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
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 Wiadomości z astronet.pl

› Nowe plany NASA ujawnione we wtorek
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› CanSat sterowany sztuczną inteligencją – projekt WindRiders
› Katalog Caldwella: C54
› Misje kosmiczne XX wieku: Program Discovery
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› Do 20 marca zapisy do konkursu Łowcy Cząstek 2026
› Katalog Caldwella: C64
› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
› Niebo w marcu 2026 roku
RSS  Najnowsze prace na astro-ph:

› Global detector network to search for high-frequency gravitational waves (GravNet): conceptual design
› Neutrino and electromagnetic signatures from Superluminous Supernovae: a case study for SN 2017egm
› BLAZ4R and the eROSITA view of z>4 blazars
› Clouds with a silicate lining: Using JWST spectra to probe atmospheric diversity in young AB Dor L dwarfs
› Disentangling auroral, cloud and magnetic spot driven variability in three early L-dwarfs with HST/WFC3
› A Probabilistic Autoencoder for Galaxy SED Reconstruction and Redshift Estimation: Application to Mock SPHEREx Spectrophotometry
› Systematic Monitoring of Extreme X-ray Variability from Weak-line Quasars
› A Fast, Hot Wind from a Nuclear Starburst
› Beyond the Largest Lyapunov Exponent: Entropy-Based Diagnostics of Chaos in Henon-Heiles and N-Body Dynamics
› The background gas humming and multi-messenger transients of stalled supermassive black hole binaries
› GJ 523b is a Massive, 170 Myr-old Mega-Earth, Likely on a Polar Orbit
› The rise of the black hole X-ray binary AT2019wey observed with TESS
› A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
› The mmax-Mecl relation in the LEGUS clusters
› A PANORAMIC of UV-optical morphologies of "Little Red Dots": Two groups of LRDs distinguished by UV half-light radius
› From dust to planets -- II. Effects of wide binary companions and external photoevaporation on planetesimal and embryo formation
› A scalable Bayesian framework for galaxy emission line detection and redshift estimation
› Photon Ring Astrometry I: A Simple Spin Measurement Technique for High-Resolution Images of M87*
› A striking excess of red quasars with steep radio spectral slopes: a dusty blow-out phase revealed through AGN-driven shocks?
› The Coldest Known Y Dwarfs: Estimates of their Effective Temperatures
› The Diffuse Gamma-ray Sky of a Milky Way Analogue: Local Diversity and Global Constraints
› Production of heavy $\alpha$-elements and $^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
› Distance estimate to NGC 6951 from supernova siblings Type IIP SN 2020dpw and Type Ib SN 2021sjt
› Deep radiative zones affect the planetary cooling and internal structure: implications for exoplanet characterisation
› Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
› Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star
› SaNDi-SHoP: Searching for Satellites'N'Disks with a Star-Hopping Program I. Analysis of the close surroundings of DI companions
› Understanding Balmer Decrements in T Tauri stars in terms of Multiflow Magnetospheric Accretion
› On the importance of laboratory experiments for interpreting exoplanet observations
› ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229
› Large-scale weak lensing convergence in nonlinear general relativity
› Large Scale Spectrophotometric Relative Flux Calibration for the Roman High Latitude Wide Area Survey
› Interstellar stereoisomerism
› From Origins to Observables: Distinguishing Dark Compact Objects with Population-Level Microlensing Signatures
› Propagating Kink Waves in Chromospheric Jet-like Structures and Coronal Plumelets
› Revisiting the Claim for a Direct-Collapse Black Hole in UHZ1 at $z=10.05$
› Dynamics and stability of magnetized AGN-blown bubbles in clusters of galaxies
› Flare-driven habitability: Expanding life's potential around low-mass stars
› Investigation on the X-ray emission of NGC 4051 during its 2009 optical/UV-X-ray dissociation phase
› Bar Properties and Star-by-Star Bar Membership via Action Conservation
› Constraints on the Physical Association between ICECAT1 Neutrinos and Fast Radio Bursts Using the Second CHIME/FRB Catalogue
