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

› Kosmiczny przegląd miesiąca AstroNETu – marzec 2026 roku
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› Katalog Caldwella: C54
RSS  Najnowsze prace na astro-ph:

› Independent Replication of Nuclear Test-Transient Correlations and Earth Shadow Deficit in POSS-I Photographic Plates
› Large Scale Structure and Environmental Effects on Dwarf Galaxy Growth
› Non-Cold Dark Matter from Memory-Burdened Primordial Black Holes
› A Solar Probe of Dark Matter Decay in the Galaxy
› Revealing the stellar population of the ultra-obscured Galactic globular cluster Glimpse-C02
› Lagrangian Bias as a Gaussian Random Field
› The multi-age stellar populations of Terzan 5 as revealed by JWST
› Imladris: a detailed and flexible model for galaxy simulations with individual stars
› Searching for unresolved massive black hole pairs through AGN photometric variability
› The Kormendy Relation in the First Billion Years: Evidence from $JWST$
› Optimisation of calibration sources for global 21-cm experiments: the REACH case
› Generalized Predictions for the Electromagnetic Signatures of Mirror Stars
› The Impact of Seyfert Jets on Galaxy Evolution Across Major Scaling Relations
› Eppur non si trovano Vol. 2: No Planetary-mass Primordial Black Holes toward the Andromeda Galaxy
› The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds
› Pegasi Ascendant: Ranking Constellation Genitives on their Aesthetic Merit
› Formation of dust grains in the winds of cool giants, PhD thesis 1992
› Traces of Helium Detected in Type Ic Supernova 2014L
› Resistive MHD Simulations of Stellar Wind-Magnetosphere Coupling in TRAPPIST-1e
› Radiative Feedback in Population III Protostellar Growth: The Impact of HI Shielding
› Predictions of the LSST Solar System (non-)Yield
› A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection
› A Novel Method to Construct Frequency-Domain Gravitational Waveform for Accelerating Sources
› Planetary Radar at the Arecibo Observatory
› A large misalignment between continuous jet and discrete ejecta in microquasar GRS 1915+105 during its obscured phase
› Calibrating optical galaxy cluster projection effects with sparse spectroscopic samples: A clustering redshift approach
› Relic Magnetic Fields from Non-Adiabatic Photon Freeze-Out at Recombination
› FAST Observations of Wave-like Structures in the Radio Dynamic Spectrum of AD Leo
› X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state
› Global asteroseismology of 19,000 red giants in the TESS Continuous Viewing Zones
› Twists in the flow: revisiting convective mixing in rotating stellar models. I. Effect on the stellar structure
› Three-Dimensional Ocean Dynamics and Detectability of Tidally Locked Lava Worlds
› Revisiting Marked Galaxy Clustering from a Joint Point Process Perspective
› A Universal 1.5 GeV Gamma-Ray Line in Active Galactic Nuclei
› A Geometric Theory of Cosmological Structure via Entropic Curvature in Wasserstein Space
› Misaligned rings around minor planets with moons
› The complex dependencies of Wolf-Rayet winds -- Insights from detailed radiative transfer models
› A comparison of pendulum models for large-amplitude longitudinal prominence oscillations
› OJAL\'A: Optimizing J-PAS Astronomy for Large-scale Analysis. A foundation model for the SED of galaxies, QSOs and stars
› Arches of chaos, heteroclinic connections of first-order MMRs and the chaotic transport of small bodies in the Sun-Jupiter system
› Predicting CO and dust emission of star-forming galaxies
› An updated picture of pre-solar history from short-lived radioactive isotopes and inferences on the birth of the Sun
› Euclid preparation. Impact of redshift distribution uncertainties on the joint analysis of photometric galaxy clustering and weak gravitational lensing
› Transport-Geometric Formulation of Peak Statistics: Curvature-Conditioned Point Processes and Response Hierarchy
› 20 years of monitoring: PKS 2155-304 and PKS 1510-089 in the eyes of Swift and Fermi. I. The case of PKS 2155-304
› Waiting time distribution of solar flares from a global perspective
› 20 years of monitoring: PKS 2155-304 and PKS 1510-089 in the eyes of Swift and Fermi. II. PKS 1510-089 and comparison
› Imaging magnetically driven astrospheres: a forward modelling approach
› Near-Earth asteroids in Main Belt-crossing orbits
› Resolving Oblique Star-Disk Collisions in Quasi-Periodic Eruptions: Numerical Requirements and the Importance of Geometry
› On the variability of the reflection nebula Van den Bergh 27 surrounding RY Tau
› A subgrid model for chemical enrichment in cosmological simulations
› High-Precision Near-Infrared Abundances of Solar Analogs in the YJ Bands
› Focal plane wavefront control with model-based reinforcement learning
› Addressing the open flux problem with a non-spherical solar coronal magnetic field model
› Universal Non-Gaussian Signatures from Transient Instabilities
› Distance and [Fe/H] of Galactic bulge clusters from member RR Lyrae I-band light curves
› Curvature-induced electroweak symmetry breaking and phase transition of a Higgs-portal dark scalar field
› ALMA Band 2 line survey of a $z = 3.44$ clumpy strongly-lensed submillimetre galaxy
› The radial component of the local Galactic magnetic field in 3D
› Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities
› Cosmological zoom-in perturbation theory as a consistent beyond point-particle approximation framework
› First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes
› Delayed Radio Flares in Neutrino-associated Blazars: The Case of TXS 0506+056
› The RRATalog: a Galactic census of rotating radio transients
