Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

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› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
› Niebo w marcu 2026 roku
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RSS  Najnowsze prace na astro-ph:

› High-resolution near-IR spectroscopy of the B[e] supergiant LHA 115-S 18: discovery of hot water vapor emission
› LISA science ground segment conventions
› SDSS-V LVM: A spatially resolved study of the physical conditions and the chemical abundance discrepancy in the Lagoon Nebula (M 8)
› Shaping the diffuse X-ray sky: Structure, Variability and Visibility
› MEOW: The increase in the obscured AGN fraction in mid-infrared from 0 < z < 6 with JWST MIRI
› Second Order Closures for the Radiative Transfer Equation: Some Are Unstable
› Where within the 3C 84 jet are $\gamma$-rays produced?
› Reinterpreting the puzzling properties of z>6 galaxies within a variable IMF framework
› Phantom-Crossing Dark Energy and the $\Omega_m$ Tug-of-War
› Unified Formation Channel of Hot and Warm Jupiters via Planet-Planet Scattering
› Detailed Analysis of the NGC 2168 Cluster, Leveraging Gaia DR3
› A systematic study of AGN feedback in a disk galaxy II: MACER prediction of X-ray surface brightness profile and comparison with eROSITA observations
› Primordial Non-Gaussianity and the Field-Level Cramer-Rao Bound
› CHANG-ES. XXXVIII. A Thin Radio Halo Shaped by Slow Cosmic-Ray Transport in the Quiescent Galaxy NGC 4565
› The Crimson Kiss of Two Giants: Helium Detonation and High-Energy Neutrino Production
› A large population of over-massive black hole quasars at z=0.3-0.8 revealed by eROSITA
› Planet-Planet Scattering Explains the Mass-Eccentricity Relation of Warm Jupiters
› Magnetic Connectivity in the Time-Dependent Corona and Heliosphere
› Carbon Nitride Monolayer Nanosheets: Astrochemical Insights into the Fate of Interstellar Hydrogen
› The GRAVITY young stellar object survey -- XV. The star-disk interaction region of the T Tauri star DO Tau
› More Than Power: Revisiting the CMB Hemispherical Power Asymmetry with Morphological Descriptors
› Cross-spectra likelihood for robust $\tau$ constraints from all satellite polarisation data
› Impact of eccentricity on the population properties of neutron star - black hole mergers
› Optical Spectroscopy of the IR Source CPM 19 and Surrounding Objects
› Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation
› Ecological modelling of hycean worlds
› Model validation and tolerancing of scalar vortex masks in the High Contrast Imaging Testbed (HCIT) facility
› Turning the knobs on dust evolution: Comparing codes, parameters and their effects on planet formation and disc observables
› Dimpled scalar vortex coronagraph laboratory demonstration
› A Multi-messenger Search for Ultra-high-energy Gamma Rays in Coincidence with Neutrinos
› Automatic search for transiting planets in TESS-SPOC FFIs with RAVEN: over 100 newly validated planets and over 2000 vetted candidates
› The Radio-wave Observations at the Lunar Surface of the photoElectron Sheath (ROLSES) instrument onboard the Intuitive Machines-1 Mission to the Moon
› Subsurface ocean salinity and dissipation rate inferred from Enceladus ice shell morphology
› Multi-Sensor Trajectory Reconstruction of the 24 April 2025 Alaska Fireball and Implications for Planetary Defense
› The Two Component Circumgalactic Medium Emission around z~2 Radio-loud Quasars
› Cluster Infall for Mass Calibration in the Stage-IV Era
› HI Gas and Star Formation in Major Galaxy Pairs from the FAST All-Sky HI Survey (FASHI)
› A Slit Mask Integral Field Unit for the Robert Stobie Spectrograph on the Southern African Large Telescope: I. Instrument Development
› SGR 1935+2154's Quiet Local Environment: Clues for Its Progenitor
› Sometimes You Just Can't Put a Ring on It: Setting Constraints on Rings around Moons from Magnetic Fields
› Enhancing cosmological constraints with nonlinear tanh transformations of Hermite-Gaussian Derivative fields
› Probing the Bias of Large-Scale Structure with Unlocalized Fast Radio Bursts
› The Fate of the Milky Way--Andromeda System: To Merge or Not?
