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Obserwatorium Astronomiczne na Suhorze

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Niebo
Temperatura
-0.3 °C
Wilgotność
94%
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0.0 km/h
Ciśnienie
1007.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Undetected past contacts with technological species: implications for technosignature science ›
Relativistic Magnetohydrodynamic Simulations of Giant Magnetar Bursts ›
Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge ›
Addressing the Impact of Solar Modulation Systematic Uncertainties on Cosmic-Ray Propagation Models ›
Identifying Exoplanets with Deep Learning VI. Enhancing neural network mitigation of stellar activity RV signals with additional metrics ›
Teen TITANS simulations -- I. Inefficient intermediate-mass black hole seeding via stellar collisions in young massive clusters ›
Bonnor-Ebert sphere collapse in filamentary structures ›
Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE ›
There and back again? Neutral outflows in z~3.5 quiescent galaxies ›
Possible stratospheric emission in the warm Neptune GJ 436 b from high-resolution spectroscopy ›
On the Origin of Coronal Picoflare Jets ›
Long-term eclipse time variations in white dwarf binaries ›
Improved Identification of Satellite Trails in ACS/WFC Imaging Using a Modified Radon Transform ›
Ly{\alpha} forest bounds on sterile neutrino production via neutrino self-interactions ›
The SB9 catalogue: status, comparison with non-single stars from Gaia DR3 and evolution to SBX ›
Scaling Relations across Galaxy Classification Schemes: I. Star Formation Rate-Stellar Mass Plane of CALIFA Nearby Galaxies ›
dfcosmic: A Python package for cosmic ray removal ›
A Bayesian Exploration of the Mass of Ursa Major III: Kinematics, Rotation and their influence on the Mass to Light Ratio ›
A Comprehensive Catalog of Radio Sources and Rotation Measures in the Perseus Molecular Cloud from Very Large Array Observations ›
MATLAS-42, A Globular Cluster-Rich Ultra-Diffuse Galaxy That Diverges from the "Failed Galaxy'' Formation Pathway ›
Probabilistic Methods for Initial Orbit Determination and Orbit Determination in Cislunar Space ›
Investigating the role of mergers in galaxy assembly in the early Universe (z > 5) ›
Modeling brightness temperature of sunspots using ALMA single-dish observations ›
The attempted polarity reversal and evolving magnetic environment of AD Leo ›
3D radiative transfer modeling of scattering polarization with partial frequency redistribution I. Verification and disk-center results for the solar Ca I 4227 {\AA} line ›
Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows ›
TROYE: Modeling Dynamic Phase Transitions in Gravitational Waves from Neutron Star-Black Hole Mergers ›
The GAPS Programme at the TNG: LXX. TOI-5734b: A hot sub-Neptune orbiting a relatively young K dwarf with an Earth-like density ›
Testing the Icy Pebble Accretion Hypothesis with Primordial Main Belt Asteroids ›
Updated Air-Shower $X_{\rm max}$ Moment Parametrizations for UHECR Composition with Latest Hadronic Interaction Models ›
A Photometric and Spectroscopic investigation of 11 TESS eclipsing contact binaries ›
MIGHTEE HI observations of low surface brightness and ultra-diffuse galaxies in the XMM-LSS field ›
Power-law Indices of EUV Intensity Power Spectrum in Flaring Coronal Active Regions ›
Euclid: An automated system to match Rubin transient alerts to Euclid observations ›
A geometric physics-informed machine learning inference for the neutron star maximum mass and the inverse problem ›
The Dispersed Matter Planet Project Sample -- Detection limits, Occurrence Rates and New Planets ›
The GUAPOS project -- VII: Physical structure and molecular environment of the G31.41+0.31 HII region ›
First Dark Photon Search Results from the Dandelion Experiment ›
Mathematical derivation and verification of the amplitude of LISA's interferometric signals on an ultra-stable interferometer testbed ›
CMB anisotropies from cosmic (super)strings in light of ACT DR6 ›
Chromaticity-Optimized Antenna Design and Bayesian Foreground Validation for the CANTAR Global 21 cm Experiment ›
Single and double headed ORCs in the LOFAR surveys ›
Cosmological Constraints on Temperature-Dependent Interaction between Dark Matter and Neutrinos ›
Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8 ›
A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks ›
Numerical simulations of cold clumps in the hot accretion flows around black holes ›
