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Obserwatorium Astronomiczne na Suhorze

Teleskop

Kamerka S

Kamerka N

Niebo
Temperatura
-1.6 °C
Wilgotność
94%
Wiatr
0.0 km/h
Ciśnienie
1023.6 hPa

Księżyc
Najnowsze prace na astro-ph:
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High Resolution VLA Radio Observations of the Boomerang Pulsar Wind Nebula ›
X-Shooting ULLYSES: Massive stars at low metallicity XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds ›
ALMA Central Molecular Zone Exploration Survey (ACES) II: 3mm continuum images ›
The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6 ›
Dynamical friction on binary stars in dark matter dominated environments ›
Little Red Dots: One Photometric Tag Concealing Diverse Spectroscopic Flavors of Massive Star Formation and Black Hole Activity ›
Cloaking Cosmic Light ›
The origin of isolated millisecond pulsars in globular clusters ›
Galactic Center Gamma-Ray Excess from a Generic Triaxial Halo ›
The First Systematic Survey of Stellar Halos in High-Inclination Galaxies Reveals Unusually Quiescent Merger Histories of Nearby Galaxies ›
ALMA Central molecular zone Exploration Survey (ACES) VI: ALMA Large Program Reveals a Highly Filamentary Central Molecular Zone ›
Willman 1 Revisited: The Kinematics, Chemistry, and Orbital Properties of a Potentially-Disrupting Dwarf Galaxy ›
ALMA Central molecular zone Exploration Survey (ACES) III: Molecular line data reduction and HNCO and HCO$^{+}$ data ›
Neural Bayesian updates to populations with growing gravitational-wave catalogs ›
Planet formation at the inner edge of the dead zone -- I: the interplay between accretion outbursts and dust growth ›
Compute System Organization for High Frequency High Order Wavefront Sensing and Control ›
Evidence for Sympathetic Flaring in TESS Data ›
BASS LVI. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances ›
Inspectorch: Efficient rare event exploration in solar observations ›
Quasars behind the disk of M31 galaxy ›
ALMA Central Molecular Zone Exploration Survey (ACES) I: Overview ›
An automated activity classification tool for optical galaxy spectra ›
Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO ›
Cosmological Constraints on Neutrino Masses in Quintessential Inflation ›
First Observation of CO$_2$ Emission and foreground absorption Toward the Galactic Center with JWST ›
A Census Before Rubin of Asteroid Families in the Main Belt ›
Glance: A Comprehensive Framework for Galactic Archaeology ›
Spatially-resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA2 ›
Constraining the Sub-Galactic Relationship Between Star Formation and the Hot Interstellar Medium in NGC 4254 ›
Stellar flare study of nearby young moving group members with TESS Data ›
Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging ›
IR-Safe and IR-Resummed Bispectra Before and After Reconstruction in Unified Lagrangian Perturbation Theory ›
Chandra X-ray Observations of Quasars with Velocity-Offset Broad Lines: Assessing the Binary Supermassive Black Hole Hypothesis ›
ALMA Central Molecular Zone Exploration Survey (ACES)-IV. Data of the two intermediate-width spectral windows ›
Detectability of Satellite Planes in Mock Observations of Isolated L* Galaxies ›
Evolution of Spatial Complexity in Flare Ribbon Substructure and Its Relationship to Magnetic Reconnection Dynamics ›
Introduction to Strong Alfv\'enic MHD Turbulence ›
Machine-learning cosmological parameters by eROSITA data ›
Formation of dusty clumps in the torus of active galactic nuclei ›
Search for Light-Mass Fractionally Charged Particles in Space with DAMPE Experiment ›
ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH? ›
AT 2024wpp: the most luminous fast-evolving optical transient linked to the merger explosion of a black-hole binary ›
Capture and Stability of Resonant Planet Pairs in Turbulent Disk ›
Rotation of a Solar Jet Driven by Plasma Flow along Helical Magnetic Fields in an Active Region ›
Constraining the onset height of coronal mass ejection driven shocks using near-Sun observations in visible and radio wavelengths ›
70 years of spectroscopy of the photosphere and the solar chromosphere at the Pic du Midi Observatory (1956-2026) ›
PLATOSpec's first results: Three new transiting warm Jupiters from the WINE survey TIC 147027702, TIC 245076932 and TIC 87422071 ›
Infall onto the Protoplanetary Disk during the Gravitational Collapse of a Molecular Cloud ›
Formation of first star clusters under the supersonic gas flow -- III. Environmental trends and halo-to-halo scatter in the Pop III IMF ›
