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Obserwatorium Astronomiczne na Suhorze

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Kamerka S

Kamerka N

Niebo
Temperatura
8.3 °C
Wilgotność
54%
Wiatr
9.7 km/h
Ciśnienie
1019.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Uncertainty-Aware Solar Flare Regression ›
The Cluster Evolutionary Reference Ensemble at Low-$z$ (CEREAL) Sample of Galaxy Clusters I: X-ray Morphological Properties and Demographics ›
Thermalization of Neutrinos in a Neutron Star Merger Simulation ›
Enhanced Neutrino Cooling from Parity-Doubled Nucleons in Neutron Star Cooling Simulations ›
The Binary Populations of Stellar Streams are Set by Cluster Dynamics ›
A differentiable and optimizable 3D model for interpretation of observed spectral data cubes ›
Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints ›
BICEP/Keck XXI: Constraints on Early-Universe Parity Violation from Multipole-Dependent Birefringence ›
Caught in the web: galaxy mergers along cosmic filaments ›
On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints ›
Study of UV line and continuum variabilities in the Broadline Seyfert 1 Galaxy ESO 141-G55 ›
Empirical signatures of velocity and density cascades in the Local Universe probed by CosmicFlows4 dataset ›
A clean broad iron line in GS 1354--64 as seen by XRISM ›
Estimating the completeness of the QUBRICS Survey with 3501 QSO redshifts from Gaia DR3 spectra ›
Isotopic Evidence for a Cold and Distant Origin of the Interstellar Object 3I/ATLAS ›
Imaging the disk-halo interface of NGC 891: a 2.7 kpc-thick molecular gas disk ›
Different polarized components of the quasar 3C 286 revealed by FAST ›
Effect of gravity-driven longitudinal flows in filaments on angular momentum transport to embedded cores ›
Multi-wavelength ALMA Imaging of HD 34282: Dust-trapping Signatures of a Vortex Candidate ›
Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation ›
A Direct View of the Chemical Properties of Water from Another Planetary System: Water D/H in 3I/ATLAS ›
Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission ›
New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity ›
Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC ›
Supernovae interacting with Si and S-rich circumstellar matter from double white dwarf mergers ›
Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor ›
The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers ›
A Delayed Radio Flare Traces Kinetic Energy Injection in the SMBHB Candidate SDSS~J143016.05+230344.4 ›
Polarimetric Tomography Applied to Synthetic Multi-Spacecraft White-Light Images: Observing Coronal Mass Ejections in 3D ›
Fuzzy Dark Matter and the Impact of Core-Halo Diversity on Its Particle Mass Constraints ›
High nitrogen and carbon isotopic ratios in the interstellar comet 3I/ATLAS ›
Understanding the formation and eruption of sigmoidal structure through data-driven modeling of magnetic evolution in solar active region 13500 ›
To What Extent Are Star Cluster Ages Encoded in Their Environments? Exploring the Spatial Distribution of Age-Related Information with PHANGS-HST Imaging and Convolutional Neural Networks ›
Flip-flop states in X-ray binaries and changing-state AGN ›
Broadband SETI: a New Strategy To Find Nearby Alien Civilizations ›
A Reproducible Black Hole-Neutron Star Merger Gallery Example for the Einstein Toolkit ›
Forecasting Catastrophe: Constraints on the Fomalhaut Main Belt Planetesimal Population from Observed Collisional Remnants ›
Study of the cosmological tensions and DESI-DR2 in the framework of the Little Rip model ›
Catching TeV emission from GRB 221009A and alike with LHAASO, LACT and SWGO ›
New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences ›
A jet formation model for astrophysical objects ›
An Attempt to Search for Unintended Electromagnetic Radiation from Starlink Satellites with the 21 Centimeter Array: Methodology and RFI Characterization ›
WD 1054-226 revisited: a stable transiting debris system ›
Hydrogen photoionization in a magnetized medium: the rigid-wavefunction approach revisited ›
Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets ›
Inefficiency of chiral dynamos in protoneutron stars and the early universe ›
Post-perihelion Coma Composition of the Interstellar Comet 3I/ATLAS from Optical Spectroscopy ›
BlackGEM observations of compact pulsating stars: Mode identification for the DOV PG 1159--035 using multi-colour photometr ›
Here Be SDRAGNs - Spiral Galaxies Hosting Large Double Radio Sources ›
Discovery of a 36-minute long-period transient ASKAP J142431.2-612611 ›
Symmetry-Protected Momentum Exchange between Dark Matter and Dark Energy ›
High-Energy Neutrino Emission in NGC1068 driven by Turbulent Magnetic Reconnection ›
The Average Age Map of the Galactic Bulge ›
Exploring the spin dependence on mass inclination and distance for the newly discovered black hole X-ray binary Swift J151857.0-572147 ›
Fine Structure and Formation Mechanism of a Sunspot Bipolar Light Bridge in NOAA AR 13663 ›
Structural Design and Performance Analysis of Laser Transmitting Telescope for Space Gravitational Wave Detection ›
