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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Chmury

Opady

Niebo
Temperatura
10.9 °C
Wilgotność
57%
Wiatr
4.8 km/h
Ciśnienie
1016.6 hPa

Księżyc
Najnowsze prace na astro-ph:
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Towards a Foundation Model for the Martian Atmosphere ›
The energy conditions and model selection in the local Universe ›
First head-to-head comparison of agentic AI applied to the analysis of simulated data of the Einstein Telescope ›
The incidence and star-formation properties of X-ray active galactic nuclei across the star-forming main sequence in DESI-eRASS1: the role of host-galaxy morphology ›
Photometry is all you need: supernova classification as a mixing problem ›
Assessing Ariel's capabilities to observe free-floating brown dwarfs ›
Delayed Radio Flares in Tidal Disruption Events from Star-Disk Collision Outflows ›
Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe ›
A 1% distance to the Large Magellanic Cloud measured by population-II pulsating stars using Gaia Data Release 3 ›
Dominated-Convergence Failure in Cosmological Perturbation Theory and a Numerical Foundation for BBGKY+ZA ›
Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability ›
Dust grain chemistry in the diffuse ISM towards the black hole transient GX 339-4 ›
Closing the UV Gap: Rest-frame EUV science from high-redshift QSOs as a legacy-defining capability ›
Supermassive black holes in six triaxial galaxies: Insights from SINFONI and MUSE observations ›
Massive Stars in the Thirties: awaiting new Hubble discoveries ›
A Deep Study of the Spiral Galaxy W2246f ›
Three-dimensional Conditional Diffusion Models for Cosmological 21 cm Lightcone Emulation ›
JWST's Dusty Blue BOAT -- GRB 221009A ›
Nebular Fingerprints of a Violent White Dwarf Merger: 3D NLTE Modelling of Type Ia Supernovae ›
Kolmogorov--Arnold Networks as Implicit Regularizers: Noise Robustness and Interpretability for Stellar Classification ›
Multi epoch spectroscopic variability of the B supergiant HD75149 ›
Ejected Surface Regolith as a Potential Source Material for Centaur Rings ›
Using GALEX UV Excess to Search for Metal-poor Halo Stars ›
Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole ›
Next-generation Exo-REM atmospheric models: application to VHS 1256 b to emulate patchy clouds ›
The MeerKAT Thousand-Pulsar Polarization Array I: Properties of the Polarization and Rotation Measure Time Series Data ›
Compact near infrared sources in the center of the extraordinary galaxy IC 860 ›
Shock wave formation in the thermosphere by an earthgrazing fireball: Empirical evidence for volatile-enhanced hydrodynamic shielding ›
Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars ›
Constraints on the Atmospheric Composition of 2002 XV$_{93}$ from JWST Spectroscopy ›
A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages ›
Recoil-regulated extreme mass-ratio inspirals in AGN disks ›
Modeling the Effect of the Heliospheric Magnetic Field on Cosmic Ray Muon Shadows ›
Development and demonstration of a Modular Astrobiological Experiments (MAEx) payload for autonomous biological monitoring in Low Earth Orbit (LEO) ›
Modeling Solitonic Cores, Stabilization of Bar, and Suppression of Bar Dissolution in DDO 168 via GPP Formalism: A Detailed Analysis of Bose--Einstein Condensate/Fuzzy Dark Matter Halo Structure and Bar Dynamics in the Dwarf Galaxy DDO 168 ›
ODIN: Rest-frame Optical Morphologies and Star Formation Activity of Ly{\alpha} Emitters at z=2.4, 3.1, and 4.5 ›
Sub-luminous Type IIP SN 2024abfl as a result of a significantly low energy Fe-core collapse ›
The Impact of the New $^{59}$Fe Decay Rates on $^{60}$Fe and $^{26}$Al Nucleosynthesis in Massive Stars ›
A Note on QPE Timing: False Alarms in O-C ›
DELOS: Detecting Shallow Transits in Kepler Photometry Using a Contrastive-Learning Framework ›
Optical transmission spectrum of HAT-P-47b: evidence for aerosols and tentative TiO absorption ›
From reflection to scattering: polarimetric signatures of funnel-type outflows. Modeling obscured ultraluminous X-ray sources ›
Multiple populations detection with the Chinese Space Station Survey Telescope main survey camera ›
Time-Domain Deep Learning for Pairwise Identification of Strongly Lensed Gravitational-Wave Candidates ›
Sub-surface structural changes associated with successive 11-yr solar activity cycles have been progressively more confined near the surface: new helioseismic results on Cycles 22 -- 25 from BiSON ›
An Obscured Tidal Disruption Event Uncovered by Its Mid- and Near-Infrared Dust Echo in a Star-Forming Galaxy ›
A New Cartwheel-like Collisional Ring Galaxy ›
MAMMOTH-Grism: Gas-phase Metallicity Gradients of Star-forming Galaxies in Protocluster Environments at Cosmic Noon ›
Enhanced All-Distance Equi-Zenith Angle Method for Cosmic-Ray Anisotropy Measurement ›
Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters ›
Model Independent Probe of Variation of Cosmic Opacity with Redshift ›
The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects ›
A Calibrated Bayesian Search for Potential Chemical Technosignatures in Polluted White Dwarf ›
The asymmetric carbon-rich chemistry of the planet-forming disk of HD 142527 triggered by late infall ›
Exploring the High-Redshift 21-cm Signal via Self-Consistent Simulations using Artificial Neural Network Emulation ›
Transient Signatures of Star-Envelope Collisions in Little Red Dots ›
Evidence of triggered star formation in the Pillars of Creation from JWST observations ›
Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine ›
Modeling carbon outgassing from chondritic planetesimals ›
Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS ›
High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy ›
Dust dynamics in disk dust traps and late planetesimal formation ›
Quantifying the effect of passband on observations in the Ca II K line ›
Detection of unidentified molecular pure rotational lines in C-rich PNe I. The fullerene-containing PN IC 418 ›