› Orbital motion detected in gamma Cas Fe K emission lines
› Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge
› Extinction curves, extinction laws, and the failure of interstellar dust models
› How well does MAGPHYS recover galaxy properties? A test using EAGLE simulated star-forming galaxies
› MAGIC observations of NGC 4278. The first low-luminosity radio galaxy with compact jets detected at TeV energies
› 3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra
› Revisiting Constraints on Primordial Curvature Power Spectrum from PBH Abundances
› Low-Frequency Stochastic Gravitational-Wave Background in Gaia DR3 catalogue
› The time-delay model and its applications to galactic archaeology
› A High-frequency Geodetic VLBI Experiment for Optical Clock Comparison
› Anomalously Strong Localized First Ionization Potential Effect Associated with a Solar Subflare
› The Persistent Radio Sources and Multi-wavelength Counterparts of Fast Radio Bursts in Massive Binary Systems
› Intracluster light is a close tracer of the dark matter halo shape
› First Detection of the Glycine Isomer Glycolamide in Hot Molecular Core
› Unlocking accretion rate diagnostics for high-mass protostars using JWST/MIRI HI lines
› Identification of low redshift groups and clusters of galaxies in the X-CLASS survey and the X-ray luminosity-temperature relation
› Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging
› How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background
› Perihelion observations of interstellar comet 3I/ATLAS with the IRAM 30-m telescope
› Semi-cosmographic constraints on decaying dark matter and dynamical dark energy: DESI DR2 BAO and 21\, cm intensity-mapping forecasts
› Upper Limits to Long-Term Variability of Solar-Type Stars from Observations of the Open Cluster M67
› The Lyman-alpha Emission in Solar Flares. II. A Statistical Study on Its Relationship with the White-light plus Soft X-ray Emission
› Formation of spirals in early stage protoplanetary discs
› 3D CMZ V: A new orbital model of our Galaxy's Center, informed by data across the electromagnetic spectrum
› Signatures of localised particle acceleration at a global coronal shock wave
› Data-calibrated point spread function prediction: General description of the method and demonstration on MUSE-NFM
› Photometric and late-time spectropolarimetric observations of GRB 250129A afterglow
› An Opacity-Free Test of the Cosmic Distance Duality Relation Using Strongly Lensed Gravitational Wave Signals with Space-Based Detector Networks
› Investigating peculiar prompt emission properties of the multi-Peaked GRB 250129A
› Microlensing by Cluster of Primordial Black Holes
› Solving the Cosmic Coincidence Problem: The Locally Pumped Dark Energy Model
› Ca2+ transient detection and segmentation with the Astronomically motivated algorithm for Background Estimation And Transient Segmentation (Astro-BEATS)
› What does it take to have $N_{\rm eff} < 3$ at CMB times?
› Kinetic Isocurvature Perturbation
› Slow-down of expanding bubbles in the early Universe
› Inside the Black Box of Big Bang Nucleosynthesis: Parameter Sensitivity Studies in Light of new LBT Data
› Analyzing Fermionic Dark Matter scenarios with anomalous compact objects
› First measurements of deuteron production spectra in p+p collisions at beam momentum of 158 GeV/c at NA61/SHINE
› Wave-particle equilibria with heavy ions in weakly collisional space plasmas
› Dark graviton sensing with magnetically levitated superconductors
› $\beta$-decay Measurements Near the $N=40$ Island of Inversion to Quantify Cooling of Accreted Neutron Star Crusts
› Cosmic Ray Boosted Dark Matter in COSINUS: Modeling and Constraints
› Astrophysical aspects of string compactifications
› Dark Matter Detection through Rydberg Atom Transducer
› Discovery of a radio jet in the Cloverleaf Quasar at z = 2.56
› Millisecond Pulsars in Globular Clusters and Implications for the Galactic Center Gamma-Ray Excess
› Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620
› On the spatial distribution of luminous blue variables in the M33 galaxy
› A Potential Link between Nuclear Winds and Cold Gas Outflows on Kiloparsec Scales in Reionization-Era Quasars
› In the grip of the disk: dragging the companion through an AGN
› Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
› Cosmology in Extended Parameter Space with DESI Data Release 2 Baryon Acoustic Oscillations: A 2$\sigma$+ Detection of Nonzero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly
› On the unique evolutionary mechanisms of massive quiescent galaxies in the epoch of reionisation
› Dark Matter and Galaxy Cross-Correlations with the Cherenkov Telescope Array Observatory
