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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Chmury

Opady

Niebo
Temperatura
1.0 °C
Wilgotność
93%
Wiatr
3.2 km/h
Ciśnienie
1004.2 hPa

Księżyc
Najnowsze prace na astro-ph:
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You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA ›
Satellite Metallicity Enhancement I: Suppressed Star Formation, Stellar Mass Loss, and Enriched Inflow of DESI and EAGLE Galaxies around Massive Clusters ›
An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos ›
Empirical estimates of how massive galaxies can be in {\Lambda}CDM ›
Identification of Compact Groups of Galaxies in IllustrisTNG300 ›
The Peculiar Velocity of Messier~87 from Microarcsecond Geodetic VLBI Astrometry ›
Discovery of 30 Repeating Fast Radio Burst Sources and Uniform Population Statistics of 80 Repeating Sources from CHIME/FRB ›
How to augment cosmic shear measurements with radio polarimetry of galaxies? ›
Thirty Circumbinary Disk Occultation Systems (KH 15D-like stars) from the OGLE Project ›
Wideband RFI Monitor Requirements, Design, and Commissioning at DRAO ›
Unmasking Stellar Feedback-Driven Bubbles: Identification and Properties Analysis ›
Specific Star Formation Rate Enhancement across the Galaxy Merger Sequence: Insights from Citizen Science Classifications ›
Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters ›
Cosmological test of a length-preserving biconnection gravity ›
Non-Parametric Equation of State Reveals Non-Conformal Behavior Beyond Neutron Star Densities ›
Gravitational-wave standard sirens and application in cosmology ›
Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes ›
The Stellar Abundances and Galactic Evolution Survey (SAGES). V. The First Data Release of the DDO51 Band ›
Chasing the neutrino blazar candidates II: SED modeling with hadronic model ›
The evolution of C4H and c-C3H2 in molecular cores ›
When Magnetic Fields Sculpt the Sky: The Riegel-Crutcher cloud in optical polarization ›
Observations of the 2023 February 27 fireball in northern Sweden using the auroral imaging system ALIS_4D ›
Beyond power spectrum to unveil systematics on HI intensity maps ›
The Status of Gravitational Vector Perturbations with Recent CMB Data ›
BOCOSUR: An all sky network for fireball detection in Uruguay ›
Reionisation time field reconstruction from 21-cm Maps: Investigating predictor coherence in WDM cosmology ›
The MaNGA Low-mass disks HUnt for CO (MaLHUCO) Survey ›
Interstellar X-ray Absorption and Scattering ›
Complexity and Multifractal Variability in Multi-Band Emission of Seyfert AGN ›
Separate Universe Super-Resolution Emulator ›
Plato's view on supermassive black hole binaries: Exploring the faint limit of ESA's Plato space mission ›
Exploring Enceladus's Interior Structure Using Electromagnetic Induction ›
JWST observations and a model for the extremely luminous obscured quasar W2246-0526 at z=4.6 ›
How to count clustered galaxies ›
Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs ›
GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate ›
High-Spin BBH Subpopulation from AGN Accretion ›
Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way ›
Physical characterization and modeling of candidate Hyper-Compact HII Regions ›
Search for quasar pairs with Gaia astrometric data. II. Photometric redshift prediction with machine learning for the MGQPC catalogue ›
Consistency between dynamical modeling and photometrically derived masses of fireballs ›
A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287 ›
Bayesian Analysis of Massive Boson Star Models for Sagittarius A* Using Near-Infrared Astrometry Data ›
Accelerating 3D Non-LTE Synthesis with Graph Neural Networks ›
Challenges to the cosmological constant model following results from the Dark Energy Survey ›
X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission ›
Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis ›
Optical Appearance of the Kerr-Bertotti-Robinson Black Hole with a Magnetically Driven Synchrotron Emissivity Model ›