Multiple protostellar outflows from a single protostar with a misaligned disk ›
F10.7 Index Prediction: A Multiscale Decomposition Strategy with Wavelet Transform for Performance Optimization ›
Galaxy evolution in the cosmic web: the relative impact of nodes and filaments in the EAGLE simulation ›
Bypassing the Lyth Bound with Entangled Gravitons: Primordial Signatures and Late-Time Noise ›
Evidence of a non-equipartition energy regime in 1803+784 Core-shift and Faraday rotation measurements from simultaneous multi-frequency polarimetric VGOS observations ›
Long-term optical variability of high-mass X-ray binaries. III. Polarimetry ›
SN 2024abvb: a Type Ibn/Icn supernova with evidence of helium and an extreme offset from its host galaxy ›
A multi-wavelength study of nearby starburst galaxy M 82 ›
Cylindrical cosmological simulations with StePS ›
Photosynthetic exergy I. Thermodynamic limits for habitable-zone planets ›
Infrared spectropolarimetry of a C-class solar flare footpoint plasma -- I. Spectral features and forward modelling ›
Characteristics of natural remanence records in fine-grained particles returned from asteroid Ryugu ›
Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources ›
Stellar structure, magnetism and the variational principle ›
Revisiting the Geminga halo at GeV energies with Fermi-LAT data ›
A Salpeter IMF and an NFW halo: Disentangling the dark and stellar mass through precise lens modelling of a double-source-plane system reinforces the canonical model of elliptical galaxies ›
The Magnetic Filling in MAD Simulations and its Impact on the Jet in M87 ›
XRISM Discovery of Multiple Ionized Fe-K Emission and Absorption Components in Centaurus A ›
Gaia Data Release 4: Modelling of drift-scan related effects in Gaia's point spread function ›
Constraints on CMBR flux due to high-z dust emission ›
Relativistic Dissipative Magnetohydrodynamics from the Boltzmann equation for 2-particle species gas ›
Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare ›
Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies ›
Black hole-Neutron star distinction based on long-term MAXI and Swift study of 42 low mass X-ray binaries ›
Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections ›
Molecular bipolar outflow in SN 1987A supports the jittering-jets explosion mechanism ›
HINORA II: Testing the Existence of the Council of Giants in {\Lambda}CDM simulations ›
A Catalog of 486 Barium Stars Identified in GALAH DR4 ›
The hybrid Nova Vul 2024 (=V615 Vul) ›
Simulations of the 21cm emission line for upcoming large-scale HI galaxy surveys ›
The no-hair theorems at work in the tidal disruption event AT2020afhd ›
MHD Simulations of Strongly Magnetized HII Region Evolution: Evidence for Ionized Gas Filamentation ›
Experimental and computational studies of the hydrogenation of carbon disulfide (CS2) on ice analogues ›
RAMSES-MCR: A consistent multi-group treatment of cosmic rays physics in momentum-space with the RAMSES code ›
Revisiting CPL with sign-switching density: to cross or not to cross the NECB ›
Scattering, Migration, Re-circularization and Relaxation to Build Out Galaxy Disks with Exponential Profiles ›
The JWST Resolved Stellar Populations Early Release Science Program. IX. The RR Lyrae Population in WLM with HST and JWST ›
Physical Predictions in Closed Quantum Gravity ›
Cosmic Ray Spectra and Metal Budget Regulated by the Galactic Wind ›
Likelihood-Based One-Class Scoring in CWT Latent Space for Confusion-Limited LISA Gravitational-Wave Detection ›
Linking Leptogenesis and Asymmetric Dark Matter: A Testable Framework for Neutrino Mass and the Matter-Antimatter Asymmetry ›
Warm dark matter from freeze-in at stronger coupling ›
Unitarity violation and restoration in radiative bound-state formation ›
Spontaneous particle creation by oscillating compact stars ›
A strongly hyperbolic viscous relativistic hydrodynamics theory with first-order charge current ›
Electromagnetic Radiation from Cosmic-Ray Scatterings on Relic Neutrinos ›
Complex Inflaton Potentials with Nonminimal Coupling: Robust Inflation and Geometric Reheating ›
Thermodynamic Gravity with Non-Extensive Horizon Entropy and Topological Calibration ›
Range Emulator: A Compact Paraxial Optical System to Emulate Long-Distance Monochromatic Laser Propagation ›
Accurate transition and hyperfine data in Ag I from Multiconfiguration Dirac-Hartree-Fock and Relativistic Coupled-Cluster methods ›
Gravitational wave radiation from periodic orbits in regular black holes ›
