Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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Zdjecie: nocny widok od południowego wschodu
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 Wiadomości z astronet.pl

› Katalog Caldwella: C109
› Łazik Perseverance odkrył potencjalne biosygnatury na Marsie
› Katalog Caldwella: C104
› Sonda Solar Orbiter dowiodła – energetyczne elektrony ze Słońca mają dwa różne źródła
› Zdjęcie z Chandry w falach radiowych i rentgenowskich
› Katalog Caldwella: C84
› Relacja z obozu astronomicznego dla starszych 2025
› Katalog Caldwella: C41
› Jakie materiały i skąd stworzyły planetoidę, z której uformowała się Bennu?
› Recenzja książki „Trinity. Historia bomby, która zmieniła losy świata”
RSS  Najnowsze prace na astro-ph:

› Systematic Effects of Chaotic Magnetic Fields on Neutron Star Tidal Deformability: Implications for Gravitational Wave Constraints on Dense Matter
› SIMBA: A Python-based single-point astrochemical solver and analysis tool
› Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Time delays & Hubble constant measurement
› Off-center black hole seed formation? Implications for high and low redshift massive black holes
› Death by Impact: Evidence for Merger-Driven Quenching in a Collisional Ring Galaxy at Cosmic Noon
› Zeeman Doppler Imaging of $\tau$Ceti: The Weakest Magnetic Field Detected in a Sun-like Star
› Origin of the double-peaked narrow emission-lines in the optical spectra of X-shaped Radio Galaxies
› DELVE Milky Way Satellite Census I: Satellite Population and Survey Selection Function
› WIYN Open Cluster Study. XCIII. An Extended Radial-Velocity Survey and Spectroscopic Binary Orbits in the Open Cluster NGC 188
› Building up JWST-SUSPENSE: inside-out quenching at cosmic noon from age, Fe-, and Mg-abundance gradients
› Star-Black Hole Interactions in Young Star Clusters
› Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Lens model comparison and H0 measurement
› VADER: A Variational Autoencoder to Infer Planetary Masses and Gas-Dust Disk Properties Around Young Stars
› Constraints on the early growth of massive black holes from PTA and JWST with L-GalaxiesBH
› Exploring the spatially-resolved capabilities of the J-PAS survey with Py2DJPAS
› Do Outer Giants Inflate Neptune-sized Planets? An Architecture-Dependent Mass-Radius Relation
› Lowering the Horizon on Dark Energy: A Late-Time Response to Early Solutions for the Hubble Tension
› No Giant Planets in the Eta Cassiopeiae System: Dynamical Implications of a Wide Binary Companion
› Phantom Crossing with Quintom Models
› Brown Dwarf Formation Through Gravitational Collapse: Insights From 3D Numerical Simulations
› SN 2024aecx: Double-Peaked Light Curves and Rapid Evolution in a Nearby Type IIb Supernova
› Space Mission Options for Reconnaissance and Mitigation of Asteroid 2024 YR4
› Predicting stellar collision outcomes of main sequence stars
› Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense
› Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning
› Search for Quintessence-Like Pseudoscalar Dark Energy Effects on $^{56}\text{Fe}$ Nuclear Transition Energies in Supernova 1991T
› When IIb Ceases To Be: Bridging the Gap Between IIb and Short-plateau Supernovae
› BOWIE-ALIGN: Weak spectral features in KELT-7b's JWST NIRSpec/G395H transmission spectrum imply a high cloud deck or a low-metallicity atmosphere
› A high fraction of close massive binary stars at low metallicity
› The Photospheric Emission of a Short-Duration Gamma-Ray Burst Emerging from a Realistic Binary Neutron Star Merger
› TESS Subgiant and Lower Red Giant Asteroseismology in the Continuous Viewing Zones
› Who Uses Whose Telescopes? Analyzing the Knowledge Geography and Research Dominance of Global Astronomical Facilities
› TESS Light Curve Analysis: A Case Study of Stellar Rotation in TIC 445493624
› Large-field CO(1-0) observations toward the Galactic historical supernova remnants: shocked molecular clouds toward the Crab Nebula
› Revisiting thermodynamics at the outskirts of the Perseus cluster with Suzaku: importance of modeling the Hot Galactic gas
› Extreme High-Energy Neutrinos: IceCube vs. KM3NeT
› Identifying Fixed Points in the Three-Body Problem Using a High-Order Transfer Map
› Cislunar Resonant Transport and Heteroclinic Pathways: From 3:1 to 2:1 to L1
› Multiple Giant Impacts and Chemical Equilibria: An Integrated Approach to Rocky Planet Formation
› A comprehensive study of comet 67P/Churyumov-Gerasimenko in the 2021/2022 apparition. I. Photometry, spectroscopy, morphology
› Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period
› TSD: An inverse problem approach for recovering the exoplanetary atmosphere transmission spectrum from high-resolution spectroscopy
