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

› Scanway S.A. i Łukasiewicz – ILOT łączą siły
› Najsłynniejsze zdjęcia Ziemi z kosmosu
› Misje kosmiczne XX wieku: program Energia-Buran
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› Start misji Artemis II – od podstaw
› Kosmiczny przegląd miesiąca AstroNETu – marzec 2026 roku
› Katalog Caldwella: C49
RSS  Najnowsze prace na astro-ph:

› Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario
› High-dimensional inference for the $\gamma$-ray sky with differentiable programming
› Primordial Neutron Stars
› Temperature asymmetry in the Milky Way's hot circumgalactic medium induced by the Magellanic Clouds
› Choice of optical transformation for photonic circuit wavefront sensors
› The Hubble sequence in JWST CEERS from unbiased galaxy morphologies
› Ghosts of eruptions past: Searching for historical Galactic supernovae using variable thermal dust echoes and machine learning
› GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy
› Positive YORP effect induced by lateral heat conduction in a crater
› Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
› EPISODE IV: Ice Inventory in the Envelope of EC 53
› Colloquium: Radio astronomy with the Arecibo 305-m telescope: In contemporaneous context
› Development of the New Optical Sensor for IceCube-Gen2
› The Fate of Frozen Carbonated Water at Europa-like Conditions
› A practical re-weighting scheme of data fitting: application to asteroids orbit determination with Gaia
› Overview of Hayabusa2 extended mission's flyby of Near-Earth Asteroid (98943) Torifune
› Validating a Non-conventional Method for Expansion of Coronal Mass Ejections (CMEs) and Investigating the Evolution of a CME Substructures Using Solar Orbiter and Wind Observations
› cTreeBalls: a fast 3-point correlation function code for clustering measurements
› FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses
› What Heats the Dense Gas in the Galactic Center?
› A Convolutional Neural Network-Derived Catalog of Solar Flares from Soft X-Ray Observations
› Polarimetry in Planetary Sciences and Astronomy
› Spectral signatures from the habitable zone
› Recent advances in modelling of global-scale collisions using smoothed particle hydrodynamics
› Photoionization modelling of circumstellar nebulae using irregular grains
› The formation of planetary systems: physics, populations, and architectures
› Recent development in high-precision high-fidelity spectrographs for exoplanet research and characterization
› Giant Planet Formation by Disk Instability
› Beyond Mass and Multiscale Environments: What Shapes Low Surface Brightness Galaxies? Evidence from MaNGA
› The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results
› Optical identification of the FASHI sources: toward the extended Local Volume
› Radio Monitoring Campaign of Active Repeater FRB 20220912A with CHIME
› Dust Processing in Protoplanetary Discs From Infall to Dispersal: the Origin of Solar System Isotopic Heterogeneities
› A New Measurement of the Extragalactic Background Light using 15\,yr of {\it Fermi}-Large Area Telescope Data
› Bounding axion dark energy
› The Cosmic Web and Its Filaments: Neutrino Mass from Topology and Persistent Homology
› Machine Learning as a Transformative Tool for (Exo-)Planetary Science
› Joining forces: 30 years optical monitoring of the Einstein Cross
› The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z = 3.55$
› Fast and Scalable Production of Stacked Prism X-ray Lenses for Astrophysics Using Two-Photon Polymerization
› Terrestrial planet formation in the era of GPU computing
› Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars
› An automated method for planetary nebula detection with SIGNALS: first applications to NGC 4214 and NGC 4449
› The evolution of the mid-infrared spectrum of SN 1987A observed with the JWST/MIRI-MRS
› Methanimine as a sink in the HCN and HNC solid state hydrogenation network
› Unseen Astronomy
› Long-period transiting exoplanets: advances in detection and characterization
› The Illusory Precision of TTV Masses: Hidden Solutions Behind Kepler-9's Tight Mass Ratio
› Detecting nitrogen-carriers in the inner regions of protoplanetary disks
› A first [CII] view of high-z quiescent galaxies
› Constraining the Molecular Kennicutt-Schmidt Relation with Multi-Transition CO Observations of Nearby Galaxies
› Nii-body: Bayesian Inference of Multiplanet Dynamics via N-body Simulations
› NCCR PlanetS: Observational and computational characterization of exoplanet atmospheres
› A TeV-based Determination of the Local Extragalactic Background Light and its Consistency with Galaxy Counts and Direct Measurements
