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Obserwatorium Astronomiczne na Suhorze

gwiazdy nad kopułą

Kamerka S

Kamerka N

Niebo
Temperatura
-0.4 °C
Wilgotność
67%
Wiatr
0.0 km/h
Ciśnienie
1016.7 hPa

Księżyc
Najnowsze prace na astro-ph:
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PowerSpectR: An R Package for Radial Power Spectrum Estimation ›
GW190711_030756 and GW200114_020818: astrophysical interpretation of two asymmetric binary black hole mergers in the IAS catalog ›
Detection and Evolution of Linear Polarization of the Galactic Center Transient MAXI J1744-294 ›
ASTRAFier: A Novel and Scalable Transformer-based Stellar Variability Classifier ›
LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators ›
The assembly and fate of a giant disc galaxy in a protocluster at $z = 3$ ›
How Robust is the Cosmic Distance with Tip of Red Giant Branch against Stellar Population Variations? ›
Accretion-powered flares from black hole-disk collisions in galactic nuclei ›
Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing ›
Super-Earth masses and stellar abundances from NIRPS reveal tentative evidence for water-rich formation around M dwarfs ›
The Structure of Molecular Gas in PHANGS-ALMA Galaxies: Cloud Spacing, Two-Point Correlation and Stacked Intensity Profiles ›
From Internal Collision to Photon Escape: First-Principles Modeling of Radiation-Mediated Shocks in Gamma-Ray Burst Photospheres ›
Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters ›
The Goldilocks problem for detecting water in terrestrial planets: Constraining water abundances in the mid-IR with LIFE ›
Hydrolyzed Hazes on Water-rich Exoplanets: Optical Constants and Detectability ›
What's the (RV) Point? A $3.5\times$ Enhancement in Super-Jupiters with Saturn-like Periods from a Critical Observation ›
Searching for GEMS: Discovery of the Nearby Post-Common-Envelope Binary System TIC-460388167 ›
Solar Extreme Ultraviolet Spectrograph and High-energy Imager (SEUSHI): Design, Development, and Pre-Flight Calibration ›
Stochastic Optical Variability and an rms-flux Relation in the Intermediate Polar EP240309a ›
Which Neutron Stars Reach the Stiffening Regime? Multimessenger Constraints on Core Sound Speed and Stellar-Mass Thresholds ›
Tracing Active Galactic Nuclei Properties Through a Changing-look Event ›
Two young open clusters in Cygnus and their vicinity: combining multicolor photometry with Gaia DR3 astrometry ›
The ZTF-ULTRASAT experiment: Characterizing the non-transients in ULTRASAT's high cadence survey ›
Detection of TeV emission during early afterglow from poorly localized GRBs with ground based IACTs ›
Multiphase Gas Structure in the Circumnuclear Region of NGC 5506 Observed with ALMA ›
Isolating Sgr A East: The First Uncontaminated X-ray Maps of a Galactic Center Supernova Remnant ›
On the Information Content of Ariel Transmission Spectra: Reassessing the Tier System ›
Too Big to Quench? I. Constraining ISM Stripping of Dwarf Satellites in Milky Way-like Halos ›
The Fate of Globular Cluster Substructure: A Kinematic Response to Galaxy Assembly ›
Dust Absorption towards Supernova Remnant W44 ›
Development of Faster and More Accurate Supernova Localization at Super-Kamiokande ›
A Search for Wide-orbit Planets Around M-dwarfs using Deep MIRI 15-micron Images ›
Resolving the 2024 Outburst of Magnetar 1E 1841-045 from its host Supernova Remnant with EP-FXT ›
A study of periodic nulling in PSR B0751+32 with FAST ›
Does the spectral break in the IceCube diffuse neutrino spectrum originate from AGN evolution? ›
The deci-Hz gravitational wave signal from the collapse of rotating very massive stars ›
Meteor clusters: tracing meteoroid fragmentation in near-Earth space ›
First Lunar Farside SETI Observations for Periodic Signals with the Low-frequency Radio Spectrometer of Chang'E-4 Mission ›
Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023--2025 Observing Seasons ›
eROSITA's cool star population explained ›
Scalable continuous gravitational wave detection in PTA data with non-parametric red noise suppression and optimal pulsar selection ›
