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

› Drugi w historii lot komercyjnej rakiety z lądowaniem boostera!
› Misje Kosmiczne XX wieku: Atlantis
› Recenzja książki „Księżyc. Jak zmienił naszą planetę, przewodził ewolucji i stworzył nas takimi, jakimi jesteśmy”
› Insekty przyszłością diety astronautów?
› W Układzie Słonecznym: Obłok Oorta
› Misje kosmiczne XX wieku: Challenger
› Galaktyczny kartograf – Teleskop Nancy Grace Roman
› Niebo w listopadzie 2025 roku
› Misje kosmiczne XX wieku: Discovery
› Japońska technologia powraca na ISS. Pierwsza misja nowej kapsuły zaopatrzeniowej HTV-X
RSS  Najnowsze prace na astro-ph:

› Variations of angular momentum $L_z$ as an indicator of orbital chaos of globular clusters in the central region of the Galaxy with a bar
› Spectropolarimetric Evolution Reveals Dual-Axis Ejecta in the Atypical Magnetar-Powered SN 2012au
› Practical Author Name Disambiguation under Metadata Constraints: A Contrastive Learning Approach for Astronomy Literature
› Reaching for the Edge II: Stellar Halos out to Large Radii as a Tracer of Dark Matter Halo Mass
› Back to basics: Little Red Dots as galaxies and dust-obscured AGNs in a synthetic NIRCam sky simulated with L-GalaxiesBH
› An Analytical Model for the Eccentricity Cascade: Hot Jupiter Formation via S-type Instability
› Large-Scale Structure in COSMOS-Web: Tracing Galaxy Evolution in the Cosmic Web up to $z \sim 7$ with the Largest JWST Survey
› Widening of Binaries via Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System
› The signature of major mergers on the hydrostatic mass bias of galaxy clusters
› TESS Investigation -- Demographics of Young Exoplanets (TI-DYE) IV: a Jovian radius planet orbiting a 34 Myr Sun-like star in the Vela association
› Intra-night optical polarization monitoring of blazars
› KOALA, a new ATLAS9 database -- I. Model atmospheres, opacities, fluxes, bolometric corrections, magnitudes and colours
› Hybrid Simulations of Supersonic Shear Flows: I) Particle Acceleration
› The Quiescent Merging Nature of the Coma Cluster Revealed by ICM Velocity Structure
› REBELS-IFU: Steeply rising star formation histories and the importance of dust obscuration in massive $z \simeq7$ galaxies revealed by multi-wavelength observations
› REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization
› XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
› Indirect forces in disc-planet interaction
› Hydrogen-Poor Superluminous Supernovae in the Nebular Phase: Spectral Diversity Due to Ejecta Ionization as a Probe of the Power Source
› Hydrogen-line profiles from accreting gas giants and their CPDs
› Jeans Model for the Shapes of Self-interacting Dark Matter Halos
› Optimization of lenslet arrays for PRIMA Kinetic Inductance Detectors
› Historical Surveys to Rubin First Look: Absolute Colors of trans-Neptunian objects
› The Dawes Review 13: A New Look at The Dynamic Radio Sky
› The impact of supermassive black holes on exoplanet habitability: I. Spanning the natural mass range
› What's Inside Matters: The Effect of Oxygen Fugacity and Initial Volatile Abundance on the Atmospheres of the TRAPPIST-1 Planets
› Mock Observations for the CSST Mission: Main Surveys -- the Mock Catalogue
› ALMAGAL V. Relations between the core populations and the parent clump physical properties
› Ubiquitous high-frequency waves and disturbances in the active region corona observed with DKIST/Cryo-NIRSP
› Unveiling the Chemical Complexity and C/O Ratio of the HD 163296 Protoplanetary Disk: Constraints from Multi-line ALMA Observations of Organics, Nitriles, Sulfur-bearing, and Deuterated Molecules
› Evolutionary Map of the Universe: A pilot survey to detect high Galactic latitude pulsars in variance images with ASKAP
› In situ Evidence of 5-minute Oscillations from Parker Solar Probe
› PRIMA General Observer Science Book Volume 2
› A High-Precision Dynamical Model of Callisto: Incorporating Rotation Effects within Multi-Layer Internal Structure Models
› EUSO-SPB2 Cherenkov Telescope: Overview and First Neutrino Constraints
› Discovery of an X-ray bridge between the comma-shaped gas and the main cluster in MCXC J0157.4-0550
› A proposal to construct the dark-matter-only counterpart of the observed Universe combining weak lensing and baryon censuses
› Accuracy and Applicability of the Hartle-Thorne and Komatsu-Eriguchi-Hachisu Methods for Modeling Rotating Neutron Stars
› SPICE -- modelling synthetic spectra of stars with non-homogeneous surfaces
› Surface figure metrology for reflective membrane mirrors based on phase-measuring deflectometry
› Measurement of cosmic-ray muon flux at CJPL-II
› Highly Polarized Intrinsic Emission and its Orthogonal Counterpart in Vela X-1
› The Spatial Evolution of Star Clusters in NGC 628 with JWST
› A Simulation Platform for Small Solar System Bodies using the Einstein-Elevator
› Galactic foreground residual biases in CMB lensing convergence reconstruction and delensing of B-mode maps
› Constraints on the canonical single-field slow-roll inflation model from observations
› Empirical prediction of plasma emission measure distributions and X-EUV spectra of late-type stars
› Evidence for the Keplerian orbit of a close companion around a giant star
› Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
› Formation and disruption of resonant chains of super-Earths: Secular perturbations from outer eccentric embryos
› Close-in compact super-Earth systems emerging from resonant chains: slow destabilization by unseen remnants of formation
› A glitch in the millisecond pulsar J0900$-$3144
› Recalibrating Inflation: Insights from Starobinsky Gravity
› Shadow-Induced Warps in Protoplanetary disks
