Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› Relacja ze Spaceshield Hack 2026 – kosmiczny hackathon prosto ze Stalowej Woli
› Astronomowie znaleźli najsilniejsze dowody na istnienie pól magnetycznych egzoplanet
› Kosmiczny przegląd miesiąca AstroNETu – maj 2026 roku
› Niebo w czerwcu 2026 roku
› Wybuch New Glenna podczas testu – Blue Origin apeluje o zbieranie szczątek
› Dalekie ekspozycje w astrokrajobrazie
› NASA przedstawiła szczegóły planów bazy księżycowej – w tym 3 nowe misje
› Creotech udostępnił strategię rozwoju na nadchodzące lata
› Starship IFT-12 poleciał: czy to krok SpaceX w stronę Księżyca?
› Masywne gromady gwiazd szybciej rozpraszają otaczające je obłoki gazowe
RSS  Najnowsze prace na astro-ph:

› Hybrid stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$
› Systematic Polarization Errors from Parallactic-Angle Dependent Leakage in Pseudo-Circular Feeds
› Enabling tomorrow's planetary defence and space resource economy: Autonomous fleet-based asteroid rendezvous missions
› A Steep-Extinction QSO at z=4.6: JWST Evidence for Abundant Small Dust Grains
› Euclid: Disky titans -- surprisingly high star formation efficiency in two brightest group galaxies at $z\sim 0.75$
› NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$
› Systematic Error in Approximate Models of the GRB Early Afterglow
› The Role of Stellar Spin in Repeating Partial Tidal Disruption Events
› HERMES: HiERarchical Modelling for Exoplanet Science
› Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions
› A New Record Census of Dwarf AGN and a Bimodal $M_{\rm BH}$-$M_{\star}$ Scaling Relation with DESI DR1
› The Life and Death of Stars That Capture Primordial Black Holes
› Euclid: Early Release Observations -- Internal kinematics and the convective-transition gap of NGC 6397
› A Massive Hot-Jupiter Companion that Disfavors Giant Planet Formation Beyond the Water-Ice Line
› Lyman-alpha Pressure Strongly Enhances Pre-Supernova Feedback at Cosmic Dawn: The First Multi-Dimensional Lyman-alpha Radiation Hydrodynamics Simulations
› Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
› The Radio-IR Correlation in the Context of Deep Radio Source Counts
› Beyond Self-Similarity: Reconciling X-Ray Scaling Relations in Galaxy Clusters and Groups
› A Cosmic Archipelago of lensed metal-poor galaxies at $z\sim6$
› Can current models predict the local black hole merger rate?
› Accretion of Primordial Black Holes in Stellar Interiors
› The effects of yields from binary massive stars as functions of metallicity
› Precision constraints on stellar physics from main sequence detached eclipsing binaries
› Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet II: radiative discs and observational signatures
› Signature of Bursty Star Formation in the High-Redshift Galaxies Detected with JWST
› Bridging the UV Gap: The HST Ultraviolet Foundation for Star Formation Science in the Era of Roman, Euclid, and HWO
› Elemental cosmic ray spectra reveal two populations of Galactic sources and an immediate transition to an extragalactic component after the knee
› Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass
› One Transit Is All You Need: Detecting Exoplanets Through Learned Stellar Behaviour with EXOVEIL
› Neutrino Fingerprints: Image-Based Encodings of IceCube Events for CNN Direction Reconstruction
› Topology of molecular clouds in the PHANGS-JWST catalogue in relation to the physical characteristics of their galaxies
› First Detection of HC5N in a Class II Disk around TW Hya
› Nereid as a Regular Satellite of Neptune
› A High-Bandwidth Backplane for Wideband Radio Interferometers and Integration with the CHORD Telescope Correlators
› The mass of the neutron star in 4U 1820-30 revisited
› Field-level constraints on cosmic birefringence with a hybrid $E$-$B$ internal linear combination
› Data-Driven Forecasting of three-Component Seismograms Using Transformer Architectures
› On a re-examination of neutron star cooling in transient sources -- No shallow heating required?
› Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements
› Dust On, Dust Off: HST Observations of the Newly Dormant Jupiter Co-orbital Comet P/2023 V6 (PANSTARRS)
› A $z \sim$ 6.2 Quasar on the Local M$_{\rm BH}$-$\sigma_{\rm \ast}$ Relation Quenching Its Host Galaxy from the Aether Survey
› Comprehensive Analysis of Optical brightness and Color Variability of Blazars in the ZTF Survey DR22
› Fifty years of primordial helium abundances: A statistical reanalysis
› COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
› A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43
› Detection of a four-carbon sugar in interstellar space
› Deficit of primordial Li7 and primordial black holes
› The caustic method applied to The Three Hundred: prospects for upcoming CATARSIS and other surveys
› Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation
› Self-interacting neutrinos in cosmological perturbation theory -- integrating the collision kernel
› Hidden-sector accretion and warped black-string seeds for high-redshift supermassive black holes
› A comprehensive Rossiter-Mclaughlin Modelling Framework in TLCM: Application to HD 2685 $=$ TOI-135 system
› The UV Side of Little Red Dots: Red, Compact, and Iron-Enhanced Rest-UV Emission with a Strong Downturn around Ly$\alpha$
› Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes
› The Gaia GSP-Spec catalogue of interstellar extinctions, and stellar luminosities, radii, and masses
› Temperature-programmed desorption of SO2 from water ice surfaces: Adsorption energy distributions
› Taxonomy of High Mass X-ray binaries from a historical perspective
› Acenaphthene Derivatives as Signatures of C$_{11}$H$_9^+$ Reactivity with Methylated Naphthalenes
› An analysis of the Type Ia SN 2024gy and a comparison of different host extinction estimation techniques
› Varstrometry for Off-nucleus and Dual sub-Kpc AGN (VODKA): Radio Classification of High-Redshift Dual AGN Candidates with the Very Large Array
› Multimodal Transformer Based Generic Mixture Density Network for Scattering Timescale Estimation of Fast Radio Bursts
› Probing the Variation of the Inner Surface-Brightness Profile of Nuclear Star Clusters on the Intermediate-Mass Black Hole Mass Measurements Using Mock Observations of ELT/MICADO and HARMONI
› Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays
› Systematically Measuring Ultra-Diffuse Galaxies. IX. A Gyr in the Life of Nearby Low Surface Brightness Galaxies
› Constraining AGN accretion physics with black hole mass-luminosity scaling relations
› Astrophysical Constraints on Color-Superconducting Gap and N$^{3}$LO Perturbative-QCD Constant $c_0$
› Constraining Scale-Dependent Growth in $f(R)$ Gravity with Future 21 cm Surveys
› J0404+1112: A 3-Hour Eclipsing White Dwarf-Brown Dwarf Probing Multiple Atmospheric Regimes
› KRONOS I: The $1{-}2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
› The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6
› Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors
› GraphShed: a parameter-free Graph-based waterShed group finder
› The CRIMSON survey I: super-stellar SiO in the directly imaged companion TWA 5 B from high-resolution M-band spectroscopy
› A Previously Underexplored Regime in TESS: Minute-Scale Eclipses Reveal Ten White Dwarf-Cool M-Dwarf Binaries
› Biased tracers, Hybrid Effective Field Theory and Modified Gravity
› Suppressed diffusion and gamma-ray emission from the Cygnus Bubble
› Longitudinal Development Analysis of Extensive Air Showers Using CORSIKA Simulations
› The VMC survey -- LV. The coherent expansion of the SMC
› Spectral Handling and Estimation of AGN Parameters (SHEAP), The first AGN fitting GPU-based code
› The OAD Flagship Ecosystem
› Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability
› Teleocosmology and quantum post-selection
› First results of a high sensitivity and transportable Ring Laser Gyroscope
› Inverse energy transfer in decaying MHD turbulence: A shell-to-shell analysis
› On-Shell Bootstrap of Loop Inflation Correlators with Spectral Dispersion
› Thermal Metastable Strings in One-Scale Models and Gravitational Waves
› Quintessential $\alpha$-attractors fit DESI
› Deconstructing the Extra-Dimensional Axion
› Probabilistic Microcausality in a Thermal Bath of Gravitons
› The decay rate of metastable cosmic strings beyond the thin-string approximation
› Lorentz-violating signatures in quasi-periodic oscillations from a magnetised Kalb-Ramond black hole
› Model-Independent Search Discards Faint Lensed-Pairs of Gravitational Wave Events in the Sub-Threshold Candidates of GWTC-4
› Gravitino Freeze-In Dark Matter with an Additional Scalar Field
› Signatures of Ultralight Dark Matter in Space-Based Laser Interferometers
› Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068
› Velocity space origins of pressure-strain interaction in multi-population distributions and its application to magnetic reconnection
