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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1016.2 hPa

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 Wiadomości z astronet.pl

› Katalog Caldwella: C28
› Katalog Caldwella: C102
› Liczba czarnych dziur we wszechświecie może być mniejsza niż wcześniej zakładaliśmy
› Sterowanie lotem za pomocą balonów – projekt DracoSat
› Katalog Caldwella: C13
› Misje Kosmiczne XX wieku: Endeavour
› Katalog Caldwella: C103
› Ćwierćwiecze działalności AstroNETu. Pierwsze papierowe wydanie
› Katalog Caldwella: C86
› AstroNET finalistą konkursu Popularyzator Nauki 2025
RSS  Najnowsze prace na astro-ph:

› Self-gravitating Superfluids: The Gross-Pitaevskii-Poisson Framework
› The Nature of Galactic Spiral Arms
› ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves
› The accretion of quasars at the epoch of reionisation: $JWST$ catches the primeval monsters slowly feasting
› Reviving sub-keV warm dark matter: a UVLF-based analysis
› The final stages of binary evolution using multi-messenger studies
› The AURORA Survey: The Mass -- Metallicity and Fundamental Metallicity Relations at $z \sim 2.3$ Based Purely on Direct $T_e$ Metallicities
› The supernova Ia progenitor problem in the 2040s
› The imprints of massive neutrinos on the 3-point correlation function of large-scale structures
› Towards an Agnostic Algorithm for Sampling Empirical Structure Models: The case of Uranus and Neptune
› Empirical instability strip for classical Cepheids II. The Small Magellanic Cloud galaxy
› Archaeological investigation of galaxies' evolutionary history in the cosmic middle ages
› On the Divergent Evolution of Io and Europa as Primordial Ocean Worlds
› SatTrack: Software for Evaluating Satellite Interference and Rim-Based Interference Mitigation Using a Reconfigurable Parabolic Antenna
› The contribution from smalls scales on two-point shear analysis: comparison between power spectrum and correlation function
› Exoplanets in reflected starlight with dual-field interferometry and a fifth Unit Telescope at VLTI
› Quantifying Systematic Age Discrepancies in Very Young Star Clusters
› SHARP: Beyond JWST -- Revealing the galaxy birth and growth with the resolution of the ELT
› Hidden Companions of the Early Milky Way I. New alpha-Enhanced Exoplanet Hosts
› The mass distribution of clumpy accretion onto the nearby young star TW Hya
› Gravitational wave oscillations in Multi-Proca dark energy models
› Surveying Ultra-hot Jupiters using Phase Curves with $\textit{Twinkle}$
› A robust morphological classification method for galaxies using dual-encoding contrastive learning and multi-clustering voting on JWST/NIRCam images
› A VERITAS view of HESS J1857+026 within a multi-wavelength analysis
› A Near-Earth Object Model Calibrated to Earth Impactors
› Constraining the Nanohertz Gravitational Wave Background with an X-ray Pulsar Timing Array from NICER observations
› Pulsed radio emission from a Central Compact Object
› Semantic Model for the SKA Regional Centre Network
› Uncovering the population of compact binary mergers and their formation pathways with gravitational waves through the Einstein Telescope
› Prediction of the Solar Polar Fields in 2026: An Unusually Weak Level Across the Last Five Solar Cycles
› Quantifying sunspot group nesting with density-based unsupervised clustering
› ODIN: A New Lyman Alpha Blob Selection Method, Sample, and Statistical Analysis at $z\sim3.1$
› ESO Expanding Horizons: Underluminous Thermonuclear Supernovae
› Super-resolution-enabled atmospheric tomography for astronomical multi-wavefront-sensor adaptive-optics systems
› On Signatures of a Possible New Physics Resonance in Atmospheric Air Showers Using a Parameterized Model
› Super-resolution wavefront reconstruction in adaptive-optics with pyramid sensors
› Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars
› The Competing Influence of Ram Pressure and Tidal Interaction in NGC 2276
› A search for late-type brown dwarfs in the Euclid Quick Data Release 1
› High-Resolution Measurements with the CTAO Southern Array: The Case for Pulsar Wind Nebulae
› CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks
› Radio studies of supernovae 1979C, 1986J and 2006X with LOFAR
› Constraining black hole spin in PG 1535+547 amidst complex multi-layered absorption
› Observations of AGN-driven feedback: dynamics and ionization of the filaments in M87
› Surrogate-Accelerated Bayesian Inversion for Exoplanet Interior Characterization
› Across the Universe: GW231123 as a magnified and diffracted black hole merger
› The contribution of the color space in LSST-like photometry for the selection of extragalactic globular cluster candidates
› Validating the performance of the Radio Neutrino Observatory in Greenland using cosmic-ray air showers
› Evolving and interacting dark energy: photometric and spectroscopic synergy with DES Y3 and DESI DR2
› The MeerKLASS L-band On-the-Fly Continuum Survey: Data Release 1
› A VLA search for compact radio sources in the explosive molecular outflows DR 21 and G5.89
› Pre-supernova O-C shell mergers could produce more $^{44}\mathrm{Ti}$ than the explosion
› Interpreting the strong clustering of ultra-diffuse galaxies by halo spin bias
› Implicit Likelihood Inference of the Neutrino Mass Hierarchy from Cosmological Data
› Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track Samples
› Magnetic field spreading from stellar and galactic dynamos into the exterior