› Superresolution of unequal-brightness thermal sources for stellar interferometry
› Apsidal motion and proximity effects in the massive binary BD+60 497
› Simulation of Wavefront-based Disturbance Observers for Large Telescopes
› Modal Identification of Mirror Vibrations at the VLT using Accelerometer Data
› Deciphering Profile Stability in Millisecond Pulsars: Timescales, Frequency Evolution, and Implications on Emission Mechanisms
› Deimos photometric properties: analysis of 20 years of observations (2004-2024) by the Mars Express HRSC camera
› An nl-model with a full radiative transfer treatment for level populations of hydrogen atoms in a spherically symmetric H II region
› Two unseen massive white dwarf candidates in close binaries
› Eleven Local Volume dwarf galaxies in the FASHI survey
› The AdvCam: Designing the future cameras for the Large-Sized Telescope of the Cherenkov Telescope Array Observatory
› Asymmetric radiation in binary systems: Implications for disk evolution and chemistry
› Investigating the capability of the Cherenkov Telescope Array Observatory to detect gamma-ray emission from simulated stationary neutrino sources identified by KM3NeT
› Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
› Evolution of low surface brightness ultra-thin galaxies: The role of dark matter halo and bar formation on disk thickness
› Cosmic dust as a prerequisite for the formation of complex organic molecules in space?
› Magnetic Reconnection as a Potential Driver of X-ray Variability in Active Galactic Nuclei
› Probing the millisecond pulsar origin of the GeV excess in the Galactic Centre with LISA
› Muon number reconstruction with IceTop using a two-component lateral distribution function
› Archival Search for IceCube Sub-TeV Neutrino Counterparts to Sub-Threshold Gravitational Wave Events from the Third Observing Run of the LIGO-Virgo-KAGRA
› Binary imposters: Mergers in massive hierarchical triple stars
› Capturing System Drift with Time Series Calibration for Global 21-cm Cosmology Experiments
› Radio detection of Cosmic Rays with the IceCube Surface Array Enhancement
› Solar Flare Hard X-ray Polarimetry with the CUbesat Solar Polarimeter (CUSP) mission
› Long-lived coronal loops in solar active regions
› The nature and evolution of a-C(:H) nanoparticle substructures and speculations on the origin of the 3-4$\mu$m emission bands
› Puffed-up Inner Rings and Razor-thin Outer Rings in Structured Protoplanetary Disks
› Increasing science yield with a twilight observing program with the SCALES instrument at Keck
› Probing Stellar Kinematics with the Time-Asymmetric Hanbury Brown and Twiss Effect
› Euclid preparation. Using mock Low Surface Brightness dwarf galaxies to probe Wide Survey detection capabilities
› Gamma-ray Analysis of Pulsar Environments and Their Theoretical Explanation
› A novel pointing technique for the enhancement of Tropospheric Delay Calibration System performances
› Parity in Composite-Field Galaxy Correlators
› Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases
› Massive Retrograde Moons May Survive During Different Hot Jupiters' Migration Scenario
› Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges
› Thermonuclear X-ray bursts across the eclipse transitions in the LMXBs EXO 0748-676 and XTE J1710-281
› Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data
› High-Dimensional Bayesian Model Comparison in Cosmology with GPU-accelerated Nested Sampling and Neural Emulators
› VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
› First detection of ices in intermediate-mass young stellar objects beyond the Milky Way
› How Theory-Informed Priors Affect DESI Evidence for Evolving Dark Energy
› Constraints on Dark Matter Structures around Gaia Black Holes
› Redefining interiors and envelopes: hydrogen-silicate miscibility and its consequences for the structure and evolution of sub-Neptunes
› Consistent Four-derivative Heterotic Truncations and the Kerr-Sen Solution
› LHAASO Galactic Plane $\gamma$-rays Strongly Constrain Heavy Dark Matter
› Bumblebee vector-tensor dark energy
› Taming the dark photon production via a non-minimal coupling to gravity
› Leptogenesis from Dark Matter Coannihilation
› Probing Flavour Deconstruction via Primordial Gravitational Waves
› Examining the influence of anisotropy on the fundamental mode of nonradial oscillation in quark stars on a complete general relativistic scheme
› Generalized Lema\^itre time for rotating and charged black holes and its near-horizon properties
› On the (Im)possibility of Electrically Charged Planck Relics
› The impact of Alfvenic shear flow on magnetic reconnection and turbulence
› Hyperons in Neutron Stars across the observed mass range: Insights from realistic $\Lambda$-N and $\Lambda$-$\Lambda$ interactions within a Microscopic Framework