› Boost operator approach to the relativistic polarized SZ effect
› Modeling the Multi-Wavelength Afterglow of Short Gamma-Ray Bursts with a Plateau Phase
› Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations I: Hydrodynamics
› Star clusters in the gamma-ray sky
› Planetary nebulae as tracers of stellar population properties: a pilot study with MUSE
› A 34.6-day transiting sub-Neptune in the TOI-1422 planetary system
› Looking at infrared background radiation anisotropies with Spitzer II. Small scale anisotropies and their implications for new and upcoming space surveys
› Mutated Hilltop Inflation in the Era of Present and Future CMB Experiments
› Probing the era of giant collisions: millimeter observations of the HD 166191 system
› An optical--mid-infrared color evolution tool for nova identification using WISE data
› Testing the cosmological Euler equation: viscosity, equivalence principle, and gravity beyond general relativity
› Implicit inference of the reionization history with higher-order statistics of the 21-cm signal
› Characterization of the ionization response of argon to nuclear recoils at the keV scale with the ReD experiment
› Keeping It Renormalizable: Minimal Baryogenesis induced Asymmetric Dark Matter
› In-situ environmental radiation background measurement in the second phase of CJPL
› NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration
› Dark Matter Capture in a Core-Collapse Supernova Revives Dark Photons
› Influence of Rotation on Fingering Convection in Planetary Cores
› Intrinsic Dimension Estimation for Radio Galaxy Zoo using Diffusion Models
› \textit{Euclid}: From Galaxies to Gravitational Waves -- Forecasting Stochastic Gravitational Wave Background Anisotropies and Their Cross-Correlation
› First Use of GPS Satellites for Beam Calibration of Radio Dish Telescopes
› Gamma-Ray Burst Light Curve Reconstruction: A Comparative Machine and Deep Learning Analysis
› Anatomy of Parity-violating Trispectra in Galaxy Surveys
› Establishing a Connection Between the Jet and the Corona in Black Hole Low Mass X-Ray Binaries
› Molecular Dynamics Simulations on Nuclear Recoils in Silicon Crystals towards Single Electron-Hole Pair Ionization Yields
› Accurate $N$-body simulations with local Primordial non-Gaussianities: initial conditions and aliasing
› Transformers for Stratified Spectropolarimetric Inversion: Proof of Concept
› Braking index of the frequently glitching PSR J0537$-$6910
› Multi-Model Framework for Reconstructing Gamma-Ray Burst Light Curves
› Survival of higher overdensity cold gas in a turbulent, multiphase medium
› EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger?
› The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
› Probing the Cosmological Principle with CMB lensing and cosmic shear
› Discovery and Analysis of Afterglows from Poorly Localised GRBs with the Gravitational-wave Optical Transient Observer (GOTO) All-sky Survey
› Euclid preparation LXXIX. Using mock low surface brightness dwarf galaxies to probe Euclid Wide Survey detection capabilities
› Recovering the Coupled Treatment of Redshift-Space Distortions and the Lightcone Effect after Diffuse Foreground Removal
› Interstellar Dust-Catalyzed Molecular Hydrogen Formation Enabled by Nuclear Quantum Effects
› Multi-modal atmospheric characterization of $\beta$ Pictoris b: Adding high-resolution continuum spectra from GRAVITY
› CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. V. Chemical composition gradients as a function of the galactocentric radius
› The evolution of the bar fraction and bar lengths in the last 12 billion years
› FlowLensing: Simulating Gravitational Lensing with Flow Matching
› Probing Anisotropic Cosmic Birefringence with Foreground-Marginalised SPT B-mode Likelihoods
› Galactic X-ray Transients in the First eROSITA All Sky Survey
› Connecting outflows with radio emission in active galactic nuclei at cosmic noon
› ZTF25abjmnps (AT2025ulz) and S250818k: A Candidate Superkilonova from a Sub-threshold Sub-Solar Gravitational Wave Trigger
› Constraints on Cosmic Birefringence from SPIDER, Planck, and ACT observations
› Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared
› Kinematic scaling relations of disc galaxies from ionised gas at $z\sim~1$ and their connection with dark matter halos
› Global Distribution of the Key Species on the Surface of Europa
› Dark Photons in the Radio Sky: I. Resonant Conversions in Halos
› Dark Photons in the Radio Sky: II. Resonant Conversions in the Intergalactic Medium
› A Bayesian Perspective on Evidence for Evolving Dark Energy
› Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
› Flavor Matters, but Matter Flavors: Matter Effects on Flavor Composition of Astrophysical Neutrinos
› Bridging the Rossby number gap in rapidly rotating thermal convection
› Demonstration that Differential Length Changes of Optical Cavities are a Sensitive Probe for Ultralight Dark Matter
› Unified nonparametric equation-of-state inference from the neutron-star crust to perturbative-QCD densities
› Earth-Scattering Induced Modulation in Low-Threshold Dark Matter Experiments
› Precision calculation of $N_{\text{eff}}$ with Neutrino Direct Simulation Monte Carlo
› The periastron regression of 2M1510 AB, the jet precession of M87* and Telisto/Planet Nine: three different scenarios for a possible common cause
› Euler-Heisenberg action for fermions coupled to gauge and axial vectors: Hessian diagonalization, sector classification, and applications
› Stochastic Limit of Growing Gravitational Wave Memory from Sources in the Early Universe and Astrophysical Sources

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