The puzzling story of flare inactive ultra fast rotating M dwarfs -- III. Investigating X-ray Activity ›
Oblique Shocks at Supernova Remnants in Massive Star Clusters: A Model for the Cosmic-Ray Knee Observed by LHAASO ›
A Natural $\gtrsim 100\times$ Telescope: Discovery of the Strongly Lensed Type II SN 2025mkn at $z=1.37$ ›
Three-dimensional transport-induced chemistry on temperate sub-Neptune K2-18b, Part II: the combined effects of atmospheric dynamics and chemical reactions ›
Chromospheric turbulence as a regulator of stellar wind mass flux ›
Flux variability of the "10 keV feature" of 4U 0115+63 ›
In-flight calibration of ESA Hera's HyperScout-H imager ›
DustPedia and Local Volume Legacy samples as benchmarks for dust evolution in galaxies ›
How many VHE gamma-ray binaries with young pulsars can be observed? ›
The evolution of exocomets and their source populations ›
A Statistical-AI Framework for Detecting Transient Flares in SDSS Stripe 82 Quasar Light Curves ›
Extended coronal line emission and new clues to a possible dual AGN in the merger J1356+1026 ›
Substructure in externally irradiated protoplanetary disks, I. spirals and rings in two-dimensional radiation hydrodynamics ›
The Stack Search Tests on FAST Data: Discovery of Six Faint Isolated Millisecond Pulsars in NGC 6517 and NGC 7078 (M15) ›
Chemistry and ro-vibrational excitation of CH$^+$ in the Planetary Nebula NGC 7027 ›
The peculiar velocity correlation function of the Cosmicflows-4 catalog ›
A Dynamical Equilibrium Linking Nanohertz Stochastic Gravitational Wave Background to Cosmic Structure Formation ›
3D kinematics of SMC star clusters: residual velocities disentangle kinematically perturbed clusters ›
Stochastic problems in pulsar timing ›
A parametric study of plasma instability cooling and its impact on intergalactic magnetic field constraints in GeV cascades ›
What you see is not necessarily what you get: Interpreting near-infrared scattering phase functions of debris discs ›
Planetesimal-Driven Instabilities in Resonant Chains of Cold Neptunes and Their Dynamical Outcomes ›
Searching for Ultracool Dwarfs in Early LSST Data Products ›
Ray-traced weak lensing convergence in screened modified gravity theories ›
Neutral Hydrogen in the Shapley Supercluster Core I: Environmental Effects on Gas Content and Galaxy Evolution ›
Exoplanet Orbital Distribution around FGK Sun-like Host Stars I: planet occurrence rate derived from the Kepler Mission and theoretical interpretations from planet formation ›
Morphological complexity of NGC 628 - a multiwavelength multiscale analysis using the ordinal pattern framework ›
Expansion kinematics of young clusters. III. The kiloparsec sample ›
Exoplanet Orbital Distribution around FGK Sun-like Host Stars II: a valley in the orbital semi-major axis distribution of sub-Neptunes ›
Optical images of Kerr-Sen black hole illuminated by thick accretion disks ›
Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide ›
A GPU-Accelerated JAX Framework for Robust Parametric Component Separation and Clustering Optimization for CMB Polarization Satellites ›
The effect of dust on vortices I: Laminar models ›
The effect of dust on vortices II: Streaming instabilities ›
Probing non-Gaussianity during reheating with SIGW in the LISA band ›
The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background ›
Disentangling cosmic distance tensions with early and late dark energy ›
Revisiting the sphaleron and axion production rates in QCD at high temperatures ›
Scalars at the Cosmological Collider: Full Shapes of Tree Diagrams and Bispectrum Searches using Planck Data ›
Quantum Simulation of Collective Neutrino Oscillations using Dicke States ›
Accretion Disks in Schwarzschild-MOG and Kerr-MOG Backgrounds: MOG Parameter in terms of Observational Quantities ›
Coalescing Compact Binary Parameter Estimation with Gravitational Waves in the Presence of non-Gaussian Transient Noise ›
Observational Quantities in Quasi-Newtonian Descriptions of Cosmological Space-Times ›
Detecting Chiral Gravitational Wave Background with a Dipole Pulsar Timing Array ›
Hard to shock DBI: wave propagation on planar domain walls ›
Probing Majoron Dark Matter with Gravitational Wave Detectors ›
