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Obserwatorium Astronomiczne na Suhorze

Teleskop

Chmury

Opady

Niebo
Temperatura
14.4 °C
Wilgotność
47%
Wiatr
8.0 km/h
Ciśnienie
1003.0 hPa

Księżyc
Najnowsze prace na astro-ph:
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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 ↓↑