Image Processing Framework for Eclipse Shadow Band Analysis ›
A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588 ›
Cooling of Isolated Neutron Stars with Hyperon-mixed Kaon-Condensation Matter ›
Small and Complex I: The Three Component Structure of $z \sim 0$ Massive Compact Quiescent Galaxies ›
Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies ›
Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations ›
Validating Coronal Magnetic Field Models Using Gaussian Separation ›
Numerical estimation of the capture ability of Neptunian mean motion resonances ›
RAYTHEIA: A high-performance ray-tracing algorithm for three-dimensional direction-dependent equations in astronomical simulations ›
Lunar ejecta as the missing piece to resolve the lunar cratering asymmetry ›
On the Problem of Prognostication of Bright Kreutz Sungrazers ›
On the residual missing mass of the Bullet Cluster ›
Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events ›
The Influence of Aliphatic Components on the Aromatic Emission Characteristics of Polycyclic Aromatic Hydrocarbons ›
Tracing the kinematic perturbations of the Milky Way spiral arms with APOGEE DR17 and Gaia DR3 ›
From Large Telescopes to the MUltiplexed Survey Telescope (MUST) ›
Cyclotron Line Variability and Accretion Dynamics in Vela X-1 ›
Application of Machine Learning to 21 cm Cosmology ›
Reionization History and Neutrino Mass ›
CosmoDRAGoN III: Shaping the Afterlife -- How Progenitors and Environments Sculpt Radio Galaxy Remnants ›
Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-Duration Magnetic Field Sector Transition ›
Isolating Broadband Radio Technosignatures (BRaTs): A Framework for Detecting Planetary-Scale Leakage ›
Astrophysical signatures of Kerr-Bertotti-Robinson black holes in a cloud of strings: ISCO, microquasar QPOs, and Bondi-Hoyle-Lyttleton accretion ›
Stellar Age Compression Reshapes Interpretations of the Milky Way Thick-Disk Formation History ›
Thermal Deformation Reduction in High-Power Interferometry with Higher-Order Laser Modes ›
Design and in-orbit calibration of the MXT optics ›
Transition region-induced kinetic Alfven wave conversion. Electric displacement field ›
Wolf-Rayet stars as tracers of gamma-ray emission: Isolated stars and stellar clusters/associations ›
STEPSIC: Initial condition generator for stereographic cosmological simulations ›
Energy-resolved pulse profiles of Vela X-1: cross-calibrating XMM-Newton and NuSTAR to trace spectral features ›
Quantum and Structural Effects Captured via a Statistical Method: the SACM Applied to HCN and HNC Colliding with CO ›
The dispersal of compact protoplanetary discs ›
High-speed single-photoelectron detection for Cherenkov astronomy ›
SAPLE: Swift Analysis Pipeline for Lightcurve Extraction ›
Comparing Results from Two Uniform Phase Curve Surveys ›
Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems ›
Breaking Free from the Swampland of Impossible Universes through the DESI Portal ›
HI absorption in MHONGOOSE -- Spin temperatures and cold neutral medium in nearby disk galaxies ›
Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks ›
Can magnetic reconnection power neutrino emission from AGN coronae? ›
An agentic framework for gravitational-wave counterpart association in the multi-messenger era ›
Astrons: Reissner-Nordstr\"om Primordial Naked Singularities ›
Co-evolution of the Milky Way high- and low-{\alpha} sequences with chemical evolution models ›
On the origin of variability in $\alpha$ Cygni variable $\epsilon$ Ori (HD 37128) using TESS observations and modelling ›
Mineral False Positives in the Search for Exoplanet Surface Biosignatures ›
Photonic integrated circuits for astronomy: A formal description of an integrated photonics-based wavefront sensor (IP-WFS) ›
Multifield stochastic inflation: Relevance of number of fields in statistical moments ›
Gas Phase Distribution in the Neutral ISM: A Comparison between Observation and Numerical Simulation ›
Machine Learning Techniques for Astrophysics and Cosmology: Simulation-Based Inference ›
Numerical Study of Some Generalizations of the Starobinsky Inflationary Model ›
