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

› Wada zwierciadła Kosmicznego Teleskopu Hubble’a
› 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
RSS  Najnowsze prace na astro-ph:

› Delayed Wind Onset in Pa 30, the Remnant of Type Iax SN 1181
› V570 Per: Characterization of a Benchmark Eclipsing Binary
› Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity?
› Mixing between AGN winds and ISM clouds produces luminous X-ray emission
› First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-IR Spectral Energy Distribution and Millimeter Polarimetry
› Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE): a likely aligned orbit for the 3 Myr planet TIDYE-1 b
› Variability-selected AGN in dwarf galaxies: the incidence of AGN in dwarf and massive galaxies is similar
› Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
› J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $
› Mid-infrared extinction toward the Galactic center
› Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre
› Large Language Model Driven Analysis of General Coordinates Network (GCN) Circulars
› Radio properties of the quasi-periodic eruption source RXJ1301.9+2747 at parsec scales
› Tidal Disruption Events
› Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core Collapse
› SN 2023taz: Implications for the UV Diversity of Superluminous Supernovae
› Simulations of a Conducting Sphere Moving through Magnetized Plasma: Alfv\'en Wings, Slow Magnetosonic Wings, and Drag Force
› Proton specific entropy as a proxy for the $O^{7+}/O^{6+}$ charge state ratio over heliocentric distance
› Constraining the Jet Energetics of the Transient X-ray Binaries MAXI J1348-630 and MAXI J1820+070 through Calorimetry
› Understanding the Origin and Dynamical Evolution of the Unique Open Star Cluster Berkeley 20 using FIRE Simulations
› A Neural Network Approach to Preferred Event Selection for Low-Latency Gravitational-Wave Alerts
› Toward Complete Merger Identification at Cosmic Noon with Deep Learning
› Relative Strengths of Fundamental and Harmonic Emissions of Solar Radio Type II Bursts
› Hyperaccretion-driven relativistic jets from massive collapsars in active galactic nucleus disks
› Deep-learning mitigation of foregrounds and beam effects in 21-cm intensity mapping using hybrid frequency differencing and PCA
› The ALMA-QUARKS survey: Evidence of a candidate high-mass prestellar core aside a bright-rimmed cloud IRAS 18290-0924
› Implications of the Two-Component Dark Energy Model for Hubble Tension
› PHR~J1724-3859: A Bipolar Planetary Nebula in Open Cluster Trumpler 25
› Solar Periodic Companion and Random Stellar Flybys: Dynamical Perturbations of Highly Eccentric Comets in the Oort Cloud
› Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter
› Electron Cyclotron Maser Emission as the Driving Mechanism in Long-Period Radio Transients
› Non-thermal processes in standard big bang nucleosynthesis: III. Reactions with slow nuclei and the overall effect
› Gravitational Wave Phase shifts of black hole mergers in AGN Disks
› Evolution of action-space coherence in a Milky Way-like simulation
› Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. IV. Broad Emission Line Evolution Sequence Among H{\alpha}, Mg II, and H{\beta}
› The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking
› Refractive indices of photochemical haze analogs for Solar System and exoplanet applications : a cross-laboratory comparative study between the PAMPRE and COSmIC experimental set-ups
› A Method for Gamma-Ray Energy Spectrum Inversion and Correction
› A JWST Transit of a Jupiter Analog: II. A Search for Exomoons
› Origin of Galaxies
› Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability
› Type Iax supernovae as a source of iron-rich silicate dust
› Galaxy-Multiplet Clustering from DESI DR2
› Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. V. Dramatic Variability in High-Ionization Broad Emission Lines
› Simple relations from complex outflows: How the $M-\sigma$ relation emerges in a multi-phase environment
› Insights on Gas Distribution and Dynamics in Massive Proto-cluster G358.46$-$0.39: Possible Multiplicity in G358.46$-$0.39 MM1a
› Explosions in the Empty: A Survey of Transients in Local Void Galaxies
› Elemental abundance ratios for the bulge of M31
› Viscous Dark Energy and Mass-Varying Dark Matter in Lyra Manifold: Cosmological Dynamics and Observational Constraints
› 21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter
› Advancing Identification method of Gamma-Ray Bursts with Data and Feature Enhancement
› Optical gains measurement with a gain scheduling camera: On-sky demonstration with PAPYRUS and perspectives
› Challenging the $\omega_0\omega_a$CDM parametrization through rational expansions in view of DESI data release
› LCS: A Learnlet-Based Sparse Framework for Blind Source Separation
› Probing the disk-jet coupling in M87
› Efficient Exoplanet Imaging Simulations of the Habitable Worlds Observatory
› Identification of periodic density structures in Solar Orbiter data: Radial evolution
› Using Light Curve Derivatives to Estimate the Fill-out Factor of Overcontact Binaries
› The VVVX quest for satellites around the Circinus galaxy
› Is There New Physics Beyond 30 TeV in the BOAT?
› Quadruple system HD 135160 in a unique 2+2 configuration
› Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data
› Catching the 2021 {\gamma}-ray flare in the blazar TXS 2013+370
› Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break
› Reporting a Deficit of Intrinsic NV Absorbers in Core-dominated, Radio-loud Quasars
› The Cherenkov Camera for the PBR mission
› The data processing system of the POEMMA-Balloon with Radio mission
› The JWST weather report from the nearest brown dwarfs III: Heterogeneous clouds and Thermochemical instabilities as possible drivers of WISE 1049AB's spectroscopic variability
› Impact of cosmic expansion on gravitational wave spectra from strongly supercooled first-order phase transitions
› The Relationship Between Emission Line and Continuum Luminosity and the Baldwin Effect in Blazars. I. The Case of the Mg II {\lambda}2798 {\AA} Emission Line
› The Atacama Cosmology Telescope: Cross-correlation of kSZ and continuity equation velocity reconstruction with photometric DESI LRGs