› Paschen Jumps in Little Red Dots: Evidence for Nebular Continua
› Enhancing event reconstruction for $\gamma$-ray particle detector arrays using transformers
› Analytic compression of the effective field theory of the Lyman-alpha forest
› Large or bright satellite constellations: Effects on observations, including on the background sky brightness
› Blueshifted lines from the inner accretion disc's rotation can explain quasar absorption "forests''
› Finding Circumbinary Planets: A Semi-Automated Transit Search of TESS Eclipsing Binaries
› IFS spectrograph designs for the Wide-field Spectroscopic Telescope: Architecture and performance gains from curved sensors
› The k-MENDEL sample of local analogs to reionization galaxies. Spectral identification of EELGs and properties of green peas in DESI
› Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith
› High-Contrast Imaging of Forming Protoplanets: VLTs, JWST, and the Promise of ELT
› The missing ultra-faint satellites of the Milky Way
› Inverse Energy Cascade in Turbulent Taylor-Couette Flows
› Resolving satellite-in situ mismatches in Net Primary Production using high-frequency in situ bio-optical observations in the subpolar Northwest Atlantic
› Love numbers of black holes and compact objects
› Minimum mass, maximum charge and hyperbolicity in scalar Gauss-Bonnet gravity
› Tidal Response of Compact Objects
› Evaluating Deep Learning Models for Multiclass Classification of LIGO Gravitational-Wave Glitches
› labrador: A domain-optimized machine-learning tool for gravitational wave inference
› Genericness of quantum damping of cosmological shear in modified loop quantum cosmology
› Probing the Kinematic Dipole with LISA: an analytical treatment
› Relative Magnification Factor of Point Sources on Accretion Disks
› Covariant scalar-tensor theories beyond second derivatives
› Short-Time Plasma Evolution: Flow Generation and Magnetogenesis
› Probing Solar Symmetrons with Direct Detection
› CMB signatures of gravity-mediated dark radiation in $\mathbf{\Delta N_{\rm eff}}$
› Classification of Symmetric Four-Body Dziobek Central Configurations and Application to the Earth--Moon System
› BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$
› Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations
› Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
› Beyond Spherical geometry: Unraveling complex features of objects orbiting around stars from its transit light curve using deep learning
› Leveraging Photometry for Deconfusion of Directly Imaged Multi-Planet Systems
› BayeSN-TD: Time Delay and $H_0$ Estimation for Lensed SN H0pe
› Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM
› Dark winds on the horizon: Prospects for detecting neutrino and hot dark matter wakes in large-scale structure
› statmorph-lsst: Quantifying and correcting morphological biases in galaxy surveys
› Aql X-1 from dawn 'til dusk: the early rise, fast state transition and decay of its 2024 outburst
› A window for water-hydrogen demixing on warm metal-rich sub-Neptunes
› Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions
› High-energy Neutrino Predictions for T Coronae Borealis: Probing Particle Acceleration in Novae
› Validation of Satellite Lifetime Predictions at Leonid Space
› The Volatile Inventory of 3I/ATLAS as seen with JWST/MIRI
› Little Red Dots on FIRE: The Ability of Bursty Galaxies to Host an Abundant Population of High-Redshift AGN
› Sunrise III: The Wavefront Correction System
› A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks
› The Baryon Budget of Galaxies across the First Billion Years
› SPACE-Timers -- A Stack-Based Hierarchical Timing System for C++
› Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions
› An Updated SynthPop Model for Microlensing Simulations I: Model Description & Evaluation
› Magnetic Connectivity in the Time-Dependent Corona and Heliosphere
› The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs
› Euclid preparation. Galaxy power spectrum and bispectrum modelling
› What Are Pulsar Companions Made of? Using Gravitational Tides to Probe Their Compositions
› Spectroscopic Redshifts for 461 Euclid Q1 Strong Gravitational Lenses from NISP Slitless Spectroscopy
› Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition
› PRECESSION 2.1: black-hole binary spin precession on eccentric orbits
› Inflation in theories with broken diffeomorphisms
› Characterization of compressible fluctuations in solar wind streams dominated by balanced and imbalanced turbulence: Parker Solar Probe, Solar Orbiter and Wind observations

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