Spatio-Spectroscopic Representation Learning using Unsupervised Convolutional Long-Short Term Memory Networks ›
Chandra Proper Motions and Milliarcsecond Astrometry of Nineteen Pulsars ›
A response-matrix-centred approach to presenting cross-section measurements ›
Hypothesis tests and model parameter estimation on data sets with missing correlation information ›
Covering Unknown Correlations in Bayesian Priors by Inflating Uncertainties ›
Plotting correlated data ›
Spectral Homogenization of the Radiative Transfer Equation via Low-Rank Tensor Train Decomposition ›
Scaling Laws for Template-Free Detection of Environmental Phase Modulation in Gravitational-Wave Signals ›
Minimal Dark Matter: Generalized Framework and Direct-Detection Sensitivity ›
Decay of a multi-axionic SU(N) symmetric color aether in the early Universe as an origin of emergence of a many-component dark matter ›
Dark Photon mediated Inelastic Dark Matter in Cosmology, Astrophysics and Colliders ›
GR-Athena++: Binary Neutron Star Merger Simulations with Neutrino Transport ›
Constraining the $\Lambda\Lambda$ interaction with terrestrial and astronomical data ›
Detection prospects of solar $g$-modes with LISA ›
The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant ›
Deep Generative model that uses physical quantities to generate and retrieve solar magnetic active regions ›
Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production ›
Unveiling Electron Density Profile in Nearby Galaxies using SDSS MaNGA ›
AstroMLab 4: Benchmark-Topping Performance in Astronomy Q&A with a 70B-Parameter Domain-Specialized Reasoning Model ›
The Cosmic Owl: Twin Active Collisional Ring Galaxies with Starburst Merging Front at $z=1.14$ ›
A solution to the tension of burning on neutron stars and nuclear physics ›
TasVisAn and InsPy -- Python Packages for Triple-Axis Spectrometer Data Visualization, Analysis, Instrument Resolution Calculation, and Convolution ›
HOLISMOKES XVII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data ›
No evidence for Keplerian taper of far-out galactic rotation ›
Quantum estimation of cosmological parameters ›
A spherical hydrodynamical model of cosmic voids in {\Lambda}CDM and beyond ›
$r$-process Heating Feedback on Disk Outflows from Neutron Star Mergers ›
New Interpretations of the Cosmological Preference for a Negative Neutrino Mass ›
The Impact of Baryonic Effects on the Dynamical Masses Inferred Using Satellite Kinematics ›
Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models ›
Joint Bayesian calibration and map-making for intensity mapping experiments ›
The Galaxy Activity, Torus, and Outflow Survey (GATOS): N. Unveiling physical processes in local active galaxies. Unsupervised hierarchical clustering of JWST MIRI/MRS observations ›
Quantifying the Effects of Parameters in Widespread SEP Events with EPREM ›
Stochastic analysis of ultra-high energy cosmic ray interactions ›
Ultra-long Gamma-ray Bursts from Micro-Tidal Disruption Events: The Case of GRB 250702B ›
MEGATRON: Disentangling Physical Processes and Observational Bias in the Multi-Phase ISM of High-Redshift Galaxies ›
The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape ›
Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity ›
Rethinking mass transfer: a unified semianalytical framework for circular and eccentric binaries. II. Orbital evolution due to nonconservative mass transfer ›
The PAU Survey: The $i$-band galaxy luminosity function from the present-day to $z = 2$ ›
Simulating Disky Broad Line Region Reverberation ›
Joint Constraints on Fuzzy and Warm Dark Matter from Satellite Populations of the Milky Way and Andromeda ›
DRAGNs in the Forest: Identifying Artifacts with Random Forest Models in the VLASS DRAGNs Catalog ›
Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events ›
NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period ›
A simple mechanism for the enhancement of the inflationary power spectrum ›
Supermassive black holes swallow stellar objects at high rates: from Little Red Dots to Black Hole Stars ›
PDRs4All XXI. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster ›
Gravitational-wave signatures of nonviolent nonlocality ›
Primordial black hole ringdown: The irreducible stochastic gravitational wave background ›
Fast and Fewrious: Stochastic binary perturbations from fast compact objects ›
Towards an anomaly detection pipeline for gravitational waves at the Einstein Telescope ›
Gravitational Ionization by Schwarzschild Primordial Black Holes ↓↑