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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
12.5 °C
Wilgotność
60%
Wiatr
0.0 km/h
Ciśnienie
1016.3 hPa

Księżyc
Najnowsze prace na astro-ph:
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Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with HMG ›
Time-resolved XRISM spectroscopy reveals the evolution and structure of the corona in MCG-6-30-15 ›
High-energy neutrino constraints on primordial black holes as dark matter ›
A first empirical derivation of the average dust attenuation law at 2 ›
Eccentricities of millisecond pulsars with intermediate-mass progenitors ›
Gaia astrometry disfavors a binary origin for long secondary periods ›
Magnetic field alignment with dense cores in the transition between cloud and core scales ›
Repopulating the pair-instability mass gap without sustained growth to massive IMBHs: the case of 47\,Tuc ›
JWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia Supernova ›
Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk ›
Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics ›
Even a precessing clock is right twice per orbit -- The super-periods of eRO-QPE2 and challenges for quasi-periodic eruption orbital models ›
Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune ›
High Resolution X-ray Spectroscopy of the Nova-Like Cataclysmic Variable BZ Cam using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow ›
Spectroscopic Characterization of WD J000801.25-350450 and its Two Co-Moving Companions ›
Kozai-driven mass loss of the circumbinary disk in D9 in orbit around the supermassive black hole Sgr A* ›
PEACC -- Precision Emitter for 21 cm Array Coherent Calibration ›
Galactic Archaeology with the Subaru `\=Onohi`ula Prime Focus Spectrograph Strategic Program ›
A Study of HH 270 with the James Webb Space Telescope ›
Near-critical magnetic fields in Kepler red giants ›
Impacts of Multidimensional Progenitor Perturbations on Core-Collapse Supernova Explosions ›
Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation ›
Spectroscopic Survey of Faint Planetary-Nebula Nuclei. VIII. The Dwarf Barium Central Star of Kohoutek 1-9 ›
Secular Light Curve of Exocomet 3I/ATLAS, and its Location on a Comet Evolutionary Diagram ›
Environmental Dependence of Galaxy properties: A study of 341 Ring Galaxies in Cosmic Voids ›
To understand the radiative processes of pulsars and fast radio bursts with the FAST ›
Estimating the Luminosities of Protostars with Limited Infrared Photometry ›
Possible Supermassive Dark Object Composed of Light Fermionic Gas with an Embedded Neutron Star Core ›
Predicting Associations between Solar Flares and Coronal Mass Ejections Using SDO/HMI Magnetograms and a Hybrid Neural Network ›
Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object II: The dynamical fate of tidal fragments ›
Daily Predictions of F10.7 and F30 Solar Indices with Deep Learning ›
A Multi-modal Fusion Network for Star-Galaxy Classification from CSST Simulated Datasets ›
Impact of Observational and Modelling Assumptions on Intergalactic Magnetic Field Constraints from TeV Gamma-Ray Bursts with the Cherenkov Telescope Array Observatory ›
Starbursts at Cosmic Dawn: Formation of Globular Clusters, Ultra-Faint Dwarfs, and Population III star clusters at z > 6 ›
Joint Observation of SGR J1935+2154 with \textit{Insight}-HXMT and KM40m during the active episode of October 2022 ›
A seeing measurement device for the PoET solar telescope ›
Inflationary magnetogenesis from non-minimal coupling in large- and small-field potentials ›
Uncovering the Dominant Spatial Scales of the Sun's Magnetic Field in Solar Cycle 24 ›
An Analytic Formalism of Inflation for Derivative Coupled Scalar Field and Validating its predictions for Some Inflationary Potentials ›
A Theoretical Investigation of He I Line Profiles for the Spectroscopic Analysis of DB White Dwarfs ›
Lorentz invariance violation search with flaring active galactic nuclei observations of the first Large-Sized Telescope of CTAO ›
A Fast Direct Solver for Mutual Coupling Analysis of Large Arrays of Reflector Antennas ›
