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Obserwatorium Astronomiczne na Suhorze

Teleskop 60cm na Suhorze

Kamerka S

Kamerka N

Niebo
Temperatura
1.7 °C
Wilgotność
94%
Wiatr
9.7 km/h
Ciśnienie
1008.1 hPa

Księżyc
Najnowsze prace na astro-ph:
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Generating background-corrected VPHAS+ HiPS with Montage ›
Metallicity regulates planet formation across all masses ›
Definition of Exoplanets and Brown Dwarfs ›
Analytic Marginalization over Binary Variables in Physics Data ›
How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood ›
Shadows of the Colossus: Hierarchical Black Hole Mergers in a 10-million-body Globular Cluster Simulation ›
XRISM constraints on the velocity power spectrum in the Coma cluster ›
Suppressed "lump" EM signature in radiation pressure dominated accreting massive black hole binaries ›
The velocity dispersion profile of nine open clusters in the solar neighborhood ›
Likelihood Reconstruction for Radio Detectors of Neutrinos and Cosmic Rays ›
Illuminating the Diffuse Radio Emission in Low-Mass Cluster: Abell 13 ›
Characterizing Low-Latency Sky Localization in Multi-Detector Gravitational-Wave Networks ›
Dynamical Dark Energy Meets Varying Electron Mass: Implications for Phantom Crossing and the Hubble Constant ›
SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations ›
Under Pressure: Decoding the Effect of High Densities on Derived Nebular Properties ›
Earth Analogs in Reflected Light: Insights from Early Spectral Characterization in Unconstrained Orbits ›
Evidence for Dynamical Dark Energy using DESI DR2 Ly$\alpha$ Forest ›
On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants ›
Tracing The Start and End of Cosmic Reionization - Exploring The Role of Ionizing Sources as drivers ›
Quasi-Biennial Oscillations and Rieger-type Periodicities in a Babcock-Leighton Solar Dynamo ›
The variability angular diameter distance and the intrinsic brightness temperature of active galactic nuclei ›
Impact of Charge Transfer Inefficiency on transit light-curves: A correction strategy for PLATO ›
The Solar Neighborhood. LV. M Dwarf Twin Binaries -- One in Five Twin Sibling Pairs Are Mismatched in Activity and/or Rotation ›
Discovery of multi-temperature coronal mass ejection signatures from a young solar analogue ›
Do Young Suns Produce Frequent, Massive CMEs? Results from Five-year Dedicated Optical Observations of EK Draconis and V889 Hercules ›
Coronal Mass Ejections from Young Suns: Insights from Solar and Stellar Observations and Models ›
The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations ›
A great diversity of spectral shapes in the ionising spectra of z ~ 0.6 - 1 galaxies revealed by HST/COS and possible detection of nebular LyC emission ›
Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation ›
Constraining the Hubble Constant using Cross-Correlation of Gravitational Wave Events with Flux-Limited Galaxy Catalog ›
RGC: a radio AGN classifier based on deep learning. I. A semi-supervised model for the VLA images of bent radio AGNs ›
Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasi-periodic Eruptions ›
Avoiding PBH overproduction in inflation model with modified dispersion relation ›
K-DRIFT: Unveiling New Imagery of the Hidden Universe ›
Photometric and Spectroscopic Studies of Four Low Mass-ratio Contact Binaries with Period Longer than 0.7 days ›
Analyzing GW231109_235456 and understanding its potential implications for population studies, nuclear physics, and multi-messenger astronomy ›
SWIFTGalaxy: a Python package to work with particle groups from SWIFT simulations ›
Instability and vertical eccentricity variation in global hydrodynamic disk simulations ›
SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit ›
Multivariate Time Series Classification of Fermi - Detected Gamma-Ray Transients Using Convolutional-Recurrent Neural Networks ›
Introducing the Seyfert-LINER Index (SLI): High Resolution ( ›
Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034 ›
Magnesium Isotopic Detection in Cool Stars: Tracing Nucleosynthetic Signatures from MgH Features ›
Multi-Modal Masked Autoencoders for Learning Image-Spectrum Associations for Galaxy Evolution and Cosmology ›
Detecting ultralight dark matter in the Galactic Center with pulsars around Sgr A* ›
Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations ›
Beyond the Local Group - I: Cosmic Filaments Govern the Spatial Alignments of Galaxy Pairs ›
Cosmic magnification on high-redshift submillimeter galaxies ›
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff ›
Discriminating Between Models of the Nanohertz Gravitational-Wave Background with Pulsar Timing Arrays ›
Prospects for Observing the Microquasar SS 433 with the LACT Array ›
Radio Follow-Up Observations of a Weak-Line Quasar Exhibiting Remarkable X-ray Variability ›
FOXES: A Framework For Operational X-ray Emission Synthesis ›
The Missing Mechanism: Picoflare Heating in the Solar Corona ›
Stellar Wind-Blown Bubbles as Environments for Late-Time Rebrightening of Gamma-Ray Burst Afterglows ›
The MDW H{\alpha} Sky Survey: Data Release 1 ›
HI Content of Group Galaxies from the FAST All Sky HI Survey ›
Discovery and Timing Follow-Up of Two FAST-Discovered Pulsars from the FAST CRAFTS Survey ›
Constraint on the physical origin of GRB prompt emission via its non-detected diffuse neutrino emission ›
The cosmochemistry of planetary systems ›
Morphological and Kinematical Diagnostic of FU Orionis-type Outburst Mechanisms ›
Impact of Subsurface Temperature Gradients on Emission Spectra of Airless Exoplanets: the Solid-state Greenhouse and Anti-Greenhouse ›
Revisiting the 150 MHz Radio Luminosity Function of Star-Forming Galaxies with LOFAR Deep Fields through a Refined Statistical Framework ›
Coronal Mass Ejections Deflected by Newly Emerging Flux: A Combined Analytic and Numerical Study ›
Detecting Intermediate-Mass Black Holes out to 20 Mpc with ELT/HARMONI: The Case of FCC 119 ›
A test of Amati relation using HII galaxy distances ›
The Velocity Map Asymmetry of Ionized Gas in MaNGA II. Correlation between Velocity Map Morphology, Star Formation, and Metallicity in Regular Disk Galaxies ›
SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope ›
SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction ›
Spatially Resolved, Multiphase Mass Outflows of the Seyfert 1 Galaxy NGC 3227 ›
Exploring the accelerating black holes from the observations of quasi-periodic oscillations in X-ray binaries ›
Testing the cosmic distance duality relation using model-independent approach ›
A Statistical Study of delta-Sunspots from Solar Cycle 23 to 25 ›
Evaluating the chromospheric structure model of AD Leo using RH1.5D and magnetic field data ›
A Search for Supermassive Black Hole Binary Candidates in 46-Year Radio Light Curves of 83 Blazars ›
Constraining and Comparing the Dynamical Dark Energy and f(R) Modified Gravity Models with Cosmological Distance Measurements ›
Revisiting Very High Energy Gamma-Ray Absorption in Cosmic Propagation under the Combined Effects of Axion-Like Particles and Lorentz Violation ›
Luminosity Functions and Detectability of Binary Neutron Star Merger-nova Signals with Various Merger Remnants ›
A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene ›
The Detectability of Lunar-Origin Asteroids in the LSST Era ›
The Sun as an X-ray star V.: A new method to retrieve coronal filling factors ›
Recasting and Forecasting Dark Matter Limits Without Raw Data: A Generalized Algorithm for Gamma-Ray Telescopes ›
Open-Source High-Fidelity Orbit Estimation for Planetary Science and Space Situational Awareness Using the Tudat Software ›
Spinning-down RU Lup. Constraints on the physics of the outflow from high-resolution spectroscopy ›
QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra ›
Fundamental effective temperature measurements for eclipsing binary stars - VI. Improved methodology and application to the circumbinary planet host star BEBOP-3 ›
Development of the Reconstruction Procedure of the Fluorescence detector Array of Single-pixel Telescopes for measuring Ultra-High Energy Cosmic Rays ›
Using Type-II Cepheids as Extragalactic Standard Candles: Distances to M31 ›
Automated Exploration of Radical-Molecule Chemistry: The Case of Oxirane + CH in the ISM ›
Fine details in solar flare ribbons: Statistical insights from observations with the Swedish 1-m Solar Telescope ›
The spatial distribution of dwarf and giant galaxies in and around Virgo cluster ›
Energetics of star-planet magnetic interactions: Novel insights from 3D modelling ›
