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Obserwatorium Astronomiczne na Suhorze

Zachód Słońca

Kamerka S

Kamerka N

Niebo
Temperatura
11.4 °C
Wilgotność
55%
Wiatr
1.6 km/h
Ciśnienie
1002.1 hPa

Księżyc
Najnowsze prace na astro-ph:
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Earth Science Foundation Models: From Perception to Reasoning and Discovery ›
Formation of stable exoplanetary systems around pulsars by capture: An exercise in computational classical mechanics ›
Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps ›
Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties ›
Depth of Maximum of Air-Shower Profiles above 10^17.7 eV Measured with the Fluorescence Detector of the Pierre Auger Observatory ›
One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN ›
Tracking down the broadband polarimetric properties of PG 1553+113 ›
The flare and spiral structure of the Milky Way's disc as traced by young giant stars ›
SIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge ›
Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory ›
$\alpha\beta q_\mathrm{th}$-mapping of planet-induced density wave damping in protoplanetary discs ›
Revisiting the ultraviolet spectroscopy of the eta Tel edge-on debris disk ›
On the Numerical Stability of the Diffusion Coefficient in Microscopic Simulations ›
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample ›
The HAges Catalog: Stellar Ages for High Priority HWO Target Stars ›
Light Propagation Prescriptions for Black Hole Movies ›
The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31 ›
A New WZ Sagittae-type Dwarf Nova KSP-OT-202104a Near the Period Minimum from the KMTNet Supernova Program ›
Quantitative Spectroscopic Diagnostics for FU Orionis-Type Young Stellar Objects ›
The Metallicity Distribution of the Ultra-Faint Dwarf Galaxy Segue 1 ›
Assessing the imprint of eccentricity in GW signatures using two independent waveform models ›
Forbidden Formation Histories: The Binary Black Hole Merger Rate Disfavors Long Delay Times ›
Extensions of Brown Hamiltonian-III. Applications to irregular satellites of giant planets ›
Machine-learning applications for weak-lensing cosmology ›
Jets from Scratch: A 3D Dynamo Origin of Long Gamma-Ray Burst Jets ›
A Spatially Resolved HI Survey of Seyfert Galaxies: the Role of AGN Feedback in Shaping Atomic Gas Reservoirs ›
Forward Modeling of Dust-Induced Stray Light in Ground-Based Coronagraphs: A Dual-Path Monitoring Approach for High-Precision Inner Corona Observations ›
On the Reparameterization Between Cartesian Position-Velocity Vectors and Orbital Elements in the Kepler Problem ›
No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114 ›
Revisiting constraints on primordial vector modes and implications for sourced magnetic fields and observed $EB$ power spectrum ›
Height Variations of Magnetoacoustic Cutoff Frequency in the Solar Atmosphere ›
Resonant shear-flow instability in anisotropic supersonic plasmas with heat flux ›
Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus ›
The Accretion Process on Protostars ›
Diversity in Evolutionary Status and Magnetic Activity among Solar-Type Twin Detached Eclipsing Binaries ›
Comparative analysis of missing data imputation methods for CSST survey: Impact on photometric redshift estimation performance ›
Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946 ›
Revisiting the 2021 Outburst of the BHC MAXI J1803-298 Using NICER, NuSTAR, and Insight-HXMT Data ›
Probing nonlinear structure formation beyond $\Lambda$CDM with the LSS bootstrap: a joint power spectrum and bispectrum analysis ›
Fizzy water ice in space: CO$_2$ adsorption, binding energies and its fate in a protoplanetary disk ›
Full non-LTE multi-level radiative transfer II. The case of a 5-level Ca ii atom with broadened excited levels ›
Comet 1P/Halley Completes 15 Orbits in 1,151 Years: Commensurability with the Solar System Quasi-Period and Evidence for Jupiter-Saturn Dynamical Coupling ›
Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational \(H(z)\) Data ›
Magnetar-powered long gamma-ray bursts and connection to superluminous supernovae and fast radio bursts ›
VLTI/PIONIER imaging of post-AGB binaries. An INSPIRING hunt for inner rim substructures in circumbinary discs ›
Self-gravity in thin protoplanetary discs: 2. Numerical convergence solved and revealing the overestimation in mass of formed planets with softening ›
The impact of flickering variability and magnetisation on the dynamics, stability and morphology of radio-loud AGN jets ›
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe ›
COOL-LAMPS IX: A Rare Duo of Quasars Each Lensed by a Single Massive Galaxy Cluster ›
Spectropolarimetric analysis of waves linked to FIP ›
UNIONS-3500 Weak Lensing: IV. 2D cosmological constraints in harmonic space ›
No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison ›
UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space ›
UNIONS-3500 Weak Lensing: I. A Galaxy Shape Catalogue in the Northern Sky ›
On the Apparent Correlation between X-ray and Neutrino Luminosities of Active Galactic Nuclei ›
DEFROST: Detecting Excess in Faraday Rotation thrOugh Sophisticated analysis Techniques ›
Tracing the sulfur depletion in starless and pre-stellar cores ›
Guitar Nebula: extreme accelerator in extreme environment ›
Apocalypse When? Solar System Constraints on an Imminent Big Rip ›
The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet ›
Detector for fast wave trains in the solar radio emission ›
A New PSF Deconvolution Algorithm: Simultaneous Spatial Resolution Enhancement and Point Source Removal for Morphological Analysis of AGN Host Galaxies ›