K-DRIFT Science Theme: New Theoretical Framework Using the Galaxy Replacement Technique for LSB studies ›
Measuring the evolution of stellar bars with the host galaxy's spin ›
Identifying Red Supergiants in the Local Group Using JWST Photometry. I. NGC 6822, Sextans A, NGC 300, WLM, and IC 1613 ›
Pre-Virialized Assembly at Cosmic Dawn: The Dynamics and Extreme Ionization of Compact Group CGG-z7 at $z\sim7.04$ ›
Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance ›
s-process nucleosynthesis in low-mass AGB stars by the $^{13}$C($\alpha$,n)$^{16}$O neutron source ›
One Hundred Years of Venus Polarimetry: PICSARR Observations of the Phase Curves ›
Hydrocarbon complexity and photochemical shielding of prebiotic feedstock molecules in exoplanet atmospheres ›
A probable inside-out dwarf nova outburst from the period bouncer candidate ASASSN-25dc ›
Disc accretion onto a binary black hole in a hierarchical triple system as an origin of the most luminous hyper-soft sources ›
Compression-Driven Kinetic Instabilities in Magnetically Arrested Disks ›
A reaction-diffusion model for describing the ring/gap structure in disks surrounding individual young stars ›
Homogenization of the Stetson Photometry with the BEST Database ›
Double White Dwarf Mergers as Progenitors of Long-Period Transients ›
Robust ellipticity measurements of 29 Galactic globular clusters ›
How interacting winds shape the mechanical feedback of massive star clusters over millions of years ›
Extreme mass loss during common envelope evolution: the origin of the double low-mass white dwarf system J2102--4145 ›
Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE ›
Non-common path aberration compensation and a dark hole loop with a pyramid adaptive optics system: Application to SAXO+ ›
ML in Astrophysical Turbulence I: Predicting Prestellar Cores in Magnetized Molecular Clouds using eXtreme Gradient Boosting ›
Nonlinear evolution of unstable solar inertial modes: The case of viscous modes on a differentially rotating sphere ›
Gas chemistry in the dust depleted inner regions of protoplanetary disks. I. Near-IR spectra and overtones ›
Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactions ›
LeMMINGs VII: 5 GHz, 50 mas e-MERLIN observations of a statistically complete sample of nearby AGN ›
Systematic selection of surrogate models for nonequilibrium chemistry ›
Evolution and formation of ultramassive white dwarf stars: The case for a 9Msun progenitor ›
A GPU-Accelerated Transient Detection Pipeline for DECam Time-Domain Surveys ›
An Alternate Pathway for H$_2$ Formation in the Early Universe: A physical process to account for the presence and coevolution of the luminous galaxies and supermassive black holes at the high redshifts ›
Multimessenger Characterization of High-Energy Neutrino Emission from the Brightest Neutrino-Active Galactic Nuclei ›
Very High Energy Gamma Rays from Ultra Fast Outflows ›
Fundamental Limits of Quantum Sensors for Gravitational Wave Detection ›
Spectral sirens cosmology from binary black holes populations with sharper mass features ›
Low-Energy and Low-Thrust Exploration Tour of Saturnian Moons with Full Lunar Surface Coverage ›
Shadows and Polarization Images of a Four-dimensional Gauss-Bonnet Black Hole Irradiated by a Thick Accretion Disk ›
Gravitational waves from warm inflation in the weak dissipative regime ›
MMS Observations of Kinetic Alfv\'en Wave Turbulence and Steep Kinetic-Range Spectra in the Outer Plasma Sheet Boundary Layer ›
Local Origin of Hidden Symmetry in Rotating Spacetimes ›
Spatiotemporal Properties of Compressible Magnetohydrodynamic Turbulence from Space Plasma ›
A Deep Learning Framework for Amplitude Generation of Generic EMRIs ›
Black Hole Mergers as the Fastest Photon Ring Scramblers ›
Flash from the Past: New Gamma-Ray Constraints on Light CP-even Scalar from SN1987A ›
A Remarkably Accurate Predictor of Sunspot Cycle Amplitude ›
Quasi-steady emission from repeating fast radio bursts can be explained by magnetar wind nebulae ›
Revisiting the Chern-Simons interaction during inflation with a non-canonical pseudo-scalar ›
Chasing the light: Shadowing, collimation, and the super-Eddington growth of infant black holes in JWST broad-line AGNs ›
Dynamical reconstruction of SPARC galactic halos within self-interacting fuzzy dark matter ›
The cosmological Mass Varying Neutrino model in the late universe ›
Principal Components for Model-Agnostic Modified Gravity with 3x2pt ›
A machine-learning photometric classifier for massive stars in nearby galaxies II. The catalog ›
Symmetry in Fundamental Parameters of Galaxies on the Star-forming Main Sequence ›
Probing neutral outflows in z ~ 2 galaxies using JWST observations of Ca II H and K absorption lines ›
Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter ›
Empirical Calibration of Na I D and Other Absorption Lines as Tracers of High-Redshift Neutral Outflows ›
The JWST Spectroscopic Properties of Galaxies at $z=9-14$ ›
A Method for Testing Diffusive Shock Acceleration and Diffusion Propagation of 1-100 TeV Cosmic Electron with Multi-wavelength Observation of Geminga Halo and Pulsar Wind Nebula ›
Imprints of gravitational-wave polarizations on projected tidal tensor in three dimensions ›
