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Obserwatorium Astronomiczne na Suhorze

Widok nad kopułą w nocy

Chmury

Opady

Niebo
Temperatura
-3.6 °C
Wilgotność
93%
Wiatr
3.2 km/h
Ciśnienie
1009.8 hPa

Księżyc
Najnowsze prace na astro-ph:
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Measuring Cometary Nuclei Behind Bright Comae: PSF Delta Decomposition with Bicubic Resampling and an Application to Interstellar Comet 3I/ATLAS C/2025 N1 ›
Sequential Convex Programming for Multimode Spacecraft Trajectory Optimization ›
Simulated Rotation Measure Sky from Primordial Magnetic Fields ›
Evolutionary Processes in the Centaur Region ›
Constraining properties of dust formed in Wolf-Rayet binary WR 112 using mid-infrared and millimeter observations ›
Estimating the masses of Narrow line Seyfert 1 galaxies using damped random walk method ›
Chemical and Isotopic Homogeneity Between the L Dwarf CD-35 2722 B and its Early M Host Star ›
X-ray, optical, and radio follow-up of five thermally emitting isolated neutron star candidates ›
Pixellated Posterior Sampling of Point Spread Functions in Astronomical Images ›
Mind the Information Gap: Unveiling Detailed Morphologies of z 0.5-1.0 Galaxies with SLACS Strong Lenses and Data-Driven Analysis ›
Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback ›
Tracing AGN-Galaxy Co-Evolution with UV Line-Selected Obscured AGN ›
In medio stat virtus: enrichment history in poor galaxy clusters ›
Role of magnetic reconnection in blazar variability using numerical simulation ›
Connecting clustering and the cosmic web:Observational constraints on secondary halo bias ›
Metal enrichment of galaxies in a massive node of the Cosmic Web at $z \sim 3$ ›
Beyond the Monsters: A More Complete Census of Black Hole Activity at Cosmic Dawn ›
SE3D: Testing the recovery of stellar population, dust and structural properties on mock-observed toy model and simulated galaxies ›
$\nabla\cdot{B}=0$ versus the Universe ›
Detection of the Cosmological 21 cm Signal in Auto-correlation at z ~ 1 with the Canadian Hydrogen Intensity Mapping Experiment ›
SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars ›
Metal-loaded outflows in sub-Milky Way galaxies in the CIELO simulations ›
Disc growth and vertical heating of lenticular galaxies in the Fornax cluster ›
Planetary Habitability Under the Light of a Rapidly Changing Star ›
Tracing ionized gas kinematics in Lyman-Break Analogs. Implications for star formation compactness and outflow properties ›
Optical and cm follow-ups of the Changing-Look event in Mkn 590 ›
KIC 5623923: A Faint Eclipsing Binary Consisting of $\delta$ Scuti pulsations ›
Internal kinematics of dwarf galaxies orbitally moving in ultralight dark matter ›
Alignment of radio jets in the microquasar V4641 Sagittarii with its high-energy structures ›
Sequential Fragmentation of C/2025 K1 (ATLAS) After Its Near-Sun Passage ›
Observations of [O I] emission in Comets C/2014 Q2 (Lovejoy) and C/2007 N3 (Lulin): Possible Influence of Solar Activity on Oxygen Line Ratios ›
The Speed of Gravity and the Fate of Dark Energy ›
Discovery of linear propadienone: Study of the chemistry of linear and cyclic H$_2$C$_3$O and H$_2$C$_3$S in TMC-1 ›
Asgard/NOTT: L-band nulling interferometry at the VLTI - III. The mid-infrared integrated optics beam combiner for NOTT ›
Cold Dark Matter and Dark Energy Based on an Analogy with Superconductivity ›
Seasonal asymmetry in vertical distribution of meteor decay time at two conjugate polar latitudes ›
Tidal Heating of the Lunar Magma Ocean ›
Symbiotic Stars (Including T Corona Borealis) Are Not Immediate Progenitors of Normal Type Ia Supernovae ›
Pile-up simulator for XRISM/Xtend onboard the X-ray Imaging and Spectroscopy Mission (XRISM) ›
Data-constrained magnetohydrodynamic simulation of global solar corona including solar wind effects within 2.5 $R_\odot$ ›
A Focused Review of Quintom Cosmology: From Quintom Dark Energy to Quintom Bounce ›
Stellar Parameters of BOSS M dwarfs in SDSS-V DR19 ›
TOI-7510: A solar-analog system of three transiting giant planets near a Laplace resonance chain ›
Exomoon search with VLTI/GRAVITY around the substellar companion HD 206893 B ›
Spatially Resolved Plasma Diagnostics of the Supernova Remnant DEM L71 using the Reflection Grating Spectrometer ›
Precise mass and radius determination for two new and one known Neptune-sized planets around G Dwarf hosts ›
A laboratory plasma experiment for X-ray astronomy using a compact electron beam ion trap (EBIT) ›
