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Obserwatorium Astronomiczne na Suhorze

Widok nad kopułą w nocy

Chmury

Opady

Niebo
Temperatura
14.9 °C
Wilgotność
72%
Wiatr
6.4 km/h
Ciśnienie
1017.6 hPa

Księżyc
Najnowsze prace na astro-ph:
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The Phenomenological Nature of Quasar-type Blazars (BZQ). I. Revisiting the Flat-Spectrum Paradigm ›
Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective ›
Detecting Gravitational-Wave Anisotropies with Simulation-Based Inference ›
Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants ›
A formation scenario of black hole-envelope systems --viscous hydrodynamics simulation in general relativity-- ›
Discovery and Analysis of a Type II Supernova Candidate at z = 3.19 from JWST's COSMOS-Web Survey ›
Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes ›
FASTAR -- I. Continuous and differentiable evolutionary stellar population models ›
Fast and Flexible Characterisation of Astronomical Light Curves Using Multi-Time Attention ›
The AGORA High-resolution Galaxy Simulations Comparison Project. XI: Solving the Non-Spherical Morphology and Evolution of Dark Matter Halos with Haskap Pie ›
Dark matter-deficient twins: FCC 224 and FCC 240 as possible analogues of NGC 1052-DF2 and DF4 ›
Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE ›
On the maximum neutrino flux of blazars in the one-zone leptohadronic model ›
The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $z\geq 3$ ›
Pitch-Angle Scattering of Cosmic Rays: Confronting Theory with Observations ›
The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation ›
Hubble Astrometry for the Local Group and Beyond in the 2030s ›
Orbital Parameters of the Unusual WR + O Binary System LS III +44 21 ›
JWST and Gemini Observations of the Active Centaur 450P/LONEOS: Nucleus and Coma Characterizations ›
A Redshift-based Red Selection of Dusty Star-forming Galaxies ›
Pushing the Limit of Asteroseismic Detection for Cool Dwarfs using TESS and Deep Learning ›
Evidence for mass-dependent spin subpopulations in GWTC-4 ›
Near UV Stellar Activity and Brightness Fluctuations of the Alpha Centauri AB Star System from Weeks to Decades -- Inputs for Reflected Light Spectroscopy with HWO ›
Constraining the Potential Index $n$ of the Early Dark Energy Model Using Cosmic Birefringence from Planck and ACT ›
The 3D Structure and Kinematics of the Local Disk-Halo Interface: Intermediate-velocity Clouds are the Minority of High-altitude Clouds in the Solar Neighborhood ›
Evolution of a long-period Cataclysmic Variable from the viewpoint of the donor star: the case of SDSS J085210.48+783246.6 ›
Radiative MHD Studies of Solar Spicules: Driving Mechanisms and the Role of Background Magnetic Field ›
Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Survey ›
FASTAR -- II. Semi-resolved evolutionary stellar population models ›
Observational Technological Innovations and Future Development of the Lijiang Coronagraph ›
Timing and Spectral Studies of PSR J2022+3842 with NICER and NuSTAR ›
New galaxy cluster in the Zone of Avoidance SRGe CL0512.7+3712. Discovery and multi-wavelength characterization ›
The XRISM measurements of the black-hole spin in Cyg X-1 are highly model-dependent ›
Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions ›
A Three-Decade VLBI Study of the Nucleus in the Lobe-Dominated Quasar 3C207 ›
Deep Learning-Enabled Prediction of Geoeffective CMEs Using SOHO and SDO Observations ›
SN~2018erx: A fast-evolving, dust-reddened Type Icn supernova with broad C II emission lines ›
The Evolution of Cataclysmic Variables Under Various Magnetic ›
High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars ›
Preliminary cosmological results using extreme accretors Quasar formalism ›
Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients ›
QPEs from Warped Disk Collisions with EMRIs: Brightness-Recurrence Diagram and Gravitational-Wave Follow-up ›
Mass distribution of neutron stars in binary systems ›
Puzzling Ultra-Diffuse Galaxy Evolution (PUDGE). II. A transformation pathway from UDGs to compact dwarfs (CDs) in galaxy clusters ›
Radio Study of G76.9+1.0 Pulsar Wind Nebula ›
Small and Complex II: Characterizing the Disk and Stellar Envelope of Edge-on $z \sim 0$ Massive Compact Galaxies ›
Cyclotron breaking: a mechanism for parallel ion cyclotron waves to heat the fast solar wind ›
Exploring biases in derived stellar parameters and the ionizing photon production efficiency ›
Shear Particle Acceleration in Structured Gamma-Ray Burst Jets: IV. Thermal {\em vs.} Non-thermal Emission of the Jet Cocoon ›
Kepler Discovery of GW Vir Pulsations of the Central Star of Planetary Nebula Kn 61 ›
The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios ›
Discovery of Short-Term {\gamma}-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449 ›