An archival summary: 15 years of ALMA observations on disks and planet formation ›
Long-Duration GRB 211211A: Internal Energy Dissipation Driven by a Long-Lived Magnetar ›
Extending Hubble into the 2030s to Resolve the Physics of LyC Escape ›
The outer rings of SN 1987A from year 1994 to 2024: morphology, light curves, and optical to mid-infrared spectra ›
The Shape of (486958) Arrokoth ›
The evolution and internal structure of Neptunes and sub-Neptunes II. Convective mixing and thermal conductivity ›
Cosmo-PINN: A Physics-Informed Neural Network for Cosmological Reconstruction ›
Determining the incidence rate of magnetic $\delta$ Scuti candidates with CoRoT ›
A new completely parameter-free clustering algorithm for unsupervised classification of BATSE gamma-ray bursts ›
The Architecture of the 14 Herculis System Suggests Primordial Ejection of a Massive Planet ›
The Northern Cross Fast Radio Burst project: VI. The INCART public database ›
Signals from the early Universe: a comprehensive search for primordial features in Planck CMB datasets ›
Efficient computation of the galaxy angular bispectrum in redshift space ›
From Images to Orbits: A Hubble 2030s Astrometric Legacy for the M31-M33 Star Cluster Systems ›
Late-time Quantum Vacuum Decay and its Cosmological Implications ›
Augmented Correlation Functions for Spectroscopic Galaxy Surveys ›
Effective chemical potential and its phenomenological implications for the Hubble parameter ›
A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino ›
When the Ringing Stops: Purely Imaginary Modes in the Ringdown Spectrum of Dynamical Black Holes ›
Signatures of loop quantum gravity in primordial black hole cosmologies ›
Visible inelasticity as a probe of tau flavor content of astrophysical neutrinos ›
Dynamical Tsallis WIMP Freeze-Out and Residual Memory Channels in the Radiation Sector ›
Statistical study of energy dissipation in magnetic structures during turbulent reconnection in the Earth's magnetotail ›
Quantum transitions of vector vortex light in gravitational waves ›
Problems of cosmology on small scales of the Universe ›
Black Hole Photon Rings Saturate the Quantum Chaos Bound ›
Propagation of waves in weakly ionized two-fluid plasmas. II. Nonlinear Alfv\'enic waves ›
Supermassive black hole seeds from direct collapse of CDM-curvature peaks ›
Characterization of Spurious Charge in SENSEI Skipper-CCDs ›
Physics Is All You Need? A Case Study in Physicist-Supervised AI Development of Scientific Software ›
Modeling spectra of MN112 ›
Evidence for a sign change of the ISW effect in the very recent universe? hot voids and cold overdensities at $z ›
Long-Lived Isomers of C$_{11}$H$_9^+$: New Experimental Insights from the PIRENEA Setup ›
Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies ›
Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections ›
Spin Precession Signatures as an Indicator of Microlensing in Strongly Lensed Gravitational Waves ›
Gravitational lensing by a spiral galaxy I: the influence from bar's structure to the flux ratio anomaly ›
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae ›
Quokka-based understanding of outflows (QED) -- IV. Limitations of H$\alpha$ as an outflow diagnostic ›
The Sesquinary Catastrophe on Deimos can reconcile its excited past with its dynamically cool present ›
Considering lensing effect on gravitational wave signals from black holes in mass gap ›
Spectral State Switching in Mrk 421: Results from the AstroSat LAXPC/SXT Observations ›
Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots ›
A multi-technique search for year-scale $\gamma$-ray quasi-periodic modulation in the high-redshift FSRQ PKS~2052$-$47 ›
Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys ›
Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS ›
An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics ›
Inspectorch: Efficient rare event exploration in solar observations ›
Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance ›
Path Measures for Stochastic Galaxy Formation on Layered Halo Graphs ›
The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters ›
A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations ›
Circular polarization images of Sgr A* for different magnetic field geometries ›
Oort Cloud Ecology -- IV. Exchanging Asteroids ›
The POKEMON Speckle Survey of Nearby M dwarfs. IV. Distance-Limited Catalog (POKEMON-DLC) ›
Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks ›
The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants ›
Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444 ›
Mars as an Exoplanet: Lessons from a Planet at the Edge of Habitability ›
CMB Acoustic Power Spectra in STVG-MOG ›
Formation of intermediate-mass black holes in young massive clusters detected with JWST: analytic mass estimates ›
Scattered light signatures of flyby-induced warps in protoplanetary discs ›
A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum ›
Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction ›
The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios ›
Bar-halo interaction: the role of orbital anisotropy ›
Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena ›
Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the $52^{\circ} ›
FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays ›
Microcanonical Hamiltonian Monte Carlo ›
Neutrino Physics and Astrophysics at Colliders ›
Gravitational Wave Signatures of $\mathrm{U(1)_X}$ Breaking and Right-Handed Neutrino Dynamics ›
Effective matter sectors from modified entropies ›
Massive boson stars: Stability and GW emission in head-on mergers ›
Enhancing online estimation of CBC parameters with the low-latency MBTA analysis ›
The reason peculiar velocities grow faster in general relativity than in Newtonian gravity ›
Isentropic hybrid stars in the Nambu-Jona-Lasinio model: effects of neutrino trapping ›
GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog ›
Inflation with vector fields revisited: non-Gaussianities ↓↑