Ionospheric VLF Radio Reflection Analysis System ›
The relation between helium white dwarf mass and orbital period under two types of opacity ›
Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation ›
Search for the potential electromagnetic counterparts of neutrino events in SDSS galaxies at z ›
The Evolving Baryonic Tully Fisher Relation: A Universal Law from Galaxies to Galactic Clusters ›
Rotation of flux ropes in the low corona ›
Simulating the Stellar Bycatch: Constraining the Prevalence of Extraterrestrial Transmitters within Radio SETI Surveys ›
Search for Radio Pulsations from Neutron Star Candidates in Detached Binaries ›
Projection Effects in Barred Galaxies Causing Wrong Interpretation of Radial Flows ›
Tails of Gravity: Persistence of Star Formation in the CMZ Environment ›
From Empirical to Physical Model: Direct Fits of Optically Thin Inverse Compton Scattering to Prompt GRB Spectra ›
Projections of Earth's Technosphere: Strategies for Observing Technosignatures on Terrestrial Exoplanets ›
Impact of Spectral Coverage on Parameter recovery in Blazar Modeling ›
Performance Calibration of the Wavefront Sensor's EMCCD Detector for the Cool Planets Imaging Coronagraph Aboard CSST ›
Radio Burst Phenomenology of AD Leonis and Associated Signatures of Propagation Effects ›
Black Hole merger rates in the first billion years in light of JWST data ›
Impact of Simulation Box Size for Weak Lensing: Replication and Super-Sample Effects ›
Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning ›
Jet reorientation revealed by intermittent jet activity in radio galaxy 0954+556 ›
The effect of sound speed on the gravitational wave spectrum of first order phase transitions in the early universe ›
A Self-Consistent Model of the Ultra High-Energy Gamma-Ray Emission of Pulsar Wind Nebulae: Insights from LHAASO and ATNF Catalogs ›
Advances and Challenges in Solar Flare Prediction: A Review ›
Rotational effects in quark stars: comparing different models ›
Molecular hydrogen in filaments at high Galactic latitudes ›
Discovery of new N-emitters over a wide redshift range ›
A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line? ›
Considerations on the process of target selection for the Comet Interceptor mission ›
The miniJPAS and J-NEP surveys: Machine learning for star-galaxy separation ›
H II regions and supernova remnants associated with molecular clouds: A pilot study with the SARAO MeerKAT Galactic Plane Survey ›
On-sky demonstration of second-stage wavefront control with a photonic lantern ›
The origin of B-type runaway stars based on kinematics ›
Multi-Resonant-Line Radiative Transfer: Lyman-Alpha Fine Structure and Deuterium Coupling ›
An improved time delay from VLA and ATCA monitoring of the gravitational lens system PKS 1830-211 ›
Hurst exponent and planetary rings ›
Evidence of an Energetic Magnetar Powering 1LHAASO J0500$+$4454 ›
Inferring the Impacts of Baryonic Feedback from Kinetic Sunyaev-Zeldovich Cross-Correlations ›
Relativistic excitation of compact stars ›
gr-Orbit-Toolkit: A Python-Based Software for Simulating and Visualizing Relativistic Orbits ›
Experimental Demonstration of an On-Axis Laser Ranging Interferometer for Future Gravity Missions ›
GREA and Dark Energy: A holographic dual ›
Astronomical Methods and Instrumentation in the Islamic World: Past, Present, Future ›
Searching Stochastic Gravitational Wave Background Landscape Across Frequency Bands ›
Hawking heating of neutron stars by dark matter ›
Periodic gravitational lensing by oscillating boson stars ›
Fibre Inflation Meets Quintessence: Implications of Perturbative Stabilisation ›
Effective-one-body modelling of eccentric supermassive black hole binaries for Pulsar Timing Array ›
Probing High Reheating Temperatures by Direct Detection Experiments ›
Two Puzzles, One Solution: Neutrino Mass and Secluded Dark Matter ›
Microseismic Noise Mitigation with Machine Learning for Advanced LIGO ›
General relativity, early galaxy formation and the JWST observations ›
Investigating impacts of dust events on atmospheric surface temperature in Southwest Asia using AERONET data, satellite recordings, and atmospheric models ›
Strangelet Searches from Neutron Stars, Binary Mergers, and Gamma-Ray Bursts with Current and Future Observatories ›
New constraints on axion with gamma-ray observations of the Crab Nebula ›
Quintessential Inflation in Light of ACT DR6 ›
Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run ›