› Random Forest Classification of MBTA Gravitational-Wave Triggers for Low-Latency Detection
› Quantum Computing Tools for Fast Detection of Gravitational Waves in the Context of LISA Space Mission
› Reconstruction of the Equations of State (EoSs) of Compact Stars using machine and deep learning regression techniques
› Nonresonant capture cross section measurement of the 29Si(p,gamma)30P reaction
› Cogenesis of baryon and lepton number asymmetries matching the EMPRESS Data
› Rotating neutron stars within the macroscopic effective-surface approximation
› Hybrid Active-Passive Galactic Cosmic Ray Simulator: experimental implementation and microdosimetric characterization
› Thermal Cesium Release in PMTs Revealed by Resonant Laser Spectroscopy and Its Correlation with Quantum Efficiency
› Virtual states and exponential decay in small-scale dynamo
› Revisiting axion dark matter with nonlinear transitions
› Axion-photon conversion in transient compact stars: Systematics, constraints, and opportunities
› Artificial Precision Timing Array: bridging the decihertz gravitational-wave sensitivity gap with clock satellites
› Massive star cluster formation III. Early mass segregation during cluster assembly
› KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
› Circumventing Cosmic Variance via Remote Quadrupole Measurements
› The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
› Is your stochastic signal really detectable?
› On the use of the Axelrod formula for thermal electron collisions in Astrophysical Modelling
› How do recollimation-induced instabilities shape the propagation of hydrodynamic relativistic jets?
› Evidence of the association of repeating fast-radio-burst sources with fast-spinning super-twisted magnetars
› Decaying vacuum energy, matter creation and cosmic acceleration
› The Relative Contributions of Accretion Disk versus Jet to the Optical and Mid-infrared Variability of Seyfert Galaxies
› Amaryllis: a digital twin of the earliest galaxies in the Universe
› Apache Point rapid response characterization of primitive imminent impactor 2024 RW$_1$
› Turbulent drag on stellar mass black holes embedded in AGN discs
› The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
› Calibrating baryonic effects in cosmic shear with external data in the LSST era
› Expanding the Ice Inventory of NGC 1333 IRAS 2A with INDRA using JWST Observations: Tracing Organic Refractories and Beyond
› Probing Solar Polar Regions
› Distinct Fe-K Line Complexes in MAXI J1744-294 Revealed by XRISM High-Resolution Spectroscopy
› Evolution of the Ionizing Photon Luminosity Function
› The advanced evolution of massive stars: I. New reaction rates for carbon and oxygen nuclear reactions
› GRB 241105A: A test case for GRB classification and rapid r-process nucleosynthesis channels
› Orbital and Pulsation Analysis of Forty-Two Heartbeat Stars Discovered in TESS Data
› A Novel Pipeline for the Identification of New Gamma-Ray Blazars from the 4FGL-Xiang Catalog Based on Multi-wavelength Flux Distributions
› Does the high-energy AMS-02 positron flux originate from the dark matter density spikes around nearby black holes?
› Granulation on a quiet K dwarf: HD 166620 I. Spectral signatures as a function of line-formation temperature
› The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
› The Schwarzschild-Couder Telescope for the Cherenkov Telescope Array Observatory
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: II. Super-Eddington Accretion
› The Orbits of Isolated Dwarfs in the Local Group from New 3D Kinematics: Constraints on First Infall, Backsplash, and Quenching Mechanisms
› The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates
› Magnetic reconnection sustains the mass budget of the solar wind
› TESLA-X: An effective method to search for sub-threshold lensed gravitational waves with a targeted population model
› Tidal Resonance in Binary Neutron Star Inspirals: A High-Precision Study in Numerical Relativity
› Coherence DeepClean: Toward autonomous denoising of gravitational-wave detector data
› Cosmological Stasis from Field-Dependent Decay
› Photon Absorption in a Doubly Special Relativity Model with Undeformed Free Propagation and Total Momentum Conservation
› Optimized quantum sensor networks for ultralight dark matter detection
› Shadows of naked singularity in Brans-Dicke gravity
› Exploring the role of accretion disk geometry in shaping black hole shadows
› A comparative study of time on Mars with lunar and terrestrial clocks
› II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
› I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
› III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
› Letter of Intent: AICE - 100m Atom Interferometer Experiment at CERN

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