› Beaming of polarized radiation in subcritical X-ray pulsars
› Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared
› Multimessenger Constraints on Production Sites of High-Energy Neutrinos from NGC 1068
› Number Theory in Quantum Physics: Minicharged Particles and the Prouhet-Tarry-Escott Problem
› Dark energy from string theory: an introductory review
› Analytical Scaling of Relativistic Drag in the Interstellar Medium
› Cherenkov plasmons emission by primordial neutrinos
› Wormhole Dynamics: Nonlinear Collapse and Gravitational-Wave Emission
› Lectures on Light Particles and Compact Objects
› Does a wormhole survive a cosmological bounce?
› An Asymptotically Causal Metamodel for Neutron Star Equations of State
› Next-to-Minimal Freeze-in Dark Matter
› Optical frequency comb Fourier transform spectroscopy of the CH$_2$$^{79}$Br$^{81}$Br, CH$_2$$^{79}$Br$_2$, and CH$_2$$^{81}$Br$_2$ isotopologues in the 1180-1210 cm$^{-1}$ region
› Gravitational wave spectrum from first-order QCD phase transitions based on a parity doublet model
› Baryogenesis in $SU(2)_{L}$ multiplet models
› Topological defect induced phase separation in a holographic system
› Stability analysis and double critical phenomenon in the Einstein-Maxwell-scalar theory
› Modeling the refractive index profile n(z) of polar ice for ultra-high energy neutrino experiments
› Differentiable Optics with dLux II: Optical Design Maximising Fisher Information
› Joint Electromagnetic and Gravitational Wave Inference of Binary Neutron Star Merger GW170817 Using Forward-Modeling Ejecta Predictions
› Higher multipoles of the cow
› Unveiling the Coma Cluster Structure: From the Core to the Hubble Flow
› Insights into the structure and kinematics of a Milky Way-like galaxy
› SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
› Evidence for a Spectral Break or Curvature in the Spectrum of Astrophysical Neutrinos from 5 TeV--10 PeV
› Super-Eddington accretion in protogalactic cores
› Primordial Physics in the Nonlinear Universe: mapping cosmological collider models to weak-lensing observables
› MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z${\sim}$2
› A galactic tug-of-war: how (not) to simultaneously fit the Milky Way satellite luminosity function and the mass-metallicity relation
› Reverberation lags viewed in hard X-rays from an accreting stellar-mass black hole
› CURLING -- III. Identifying Candidates of Wide-separation Gravitationally Lensed Quasars from the CatNorth Catalogue
› Gravitational Waves from Hyperbolic Encounters of Primordial Black Holes in Dwarf Galaxies
› Strong gravitational-wave lensing posterior odds
› Reexamining Evidence of a Pair-Instability Mass Gap in the Binary Black Hole Population
› Constraints on Axion-photon coupling from the Global 21-cm Signal
› Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeV
› Topological Signatures of Heating and Dark Matter in the 21 cm Forest
› Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae
› Primordial black holes: constraints, potential evidence and prospects
› Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
› Multi-Tracer Cross-Correlations of the Unresolved $\gamma$-Ray Sky
› The early r-process nucleosynthesis scenarios
› Supernova interactions with aspherical circumstellar material I: calculations of light curves, AB magnitudes, spectra, and polarisation
› Direct Abundance Maps and Radial Metallicity Gradients of two Galaxies at z~4-5 in the GARDEN Survey
› Resolution Dependence in Magnetohydrodynamic Simulations of Neutrino-Driven Core-Collapse Supernovae
› Physics-Informed Neural Networks for Modeling Galactic Gravitational Potentials
› The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
› AT 2025abao: The fourth luminous red nova in M 31
› Single- and double-headed odd radio circles in the LOFAR surveys
› Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources
› TESS Planet Occurrence Rates Reveal the Disappearance of the Radius Valley Around Mid-to-Late M Dwarfs
› Stochastic Particle Acceleration during Pressure-Anisotropy-Driven Magnetogenesis in the Pre-Structure Universe
› Gravitational-Wave Propagation Through the Axiverse
› Advanced Virgo Plus for O5 -- Design Report Overview
› Data-calibrated point spread function prediction: General description of the method and demonstration on MUSE-NFM
› e-CALLISTO FITS Analyzer: A Software Framework for CALLISTO Solar Radio Data
› Single vs. Binary Origin: The Diversity of Stripped-Envelope Supernova Remnants
› Formation and disruption of wide binaries in star clusters revealed by N-body simulations
› Enabling fundamental understanding of Nature with novel binning methods for 2D histograms
› Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
› The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions
› Unique gravitational wave signatures of GLPV scalar-tensor theories
› Investigating Production of TeV-scale Muons in Extensive Air Shower at 2400 Meters Underground
› High-Q Superconducting Lumped-Element Resonators for Low-Mass Axion Searches
› Development and Testing of a Modular Large-Area Cosmic Ray Telescope Using Scintillator-Fiber Hybrid Design for Millimeter-Level Muon Tracking
› The phases of QCD reached in terrestrial and cosmic colliders
› Probing the Scalar Hair of Rotating Horndeski Black Holes through Thick Disk Images
› Linear stability of nonrelativistic Proca stars
› Microscopic Description of Critical Bubbles
› Analytic force-free jet from disk-fed rotating black holes
› Conventional and Unitarity-Conserving Peccei-Quinn Inflation Models and ACT

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