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Obserwatorium Astronomiczne na Suhorze

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Księżyc
Najnowsze prace na astro-ph:
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Bridging scales: How much do supermassive black holes grow in the suppressed Bondi regime? ›
JWST/NIRSpec Reveals a Small Population of Dominant Dust-Obscured Ionizing Sources in Galaxies at 1 < z < 3 ›
An almost NIRCam-dark dusty star-forming galaxy at z=6.63 ›
Where Giants Dwell: Probing the Environments of Early Massive Quiescent Galaxies ›
The binary landscape of massive stars at low $Z$: Insights from the BLOeM Campaign ›
Evidence for in-situ acceleration of relativistic particles in the wings of X-shaped radio galaxies ›
Highly Efficient Identification of Extreme Emission Line Galaxies in the Local Universe: >8000 New Green Pea Candidates at 0.12 < z < 0.36 ›
Bridging scales: Modeling suppressed Bondi accretion on black holes and its impact on galaxy growth ›
Radiation-mediated shocks in gamma-ray bursts: spectral evolution ›
Kinematic scaling relations of disc galaxies from ionised gas at $z\sim~1$ and their connection with dark matter halos ›
No TiO detected in the hot Neptune-desert planet LTT-9779 b in reflected light at high spectral resolution ›
Gravity-Selected Galaxy Clusters: a Tight Mass-Richness relation and an unclear Compton $Y$-richness trend ›
Isolating the gravitational influence of Uranus's winds requires close passages inward of the rings ›
Identification of Candidate Halos Hosting Massive Black Hole Seeds in the \textit{Renaissance} Simulations with Support Vector Machines ›
Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem ›
How to evaluate the sufficiency and complementarity of summary statistics for cosmic fields: an information-theoretic perspective ›
3D MHD simulations of coronal loops heated via magnetic braiding I. Continuous driving ›
3D MHD simulations of coronal loops heated via magnetic braiding II. Automatic detection of reconnection outflows and statistical analysis of their properties ›
WATSON-Net: Vetting, Validation, and Analysis of Transits from Space Observations with Neural Networks ›
Symbolic Regression Is All You Need: From Simulations to Scaling Laws in Binary Neutron Star Mergers ›
Probing the Molecular Hearts of Extreme Bipolar Planetary Nebulae with ALMA ›
Model of super-Alfv\'enic MHD turbulence and structure functions of polarization ›
Kinetic Theory and the Mechanics of Isothermal Gas Spheres: Derivation of the Classical Emden--Chandrasekhar Equation via the Vlasov--Poisson Formalism ›
JWST Reveals Carbon-rich Chemistry in a Transitional Disk ›
Analytical Description of Baryonic Matter Fluctuations Using Jeans Filtering Functions in Second-Order Cosmological Perturbation Theory ›
An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi ›
Stellar Populations with MaNGA: Iron Kink and Nitrogen Fuzz ›
Detection Prospects for AGNs with the Cherenkov Telescope Array ›
Gas excitation of post-starburst galaxies at 0.6 < z < 1.3 ›
Modelling Millisecond Pulsar Populations in Globular Clusters with NBODY6++GPU ›
CoronaGraph Instrument Reference stars for Exoplanets (CorGI-REx) I. Preliminary Vetting and Implications for the Roman Coronagraph and Habitable Worlds Observatory ›
Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation ›
Measuring the magnetic fields in the chromospheres of low-mass stars ›
Probing Intrinsic Ellipticity in Neutron Star Binaries ›
Low-Frequency Noise Performance of Microstrip-Coupled Lumped-Element Aluminum KIDs using Hydrogenated Amorphous Silicon Parallel-Plate Capacitors for NEW-MUSIC ›
Continuum variability in multi-epoch quasar spectra from the Sloan Digital Sky Survey ›
Improved Modeling of Quasi-Static Thermal and Optical Response of Lumped-Element Aluminum Manganese KIDs ›
Search for host galaxies of unlocalized Fast Radio Bursts in the SDSS IV catalog ›
The Dawn of Gravitational Wave Astronomy at Light-year Wavelengths: Insights from Pulsar Timing Arrays ›