Relativistic mean-field models of neutron-rich matter ›
Pyramid Interferometers: Direct Access to Cosmological Gravitational Wave Chirality ›
Cosmic Dynamics in Einstein-Cartan Theory: Analysing Hubble Tension through Curvature and Torsion field ›
Testing the equivalence principle across the Universe: a model-independent approach with galaxy multi-tracing ›
Hidden in Pixels I: Discovery of dual "little red dots" indicates excess clustering on kilo-parsec scales ›
The SRG/eROSITA all-sky survey: Constraints on Ultra-light Axion Dark Matter through Galaxy Cluster Number Counts ›
Comparative Analysis of EMCEE, Gaussian Process, and Masked Autoregressive Flow in Constraining the Hubble Constant Using Cosmic Chronometers Dataset ›
Prospects for Deep-Learning-Based Mass Reconstruction of Ultra-High-Energy Cosmic Rays using Simulated Air-Shower Profiles ›
Improved photometric redshift estimations through self-organising map-based data augmentation ›
Mapping atmospheric features of the planetary-mass brown dwarf SIMP 0136 with JWST NIRISS ›
J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 ›
Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe ›
The Dependence of Halo Clustering on Subhalo Anisotropy and Planarity ›
Modeling nonlinear scales for dynamical dark energy cosmologies with COLA ›
Molecular diversity as a biosignature ›
Seyfert Galaxies as Neutrino Sources: An Outflow$-$Cloud Interaction Perspective ›
The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A ›
libyt: an In Situ Interface Connecting Simulations with yt, Python, and Jupyter Workflows ›
Destruction of the interstellar dust by a supernova ›
A Novel, Beam-based Formalism for Active Impedance of Phased Arrays ›
Neutrino opacities in magnetic fields for binary neutron star merger simulations ›
Intracluster light as a dark matter tracer: how their spatial and kinematic relationship is shaped by satellite demographics ›
Multigroup Thermal Radiation Transport with Tensor Trains ›
Nested, asymmetric H-He circumstellar shells in the Type Icn/Ibn SN 2024abvb ›
Validating the Angular Sizes of Red Clump Stars with Intensity Interferometry ›
The Local Tremaine-Weinberg Method for Galactic Pattern Speed: Theory and its Application to IllustrisTNG ›
Merger-driven buildup of the $M_{\rm BH}$ - $M_*$ relation bridging high-$z$ overmassive black holes with the local relation ›
Correlations Between kHz QPOs and Spectral Parameters from Time-Resolved Spectro-Temporal Analysis of 4U 1728-34 ›
Revisiting the Excess of Bar-like Structures in TNG50 Early-type Galaxies: Consistency and Tension with Observations ›
Turning JWST/MIRI backgrounds into a survey of diffuse molecular hydrogen ›
Model-independent test of the cosmic distance duality relation with recent observational data ›
Relic Magnetic Fields from Non-Adiabatic Photon Freeze-Out at Recombination ›
Non-minimally coupled quintessence with sign-switching interaction ›
A 1151-Year Quasi-Commensurability of the Solar System: Empirical Detection, Statistical Characterization, and the Anomalous Exclusion of Uranus ›
Harmonic phase diagnostics of long secondary periods. Testing predictions of oscillatory convective dipole modes in the OGLE sample ›
Planet-induced Periodic Modulation of Stellar Activity in GJ~436: Insights into a Warm Neptune's Magnetic Field ›
VST-SMASH: VST Survey of Mass Assembly and Structural Hierarchy I. Survey presentation and deep photometry of IC 5332: tracing the mass assembly in the challenging faintest-end regime ›
Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition ›
NucleiML: A machine learning framework of ground-state properties of finite nuclei for accelerated Bayesian exploration ›
Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data ›
WIMP Dark Matter within the dark photon portal ›
Finite-temperature Yang-Mills theories with the density of states method: towards the continuum limit ›
Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model ›
Towards a complete scheme of cosmological neutrino self-interactions: Collision term for a wide range of mediator masses ›
Dark energy from string theory: an introductory review ↓↑