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: widok od południa
widok od południa
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
9.9 °C

Wilgotność
 54%

Wiatr
4.8 km/h

Ciśnienie
1018.6 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Do 13 marca zapisy do konkursu Łowcy Cząstek 2026
› Katalog Caldwella: C64
› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
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› Misje kosmiczne XX wieku: program Sojuz
› Pixinsight cz. VII – XTerminatory
RSS  Najnowsze prace na astro-ph:

› unxt: A Python package for unit-aware computing with JAX
› A second visit to Eps Ind Ab with JWST: new photometry confirms ammonia and suggests thick clouds in the exoplanet atmosphere of the closest super-Jupiter
› Binary Black Holes population synthesis based on the current LVK observations
› Worlds Next Door. IV. Mapping the Late Stages of Giant Planet Evolution with a Precise Dynamical Mass and Luminosity for $\epsilon$ Ind Ab
› Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars
› Gamma-ray Signatures of r-Process Radioactivity from the Collapse of Magnetized White Dwarfs
› Red-Giant Asteroseismology of Low-Mass Population III Stars
› Detecting Axion-like particles using Cosmic Variance Cancellation with CMB and Radio surveys
› 16 new quasars at the end of the reionization unveiled by self-supervised learning
› Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
› Recalibration of Pre-SM4 STIS Echelle Throughputs
› Rederivation of STIS Secondary Echelle Mode Traces
› Do the Amati and Yonetoku Relations Evolve with Redshift for Swift GRBs?
› Accretion Disk Evolution in GX 339-4 Across Spectral States Using NuSTAR, NICER, and Insight-HXMT Observations
› Recovering the infall mass for Milky Way satellite galaxy Sextans
› Spectral characteristics of fast rotating metal-poor massive stars
› Optimising the global detection of solar-like oscillations. Tuning the frequency range for asteroseismic detection predictions and searches
› Spitzer + HST parallaxes of 13 late T and Y dwarfs
› Variable magnetic field and adaptive mixing-length: reproducing Li abundances and constraining rotational evolution of solar-type stars in clusters
› Electron densities and filling factors of extragalactic HII regions: NGC 2403 and NGC 628
› Correcting Ionospheric Faraday Rotation for the VLA and MeerKAT
› Winding, Unwinding, Rewinding the Gaia Phase Spiral
› A Multi-Level Parallel Pipeline for SPHERE-3 Detector Simulation: From EAS Generation to Image Approximation
› Parallel Version of CORSIKA Code with Cherenkov Option for SPHERE-3 Project
› Two Low Mass-Ratio Microlensing Planets and Two Types of Central-Resonant Degeneracy
› Time-dependent photospheric radiative transfer in structured GRB jets: spectral evolution and polarization diagnostics
› The Influence of Clouds and Deuterium-Burning on Brown Dwarf Habitable Zones
› Dynamics of thin accretion disks and accretion around a charged-PFDM black hole
› POLISH'ing the Sky: Wide-Field and High-Dynamic Range Interferometric Image Reconstruction with Application to Strong Lens Discovery
› Modern Rate-of-Decline Relations for Novae
› Characterizing the Instrumental Profile of LAMOST
› Detection of afterglow emission up to 100 GeV through a stacking analysis of gamma-ray bursts
› HAWC J0630+186 Could Not Be Powered by PSR J0630+19
› A Robust Geometric Distortion Solution for Main Survey Camera of CSST
› Joint Diagnostics of Circumsolar Sky Brightness Using Coronagraphic Measurements and Aerosol Optical Inversions at Mauna Loa
› HI Observations of Giant Low Surface Brightness Galaxies
› Weighing Hidden Companions of Compact Object Candidates via Rotational Broadening
› Searching for Black Hole Candidates in Quiescence by Using Multi-band Observations in Globular Cluster M22 (NGC6656)
› Mass Production of 2023 KMTNet Microlensing Planets I: Low Mass Ratio
› Atmospheric Collapse and Habitability on Tidally-Locked Exoplanets
› Statistical consistency of sign-switching vacuum energy with cosmological observations
› Half-year Evolution of a Decaying Solar Active Region and Peripheral Dimming Regions
› Optical QPOs with different periodicities in CSS and ZTF light curves of the quasar 4C 50.43
› Constraints on Neutrino Mass with Void Weak Lensing Effect
› Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