JW-Flare: Accurate Solar Flare Forecasting Method Based on Multimodal Large Language Models ›
Design of a Six-band, 2.4-Octave (80--420 GHz) Hierarchically Summed Phased-Array Slot-Dipole Antenna Array for NEW-MUSIC ›
Evolution of the radio source position uncertainties in radio astrometric catalogs over the past three decades ›
Models of long-period variables of the globular cluster 47 Tuc ›
Mock Observations for the CSST Mission: HSTDM--Synthetic Data Generation ›
J-PAS: A Neural Network Approach to Single Stellar Population Characterization ›
Multiwavelength spectral and temporal analysis of VHE Blazar 1ES 1959+650: Tracing emission mechanisms across flux states ›
Detection of Lensed Gravitational Waves from dark matter halos with deep learning ›
Superhot (> 30 MK) flare observations with STIX: Joint spectral fitting ›
Not all roads lead to merger: AGN disc properties influence the interactions of highly unequal mass black holes ›
Emission-Line and Continuum Reverberation Mapping of the NLS1 Galaxy WPVS 48 ›
Numerical Simulation of Impact Cratering and Induced Seismic Waves in Sand Targets ›
Interstellar medium phases and abundances in the central parsec: A JWST MIRI/MRS view of the Galactic center ›
Little red dots as embryos of active galactic nuclei ›
Radio Burst from a Stellar Coronal Mass Ejection ›
Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections ›
Variability of optical spectral index to support a central sub-parsec binary black hole system in quasar SDSS J001224-102226.51 ›
A magnetic field study of two fast-rotating, radio bright M dwarfs. StKM 1-1262 and V374 Peg ›
Recombination Clumping Factor of Physically Defined Intergalactic Medium at the Epoch of Reionization ›
Ray-trax: Fast, Time-Dependent, and Differentiable Ray Tracing for On-the-fly Radiative Transfer in Turbulent Astrophysical Flows ›
Rapid-response characterization of near-Earth asteroid 2024 YR4 during a Torino Scale 3 alert ›
Bright Cosmic-Ray Source as a Solution to Auger-TA Tensions ›
Compelling Evidence for a Harmonic in the Light Curve of the Supermassive Black Hole Binary Candidate PKS J1309+1154 ›
POLAR-2 - Latest Developments of the Next Generation GRB Polarimeter ›
Ultra extreme high-frequency-peaked BL Lacs: a potential population of MeV synchrotron blazars? ›
Comprehensive Study of the Lunar Energetic Particle Environment with LunPAN ›
Development of a planar cable-driven parallel robot for submillimeter and terahertz beam mapping measurements ›
Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum ›
Revisiting the Hubble tension problem in the framework of holographic dark energy ›
TIME Commissioning Observations: I. Mapping Dust and Molecular Gas in the Sgr A Molecular Cloud Complex at the Galactic Center ›
Adsorption and condensation of molecules on astrophysical dust grain surfaces: Ab-initio calculalations and kinetic Monte Carlo simulations ›
From M100 to NGC 7331: A Multiband Study and Physical Parameters in Nearby Galaxies ›
Global Distribution of the Key Species on the Surface of Europa ›
Collisions in a system of conical jet/counterjet outflows ›
A ring-shaped starburst as a galactic wind-generating mechanism: Morphology, emission, and mass ejection ›
Probing Time-Dependent Physics with Phase-Folding CMB Maps ›
Warped Disk Galaxies: Statistical Properties from DESI Legacy Imaging Surveys DR8 ›
Mitigating Nonlinear Systematics in Weak Lensing Surveys II: Stability and Diagnostics with Intrinsic Alignment ›
Abiogenesis on Different Star Types; a Dissipative Photochemical Perspective ›
Massive Inflationary Amplitudes: New Representations and Degenerate Limits ›
Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors ›
Did our Universe Tunnel out of the Wrong Higgs Vacuum? ›
Progress on the ALETHEIA project and new approaches to events overlap mitigation ›
Emergent Dark Matter ›
Impact of reactor antineutrinos on the neutrino floor in low-mass WIMP-like dark matter searches ›