› Selected topics on: 1) proposal of interpreting the Crab supernova with a GRB 2) progress in identifying the seven GRBs episodes 3) the role of Sagittarius A in identifying the dark matter component (the X fermion)
› Systematic search of laser and phase modulation noise coupling in heterodyne interferometry
› Investigating the AGN variability timescale -- black hole mass relationship with Gaia, SDSS and ZTF
› Constraining primordial non-Gaussianity from DESI DR1 quasars and Planck PR4 CMB Lensing
› On the complex nature of coronal heating
› Asymptotic behaviour of galactic small-scale dynamos at modest magnetic Prandtl number
› Equilibriums of extremely magnetized compact stars with force-free magnetotunnels
› Creation of spin-3/2 dark matter via cosmological gravitational particle production
› Fermion Thermal Field Theory for a Rotating Plasma (with Applications to Neutron Stars)
› Deviations from Gaussian White Noise in Stochastic Inflation
› A Search for Binary Black Hole Mergers in LIGO O1-O3 Data with Convolutional Neural Networks
› Ghost-free 2-form fields in cosmology: implications for gravitational parity violation
› Origin of Quasi-Periodic Oscillations and Accretion Process in X-Ray Binaries around Quantum Lee-Wick Black Hole
› In situ substrate birefringence characterization in gravitational wave detectors using a heterodyne polarimetry method
› Kinetic-Theory Bounds on the Equation of State of Dense QCD Matter
› GW231123: Overlapping Gravitational Wave Signals?
› Quantum state of interacting primordial inhomogeneities: de-squeezing and decoherence
› Baryogenesis and EDMs in the 2HDM+CS
› Boiling away asymmetries: low-scale phase transitions, gravitational waves and leptogenesis
› Revisited apparent horizon entropy and GSL in modified gravity
› Trails of clouds in binary black holes
› Revisit the periodicity of SGR J1935+2154 bursts with updated sample
› Nonlinear Hall effect in the stationary cylinder with a radial heat flux
› Environment matters: stronger magnetic fields in satellite galaxies
› X-ray Binaries: a potential dominant contributor to the cosmic ray spectral knee structure
› Forecasted Detection Limits on the (Dark) Matter Density in Supermassive Black Hole Binaries for LISA
› Novel Quantity for Probing Matter Perturbations Below the Fresnel Scale in Gravitational Lensing of Gravitational Waves
› Baryon Acoustic Oscillations in tomographic Angular Density and Redshift Fluctuations
› The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
› Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
› Discovery of a 21 cm absorption system at z=2.327 with CHIME
› Insights into the structure and kinematics of a Milky Way-like galaxy
› Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk
› SpecCLIP: Aligning and Translating Spectroscopic Measurements for Stars
› J-PAS: Forecasting constraints on Neutrino Masses
› Mass Proxy Quality of Massive Halo Properties in the IllustrisTNG and FLAMINGO Simulations: I. Hot Gas
› On the computational feasibility of Bayesian end-to-end analysis of LiteBIRD simulations within Cosmoglobe
› IGR J17091-3624: Newly Formed Periodic Dips and Multiwavelength Activity During the 2025 Outburst
› Probing Picohertz Gravitational Waves with Pulsars
› Auriga Streams III: the mass-metallicity relation does not rule out tidal mass loss in Local Group satellites
› Carnegie Supernova Project: Fast-Declining Type Ia Supernovae as Cosmological Distance Indicators
› Observation of the Galactic Center in the Sub-MeV Gamma-Ray Band with an Electron-Tracking Compton Camera
› Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes
› Dynamical Dark Energy Meets Varying Electron Mass: Implications for Phantom Crossing and the Hubble Constant
› A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene
› SN 2024cld: unveiling the complex mass-loss histories of evolved supergiant progenitors to core collapse supernovae
› A Wind-Driven Origin for the Firework Morphology of the Supernova Remnant Pa 30
› Inflationary relics from an Ultra-Slow-Roll plateau
› Exoplanets synchronization: Learning from Venus' retrograde rotation
› SPHEREx Pre-Perihelion Mapping of $\mathrm{H_2O}$, $\mathrm{CO_2}$, and $\mathrm{CO}$ in Interstellar Object 3I/ATLAS
› The magnetic origin of the outer boundaries of sunspots
› The Polarized X-ray Universe: Insights and Discoveries
› Inference of Neutron Star Mass Distributions and the Equation of State from Multi-messenger Observations
› A Comprehensive Interpretation of Fermi-LAT Pulsars: Fundamental-Plane Death Border, Visibility Thresholds, and GeV-TeV Unification
› Systematic biases in parameter estimation on LISA binaries: The effect of excluding higher harmonics for non-spinning binaries
› Towards model-independent identification of lensed gravitational waves using Kramers-Kronig relation
› Primordial black hole formation in k-inflation models
› Return of the Lepton Number: Sterile Neutrino Dark Matter Production and the Revival of the Shi-Fuller Mechanism
› A Compact Story of Positivity in de Sitter
› Gravitational waves induced by matter isocurvature in general cosmologies
› Cosmic Structure Strikes Back: The Elimination of Vector-Mediated Nonstandard Interaction Models as a Mechanism for Sterile Neutrino Dark Matter Production
› Inflation from entropy
› Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model
› Chiral magnetic effect amplified baryogenesis at first-order phase transitions

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