Inpainting over the cracks: challenges of applying pre-merger searches for massive black hole binaries to realistic LISA datasets ›
Global evolution of electric fields during planet encircling dust storms on Mars ›
Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst ›
Photometric metallicity of Galactic RR Lyrae stars in the Gaia DR3 era ›
From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies ›
The Galaxy Luminosity Functions in ASTRID: Predictions for LSST ›
Phase-resolved field-space distance bounds in ekpyrotic, bouncing and cyclic cosmologies ›
On the Anticipation of Lunar Travel in the Early 20th Century: A Pedagogical Exercise ›
Tunneling and tidal stripping in multifield ultralight dark matter halos ›
How much dark matter really matters? ›
Minimal Majoron Dark Matter ›
Secondary Gravitational Wave Signatures from 5D Rotating Primordial Black Holes in the Dark Dimension ›
Inspiral gravitational waveforms from charged compact binaries with scalar hair ›
The Gravitational Spectral Radio Forest: A Signature of Primordial Black Holes ›
Fixing the Renormalization of Inflationary Loops via Ward Identities ›
Geodesics Structure and Thermodynamic Properties of Gaussian Black Hole in Quadratic Ricci Scaler Gravity ›
Calorimetric approach to paleo-detection of dark matter ›
Quantum Field Theory of Black Hole Perturbations with Backreaction VI. Apparent Horizons, Quasi-Local Mass and Effective Classical Metrics ›
Thin Accretion Disks around Rotating Charged Black Holes in an Effective Higher-Curvature Spacetime ›
Exploring the interplay between star formation efficiency and dust in regulating the UV luminosity of early systems in the JWST and ALMA era ›
TeV to PeV neutrinos from AGN coronae ›
Ram-Pressure Stripping Caught in Action in a Forming Cluster at $z \sim 2.5$ ›
Equation of state during (p)reheating with trilinear interactions ›
Dark Matter and the Early Formation of Supermassive Black Holes ›
Edges In Coadded Images ›
Testing common approximations of neutrino fast flavor conversion ›
Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region ›
Solving the cooling flow problem with combined jet-wind AGN feedback ›
Sub-GeV dark matter in neutron stars: halo morphologies and their suppression by vacuum-like pressure ›
Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. I. Hydrodynamics ›
Oscillations of dark matter halos in galaxies and their effects on motion of stars ›
Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings ›
Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology ›
Interpreting the strong clustering of ultra-diffuse galaxies by halo spin bias ›
Exposure-averaged Gaussian Processes for Combining Overlapping Datasets ›
Scalable Gaussian Processes for Integrated and Overlapping Measurements Via Augmented State Space Models ›
Intermittent Turbulence, Fast Flavor Conversion, and Observable Supernova Probes ›
Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC ›
Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales ›
Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots ›
Optimizing Deep Learning Photometric Redshifts for the Roman Space Telescope with HST/CANDELS ›
Morphological Fingerprints of Forbush Decreases and Their Relation to Geomagnetic Storm Severity ›
Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy ›
Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars ›
Gamma-ray Signatures of r-Process Radioactivity from the Collapse of Magnetized White Dwarfs ›
Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179 ›
Novel insights into the Coma Cluster kinematics with DESI. I. Linking mass profile, orbital anisotropy, and galaxy populations ›
Artificial precession and instability in solar system and planetary simulations: analytic and numerical results ›
An Old, Low-mass, Metal-poor Hypervelocity Star Candidate Consistent with a Galactic Center Origin ›
Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation ›
Studying spherical collapse and its implications in the Eddington-inspired Born-Infeld gravity theory ›
Satellite Metallicity Enhancement I: Suppressed Star Formation, Stellar Mass Loss, and Enriched Inflow of DESI and EAGLE Galaxies around Massive Clusters ›
Empirical estimates of how massive galaxies can be in {\Lambda}CDM ›
FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics ›
A New Timing Signature of Black Hole Spin: Time-Delay Asymmetry in Kerr Accretion Flows ›
Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object ›
Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects ›
On the universality of late-time ringdown tail ›
Towards Stochastic Inflation in Higher-Curvature Gravity ›
Binary Neutron Stars from the Moon: Early Warnings and Precision Science for the Artemis Era ›
Scalar fields around black hole binaries in LIGO-Virgo-KAGRA ›
KM3-230213A and IceCube Neutrino Events from Metastable Dark Matter of Primordial Black Hole Origin ›
Excitation factors for horizonless compact objects: long-lived modes, echoes, and greybody factors ›
Connecting the Dots: A Machine Learning Ready Dataset for Ionospheric Forecasting Models ›
astroCAMP: A Community Benchmark and Co-Design Framework for Sustainable SKA-Scale Radio Imaging ›
Modeling the frequency-domain ringdown amplitude of comparable-mass mergers with greybody factors ›
Design of low-energy transfers in cislunar space using sequences of lobe dynamics ›
A Threshold Model for Micrometeoroid Atmospheric Entry: Filippov Dynamics, Survival Estimates, and Survivor-Only Inverse Limits ›
Gravitational Properties of the Monopole Bag ›
Helicity-dependent corrections to black-hole shadows from the gravitational spin Hall effect ›
Monochromatic neutrinos from scotogenic dark matter ↓↑