A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales ›
Imaging and polarization patterns of various thick disks around Kerr-MOG black holes ›
Conservation of magnetic-helicity fluctuations due to spatial decorrelation of fluxes in decaying MHD turbulence ›
Phase transition during inflation and the gravitational wave signal at pulsar timing arrays ›
Approximate reconstruction of inflationary potential with ACT observations ›
Nature-inspired optimization, the Philippine Eagle, and cosmological parameter estimation ›
Genetic algorithm demystified for cosmological parameter estimation ›
The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation ›
Dynamic Diffusion Schr\"odinger Bridge in Astrophysical Observational Inversions ›
On the prospects of thermalization of axion-SU(2) inflation ›
The fine structure of the mean magnetic field in M31 ›
Consistent Initial Conditions for Early Modified Gravity in Effective Field Theory ›
Three-dimensional equation of state extension of quark matter in Fermi-liquid theory ›
UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5 ›
Interpreting Hubble tension with a cascade decaying dark matter sector ›
Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at $z \sim 7.6$ ›
Inflation from a generalized exponential plateau: towards extra suppressed tensor-to-scalar ratios ›
Beyond Extreme Burstiness: Evolving Star Formation Efficiency as the Key to Early Galaxy Abundance ›
Machine learning analysis of Photometric data from the Dark Energy Survey ›
Cepheid Metallicity in the Leavitt Law (C--MetaLL) survey: VII. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample ›
Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions ›
On the optical emission in the mini-outburst of the black hole X-ray binary MAXI J1348-630 ›
Probing the H0 Tension with Holographic Dark Energy in Unimodular Gravity: Insights from DESI DR2 ›
Radio Astronomy in the Era of Vision-Language Models: Prompt Sensitivity and Adaptation ›
Second Generation Planet Formation in Post-AGB Discs: Testing the Role of Gravitational Instability ›
Disentangling Milky Way halo populations at low metallicities using [Al/Fe] ›
Reionization optical depth and CMB-BAO tension in punctuated inflation ›
Witnessing downsizing in the making: quiescent and breathing galaxies at the dawn of the Universe ›
Quintessential inflation studied through Semiclassical Methods ›
Both Stellar Mass and Gravitational Potential Shape the Gas-Phase Metallicity ›
A Photometric Classifier for Tidal Disruption Events in Rubin LSST ›
Ionization Sources of the Local Interstellar Clouds: Two B-stars, Three White Dwarfs, and the Local Hot Bubble ›
FlowLensing: Simulating Gravitational Lensing with Flow Matching ›
Using simultaneous mass accretion and external photoevaporation rates for d203-504 to constrain disc evolution processes ›
The richest clusters in the Coma and Leo superclusters: Properties and evolution ›
Re-envisioning Euclid Galaxy Morphology: Identifying and Interpreting Features with Sparse Autoencoders ›
The chemical DNA of the Magellanic Clouds IV. Unveiling extreme element production: the Eu abundance in the Small Magellanic Cloud ›
Discovery of Seven Cold and Distant Brown Dwarfs with JWST RUBIES ›
JWST provides a new view of cosmic dawn: latest developments in studies of early galaxies ›
JWST Lensed Quasar Dark Matter Survey III: Dark Matter Sensitive Flux Ratios and Warm Dark Matter Constraint from the Full Sample ›
In-Orbit GRB Identification Using LLM-based model for the CXPD CubeSat ›
Towards direct imaging and orbital parameter estimation of supermassive black hole binaries with spaceborne VLBI ›
Euclid preparation. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution ›
On the problem of initial conditions for inflation ›
Bayesian network 3D event reconstruction in the Cygno optical TPC for dark matter direct detection ›
Discrete Chi-Square Method beats Discrete Fourier Transform and other similar parametric time series analysis methods ↓↑