The effects of stellar activity cycles on planetary atmospheric escape and the HeI 1083nm transit signature ›
Can KM3-230213A be compatible with a cosmogenic origin? ›
The AMBRE Project: Line-broadening and stellar rotation of ESO/FEROS archived spectra ›
The role of supercluster filaments in shaping galaxy clusters ›
The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model ›
Alma Luminous Star catalogue IV: A Massive star census in the Magellanic Clouds ›
The Programmable Liquid-crystal Active Coronagraphic Imager for the 4-m DAG telescope (PLACID) instrument: installation and commissioning update ›
The Cosmic Baryon Cycle in IllustrisTNG: flows of mass, energy, and metals ›
First detection of ultra-high energy emission from gamma-ray binary LS I +61 303 ›
The influence of a stably stratified layer on the hydromagnetic waves in the Earth's core and their electromagnetic torques ›
From Rare Events to a Population: Discovering Overlooked Extragalactic Magnetar Giant Flare Candidates in Archival Fermi Gamma-ray Burst Monitor Data ›
The MiMO Catalog: Physical Parameters and Stellar Mass Functions of 1,232 Open Clusters from Gaia DR3 ›
Validating Open Cluster Candidates with Photometric Bayesian Evidence ›
The Near-Ultraviolet Spectra of FU Orionis Accretion Disks ›
Solar flare forecasting with foundational transformer models across image, video, and time-series modalities ›
MIGHTEE-HI: The HI mass-stellar mass relation of massive galaxies and the HI mass function at 0.25 ›
Improved UVIS Aperture Corrections derived from Focus Diverse PSF Maps ›
A targeted radio survey of infrared-selected bow shock candidates ›
Dynamical friction shear and rotation in Chaplygin cosmology ›
Separation of gain fluctuations and continuum signals in total power spectrometers with application to COMAP ›
Unveiling stellar (and planetary) internal dynamics with the fully compressible MUSIC code ›
Galactic bars and active galactic nucleus fuelling in the second half of cosmic history ›
Unveiling the collision between molecular outflows: observational evidence and hydrodynamic simulations ›
Discovery of SN 2025wny: a Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01 ›
The MandelZoom project II: the impact of stellar feedback on black hole accretion through an $\alpha$-disc in dwarf galaxies with a resolved interstellar medium ›
Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44 ›
Dark Energy Survey Year 6 Results: Clustering-redshifts and importance sampling of Self-Organised-Maps $n(z)$ realizations for $3\times2$pt samples ›
Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies ›
COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars ›
Cosmic magnification on multi-catalogue Herschel submillimetre galaxies ›
The Compressed 3D Lyman-Alpha Forest Bispectrum ›
HST-COS Transit Spectroscopy of KELT-20b: First Detection of Excess Far-ultraviolet Absorption From an Ultra-hot Jupiter ›
Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach ›
Propellantless space exploration ›
A Search for Ultra-Light Vector Dark Matter with a Rotating Torsion Balance ›
Beyond Point Matching: Evaluating Multiscale Dubuc Distance for Time Series Similarity ›
Electroweak Baryogenesis with \texttt{BARYONET}: a self-contained review of the WKB approach ›
Superhorizon Isocurvature as a Window into Dark Matter Production ›
Seafloor Topography Enhances KM3NeT Sensitivity to ANITA-like Events ›
Bubble wall velocity with out-of-equilibrium corrections ›
Zernike Mode Sorting with Vortex Phase Filters: Perfect Coronagraphs and Ideal Wavefront Sensors ›
Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework ›
The Ultra Slow-Roll Phase Of Warm Inflation In Braneworld Cosmology ›
Symmetry principles of gravitational perturbations in thermal environments ›
Thermodynamic Geodesics in Bardeen Regular Black Hole: Conventional vs. Modified Geometrothermodynamics Metrics ›
Refined Low-Energy Supernova Constraints on Lepton Flavor Violating Axions ›
Some Properties of Multi-Component Axion Dark Matter ›
Primordial black hole formation from collapsing domain walls with full general relativity ›
Exploring the Landscape of Spontaneous CP Violation in Supersymmetric Theories ›
Tensor network methods for quantum-inspired image processing and classical optics ›