› Detection of a highly stable orbital-period signal in GRACE-FO one-way intersatellite ranging using a synchronization-free differential observable (origin currently unidentified)
› On the Theory of Bulk Viscosity of Cold Plasmas
› The significance of Halley's Comet in the Bayeux Tapestry
› The Physics of Black Holes and Their Environments: Consequences for Gravitational Wave Science
› Low-frequency radio telescopes sensitivity to light dark matter
› 511 keV Gamma Ray Echo from Particle Decays in Supernovae
› Improved cosmological constraints on axion-lepton interactions
› Computational and Experimental Comparison of CLF5605 and roamx-0201 Martian Helicopter Rotor Airfoils
› IonCast: A Deep Learning Framework for Forecasting Ionospheric Dynamics
› The effects of dark energy on the matter-gravity coupling
› Power-law Bianchi type I inflation with multiple vector fields
› Divergence in tracing the flavors of astrophysical neutrinos: can JUNO help IceCube?
› Gravitational Bound State Perturbations Inside Black Holes and Isospectrality
› Dynamical Evolution and Graceful Exit in Quartic Warm Inflation
› A New Definition of Horndeski Theory and the Possibility of Multiple Scalar Field Extensions
› Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors
› Wavelengths and Energy Levels of Neutral Manganese (Mn I) Determined Using High-Resolution Fourier Transform and Grating Spectroscopy
› Turbulence in the terrestrial magnetosheath: space-time correlation using the Magnetospheric Multiscale mission
› Relativistic mean-field model with density- and isospin-density-dependent couplings
› Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
› Formation of neutron stars inside planetary nebulae via accretion-induced collapse and core-merger-induced collapse from white dwarf binaries
› A Novel Density Profile for Isothermal Cores of Dark Matter Halos
› Isolated Binary Black Hole Formation and Merger Rates from Galaxy Evolution
› Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology
› UHECR deflections in the coherent Galactic magnetic field
› Structure Formation with Warm White Noise: Effects of Finite Number Density and Velocity Dispersion in Particle and Wave Dark Matter
› Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
› Detection of a Type-C QPO during the soft-to-hard transition in Swift J1727.8-1613
› Smoking gun signature from axion and the constraints with radio telescopes
› Spectroscopic Characterization of redMaPPer Galaxy Clusters with DESI
› Analytical Transit Light Curves for Arbitrary Power-Law Limb Darkening: A Unified Framework
› Understanding the Drag Torque in Common Envelope Evolution
› Cool Gas in the Circumgalactic Medium of Massive Post Starburst Galaxies
› JWST's PEARLS: A Candidate Massive Binary Star System in a Lensed Galaxy at Redshift 0.94
› Investigating the Growth of Little Red Dot Descendants at z
› DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
› Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397
› Dance to Demise -- How Massive Stars May Form Dense Circumstellar Shells Before Explosion
› MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
› The source of the cosmic-ray excess in the Centaurus region -- constraints on possible candidates, mass composition and cosmic magnetic fields
› Unlocking 21cm Cosmology with SBI: A Beginner friendly NRE for Inference of Astrophysical Parameters
› Detecting Local and Integrated Relativistic Effects by Multi-Tracing a Single Galaxy Population in Harmonic Space
› Gravitational Recoil and Suppression of Super Massive Black Hole Seeds in the Early Universe
› Dust Attenuation of Lyman-Werner Feedback: Reassessing Early Super Massive Black Holes Seed Formation
› A simple, flexible method for timing cross-calibration of space missions
› Kinematics of Stellar Streams from Globular Clusters Depend on Black Hole Retention and Star Mass: A Selection Effect for Dark Matter Inference
› Bayesian Gaussian Methods for Robust Background Modeling in CALorimetric Electron Telescope (CALET) Gravitational-Wave Searches
› Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly
› Orbital decay candidates reconsidered: WASP-4 b is not decaying and Kepler-1658 b is not a planet
› The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-6
› Efficient analytic approximation for small-scale non-cold relic perturbations
› XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105
› An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise
› The interstellar flux gap: From dust to kilometer-scale objects
› Kerr Black Hole Shadows in Dispersive Plasma: Frequency-Dependent Geodesics and Shadow Distortions
› JWST/NIRCam observations of HD~92945 debris disk: An asymmetric disk with a gap
› Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem
› Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections
› Recalibrating Inflation: Insights from Starobinsky Gravity
› Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions
› JWST observes the assembly of a massive galaxy at z~4
› Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs
› Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes
› Magnetic Fields in the Shapley Supercluster Core with POSSUM: Challenging Model Predictions
› Detector Response to Gravitational Wave Polarizations in Gravitational Quantum Field Theory
› Understanding large-scale dynamos in unstratified rotating shear flows
› Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
› A waveform and time digitization mainboard prototype for the hybrid digital optical module of TRIDENT neutrino experiment
› Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models
› Using tunable coherence for reaching micrometer coherence lengths and suppressing stray light in a power-recycled Michelson interferometer
› Constraints on the Variation of the QCD Interaction Scale $\Lambda_{\text{QCD}}$
› Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
› A General Framework for the Spontaneous Scalarization of Regular Black Holes
› Large-Scale Calculations of $\beta$-Decay Rates and Implications for $r$-Process Nucleosynthesis
› Generating optimal Gravitational-Wave template banks with metric-preserving autoencoders

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