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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl
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› Satellite Metallicity Enhancement I: Suppressed Star Formation, Stellar Mass Loss, and Enriched Inflow of DESI and EAGLE Galaxies around Massive Clusters
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› Identification of Compact Groups of Galaxies in IllustrisTNG300
› The Peculiar Velocity of Messier~87 from Microarcsecond Geodetic VLBI Astrometry
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› Thirty Circumbinary Disk Occultation Systems (KH 15D-like stars) from the OGLE Project
› Wideband RFI Monitor Requirements, Design, and Commissioning at DRAO
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› Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters
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› The Status of Gravitational Vector Perturbations with Recent CMB Data
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› JWST observations and a model for the extremely luminous obscured quasar W2246-0526 at z=4.6
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› Bayesian Analysis of Massive Boson Star Models for Sagittarius A* Using Near-Infrared Astrometry Data
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› Challenges to the cosmological constant model following results from the Dark Energy Survey
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› Image Processing Framework for Eclipse Shadow Band Analysis
› A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588
› Cooling of Isolated Neutron Stars with Hyperon-mixed Kaon-Condensation Matter
› Small and Complex I: The Three Component Structure of $z \sim 0$ Massive Compact Quiescent Galaxies
› Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies
› Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations
› Validating Coronal Magnetic Field Models Using Gaussian Separation
› Numerical estimation of the capture ability of Neptunian mean motion resonances
› RAYTHEIA: A high-performance ray-tracing algorithm for three-dimensional direction-dependent equations in astronomical simulations
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› On the Problem of Prognostication of Bright Kreutz Sungrazers
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› Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events
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› STEPSIC: Initial condition generator for stereographic cosmological simulations
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› SAPLE: Swift Analysis Pipeline for Lightcurve Extraction
› Comparing Results from Two Uniform Phase Curve Surveys
› Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems
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› An agentic framework for gravitational-wave counterpart association in the multi-messenger era
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› DESI DR2 Galaxy Luminosity Functions
› Changing-Look AGN Powered By Disk Tearing
› A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy
› Comparing galaxy merger orbits in hydrodynamical simulation and in dark-matter-only simulation
› Tracing the Trace Anomaly of Dense Matter inside Neutron Stars
› Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows
› OzDES Reverberation Mapping of Active Galactic Nuclei: Final Data Release, Black-Hole Mass Results, & Scaling Relations
› Reaching diffraction-limited localization with coherent PTAs
› The abundance of thin dwarf galaxies: a challenge for cosmological simulations
› KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
› Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference
› Resolving the Core-Cusp and Diversity Problems with a Baryon-Correlated Dark Matter Profile
› Revisiting the Reported Period of FRB 20201124A Using MCMC Methods
› Possible evidence for a pair-instability supernova nature of ultra-early JWST sources
› New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
› Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics
› Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN
› The early r-process nucleosynthesis scenarios
› Impact of Rastall gravity on hydrostatic mass of galaxy clusters
› Rarity of rocket-driven Penrose extraction in Kerr spacetime
› Studying dark gaps in Ly-$\alpha$ forest transmission with large reionization simulations
› A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A
› Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
› Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts
› Large-scale and local environmental drivers of quenching: tracing H$\alpha$ concentration in X-ray and optical galaxy groups
› Inferring the population properties of galactic binaries from LISA's stochastic foreground
› Magnetic structure of coronal dark halos
› Variational views for self-supervised learning in radio astronomy
› Primordial Black Hole Formation in Rastall Gravity: Shifted Collapse Threshold and Exponential Abundance Sensitivity
› Inefficiency of chiral dynamos in protoneutron stars and the early universe
› Cosmological peculiar velocities in general relativity
› The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
› Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy
› Organosulfur Chemistry on sub-Neptunes: Implications for hazes and biosignatures
› Early emission characterization of TDE 2025aarm
› ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser
› Large-scale Morphology of the Optical F-corona from a Total Solar Eclipse Observation During the Artemis II Lunar Flyby
› Long-Term Dynamical Evolution and Ejection of Near-Earth Asteroids
› The apparent Large Magellanic Cloud star cluster age gap
› Sub-Neptunes Show a Stronger Correlation with Cold Jupiters than Super-Earths Especially in Metal-rich Systems
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› Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity
› A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications
› PySME v1.0: improved modelling of stellar spectra for survey-scale applications
› How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4
› On the origin of the environmental step: A BayeSN view of the ZTF SN Ia DR2
› String Thresholds, Dynamical Gauss--Bonnet Couplings, and Starobinsky Attractors
› Neutron Star Eclipses as Axion Laboratories
› Parameter inference of millilensed gravitational waves using neural spline flows
› How Many Times Should We Matched Filter Gravitational Wave Data? A Comparison of GstLAL's Online and Offline Performance
› New Methods for Offline GstLAL Analyses
› Inflation Model Based on Virasoro Squeezing
› Searching for dark photon dark matter from terrestrial magnetic fields
› Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
› Orbital dynamics and precession in magnetized Kerr spacetime
› Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look
› Boson Stars Hosting Black Holes
› Properties of Stable Massive Quark Stars in Holography
› Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model
› Curvaton-assisted hilltop inflation
› Cosmological long-wavelength solutions in non-adiabatic multi-fluid systems
› The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
› An approximate Kappa generator for particle simulations
› Effects of isovector spin-orbit interaction on the charge-weak form factor difference in $^{48}$Ca, $^{208}$Pb, $^{90}$Zr and $^{62}$Ni
› Searching for axions with time resolved pulsar polarimetry
› Preliminary study on the impact of stress-energy tensor compared to scalar field in Nonminimal Derivative model
› Outer-Crust Equations of State for Neutron Stars
› Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection
› Hadronic lensing
› Adaptive ray tracing, image diagnostics, and photon ring signatures of rotating dark-matter-dressed black holes

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