Inverse Compton scattering occurring in a reverse-shock scenario involving a kilonova: A channel of TeV gamma-ray photons ›
Signs of Sulphur fractionation under high magnetic field strength ›
A Unified [CII] Morpho-Kinematic Corpus for 31 Star-Forming Galaxies at z = 4.26-5.68: The High-z Kinematic Corpus Z1 ›
Compact dusty starbursts at cosmic noon linked to high-energy neutrinos ›
Discovery of Molecular and Atomic Gas associated with HESS J1646-458 (Westerlund 1): Spatial TeV Gamma-Ray and Interstellar Proton Correspondence ›
Constraining the Inclination of Binary System Orbits with the Astrometric Excess Noise from Gaia DR3 ›
Long-Term Clustering Pattern of Solar Active Regions and Their Potential Connection with Magneto-Rossby Waves ›
The Gas-Phase Mass-Metallicity Relation of Dwarf Galaxies Across Large-Scale Environments Using the CAVITY Parent Sample ›
Legacy analysis of Milky Way dwarf spheroidal satellite galaxies: an update ›
Superfluid fraction and effective ion mass in the crystalline crust of a neutron star: role of interband response ›
Machine Learning-based Separation of the He I 10830{\AA} Chromospheric Signal: Quantitative Analysis of Chromosphere-Corona Intensity in the Quiet Sun ›
Reassessing high-energy emission correlations in gamma-ray bursts using a large, homogeneous sample of X-ray afterglows ›
Extreme color-magnitude variability: connection to changing-look AGNs ›
Beyond the [OIII]$\lambda$4363 auroral line: [NeIII]$\lambda$3868 as a direct tracer of electron temperature ›
Lithium-rich M-dwarfs at the ZAMS: Evidence for planetary engulfment? ›
The transitional Type Ibn/IIn SN 2022pda, with pre-explosion outbursts and a double-peaked light curve ›
skysurvey: a pure python package to simulate the transient sky ›
Core-collape supernovae and supernova neutrinos ›
Diversity of morphology of type II spicules in MURaM-ChE simulations ›
Gaia FGK Benchmark Stars: Impact of Spectral Resolution on Stellar Abundances ›
Chronos: Towards a self-consistent and absolute stellar age scale. I. A Bayesian hierarchical lithium-age model: Validation on the Pleiades cluster ›
Building on SVOM : the CATCH satellite constellation for transient astronomy ›
Reversible-jump MCMC reveals binary black hole subpopulations with distinct redshift evolution ›
Compactness Peaks and Subpopulations: Probing Stellar Physics and Formation Channels of Merging Binary Black Holes ›
Interstellar extinction, polarization efficiency, and grain alignment in the direction towards bright-rimmed clouds and cometary globules ›
Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension ›
X-ray Polarization Signatures from Comptonization by Magnetic Reconnection Plasmoids ›
Understanding hydrodynamical wave-driven shear mixing in stellar radiation zones. Looking in the mirror of the dyapicnal oceanic mixing ›
GRB 260310A / SN 2026fgk: A Multi-Wavelength Study of a Nearby Underluminous Long GRB and SN with a Complex Afterglow ›
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions ›
The imprints of the instantaneous appearance of a conformal Killing vector field on the evolution of self-gravitating fluid spheres ›
Quantification of atmospheric carbon dioxide from the Geostationary Operational Environmental Satellite (GOES East) ›
Aurora Hunter: A Two-Stage Framework for Probabilistic Visibility Forecasting ›
Production of Leptophilic Bosons in Ultradegenerate Relativistic Matter ›
Neutron Star Bounds on Muonic Fifth Forces from Picometer to Kilometer Scales ›
Solar Axions from Nuclear Transitions ›
Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks ›
Efficient Nonlinear Uncertainty Quantification for Spaceflight Leveraging Nonlinear Expansions ›
Leptogenesis without on-shell right-handed neutrinos ›
Wideband Balanced Photodetectors for Classical and Quantum Light Detection from Optical, EUV, to X-rays ›
Thermal Spin Polarization Driven by Nuclear Spin-Orbit Coupling in Neutron Star Pasta ›
Bayesian Estimation of Spectroscopic Parameters: Application to the Atomic Nitrogen Bound-Bound System ›
Gravitational Wave Propagation in K-essence Cosmology: Theory and Observational Constraints ›
Pulse magnet of 10 T for power laser experiments with x-ray free-electron laser diagnostics ›
Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks ›
Exploring the ex-situ components within Gaia DR3 ›
Many-body atomic response functions of xenon and germanium for leading-order sub-GeV dark matter-electron interactions in effective field theory ›
Turbulence in Magnetised Neutron Stars ›
SDSO1 is a Shocked Ghost Planetary Nebula in Front of M 31 ›
A tunable Monte Carlo method for mixing correlated-k opacities. PRAS: polynomial reconstruction and sampling ›
The Magnetic Origin of Primordial Black Holes: A Viable Dark Matter Scenario ›
Multi-messengers from the radioactive decay of $r$-process nuclei ›
