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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RSS  Najnowsze prace na astro-ph:

› Self-acceleration of Hardening Binaries
› Discovery of Quasar Variability and Early Accretion Disk Signatures at Cosmic Dawn
› Coverage is not enough: Frequentist tests of simulation-based inference for primordial non-Gaussianity
› Stellar mass and morphology segregation in pairs and multiplets in the cosmic web
› Merge and Strip II: Imprint of galaxy formation physics and viscosity on baryon-dominated dwarf galaxies
› On the isotropy of viscosity in accretion discs
› Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation
› NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way
› Implications of \textit{SARAS3} data for Coulomb-like interacting dark matter
› Recommendations for the Astronomy Graduate Admissions Process
› The complex history of NGC 1427A revealed by its star clusters and star formation history
› Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the far-Infrared in the Era of Next-Generation Radio Telescopes
› Non-uniform particle injection into black hole jets by radiative magnetic reconnection
› Neural Posterior Estimation for UHECR source inference from 3D propagation simulations
› A Coordinate System for Dynamical Instabilities in Hierarchical Systems in REBOUND
› Chemistry and Isotope Ratios of Substellar Atmospheres in the $\beta$ Pictoris Young Moving Group
› The Outer Space Treaty Won't Save Us From Ourselves
› Millimeter-wave Detections of Symbiotic Stars in SPT and ACT Data
› Formation and Redshift Evolution of Dark Matter Spikes
› Status of the COSmological Microwave Observations CALibrator
› Analysis of spatial velocities of several samples of open star clusters
› Validating z > 7.5 Lyman Break Galaxy candidates in the COSMOS field with JWST/PASSAGE
› Resolving the Unresolved Galactic Winds in Multi-phase Models. I. Methodology and Application
› Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI
› XRISM/Resolve observations of Hercules X-1: a pulsating, highly broadened Fe K emission line from the neutron star accretion column
› Statistically Significant Linear Alignments Among High-Confidence Transient Candidates on POSS-I Photographic Plates
› Type Ib Supernovae are bluer than Type Ic Supernovae
› Cross-Comparison of Galaxies Detected in the CSST Spectroscopic Survey and the SKA HI Survey
› A structural degeneracy explains reionization tensions and limits dark matter constraints
› The atmosphere of the warm Neptune GJ 436 b probed with ESPRESSO
› Black Hole Supernovae Outcomes Across a Wide Progenitor Range
› Powerful parametric instability of Alfven waves in astrophysical pair plasma
› Speckle Interferometry at SOAR in 2024 and 2025
› Non-Equilibrium Ionisation in Photoionised Haloes: Implications for Shock Stability and Absorption-Line Signatures
› On the Radial Evolution of the Solar Wind : The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations
› The Days Drag On on WASP-121 b: Interpreting its NIRISS Spectroscopic Phase Curve with General Circulation Models
› Zooming in on the GeV $\gamma$-ray flare of the blazar PKS 1725+123 with a multimessenger lens
› A Point-Spread Function for the Extreme Ultraviolet High-Resolution Imager on board Solar Orbiter
› MHD simulations on the large-scale propagation of high-speed solar wind streams
› A Short-timescale Negative Optical Continuum Lag in SDSS J083717.88+191647
› Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind
› Alleviating the Hubble Tension Using $\Lambda$sCDM Model: A Coupled Dark Energy - Dark Matter Interaction
› Constraints on Phenomenological Amplitudes of CMB Anisotropy with Multi-Datasets
› Radio Signature of Higher Atmospheric Meridional Flow and Implications for Magnetic Trees in the Sun
› On the Dust Substructures Triggered by Two Super-Earths Migrating in Low-viscosity Disks
› Constraints on Halo Gas Profiles from Joint kSZ and Galaxy Clustering Analysis of ACT DR6 and CMASS
› Cosmology since the first Astro/Cosmo Moriond meeting// The emergence of the Big Bang 2.0
› A Comprehensive Study of Morphology and Kinematics in Extended Nebulae Around UV Luminous Quasars at $z\approx1$
› 4HWC J2029$+$3641: a Pulsar Wind Nebula Powered by PSR J2030$+$3641?
› Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter
› The connection between solar coronal abundances and the underlying lower atmospheric properties
› Baryons in the Darkest Sites of the Universe
› Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations
› Probing the kinematics of FU Orionis objects through high-resolution near-infrared spectroscopy
› JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line
› CHANG-ES XXXIX. Magnetic field structure in edge-on galaxies: Stacking Stokes parameters
› Constraints for Nuclear Astrophysics from an Unusual Presolar Silicate-Oxide Aggregate Grain Found in Primitive Ordinary Chondrite Meteorite Hills 00526
› Revisiting the Rheology of Neutron Star Crusts with Molecular Dynamics
› Fragmentation in the Serpens/Aquila Star-forming Region
› Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2
› Beyond collective fluctuations: probing micro-image swarms in lensed quasars with intensity interferometry
› Hadronic Scenario for Galactic PeVatron LHAASO J1912+1014u Supported by Fermi-LAT $\gamma$-ray Data and FUGIN CO Data
› A Search for Variability of Ultracool Dwarfs with the Zwicky Transient Facility
› Low-luminosity Wolf-Rayet stars: a model-data comparison
› Mean tropical year length at arbitrary ecliptic longitude
› The first detection of an atmosphere on a trans-Neptunian object beyond Pluto
› The Impact of the Magnetised Cosmic Web on Ultra High Energy Cosmic Ray Propagation
› Design, Testing, and Commissioning of the Sun Yat-sen University (SYSU) 80 cm Infrared Telescope
› The chemical fingerprint of the Gaia BH3 system. Evidence for early cluster enrichment from the analysis of 51 elements
› Investigating cosmic distance duality and dark energy evolution through intermediate and high-z probes
› Modeling large glitches with core superfluidity in a Hybrid star
› Morphological and Star Formation Properties of Cosmic Noon Massive Quiescent Galaxies
› Unravelling the complex structure of the Fe II emission region in Type 1 active galactic nuclei
› Using Ly$\alpha$ Transmitted Spectrum to Probe IGM Transmission and Identify Ionized Structures in Cosmic Reionization
› Astrochemical Inheritance of Terrestrial Planets Water from Local Wet Silicates
› ENGRAVE follow-up of a type IIb supernova spatially coincident with the sub-threshold gravitational wave trigger S250818k
› A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XXI. Statistical properties of individual HII regions in perturbed galaxies
› Is XRISM/Resolve probing a "raining" absorber in Mrk 509?
› Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS
› Operating the Fabry-P\'erot systems of the European Solar Telescope in multi-aperture mode
› Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters
› Characterizing the bolometric-photoevaporative transition in young sub-Neptunes with radiation-hydrodynamic simulations
› JWST high-contrast spectroscopy with speckle modelling: Atmospheric retrievals of the T dwarf companion HD 19467 B
› Optical activity, orbital modulation, and broadband SED constraints for RX J1553.0+4457
› Outstanding Questions in Giant Planet Theory
› Chromospheric dynamics and the O I 135.6~nm spectral line
› A study of the kinematic and volumetric co-evolution of Earth-directed CMEs
› A Statistical Survey of Faint Solar X-ray Transients Observed by NuSTAR
› PDRS : A Linear $\mathcal{O}(N)$ Algorithm for Segmentation of High-Activity Regions in Irregularly Sampled Time Series
› Role of General Users in the Lifecycle of Scientific Software
› AGN STORM 2. XII. Ground-Based Optical Photometry and Lag Measurements of Mrk 817
› Foundations for Discovery: A Coordinated Fleet Approach to NASA Astrophysics
› Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias
› Wavelength-Dependent Evolution of Full-Field Transfer Matrices in Photonic Lanterns
› Bounds on massive graviton-like particles from searches for axion-like particles coupling to photons
› Observations of Atmospheric Helium and Oxygen with SPHEREx
› Series solutions to the TOV equations
› Three-flavor supernova neutrino simulation using a hybrid quantum-classical algorithm with qutrits
› Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333
› Scalar-Electromagnetic Couplings as Source of Deformed Black Hole: From Shadows to Thermodynamic Topology
› Pole Structure of Kerr Green's Function
› Reviving Motivated Inflationary Potentials with $K$-inflation in the light of ACT
› Spinning charged test particle dynamics around a Schwarzschild black hole embedded in a homogeneous magnetic field
› Helicity-dependent corrections to black-hole shadows from the gravitational spin Hall effect
› Distributions of particles accelerated by strong Alfv\'enic turbulence
› Testing General Relativity Through Gravitational Wave Classification: A Convolutional Neural Network Framework
› Hadronic lensing
› MPI-Rockstar: a Hybrid MPI and OpenMP Parallel Implementation of the Rockstar Halo finder
› Non-minimally coupled gravity constraints from DESI DR2 data
› Observational Insights on DBI K-essence Models Using Machine Learning and Bayesian Analysis
› Geometric Cosmology models: statistical analysis with observational data
› NASA Exoplanet Exploration Program (ExEP) Science Gap List
› CONCERTO: forward modeling of interferograms for calibration
› Is the Peculiar Galactic Center Transient Swift J174610.4-290018 A Nova Outburst?