Joint probabilistic inference of galaxy redshifts and rest-frame spectra from photometric fluxes with latent diffusion ›
Revisiting the greenhouse effect of non-greenhouse gases in the atmospheres of Earth-like planets ›
Search for long-term variability of HESS J1745-290 ›
Milky Way Dynamics Favor Dark Matter over Modified Gravity Models ›
Characterizing Pulsar Distances Using HI Kinematics ›
Can We Distinguish the Source Region Location of Filament/Prominence Eruptions from the Sun-as-a-star H$\alpha$ Spectrum? ›
Magnetic Evolution of Highly-Sheared Region in Active Region 13842 Producing Large X9.0 Flare ›
Mitigating residual foregrounds and systematic errors in SKA1-Low AA* EoR observations via Bayesian Gaussian Process Regression ›
Demonstrating the Use of the Spherical Fourier Bessel Basis for Large Scale Clustering Systematics Discovery and Mitigation with eBOSS ›
Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova ›
Designing a low-loss high reflectivity mirror for gravitational waves detectors by combining a dielectric metasurface and a multilayer stack ›
Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering ›
Neural Posterior Estimation of Terrain Parameters from Radar Sounder Data ›
Primordial Black Hole Hotspots Beyond Flat Spacetime ›
Revisiting predictions for cosmic-ray antinucleon fluxes from Galactic Dark Matter ›
The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response ›
Black hole mass and distance from accretion disk astrophysical observables ›
Quasiparticle Quality Factors in Superconducting Resonators: Effects of Bath Temperature and Readout Power ›
General Grad-Shafranov Equation ›
Neutron stars in a conservative $f(R,T)$ gravity ›
Asymmetric Reheating of Dark QED ›
A study on Dusty Plasma Physics and the examination of Jeans Criteria for the Milky Way ›
Controlled Penumbral Inflation from Monodromic Valleys ›
Uncertainty in Physics and AI: Taxonomy, Quantification, and Validation ›
Symfind: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos ›
Robust 1-norm periodograms for analysis of noisy non-Gaussian time series with irregular cadences: Application to VLBI astrometry of quasars ›
Ultraheavy Ultrahigh-Energy Cosmic Rays ›
Quantum coherence and the invisible Universe: Subradiance as a dark matter mechanism ›
A Sample of Active Galactic Nuclei with Intermediate-mass Black Holes Extended to $z \approx$ 0.6 ›
The Two-component Model of the 'spokes' in Saturn's Rings ›
Non-Gaussianity of Tensor Induced Density Perturbations ›
LITMUS: Bayesian Lag Recovery in Reverberation Mapping with Fast Differentiable Models ›
Ward Identity Constraints on Loop Corrections in Non-Attractor Inflation ›
GW231123: A Possible Primordial Black Hole Origin ›
Deep Learning for CMB Foreground Removal and Beam Deconvolution: A U-Net GAN Approach ›
Evidence of the pair instability gap from black hole masses ›
Observation of Galactic center in the sub-MeV gamma-ray band with electron-tracking Compton camera ›
The Noise of Vacuum ›
RX Gru: a short-period pre-main-sequence eclipsing binary with a distant circumbinary companion ›
Jittering jets promote dust formation in core-collapse supernovae ›
BGRem: A background noise remover for astronomical images based on a diffusion model ›
DESI DR2 Galaxy Luminosity Functions ›
Changing-Look AGN Powered By Disk Tearing ›
A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy ›
Comparing galaxy merger orbits in hydrodynamical simulation and in dark-matter-only simulation ›
Tracing the Trace Anomaly of Dense Matter inside Neutron Stars ›
Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows ›
OzDES Reverberation Mapping of Active Galactic Nuclei: Final Data Release, Black-Hole Mass Results, & Scaling Relations ›
Reaching diffraction-limited localization with coherent PTAs ›
The abundance of thin dwarf galaxies: a challenge for cosmological simulations ›
KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature ›
Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference ›
Resolving the Core-Cusp and Diversity Problems with a Baryon-Correlated Dark Matter Profile ›