The Milky Way Tomography with Subaru Hyper Suprime-Cam. II. Global halo structure ›
The Milky Way Tomography with Subaru Hyper Suprime-Cam: Implications for the past orbit of the Large Magellanic Cloud ›
Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign ›
Miscibility and Transport Properties in Hydrogen-Neon Mixtures ›
Multi-TeV $\gamma$-ray candidates from GRB 221009A: a downturn in the intrinsic $\gamma$-ray spectrum, an echo of the prompt emission phase, and intergalactic electromagnetic cascades ›
A Path to Constraints on Common Envelope Ejection in Massive Binaries: Full Evolutionary Reconstruction of Three Black Hole X-ray Binaries ›
Probing the Origin of Magnetar X-ray Polarization Diversity: A Multi-wavelength Geometrical Study of 1E 1547.0-5408 and 1E 2259+586 ›
Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations ›
Searching for Gamma Ray Bursts associated with CHIME Fast Radio bursts ›
Ages and masses of asymptotic giant branch stars from the period--luminosity diagram ›
Vertical Structure of Local Disk Galaxies revealed by DESI Imaging Data ›
Magnetic Reconnection at Hyperbolic Flux Tube associated with a Confined Flare in NOAA Active Region 12268 ›
Spatio-temporal analysis of helioseismic quasi-biennial oscillations ›
Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds ›
Thermal Segregation and Reddening in Europa's Double Ridges ›
Reionization Topology as a Probe of Self-Interacting Dark Matter ›
The demise of the synchronous moon that gave Mars its triaxiality. The role of solar tides and a palaeo ocean ›
Inferring Unreported Measurement Uncertainties via Information Geometry in Astrophysics ›
A consistent MOND modelling of the Bullet Cluster ›
Improving Solar Flare Soft X-ray Classification With FOXES: A Framework For Operational X-ray Emission Synthesis ›
Systematic census of RR Lyrae stars in Milky Way stellar streams ›
A Turbulence-Driven Magnetic Reconnection Model for the High-Energy Neutrino Emission from NGC 1068 ›
Plasma lensing modeling of substructures on pulsar scintillation screens ›
Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b ›
Seasonal Variability of Pluto's Haze Formation Revealed by Laboratory Simulations ›
On the origin of the BAOtr-DESI tension ›
Lunar nutation effect defines the sign of the Earth rotation rate for now, but this may change soon ›
White Dwarfs with Infrared Excess from DESI EDR ›
From Fragments to Flares: Migration, Tidal Disruption, and Observable Bursts in Massive Protostellar Disks ›
Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid ›
Space-Clock Elevator: Multi-Stage Orbital Transport via Rotating Tethers and Elliptical Nodes ›
Observations of highly inclined disks with ALMA. Results from 12CO gas and continuum observations ›
First observational constraints on cosmic backreaction over an extended redshift range ›
Streaming instabilities in weakly ionized protoplanetary discs: the Ambipolar Streaming Instability (AmSI) ›
A Comparative Study of TeV Gamma-Ray Sources with Various Objects ›
Statistical Study of Balmer Continuum Enhancement in Solar Flares ›
Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948 ›
The high-altitude, inner-disc, and chemically peculiar open cluster UBC 1052 ›
Compact CO emission and no evidence of radial drift. ALMA observations of the faintest planet-forming disks in Lupus ›
GeV gamma-ray emission in the field of the shell-type supernova remnant Vela Jr revisited ›
A Ring of Fire Orphan {\gamma}-Ray Flare in the Neutrino Candidate 3C 120 ›
A Falsifiable Timing Test for the Double-White-Dwarf Model of Long-Period Transients ›
Ultra-fast simulations of the solar dipole and open flux ›
Extragalactic microlensing through Ultra Diffuse Galaxies ›
From Dust to Planets -- A Chemical Perspective ›
Compact Hydrogen Sulfide Emission Indicates Sulfur-bearing Ice Sublimation in the Inner Disk of HD 163296 ›
The environmental imprint on molecular layering in the dusty streamer of M512 ›
Emergence of Complex Structures ›
Scale-dependent surface and volume density properties of filaments in molecular clouds ›