› XRISM/Resolve observations of Hercules X-1: vertical structure and kinematics of the disk wind
› Combining spectral analysis and narrow band pass filtering to predict solar cycle parameters in the next solar grand minimum
› ExTraSS: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients
› Emission line models for the lowest mass core-collapse supernovae -- II. 3D NLTE radiative transfer modelling of a $9.0\,M_\odot$ neutrino-driven explosion
› Constructing Earth Formation History Using Deep Mantle Noble Gas Reservoirs
› Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
› A universal scaling law for gravitational waves induced during inflation
› BeppoSAX-WFC catalog of fast X-ray transients
› The Intermediate-Mass Black Hole Reverberation Mapping Project: Stable Optical Continuum Lags of an IMBH in the Dwarf Galaxy NGC 4395 Over Years
› Evolution of Mean Orbital Spacing in Planetary and Satellite Systems under Tidal Dissipation and Nebular Drag
› The r-Process: History, Required Conditions, Astrophysical Sites, and Observations
› The JWST EXCELS survey: The ages and abundances of $3
› Helium superluminous SN 2021bnw : an explosion of a massive star with a pre-outburst
› A broadband search for coherent radio emission in cataclysmic variables
› Unexpectedly Weak General Relativistic Effects in Strongly Relativistic Tidal Disruption Events
› A user-friendly package and workflow for generating effective homogeneous rheologies for the study of the long-term orbital evolution of multilayered planetary bodies
› Redshift Dipoles from Non-Geodesic Observer Congruences in Covariant Cosmology
› Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star
› How Overmassive Black Holes Formed at Cosmic Dawn
› Eppur non si trovano Vol. 2: No Planetary-mass Primordial Black Holes toward the Andromeda Galaxy
› Stochastic problems in pulsar timing
› Kozai-driven mass loss of the circumbinary disk in D9 in orbit around the supermassive black hole Sgr A*
› Sub-Neptunes as Soot Factories: Deep Atmosphere Hydrocarbon Formation and Quenching as the Origin of Sub-Neptune Aerosol Trends
› Plate Sensitivity Is Invariant Across Geomagnetic Storm Intensity at Harvard and Palomar: A Protocol for Artifact Control in Historical Plate Archive Studies
› The Leiden/ESA Astrophysics Program for Summer Students (LEAPS)
› First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST
› A graph-based Neural Network surrogate model for accelerating semi-analytical model of galaxy formation and evolution
› The Tracking Tapered Gridded Estimator for the 21-cm power spectrum from the Murchison Widefield Array (MWA) drift scan observations -- III. Improved upper limits at $z = 8.2$ from multiple pointings
› Quantum Parity Detectors: a qubit based particle detection scheme with meV thresholds for rare-event searches
› DIPLI: Deep Image Prior Lucky Imaging for Blind Astronomical Image Restoration
› Mass and distance of AGN black holes from warped accretion disks
› Stripped-Envelope Supernovae for QCD Axion Detection
› Non-Thermal Production of Sexaquark Dark Matter
› Plotting correlated data
› Kinetic Route to Helicity-Constrained Decay
› Measuring Primitive Accumulation: An Information-Theoretic Approach to Capitalist Enclosure in PIK2, Indonesia
› Conventional and Unitarity-Conserving Peccei-Quinn Inflation Models and ACT

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