Revisiting the Reported Period of FRB 20201124A Using MCMC Methods ›
Possible evidence for a pair-instability supernova nature of ultra-early JWST sources ›
New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing ›
Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics ›
Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN ›
The early r-process nucleosynthesis scenarios ›
Impact of Rastall gravity on hydrostatic mass of galaxy clusters ›
Rarity of rocket-driven Penrose extraction in Kerr spacetime ›
Studying dark gaps in Ly-$\alpha$ forest transmission with large reionization simulations ›
A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A ›
Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation ›
Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts ›
Large-scale and local environmental drivers of quenching: tracing H$\alpha$ concentration in X-ray and optical galaxy groups ›
Inferring the population properties of galactic binaries from LISA's stochastic foreground ›
Magnetic structure of coronal dark halos ›
Variational views for self-supervised learning in radio astronomy ›
Primordial Black Hole Formation in Rastall Gravity: Shifted Collapse Threshold and Exponential Abundance Sensitivity ›
Inefficiency of chiral dynamos in protoneutron stars and the early universe ›
Cosmological peculiar velocities in general relativity ›
The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III ›
Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy ›
Organosulfur Chemistry on sub-Neptunes: Implications for hazes and biosignatures ›
Early emission characterization of TDE 2025aarm ›
ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser ›
Large-scale Morphology of the Optical F-corona from a Total Solar Eclipse Observation During the Artemis II Lunar Flyby ›
Long-Term Dynamical Evolution and Ejection of Near-Earth Asteroids ›
The apparent Large Magellanic Cloud star cluster age gap ›
Sub-Neptunes Show a Stronger Correlation with Cold Jupiters than Super-Earths Especially in Metal-rich Systems ›
A SPHEREx Pipeline and Spectral Library for Ultracool Dwarfs ›
Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity ›
A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications ›
PySME v1.0: improved modelling of stellar spectra for survey-scale applications ›
How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 ›
On the origin of the environmental step: A BayeSN view of the ZTF SN Ia DR2 ›
String Thresholds, Dynamical Gauss--Bonnet Couplings, and Starobinsky Attractors ›
Neutron Star Eclipses as Axion Laboratories ›
Parameter inference of millilensed gravitational waves using neural spline flows ›
How Many Times Should We Matched Filter Gravitational Wave Data? A Comparison of GstLAL's Online and Offline Performance ›
New Methods for Offline GstLAL Analyses ›
Inflation Model Based on Virasoro Squeezing ›
Searching for dark photon dark matter from terrestrial magnetic fields ›
Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog ›
Orbital dynamics and precession in magnetized Kerr spacetime ›
Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look ›
Boson Stars Hosting Black Holes ›
Properties of Stable Massive Quark Stars in Holography ›
Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model ›
Curvaton-assisted hilltop inflation ›
Cosmological long-wavelength solutions in non-adiabatic multi-fluid systems ›
The new generation lunar gravitational wave detectors: sky map resolution and joint analysis ›
An approximate Kappa generator for particle simulations ›
Effects of isovector spin-orbit interaction on the charge-weak form factor difference in $^{48}$Ca, $^{208}$Pb, $^{90}$Zr and $^{62}$Ni ›
Searching for axions with time resolved pulsar polarimetry ›
Preliminary study on the impact of stress-energy tensor compared to scalar field in Nonminimal Derivative model ›
Outer-Crust Equations of State for Neutron Stars ›
Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection ›
Hadronic lensing ›
Adaptive ray tracing, image diagnostics, and photon ring signatures of rotating dark-matter-dressed black holes ↓↑