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Obserwatorium Astronomiczne na Suhorze

Widok nad kopułą w nocy

Chmury

Opady

Niebo
Temperatura
13.4 °C
Wilgotność
39%
Wiatr
8.0 km/h
Ciśnienie
1011.2 hPa

Księżyc
Najnowsze prace na astro-ph:
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The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries ›
A New Robust Constraint on the Self-interaction Cross-section of Dark Matter with Double Radio Relic Clusters ›
The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy ›
Self-consistent numerical simulations for the formation and dynamics of solar prominences ›
Deep Learning galaxy cluster's structural parameters from Weak Lensing observations ›
Towards a measurement of the primordial helium isotope ratio ›
Radiation Total Dose for PRIMA: Cold Exposure with Alpha Particles ›
Confirmation of Fe I on MASCARA-5 b's Dayside Observed With EXPRES ›
EMBER: Machine-Learning Detection of Modulated Ion Acoustic Waves and Associated Core-Electron Heating in the Solar Wind with Parker Solar Probe ›
Smaller Than Earth Habitability Model (STEHM): The Lower Size Limit for Atmosphere Retention in the Habitable Zone ›
A Detailed View of the Large-Scale Sloshing Cold Front in RXJ2014.8-2430 ›
Correspondence between a decaying dark matter sector scenario and scalar field model ›
Extinction law and stellar mass in the Nuclear Bulge from kinematically-selected red clump stars ›
Ultra-deep imaging of nearby dwarf irregular galaxies: stellar haloes and disk structure ›
ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) III. Optical He I line profiles of the accreting super Jupiter Delorme 1 (AB)b ›
Exploring RR Lyrae Variable Stars in the Vera C. Rubin Observatory Data Preview 1 ›
A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications ›
Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts ›
Training a neural network to rapidly identify candidate gravitational-wave events in the lower mass gap ›
Maximal mass of neutron stars constrained by neutron star observations ›
Measuring $f\sigma_8$ and BAO scale in the Local Universe: a joint real and redshift space analysis from CosmicFlows-4++ ›
A consistent formulation of stochastic inflation I: Non-Markovian effects and issues beyond linear perturbations ›
XMAGNET -- Stir before serving: a Lagrangian perspective on mixing-driven condensation in the intracluster medium ›
Multi-messenger Constraints on a Primordial Black Hole Origin of the KM3-230213A Event ›
Red Quasars: Selecting Candidates in SDSS DR16 and Estimating Their Physical Parameters ›
The NIKA2 Cosmological Legacy Survey in COSMOS: Final 1.2mm and 2mm source catalogs and redshift distribution of dusty star-forming galaxies ›
Kinematic properties of the TW Hya association ›
The Rocky Planet Picture Show: Implementation of Surface Reflection and Emission in $\texttt{POSEIDON}$ with Application to and Interpretation of JWST Data ›
Beyond Bragg-Mirrors for Gravitational Wave Telescopes: A Fabrication Tolerant Hybrid Metasurface-Bragg Mirror Design ›
A bright wideband radio burst from the isolated neutron star 2XMM J104608.7$-$594306 ›
DESI and Gravitational Wave Constraints Challenge Quintessential {\alpha}-Attractor Inflation ›
Life After the Quasar: Overmassive Black Holes and Remnant Ionised Bubbles in and Around Two z~6.6 Galaxies ›
Magnetic loops in the solar transition region ›
Upstream neutrino production and delayed jet emission in the blazar GB6 J1542+6129 ›
A Global 7% Systemic Sensitivity Floor in Gaia DR3: Multi-Wavelength Validation using 2MASS, Pan-STARRS and the 0.75-Magnitude Offset ›
$4\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback ›
Optimization of Weak Lensing Lightcone Simulations for Higher-Order Statistics in the LSST era ›
PEARLS: Two Distinct Populations of AGN Hosts Moving Between Star Formation and Quiescence ›
Gravitational particle production, the cosmological tensions and fast radio bursts ›
Study of cosmic ray impacts on cryogenic high sensitivity detectors ›
Novel Chemical Pathways for the Formation of Nucleobase Precursors via Benzene {\pi}-Bond Addition to HCN ›
Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection ›
Pre-inflationary QCD axion stars after moduli domination ›
Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries ›
Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023 ›
High-resolution ro-vibrational and rotational spectroscopy of the open-shell, linear CCH$^+$ ion ($^3\Pi$) ›
Anisotropy of Cosmic Background Photons from Annihilating/Decaying Dark Matter ›
IceCube Results and Perspective for Neutrinos from LHAASO Sources ›
Hyperactive Magnetar Eruptions: Giant Flares, Baryon Ejections, and Fast Radio Bursts ›
Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources ›
Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology ›
Ripples in the baryon to dark matter ratio in $\Lambda$CDM: implications for galaxy formation ›
Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun ›
An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4 ›
KL Dra as a Benchmark Laboratory for Accretion-Disk Physics: Constraints from TESS and Ground-Based Surveys ›
Searching for Isolated Black Hole Candidates within 15 pc of the Solar System in Gaia DR3 ›
Maximum Energy of Particles Accelerated in GRB Afterglow Shocks ›
An essential building block for cosmological zoom-in perturbation theory ›
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum ›
A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A ›
Deeper detection limits in astronomical imaging using self-supervised spatiotemporal denoising ›
The hydrodynamics of stratified ultra-relativistic outflows and the origin of GRB X-ray plateaus ›
The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc ›
Interstellar Dust Transport Through the Heliosphere Including the Sector Region ›
A systematic study of AGN feedback in a disk galaxy using MACER II: predictions of X-ray surface brightness profiles and comparison with eROSITA observations ›
Weighing the mass of LHS 3844 b ›
The RRATalog: a Galactic census of rotating radio transients ›
Scale-dependent surface and volume density properties of filaments in molecular clouds ›
Impact of Baseline, Cadence, and Host Contamination on AGN Variability Metrics: A Systematic Study with ZTF ›
Benchmarking Two Chemical Networks used in General Circulation Models of Hot Jupiters ›
Calibration-Induced Systematics in SALT3 Training and Their Impact on Dark Energy Constraints from Stage IV Supernova Surveys ›
The Deep Newtonian Regime in Late-Time Blast Waves: Inevitable Transition and Distinct Flux Signatures ›
SWIM: Stochastic Warm Inflation Module to generate and analyse Warm Inflationary power spectrum ›
Waveform Modelling for the Laser Interferometer Space Antenna ›
Weaving Life into Regolith: Engineered Autotrophic-Heterotrophic Consortia for Autonomous Biofabrication from Granular Feedstocks ›
Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620 ›
Stochastic Inflation in Numerical Relativity ›
High Frequency Spectrum of Primordial Gravitational Waves ›
Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes ›
Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints ›
Gravitational Sommerfeld Effects: Formalism, Renormalization, and Perturbation to $O(G^{10})$ ↓↑