› The Broadband X-ray Spectral Properties during the Rising Phases of the Outburst of the New Black Hole X-ray Binary Candidate Swift J1727.8-1613
› ler: LVK (LIGO-Virgo-KAGRA collaboration) event (compact-binary mergers) rate calculator and simulator
› The Large Smooth Patch on Comet 9P/Tempel 1: Remnant of a Recent Past Event
› gwsnr: A Python package for efficient signal-to-noise ratio calculations of gravitational waves
› A recoiling supermassive black hole in a powerful quasar
› New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
› Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer
› Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
› KID Detector Readout Electronics Development for Habitable Worlds Observatory
› Southern massive stars at high angular resolution. Physical separations and mass ratios
› The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth
› Stacking transmission spectra of different exoplanets
› Large-Scale Structure Probes of the Post-Inflationary Axiverse
› Episodic Star Formation -- I. Overview and Scatter of the Star-Forming Main Sequence
› Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
› Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars
› Joint Optical-HI mock catalogues and prospects for upcoming HI surveys
› Uniform models of neutron and quark (strange) stars in General Relativity
› One-Loop Tensor Power Spectrum from a Non-Canonical Spectator Field during Inflation
› Captured are circularized: A relativistic treatment of extreme mass ratio inspirals crossing accretion disks
› Validating Digital Twins of the Local Universe with the Thermal Sunyaev-Zel'dovich Signal
› Constraining reionization morphology and source properties with 21cm galaxy cross-correlation surveys
› Skewness in the Hellings-Downs curve
› A model-independent measurement of the Hubble constant from gravitational-wave standard sirens and electromagnetic observations
› The impact of cosmic filaments on starburst galaxies across cosmic times
› MXDFz4.4: A LyC emitter 250Myr after the epoch of reionization and a first test of Ly-alpha morphology as a tracer of LyC escape at high redshift
› Mock Catalogs of Strongly Lensed Gravitational Waves via A Halo Model Approach with Ground-based Detectors
› Spectroscopic galaxy redshifts in the Peanut cluster -- a massive nearly head-on cluster merger shortly after pericenter passage
› FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology
› Warm Inflation Beyond the Markovian Limit
› Type Ia supernovae interacting with a close circumstellar material (SNe Ia-CSM) are SNe Ia inside planetary nebulae (SNIPs)
› SLSim: a strong lensing population simulation package
› The ALMA-QUARKS survey: Investigating Thermal Feedback of Massive Protostars in Hot Molecular Cores
› X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state
› POSEIDON II: The Anti-Aligned Orbit of the Warm Neptune TOI-1710 A b
› cuRAMSES: Scalable AMR Optimizations for Large-Scale Cosmological Simulations
› A Search for Wide-orbit Planets Around M-dwarfs using Deep MIRI 15-micron Images
› JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust
› A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling
› UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space
› Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus
› Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts
› The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations
› Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys
› Constraints on Dynamical Dark Energy from Multiple Probes in the Full Dark Energy Survey
› Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply
› Multi-Scale Magnetic Field Observations Reveal how Colliding Flows Trigger Star Formation
› Interstellar Scintillation of Three Nearby Pulsars with FAST
› Is the Dark Comet 1998 KY$_{26}$ the Spacecraft Phobos 1?
› A study of the Physical Properties and Star Formation Activity of a Large Sample of Molecular Clouds: I Distances
› Local relaxation and scale-dependent alignment in compressible, magnetized turbulence
› Towards holographic color superconductivity in QCD
› Exceptional Lines and Excitation of (Nearly) Double-Pole Quasinormal Modes: A Semi-Analytic Study in the Nariai Black Hole
› Eigenmodes in an ultra-relativistic ultra-magnetized pair QED-plasma
› Light rings, gravitational lensing, and ISCOs of exotic compact objects in Einstein-scalar-Maxwell theories
› Intrinsic Nonlocality of Spin- and Polarization-Resolved Probabilities in Strong-Field Quantum Electrodynamics
› Theoretical and Observational Bounds on Dynamical Chern-Simons Gravity as an Effective Field Theory
› Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment
› The structure of multi-axion solutions to the strong CP problem
› Dynamic Alignment as a Statistical Survival Effect
› Predictive radar tracking reveals >500 mV/m electric-field transients during the May 2024 superstorm

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