› An SDSS-V 3D Tomographic Na I Map of the ISM: An Initial Study Towards the Smith Cloud
› Improved reconstruction of the century-long solar magnetic field by incorporating morphological asymmetry in sunspots
› Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
› GPU-Accelerated X-ray Pulse Profile Modeling
› Spin-Orbit Misalignments of Eccentric Black Hole Mergers in AGN Disks
› Effect of stochastic kicks on primordial black hole abundance and mass via the compaction function
› Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter
› Probing the wind and evolutionary state of the quiescent luminous blue variable Var$\,$2 in the Galaxy M33: constraints from self-consistent non-LTE modeling
› Evidence for Neutrino Emission from X-Ray-bright Active Galactic Nuclei with IceCube
› Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
› Searching for Exotrojans in Pulsar Systems
› Graph-Based Light-Curve Features for Robust Transient Classification
› Measuring cosmic dipole with the GRB luminosity-time relation
› It's always the quiet ones: Single Degenerate Double Detonation Type Ia Supernova from Quiescent Helium Accretion
› Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
› Prospects for Observing the Microquasar SS 433 with the LACT Array
› Equation-of-state-informed pulse profile modeling
› Searching Within Galaxies for the Earliest Signs of Quenching With Spatially Resolved Star Formation Histories in UVCANDELS Galaxies at z< 0.3
› The Scoured Spike: Suppression of Indirect Dark Matter Signals by a Hidden Companion
› Fast Radio Bursts from White Dwarf Binary Mergers: Isolated and Triple-Induced Channels
› The broad-lined type Ic supernova 2020lao experienced an energetic explosion with no central-engine signatures
› How Dark Sector Equations of State Govern Interaction Signatures
› Detection of 27 candidate circumbinary planets through apsidal precession of eclipsing binaries observed by TESS
› Stochastic gravitational-wave background search using data from five pulsar timing arrays
› Beyond Two Parameters: Revisiting Dark Energy with the Latest Cosmic Probes
› KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
› The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591
› Abundance of cosmic voids in EFT of dark energy
› A global view of post-interaction white dwarf-main sequence binaries
› Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes
› Cosmogenic 10Be as a Tracer for Recent Heliospheric Encounters with Interstellar Cold Clouds
› Time delay measurements with Broken Power Law model
› The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
› A redshift survey of the nearby galaxy cluster Abell 2199 : No upturn of the faint-end slope of galaxy luminosity function
› Searching for the Shortest-wavelength Aromatic Infrared Bands: No Evidence for the Predicted 1.05 $\mu$m Polycyclic Aromatic Hydrocarbon Feature
› Revisiting CPL with sign-switching density: To cross or not to cross the NECB
› The impact of strong lensing on Hubble constant measurements with gravitational-wave dark sirens
› Bridging the Prandtl number gap: 3D simulations of thermohaline convection in astrophysical regimes
› The Stellar Mass Function for Nine Massive Galaxy Clusters in the Local Universe
› A hot, nebular-dominated galaxy interacting with a pristine PopIII system uncovered by JWST
› Identifying AGNs from X-ray detections-I: Metallicity calibrations in AGNs with X-ray luminosity as the primary input parameter
› The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6
› Searching for Fast Astronomical Transients in Archival Photographic Plates
› A turbulence index independent framework for deriving solar wind speed and coronal electron density from radio spectral broadening
› Parallel adaptive reweighting importance sampling for Bayesian astrophysics
› The full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT
› Little Red and Blue Dots: simply stratified Broad Line Regions
› Detecting light dark matter with prompt-delayed events in neutrino experiments
› Time as a test-field: the no-boundary universe in motion and a smooth radiation bounce
› Gravitational waves from supermassive right-handed neutrinos produced at preheating
› Anomalous Dynamical Screening of Relativistic Plasma in a Magnetic Field
› The tidal response of a relativistic star
› Structure Formation with Dark Magnetohydrodynamics
› astroCAMP: A Community Benchmark and Co-Design Framework for Sustainable SKA-Scale Radio Imaging
› Shocks, compressible perturbations, and intermittency in the very local interstellar medium: Voyager 1 and 2 observations and numerical modeling
› Detection prospects of solar $g$-modes with LISA

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