The RoPES project with HARPS and HARPS-N III. Two candidate planets orbiting the G-type star HD 161098 ›
Global m=1 slow mode in near-Keplerian self-gravitating torus: applications to stellar nuclear disks and AGN molecular tori ›
Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal ›
The magnetic sensitivity of the Ca II H and K lines ›
Galactic Diffuse Gamma-Ray and Neutrino Emission from Cosmic-Ray Interactions in Stellar Atmospheres ›
Combining the Mass--Radius Posteriors of J0030+0451 Allowing for Unknown Model Systematics ›
Investigation of gravitational stability of protoplanetary disks based on statistical analysis of their masses ›
Multi-fluid multi-species models for inverse FIP-effect ›
Prominence signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics ›
Do little red dots really form a distinct class of astronomical objects? ›
Cosmological inference with halo clustering reconstructed from the redshift-space galaxy distribution ›
A bright flare in the obscured state of GRS 1915+105 as seen by NICER and Swift ›
The GAPS Programme at TNG. LXXIII. Confirmation of the hot sub-Neptune TOI-4602 b (HD 25295 b), a key target for future atmospheric characterization ›
NGC 1647: A young open cluster with a broad main sequence observed with LAMOST ›
Origin and characterization of super-Earths and sub-Neptunes ›
The nature of tilted supercritical accretion discs ›
Effective Stability of Near-Rectilinear Halo Orbits in the Earth-Moon System ›
Exact Gravastar Solution ›
Generalized Kolmogorov systems with applications to astrophysics and biology ›
Toward Neutrino and Dark Matter Detection with Ancient Minerals: TEM Study of Heavy-Ion Tracks in Olivine ›
Spin-($0$, $1$, $\frac{1}{2}$) Field Perturbations, Quasinormal Modes, Overtones, Greybody Factors and Strong Cosmic Censorship of Einstein-Skyrme Black Holes ›
Testing the Kerr hypothesis beyond the quadrupole with GW241011 ›
Induced Multi-phase Inflation with Reheating: Leptogenesis and Dark Matter Production in Metric versus Palatini ›
Ion pickup and velocity space thermalization at outer planet moons ›
Geometrically Significant Surfaces of Black Holes from a Single Scalar ›
Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity ›
Discussion on the equivalence of two relativistic point-particle Lagrangians ›
Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals ›
Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models ›
Radiatively Corrected Hybrid Inflation: Parameter Scans and Machine Learning with ACT and Future CMB Experiments ›
Probing Yukawa Gravity with Modulated Newtonian Cancellation in the CHRONOS Detector ›
Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars ›
Helicity-supported stationary spacetimes: A class of finite-energy, horizonless, axisymmetric solutions ›
Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas ›
JWST reveals the diversity of nuclear obscuring dust in nearby AGN: nuclear isolation of MIRI/MRS datacubes and continuum spectral fitting ›
Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order ›
The Quintom theory of dark energy after DESI DR2 ›
Euclid preparation. LXXXIX. Accurate and precise data-driven angular power spectrum covariances ›
Non-relativistic effective theories for fields with general potentials and their implications for cosmology ›
Comparative Study of Early-Universe Epochs in an $f(R,L_m)$ Gravity Model with Effective Curvature--Matter Interaction and $\Lambda$CDM Cosmology ›
Population III star formation near high-redshift active galactic nuclei ›
Prototyping of 6.2-mm-Pitch Fiber Positioner Modules for Stage-V Telescope Instrumentation ›
JWST Spectroscopic Insights Into the Diversity of Galaxies in the First 500 Myr: Short-Lived Snapshots Along a Common Evolutionary Pathway ›
A fast machine learning tool to predict the composition of astronomical ices from infrared absorption spectra ›
Gravitational waves reveal the pair-instability mass gap and constrain nuclear burning in massive stars ›
Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity ›
Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints ›
On Atomic Line Opacities for Modeling Astrophysical Radiative Transfer ›