5PN eccentric waveforms for intermediate-mass-ratio-inspirals (IMRIs) from post-Newtonian and black hole perturbation theory ›
Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCs ›
Investigating the correlations between IceCube high-energy neutrinos and Fermi-LAT $\gamma$-ray observations. II ›
Calibrating Bayesian Tension Statistics using Neural Ratio Estimation ›
New Constraints on Lorentz Invariance Violation at High Redshifts from Multiband of GRBs ›
Cool-Core Destruction in Merging Clusters with AGN Feedback and Radiative Cooling ›
Chasing the Light: Shadowing, Collimation, and the Super-Eddington Growth of Infant Black Holes in JWST BLAGNs ›
The Simons Observatory: Quantifying the impact of beam chromaticity on large-scale B-mode science ›
A Detection of Circumgalactic Dust at Megaparsec Scales with Maximum Likelihood Estimation ›
Neutrinos as a new tool to characterise the Milky Way Centre ›
On the accuracy of posterior recovery with neural network emulators ›
Exploring the presence of a fifth force at the Galactic Center ›
The Lyman-alpha and Continuum Origins Survey II: the connection between the escape of ionizing radiation and Lyman-alpha halos in star-forming galaxies ›
Dispu$\tau$able: the high cost of a low optical depth ›
DeepVoid: A Deep Learning Void Detector ›
Monte Carlo simulations of relativistic shock breakout from a stellar wind ›
Insights into the structure and kinematics of a Milky Way-like galaxy ›
Non-linear Dynamics and Primordial Black Hole Formation During Kination ›
Preferential Positron Acceleration in Relativistic Magnetized Electron-Positron-Ion Shocks ›
Simulation-Based Inference for Direction Reconstruction of Ultra-High-Energy Cosmic Rays with Radio Arrays ›
High-resolution Giant Metrewave Radio Telescope H{\sc i} 21\,cm imaging of the host galaxy of FRB\,20250316A ›
Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes ›
Magma ocean interactions can explain JWST observations of the sub-Neptune TOI-270 d ›
Feeding the Dead: Neutral Gas Inflow in a Long-Quenched Ancient Massive Galaxy at $z\sim 2.7$ Observed with JWST/NIRSpec ›
High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates I. X-ray Coronae ›
Clumpy Outflows from Super-Eddington Accreting Black Holes I: Radiation Hydrodynamics Simulations and Observational Implications ›
Binding energy of compact stars and their non-radial oscillations ›
Assessing the star formation history of all-sky and part-sky 100pc white dwarf samples ›
High Resolution ( ›
Physical properties of long-rising type II supernovae -- Bayesian analytic modeling and spectrophotometric correlations ›
Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum ›
Modeling Binary Lenses and Sources with the BAGLE Python Package ›
First Statistical Detection of MgII-traced Cool Gas Outflows with JWST Towards Cosmic Dawn ›
SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope ›
The Oxygen Valve on Hydrogen Escape Since the Great Oxidation Event ›
Insights for Early Dark Energy with Big Bang Nucleosynthesis ›
The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM ›
Kinematics of H I and O VI Absorbers: Insights into the Turbulence Driver of the Multiphase Circumgalactic Medium ›
Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline ›
CLiMB: A Domain-Informed Novelty Detection Clustering Framework for Galactic Archaeology and Scientific Discovery ›
Properties and Possible Physical Origins of $\gamma$-ray Emission in Extreme Synchrotron Blazars ›
Discovery of Galactic center ejected star in DESI DR1 ›
Population synthesis of double white dwarfs: evolutionary effects on system properties ›
Experimental and numerical modeling of liposome congregation in meteorite craters of Early Earth ›
Magnetic structure of coronal dark halos ›
SMMAN: quasi-Simultaneous Multi-wavelength Monitoring of gamma-ray-loud AGNs with the Nanshan 26-m radio telescope ›
The morphological stability of open clusters: a new 2D perspective ›
HelioSpectrotron 5000: An interactive multi-resolution solar spectral atlas ›
Thermodynamic Consistent Description of Compact Stars of Two Interacting Fluids: The Case of Neutron Stars with Higgs Portal Dark Matter ›
Resolving the QCD Axion Domain Wall Problem with a Light Axion ›
Stable Islands of Weak Gravity ›
Marginal IR running of Gravity as a Natural Explanation for Dark Matter ›
Probing cosmic strings via gravitational-wave lensing ›
Equivalence of scalar-tensor theories and scale-dependent gravity ›
GraviBERT: Transformer-based inference for gravitational-wave time series ↓↑