Ly$\alpha$ visibility from z = 4.5 to 11 in the UDS field: Evidence for a high neutral hydrogen fraction and small ionized bubbles at z $\sim$ 7 ›
The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history ›
Dynamical Evolution of Quasi-Hierarchical Triples ›
Prospective constraints on dark energy from nanohertz individual gravitational wave sources ›
X-ray Transmission Through Photoionized Gas with Moderate Thomson Optical Depth ›
Nonlinear Independent Component Analysis Scheme and its application to gravitational wave data analysis ›
A Differentiable Surrogate Model for the Generation of Radio Pulses from In-Ice Neutrino Interactions ›
Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies ›
The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES ›
GroundBIRD Telescope: Systematics Modelization of MKID Arrays Response ›
Mapping CO Ice in a Star-Forming Filament in the 3 kpc Arm with JWST ›
CHRONOS: Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter ›
Constraining the strangeness enhancement scenario of the UHECR muon puzzle with LHC experiments ›
The SRG/eROSITA All-Sky Survey. Detection of shock-heated gas beyond the halo boundary into the accretion region ›
Clustering analysis of medium-band selected high-redshift galaxies ›
The anisotropic expansion rate of the local Universe and its covariant cosmographic interpretation ›
Covariant cosmography in the presence of local structures: comparing exact solutions and perturbation theory ›
The First Dedicated Survey of Atmospheric Escape from Planets Orbiting F Stars ›
Intrinsic alignment of disks and ellipticals across hydrodynamical simulations ›
A 3D Chemodynamical Census of Inner-Galaxy Metal-poor Giants to [Fe/H]~-3.5 ›
The Cosmic Baryon Cycle in IllustrisTNG: flows of mass, energy, and metals ›
Solar photospheric velocities measured in space: a comparison between SO/PHI-HRT and SDO/HMI ›
A Comparison of Galacticus and COZMIC WDM Subhalo Populations ›
Nominal thresholds for good astrometric fits, and prospects for binary detectability, for the full extended Gaia mission ›
The Challenge in Illuminating the Invisible: Constraining LyC Escape with Bayesian Modelling and Symbolic Regression ›
Grand Unification Higgs-$\mathcal{R}^2$ Inflation: Complementarity between Proton Decay and CMB Observables ›
Testing the cosmological Euler equation: viscosity, equivalence principle, and gravity beyond general relativity ›
Type Iax supernovae as a source of iron-rich silicate dust ›
Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon ›
Astrometric view of companions in the inner dust cavities of protoplanetary disks ›
Polarimetric and spectropolarimetric observations with FoReRo2: Instrument overview and standard star monitoring ›
The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations ›
Discovering gravitational waveform distortions from lensing: a deep dive into GW231123 ›
Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution ›
SN 2024abvb: A Type Icn Supernova in the Outskirts of its Host Galaxy ›
Mathematical Anatomy of Neutrino Decoherence in Red Turbulence: A Fractional Calculus Approach ›
Euclid preparation. Galaxy power spectrum modelling in redshift space ›
Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos ›
Statistical Validation and Photometric Characterization of the Hot Jupiter Candidate TOI 7475.01 ›
Euclid preparation. Impact of galaxy intrinsic alignment modelling choices on Euclid 3x2pt cosmology ›
Certified Uncertainty for Surrogate Models of Neutron Star Equations of State via Mondrian Conformal Prediction ›
New axion bounds derived from the 100-parsec Gaia DR3 white dwarf luminosity function ›
Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs ›
Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate ›
Simultaneous Misalignment and Mode Mismatch Sensing in Optical Cavities Using Intensity-Only Measurements ›
Explainable classification of astronomical uncertain time series ›
Simultaneously search for multi-target Galactic binary gravitational waves ›
General form for Pseudo-Newtonian Potentials, imitating Schwarzschild geodesics ›
Incorporating curved geometry in cosmological simulations ›
Cosmological Perturbation in New General Relativity: Propagating mode from the violation of local Lorentz invariance ›
Novel very-high-frequency quasi-periodic oscillations of compact, non-singular objects ›
Scattering of non-relativistic finite-size particles and puffy dark matter direct detection ›
Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors ›
Enhancing low energy reconstruction and classification in KM3NeT/ORCA with transformers ›
Apparent Phantom Crossing in Gauss-Bonnet Gravity ›
Gravitational Noether-Ward identities for scalar field ›
Kerr-Newman-de Sitter black holes in $f(R)$ gravity with constant curvature: horizon structure and extremality ›
Limits of vacuum-template subtraction for LISA massive black hole binary sources in realistic environments ›
New solution to the hyperon puzzle of neutron stars: Quantum many-body effects ›
Kinetic Route to Helicity-Constrained Decay ›
Using thermodynamics to learn gravitational wave physics ›
Modified Teukolsky formalism: Null testing and numerical benchmarking ↓↑