Graph-based Summary Statistics for Revealing the Stochastic Gravitational Wave Background in Pulsar Timing Arrays ›
The Colors of Ices: Measuring ice column density through photometry ›
Low-noise Fourier Transform Spectroscopy Enabled by Superconducting On-Chip Filterbank Spectrometers ›
Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference ›
Magnetized Shocks Mediated by Radiation from Leptonic and Hadronic Processes ›
Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum ›
Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network ›
Phase-space perturbation theory for cosmic large-scale structure ›
Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties ›
Effects of the radiative interior on solar inertial modes ›
Cygnus X-3: A variable petaelectronvolt gamma-ray source ›
Early thin-disc assembly revealed by JWST edge-on galaxies ›
BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion ›
Twenty-four thousand hours of GREENBURST observations with the GBT ›
Extreme-Value Distribution Analysis of the Second CHIME/FRB Catalog: Assessing the Rarity of the One-off FRB 20250316A ›
SN 2017ati: A luminous type IIb explosion from a massive progenitor ›
A Minimal Interpretation of the Galactic Cosmic-Ray Proton and Helium Spectra from GeV to PeV Energies ›
Stone Skipping Black Holes in Ultralight Dark Matter Solitons ›
Predicting New Concept-Object Associations in Astronomy by Mining the Literature ›
The Physical Properties of PS1-12sk and the implications for its Progenitor System ›
Spectral Universality of Turbulent Fluctuations in Relativistic Flows ›
Outflow from unmagnetized shocked radiative transonic accretion disk around a black hole ›
Characterizing the Instrumental Profile of LAMOST ›
Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments ›
Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity ›
Reconnection-driven State Transitions in Flat Spectrum Radio Quasars ›
Mass Inventory of the Solar System Beyond the Sun: A Systematic Compilation with Uncertainty Budget ›
TESS light curves of two new magnetic cataclysmic variables: an asynchronous polar at the period minimum, and an eclipsing system with a large spin-to-orbit ratio ›
Measurement of the Orbital Parameters, Spin and Spectral Evolution During the Main High State of Her X-1 with Insight-HXMT ›
Direct N-body simulations of rotating and extremely massive Population III star clusters ›
An inverted infall profile for the collapse of the massive star-forming IRDC SDC335.579-0.292 ›
Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters ›
Monitoring Volatile Evolution in Disrupting Comet D/2021 A1 (Leonard) with NOEMA and APEX ›
Beyond $f(\phi)\mathcal{G}$: Gauss--Bonnet inflation with $\mu(\phi,X)$ ›
UMI: GPU-Accelerated Asymmetric Robust Estimator for Photometric Detrending in Exoplanet Transit Searches ›
The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time ›
Optical images of Kerr-Sen black hole illuminated by thick accretion disks ›
Validating Prior-informed Fisher-matrix Analyses against GWTC Data ›
Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory ›
Supernova production of axion-like particles coupling to electrons, reloaded ›
Exploring Leptogenesis in the Era of First Order Electroweak Phase Transition ›
Possible evidences for physics beyond $\Lambda$CDM from DESI DR2 data ›
Studying Ionospheric Phase Structure Functions Using Wide-Band uGMRT (Band-4) Interferometric Data ›
Comparing astrophysical models to gravitational-wave data in the observable space ›
Completing Axion Double Level Crossings ›
Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair ›
Scattering of massive particles from black holes and naked singularities ›
False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE ›
A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind ›
Quasi-pole inflation in metric-affine gravity ›
Reheating in geometric Weyl-invariant Einstein-Cartan gravity ›
The global structure of the time delay likelihood ›
Accelerated Time-domain Analysis for Gravitational Wave Astronomy ›
Probing soft signals of gravitational-wave memory with space-based interferometers ↓↑