› Epicyclic Density Variations in the Indus Stellar Stream
› Reliable Tests of Faint-end UV Luminosity Functions in Strong Lensing Fields
› The Key to Unlocking Exoplanet Biosignatures: a UK-led IR Spectrograph for the Habitable Worlds Observatory Coronagraph
› $\Lambda$ effect in rotating hydrodynamic convection
› Low-energy atmospheric neutrino flux calculation with accelerator-data-driven tuning
› Hidden Vela Supercluster Revealed by First Hybrid Redshift & Peculiar Velocity Reconstruction
› Testing Screened Modified Gravity with Strongly Lensed Gravitational Waves
› From planetesimals to planets with N-body simulations in the giant-planet formation region
› Accurate spectroscopic redshift estimation using non-negative matrix factorization: application to MUSE spectra
› Beyond Fermi-II: Intermittent Particle Acceleration by Relativistic Turbulence in Astrophysical Plasmas
› Pure Natural Inflation Passes the ACT
› Exploring the $S_8$ Tension: Insights from the CatNorth 1.5-Million Quasar Candidates
› Empirical flare energy limits for the largest historical sunspots
› Detection and Astrometry of the Ba-Bb Subsystem in $\alpha$ Piscium: First Dual-Field Interferometry at the CHARA Array
› The Salamander: A case study of the magnetic field and peculiar morphology of G309.8-2.6 through radio polarimetry
› Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
› The statistics and structure of dissipation in subsonic and supersonic turbulence
› Temporal Variation of the Coronal Parameter in a Jetted Tidal Disruption Event: Swift J1644+57
› CubeSats Reach the Millisecond X-Ray Domain: Crab Pulsar Timing with SpIRIT/HERMES
› The period clustering of magnetars and X-ray dim isolated neutron stars
› Characterizing the 3D evolution of two successive CMEs heading for Mercury
› Obscured Star Formation in the Dwarf Galaxy DDO 43? A Comparative UV-IR Analysis
› Fast X-ray Transients produced by Off-axis Jet-Cocoons from Long Gamma-Ray Bursts
› ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon
› Shaken, not stirred: inefficient mixing of CM- and CI-like materials
› Supernova scores for active anomaly detection
› Understanding the impact of binary mass transfer in the accretor's measurable parameters
› Joint Bayesian Source and Lens Reconstruction for Multi-messenger Binary Black Holes
› POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization
› Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
› Going Wide and Deep with Roman: The z~6-9 UV luminosity function in a Roman Deep Field
› Multi-spacecraft constraints on relativistic solar energetic particle transport in the widespread 28 October 2021 event
› FEAST: a NIRSpec/MOS survey of emerging young star clusters in NGC 628
› Mass regulates the emerging timescale of young star clusters
› A Modified Conveyor Belt Model: Implications for Surface Density Thresholds for Massive Star Formation
› The rotational and magnetic properties of Polaris from long-term spectropolarimetric monitoring
› The role of mass loss in constraining quenching time in dwarf galaxies from AGB and RGB star counts
› Forward-modelling Milky Way Cepheids: selection effects and physical priors in the Gaia-HST calibration
› ODIN: Spectroscopic Validation of Ly$\alpha$-Emitting Galaxy Samples with DESI
› Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
› Data reduction method for OPTICAM multiband time series of transiting exoplanets
› Far-infrared Polarization Properties of Nearby Star-forming Regions: A New Compendium of SOFIA/HAWC+ Observations
› Dark Matter Recoupling
› Probing Physics Beyond the Standard Model through Combined Analyses of Next-Generation Type Ia Supernova, CMB, and BAO Surveys
› Black Hole Properties of Type-1 Active Galactic Nuclei in the North Ecliptic Pole Wide Field: I. Mid-infrared Sources with Optical Counterparts
› Different polarized components of the quasar 3C 286 revealed by FAST
› Multi-wavelength ALMA Imaging of HD 34282: Dust-trapping Signatures of a Vortex Candidate
› Scattering from compact objects: Debye series and Regge-Debye poles
› Binary-boosted Dark Matter
› Scalar shortcut to beyond-Kerr ringdown tests and their complementarity with black-hole shadow observations
› All-Loop Renormalization and the Phase of the de Sitter Wavefunction
› Axion-neutrino interactions in seesaw models and astrophysical probes