› A post-perihelion constraint on the CO$_{2}$/H$_{2}$O ratio of interstellar comet 3I/ATLAS from [O I] forbidden lines
› Probing Dust Composition in Distant Galaxies with JWST Mid-IR Spectroscopy of Quasars with Foreground 2175 {\AA} Absorbers II. Measurements of Grain Composition and Extinction Properties
› X-ray spectral and temporal evolution of atoll source 4U 1820-30 with AstroSat: detection of high frequency quasi-periodic oscillation
› The 'Forgotten' Neutrons: Implications for the Propagation of High-Energy Cosmic Rays in Magnetized Astrophysical and Cosmological Structures
› Fitting the light curves of tidal disruption events with non-parabolic model
› Development of a one-dimensional position sensitive detector for Compton X-ray polarimeters
› Binary neutron star mergers with a subsolar mass star
› Bulge Fossil Fragments as a new population of factories of gravitational wave sources in the Galaxy
› Verification of the Polarimetric Capability of the East Asia VLBI Network
› Core and mantle thermal evolution constraints on the onset of plate tectonics and a long-lived geodynamo
› Star-Galaxy Classification in Deep LSST Data with Random Forest: A Pilot study on the Data Preview 1 Release
› Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part I : the design, development and laboratory characterization
› Interaction between vegetation and Snowball phases in the late Proterozoic Earth
› Calibration of key parameters during the in-orbit phase for the Taiji-2 gravitational reference sensor
› Jet Power Estimates of FSRQs PKS 1441+25 and Ton 599 from Broadband SED Modeling
› Cluster gravitational redshifts: uncertainties and survey requirements
› Development of ProtoPol: a medium resolution echelle spectro-polarimeter for PRL telescopes, Mt Abu, India -- Part II : the data-reduction pipeline, on-sky characterization $\&$ performance verification and first science results
› Tracing neutral hydrogen in UGCA 320: A MHONGOOSE perspective on an edge-on dwarf galaxy in a group environment
› Eclipsing binary classification with machine learning techniques
› Probing the Solar Corona and the Solar Wind Using Angular Broadening Observations with the SKA
› The Effect of Expansion and Instabilities in the Thermodynamic Regulation of the Young Solar Wind Plasma
› Implementation of a Near-Realtime Recording and Reporting System of Solar Radio Bursts
› Advancing weak lensing mass mapping with a mask-aware HEALPix transformer
› The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
› Bayes-SCF: A Bayesian filter to mitigate foreground leakage in the 21-cm power spectrum
› The Impact of Fuzzy Dark Matter Dynamics on the Accumulation and Fragmentation of Primordial Gas
› Particle Physics and Gravitational Waves as complementary windows on the Universe
› POP-CORN: Validation of a new coronal hole detection tool based on neural networks
› Structural Analysis of a Scalar-Tensor Realization of Interacting Dark Energy
› Inferring the mass of the circumgalactic medium using X-ray resonant scattering
› Ice chemistry that can be unveiled with the JWST: SynthIceSpec, a synthetic spectrum generator to test spectral limits. Solid CO_2 as a dust thermometer and solid CH_3CN detectability in cold cores
› Painting a full radio sky -- Empirical mock catalogues with multiple source populations for future radio surveys
› Double-Adiabatic Equations of State for Relativistic Plasmas
› Interpretation of 21 cm Auto Power Spectrum Measurement at $z\sim 1$ by the Canadian Hydrogen Intensity Mapping Experiment
› Nonlinear Information from DESI Luminous Red Galaxies: An Emulator-Based Analysis of Pre- and Post-Reconstruction Power Spectra
› Identifying Surface Degeneracies in Single-Visit Reflected Light Observations of Modern Earth using the Habitable Worlds Observatory
› Bayesian analysis of $\alpha$-Starobinsky model with Planck, ACT and DESI data
› CMB constraints on dark matter-proton scattering: investigating prior-volume effects using profile likelihoods
› Parameterizing Dark Energy at the density level: A two-parameter alternative to CPL
› Testing Dark Energy with Black Hole Ringdown
› Cosmological coupled black holes immersed in dark sector
