) Nozzle Shocks in Tidal Disruption Events
› Observational constraints on 3-forms dark energy
› Inference of Neutron Star Mass Distributions and the Dense Matter Equation of State from Multi-messenger Observations
› Reconnection-Driven Turbulent Fluctuations in the Magnetically Dominated Collisionless Regime
› Are Primordial Black Holes Truly Fine-Tuned?
› The Progenitor of the Type II-Plateau SN 2025pht in NGC 1637: The Dustiest, Most Luminous Red Supergiant So Far?
› Semi-analytical approach to Ly$\alpha$ multiple-scattering in 21-cm signal simulations
› Realizing the phantom-divide crossing with vector and scalar fields
› Gamma-Ray Bursts: Evidence for a Common Origin of X-ray Plateaus with Diverse Temporal Decay Index
› Radiation-hydrodynamics of star-disc collisions for quasi-periodic eruptions
› Tidal triggers and the predictability of solar activity
› New Dynamical Measurements from a Lensed Quasar Sample: Joint Analysis Constrains the Mass Profile Evolution of Lens Galaxies
› The impact of the formation channel on gravitational-wave-galaxy cross-correlations
› Transient X-ray Sources as Extremely Eccentric Mass-Transfer Binaries with Compact Companions
› Probing inflationary features with galaxy ultraviolet luminosity function observables
› LCEz4-M1: A Lyman Continuum Emitter Candidate at z = 4.444 in the MUSE Hubble Ultra Deep Field
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion
› New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity
› Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for $\epsilon$ Ind Ab
› Spectroscopic galaxy redshifts in the Peanut cluster - a massive nearly head-on cluster merger shortly after pericenter passage
› A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884
› The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
› Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
› Revisiting Marked Galaxy Clustering from a Joint Point Process Perspective
› Shortest period for outer orbit in compact hierarchical triple? Discovery of SB1 around V0885 Per
› Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy
› The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
› Measurement of the Weyl Potential Evolution and $E_G$ Statistic from KiDS-1000, BOSS and 2dFLenS
› uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo
› Mean tropical year length at arbitrary ecliptic longitude
› The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
› Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722)
› UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space
› Beyond AI as Assistants: Toward Autonomous Discovery in Cosmology
› Photometric classification of quasars from DES and photo-$z$ estimation with Machine Learning
› Blue-tilted Runnings and the JWST Early Galaxy Tension
› Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions
› Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in TIGRESS++ Simulations
› Probabilistic Data-Driven Modelling of Astrophysical Transients: The Neural Process Family for Ultrafast and Class-Agnostic Light Curve Reconstruction with NightLANP
› Ejected Surface Regolith as a Potential Source Material for Centaur Rings
› Harmonics as a Hidden Window into the Turbulent Convective Envelope of non-Blazhko RRab Stars
› Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data
› Gravitational Bound State Perturbations Inside Black Holes and Isospectrality
› An Enhanced "Flux-Corrected Transport"-Based Plasmasphere Refilling Model
› Loop-Level Lepton Flavor Violation and Diphoton Signals in the Minimal Left-Right Symmetric Model
› Non-minimally coupled loop quantum inflation with inverse-volume corrections
› Non-local gravity effects in cosmological dynamics probed by IceCube/KM3NeT signals and dark matter relic abundance
› Massive hybrid stars within the extended three-flavor quark-meson diquark model

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