Point-like and Narrow-lined: A Potentially New Population of Objects Discovered by JWST ›
Systematic Effects of Chaotic Magnetic Fields on Neutron Star Tidal Deformability: Implications for Gravitational Wave Constraints on Dense Matter ›
High five from ASTEP: Three validated planets and two eclipsing binaries in a diverse set of long-period candidates ›
Infall Explains the Disk Kinematics of AB Aur Without Gravitational Instability ›
Control variates from Eulerian and Lagrangian perturbation theory: Application to the bispectrum ›
Gamma-Ray Spectra of $R$-Process Nuclei ›
How precisely can we measure the ages of subgiant and giant stars? ›
Extremely UV-bright starbursts at the end of cosmic reionization ›
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5 ›
Evidence of dynamical dark energy found via the DESI DR2 Lyman$\alpha$ forest ›
Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet ›
Accessing the homogeneity scale with 21 cm intensity mapping surveys ›
Enhanced antineutrino emission from $\beta$ decay in core-collapse supernovae with self-consistent weak decay rates ›
First detection of X-ray polarization from the long-period X-ray pulsar 4U 1954+319 ›
Identification of periodicities with arbitrary shapes in AGN light curves ›
Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension ›
The contribution of the color space in LSST-like photometry for the selection of extragalactic globular cluster candidates ›
Joint constraints on $R_h=ct$ cosmology from DESI DR2 BAO, CC, and SN\textit{Ia} Pantheon$^+$ sample ›
Exploring the Limits of Machine Learning Classification of Neutron Star Matter Models ›
The Origin of Spin-Alignment of Dark Matter Subhalos ›
A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements ›
A Guided Unconditional Diffusion Model to Synthesize and Inpaint Radio Galaxies from FIRST, MGCLS and Radio Zoo ›
MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$ ›
Origin of Coronal Extreme Ultraviolet Shockwaves without a Coronal Mass Ejection Event ›
AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function ›
Gravitational Baryogenesis in $f(R)$ Cosmologies ›
BASS LV. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances ›
Capture and Stability of Resonant Planet Pairs in Turbulent Disk ›
IGR J12580+0134: A Possible Repeated Partial Tidal Disruption Event Inferred from Late-Time Radio Re-brightenin ›
Stochastic Particle Acceleration during Pressure-Anisotropy-Driven Magnetogenesis in the Pre-Structure Universe ›
Discovery of a Strong-lens Galaxy Pair with the Smallest Projected Separation ›
Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS ›
A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5 < z < 6.0$ at a Critical Stellar Mass of $10^{10}M_\odot$ Revealed by JWST ›
Irregular Repeating Tidal Disruption Events due to Diffusive Tides ›
A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar? ›
Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with hyperconical modified gravity ›
Validating z > 7.5 Lyman Break Galaxy candidates in the COSMOS field with JWST/PASSAGE ›
Foundations for Discovery: A Coordinated Fleet Approach to NASA Astrophysics ›
Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks ›
Peculiar velocities at low Galactic latitude ›
Information Content of the Cosmic Web ›
Statistical methods for partitioning ribbon and globally-distributed flux using data from the Interstellar Boundary Explorer ›
Fundamental Physics and Cosmology with TianQin ›
Search for primordial black holes from gravitational wave populations using deep learning ›
About electroweak domain walls in Majoron models ›
Cosmic-ray boosted inelastic dark matter from neutrino-emitting active galactic nuclei ›
Theoretical Signatures of QCD Phase Transitions in Compact Astrophysical Systems ›
Scalaron dark matter dynamics: effects of Higgs non-minimal coupling to gravity ›
Vector Resonant Relaxation and Statistical Closure Theory. II. One-loop Closure ›
GW250114 reveals black hole horizon signatures ›
Quantum Damping of Cosmological Shear: A New Prediction from Loop Quantum Cosmologies ›
Direct detection of solar chameleons with electron recoil data from XENONnT ›
Klein Bottle Cosmology ›
Constraining meV Axion Dark Matter with ALMA Observations of the Galactic Center Magnetar SGR 1745-2900 ›
Gravitational Foundations and Exact Solutions in $n$-Dimensional Fractional Cosmology ›
Baryon-dark matter coincidence in Randall-Sundrum Model ›
Infrared Spectral Gap in a Gluonic Dark Sector and the Galactic Acceleration Scale ›
Gauge-independent approach to inflation in quadratic gravity ›
Transport of electrons in tangled magnetic fields ›
Detection of Gravitons by Measuring Excess of Photon Luminosities from Interstellar and Intergalactic Hydrogen ›
Dynamic Alignment as a Statistical Survival Effect ↓↑