› Cosmological correlators from the Inflation end to CMB sky via reheating
› Fixing the center-of-mass frame of numerical relativity waveforms using the post-Newtonian center-of-mass charge
› ACT-Planck data and phase transitions from a viable no-scale Standard Model completion
› The Universe Originating from an Empty Planck-Size Torus
› UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
› Cogenesis of visible and dark matter in type-I Dirac seesaw
› Primordial black hole formation from transient $f(T)$ cosmology
› Critical Behavior of Photon Rings in Kerr-Bertotti-Robinson Spacetime
› A Telescope System for Charge and Position Measurement of High Energy Nuclei
› Non parametric constraints of gravitational-electromagnetic luminosity distance ratio
› Bayesian analysis of proton-proton fusion in chiral effective field theory
› QED cross sections in strong magnetic fields
› On the double-adiabatic equations in the relativistic regime
› Halo Spin Depends on The Distance to Cosmic Filament
› Bloodhound Unleashed: Particle-based Substructure Tracking for Cosmological Simulations
› Semi-Supervised Learning for Lensed Quasar Detection
› The Search for Stable Nickel: Investigating the Origins of Type Ia Supernovae with Late-time NIR Spectroscopy from the Carnegie Supernova Project-II
› Differentiable Fuzzy Cosmic-Web for Field Level Inference
› Evidence for Phenylium Reactivity under Interstellar Relevant Conditions
› Cosmological constraints from galaxy clustering and galaxy-galaxy lensing with extended SubHalo Abundance Matching
› Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
› Breaking the Mass-sheet Degeneracy in Time-delay Cosmology with Lensed and Unlensed Type Ia Supernovae
› Orientation of orbital planes of planetary systems detected in microlensing campaigns
› Simulation based inference of the ionization history from the 2D 21 cm power spectrum
› Optimization procedure of the baffle of the GroundBIRD Telescope to mitigate stray light
› Cloudy solutions for the clear skies of WASP-80b: 3D cloud feedback on the atmosphere and spectra of a warm Jupiter
› Catalog of Mock Stellar Streams in Milky Way-Like Galaxies
› Spatial Variations of Polarized Synchrotron Emission in the QUIJOTE MFI Data using Neural Networks
› Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach
› Abundance Stratification in Type Iax SN 2020rea with TARDIS
› Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
› HST view of NGC 5044: Constraints on Filament Widths, Magnetic Support, Multiphase Structure, and Comparison with Cluster Environments
› A fast method for deriving relative small-scale magnetic field variations from high-resolution spectroscopy
› Searching for Unparticles with the Cosmic Microwave Background
› Graph Path Likelihood for Galaxy Formation on Layered Halo Graphs
› What Shape is the Inflationary Bispectrum?
› Stellar characterization with photometric colors from J-PLUS and 2MASS surveys
› Improved dark matter measurements with flexible modeling of resolved strongly-lensed quasar narrow-line emission
› Impact of Antenna Structure and Orientation on Forward-Modelled Global 21 cm Signal Recovery
› Unlocking HST's Stellar Treasure Trove: Stellar Activity Minima for HAT-P-11 Offer Prime Windows for Transmission Spectroscopy
› Notes on Gravitational Physics
› Wideband Search for Axionlike Dark Matter Using Octupolar Nuclei in a Crystal
› pylevin: Efficient numerical integration of integrals containing up to three Bessel functions
› The Cosmic Horizon of Neutrinos
› Dark Matter and Electroweak Baryogenesis with Spontaneous $CP$ Violation in the Early Universe
› Designing trajectories in the Earth-Moon system: a Levenberg-Marquardt approach
› Light scalars in light of UV/IR mixing: classicalization via synergy between Vainshtein and chameleon screenings
› Fifty shades of grayness: parametrizations of spectral distortions and applications in cosmology
› Conformal symmetry in force-free electrodynamics
› A Unified Interpretation of Supernova, GRB, and QSO Time Dilation Signals in a Generalized Cosmological Time Framework
› A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model
› Breaking the degeneracy among regular black holes with gravitational lensing

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