The PLUTO Code on GPUs: A First Look at Eulerian MHD Methods ›
Toward a Unified Understanding of the Dense Matter Equation of State ›
Anisotropic flows in heavy-ion collisions at HADES with Skyrme pseudopotential ›
Resolving white dwarf binaries within globular clusters with LISA ›
Chiral phonons in metal-organic frameworks as quantum sensors for the direct detection of dark matter ›
Anisotropic Bianchi-I cosmological model in non-conservative unimodular gravity ›
Natural inflation in Palatini $F(R)$ ›
Halo mass functions at high redshift ›
Primordial Black Hole Hot Spots and Nucleosynthesis ›
Gravitational Wave Evidence of Spin Energy Extraction from Stellar-Mass Black Holes ›
Has ACT measured radiative corrections to the tree-level Higgs-like inflation? ›
The Glow of Axion Quark Nugget Dark Matter: (III) The Mysteries of the Milky Way UV Background ›
Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography ›
Connecting JWST discovered N/O-enhanced galaxies to globular clusters: Evidence from chemical imprints ›
Diversity of low-mass planet atmospheres in the C-H-O-N-S-Cl system with interior dissolution, nonideality, and condensation: Application to TRAPPIST-1e and sub-Neptunes ›
A Simulation Based Inference Approach to the Dynamics of the MW-LMC System - Validation ›
Metallicity fluctuation statistics in the interstellar medium and young stars -- II. Elemental cross-correlations and the structure of chemical abundance space ›
Primordial Power Spectrum and Bispectrum from Lattice Simulations of Axion-U(1) Inflation ›
LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data ›
Viability of generalized $\alpha$-inflation from Planck, ACT, and DESI Data ›
Preferential Positron Acceleration in Relativistic Magnetized Electron-Positron-Ion Shocks ›
An Accurate Comprehensive Approach to Substructure: IV. Dynamical Friction ›
Analysis of mass-transferring binary candidates in the Milky Way ›
Colors of Life in the Clouds: Biopigments of atmospheric microorganisms as a new signature to detect life on planets like Earth ›
Relativistic Jets and Winds in Radio-Identified Supermassive Black Hole Binary Candidates ›
A Vertically Orientated Dark Matter Halo Marks a Flip of the Galactic Disk ›
The dark matter wake of a galactic bar revealed by multichannel Singular Spectral Analysis ›
State-Dependent X-ray Variability in Cygnus X-1: A 12-Year NuSTAR Timing Study of Accretion Flow Geometry ›
Strategy for identifying Vera C. Rubin Observatory kilonova candidates for targeted gravitational-wave searches ›
XRISM-Subaru views of Abell 754: Energetic ICM Motions Revealed by XRISM/Resolve ›
Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasiperiodic Eruptions ›
A targeted radio survey of infrared-selected bow shock candidates ›
High-inclination Centaur reservoirs beyond Neptune ›
The Distribution of Earth-Impacting Interstellar Objects ›
Accretion Geometry of the New Galactic Black Hole Candidate AT2019wey in the Hard State ›
SDSS-ALMA Legacy Value Archival Gas Exploration (SALVAGE) -- I: global star formation is governed by central (not global) molecular gas ›
Large Scale White Noise and Cosmology ›
Shaping the Mantle: The Role of the Superheated Core After Giant Impacts ›
The Atacama Cosmology Telescope: Cross-correlation of kSZ and continuity equation velocity reconstruction with photometric DESI LRGs ›
Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data ›
Spectrophotometric evidence for a metal-bearing, carbonaceous, and pristine interstellar comet 3I/ATLAS ›
General relativity and the bulk-flow puzzle ›
Learning Efficient Representations of Neutrino Telescope Events ›
Observational constraints using Bayesian statistics and Deep Learning in $f(Q)$ gravity ›
AstronomyCalc: A python toolkit for teaching Astronomical Calculations and Data Analysis methods ›
Pulse and Polarization Structures in Axion-Converted X-rays from Pulsars ›
Optical Images of Mini Boson Stars in Palatini $f(R)$ Gravity ›
Scalar-assisted magnetogenesis during the radiation-dominated epoch ›
Chronology Protection of Rotating Black Holes in a Viable Lorentz-Violating Gravity ›
StrCGAN: A Generative Framework for Stellar Image Restoration ›
CMB observables and reheat temperature as a window to models of inflation and freeze-in dark matter production ›
Latest results from CUORE and prospects for CUPID ›
Coupling between gravitational and electromagnetic perturbations on Kerr Spacetime ›
The effects of dark energy on the matter-gravity coupling ↓↑