› Dark matter trio in classically conformal theories: WIMP, supercooling, and monopole
› Dual Cutler-Vallisneri Corrections: Mitigating PSD Drift in Zero-Latency Gravitational-Wave Searches
› Binary Black Hole inspirals cannot hide their eccentricity
› Non-perturbative determination of the QCD Equation of State up to the electroweak scale
› Deep Learning Search for Gravitational Waves from Compact Binary Coalescence
› Renormalisation and matching of massless scalar correlation functions in Soft de Sitter Effective Theory
› Optical calibration systems of the Pacific Ocean Neutrino Experiment
› Relativistic Corrections to the Formation Rate of Extreme Mass-Ratio Inspirals
› Circumstellar Medium of Supernovae as New Probes for Feebly-interacting Particles
› Cosmological Spacetimes with Sign-Changing Spatial Curvature and Topological Transitions
› Possible Extragalactic Origins of Five LMC Globular Clusters: Proper Motion Deviations in Gaia DR3
› Euclid Quick Data Release (Q1) -- Characteristics and limitations of the spectroscopic measurements
› Radio Spectral Energy Distribution of Low-$z$ Metal Poor Extreme Starburst Galaxies: Novel insights on the escape of ionizing photons
› Meta-learning for cosmological emulation: Rapid adaptation to new lensing kernels
› One-loop renormalization of the effective field theory of inflationary fluctuations from gravitational interactions
› Freezing of the renormalized one-loop primordial scalar power spectrum
› Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
› GRB 221009A: Observations with LST-1 of CTAO and Implications for Structured Jets in Long Gamma-Ray Bursts
› Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions
› Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
› Lyman-$\alpha$ Escape through Anisotropic Media
› The detection of high X-ray polarization from an accretion disc corona source and its modelling via Monte Carlo radiation transfer simulation
› Reheating with Thermal Dissipation and Primordial Gravitational Waves
› Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
› XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
› Scalar field dark matter and stepped dark radiation in an extended Wess-Zumino dark radiation model
› The Response of Planetary Atmospheres to the Impact of Icy Comets III: Impact Driven Atmospheric Escape
› Simulation-Based Prediction of Black Hole Spectra: From $10M_\odot$ to $10^8 M_\odot$
› Reconstructing Gamma Ray Burst Energy Relations with Observational H(z) data in Neural Network Framework
› Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
› On the Influence of Pluto on Twotino Dynamics Through Their Mutual 4:3 Mean Motion Resonance
› Accretion Geometry of Black Hole X-ray Binaries: Insights from X-ray Observations
› Nemesis: A Multi-Scale, Multi-Physics Algorithm for Astrophysics
› Hunting for methanol in the water rich, planet forming disk around HL Tau
› X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates
› WIMP Dark Matter Searches in Reticulum II Using MeerKAT
› Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation
› BlackGEM observations of compact pulsating stars: Mode identification for the DOV PG 1159-035 using multi-colour photometry
› The Formulation of Scaling Expansion in an Euler-Poisson Dark-fluid Model
› Non-thermal production of heavy vector dark matter from relativistic bubble walls
› Photon proliferation from multi-body dark matter annihilation
› Perturbative unitarity bounds on field-space curvature in de Sitter spacetime: purity vs scattering amplitude
› No Hiding in the Dark: Cosmological Bounds on Heavy Neutral Leptons with Dark Decay Channels
› Exploring the Landscape of Spontaneous CP Violation in Supersymmetric Theories
› New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis
› Symmetry of Bounce Solutions at Finite Temperature
› Bounds on screened dark energy from near-Earth space-based measurements
› $\mathcal{R}^2$-corrected Tachyon Scalar Field Inflation, the ACT Data, and Phantom Transition
› On the modeling and mitigation of interference fringes in polarimetric instrumentation
› Black hole scalar sirens in the Milky Way
› Analysis of Tidal Perturbations Due to Asymmetric Response of LARES 2 and LAGEOS
› Modified Teukolsky formalism: Null testing and numerical benchmarking

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