Validation of field cage and cathode for low radioactivity operation with the CYGNO experiment ›
Lensing, not luck! Detection prospects of strongly lensed gravitational waves ›
Charge Trap Analysis in a SENSEI Skipper-CCD: Understanding Low-Energy Backgrounds in Rare-Event Searches ›
Observable Signatures of Quarkyonic Phase in Neutron Stars ›
Scheduling multiple agile Earth observation satellites with multiple observations ›
Galactic Positrons from Thermonuclear Supernovae ›
Evolutionary optimization of cosmological parameters using metropolis acceptance criterion ›
Ultra-high-energy Cosmic Ray Sources can be Gamma-ray Dim ›
GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump ›
Breaking boundaries: extending the orbit-averaged Fokker-Planck equation inside the loss cone ›
A Quadratic Equation of State to Cosmic Acceleration: Entropy Evolution and Phantom Crossing ›
galsbi: A Python package for the GalSBI galaxy population model ›
The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum ›
Structure and Dynamics of the Young Massive Star Cluster Westerlund 1 ›
Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations ›
Forecasts for interacting dark energy with time-dependent momentum exchange ›
The Route to Unveil the Cosmic Genealogy of Supermassive Black Hole Binaries Using Nano-Hertz Gravitational Waves and Galaxy Surveys ›
Magnetorotational instability in a solar near-surface mean-field dynamo ›
Modeling the Light Curve and Spectra of SN 2023aew ›
The mantle-inner core gravitational mode of oscillation in a strong magnetic field regime ›
Radiation-magnetohydrodynamic Simulations of Accretion Flow Formation After a Tidal Disruption Event ›
Tracing cosmic voids with fast simulations ›
Hybrid Quark Stars with Quark-Quark Phase Transitions ›
SAMPLE -- Stratospheric Altitude Microbiology Probe for Life Existence -- A Method of Collection of Stratospheric Samples Using Balloon-Borne Payload System ›
Harnessing the potential of PyStoch: detecting continuous gravitational waves from interesting supernova remnant targets ›
Radio signatures of AGN-wind-driven shocks in elliptical galaxies: From simulations to observations ›
Radio Emission from a Nearby M dwarf Binary ›
The 300 TeV photon from GRB 221009A: a Hint at Non-linear Lorentz Invariance Violation? ›
Carpet-3 300 TeV Photon Event as an Evidence for Lorentz Violation ›
DIPLODOCUS I: Framework for the evaluation of relativistic transport equations with continuous forcing and discrete particle interactions ›
Fractality of open clusters in singles, pairs, and groups ›
Search for Past Stellar Encounters and the Origin of 3I/ATLAS ›
Fast X-ray Transient Detection with AXIS: application to Magnetar Giant Flares ›
Assessing the feasibility range of Solar-powered Planetesimals Redirection operations for Terraforming ›
Neural Enhancement of the Traditional Wang-Sheeley-Arge Solar Wind Relation ›
Stellar halo subtraction alternative for accreting companions' characterization with integral field spectroscopy: Analytical and on-sky demonstration on the PDS70, HTLup, and YSES1 systems ›
Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases ›
The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666 ›
von Karman - Howarth Similarity of Spatial Correlations and the Distribution of Correlation Lengths in Solar Photospheric Turbulence ›
CHRONOS: Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter ›
MEGATRON: the impact of non-equilibrium effects and local radiation fields on the circumgalactic medium at cosmic noon ›
A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane ›
JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the Explosion ›
Spatio-Temporal Evolution of the March 2022 ICME Revealed by Multi-Point Observations of Forbush Decreases ›
DIPLODOCUS II: Implementation of transport equations and test cases relevant to micro-scale physics of jetted astrophysical sources ›
Non-linear structure formation with elastic interactions in the dark sector ›
A family of binaries with an extreme mass ratio ›
Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-Significance Gravitational Wave Event S250818k ›
Close-in faint companions mimicking interferometric hot exozodiacal dust observations ›
Pre-perihelion Development of Interstellar Comet 3I/ATLAS ›
Debiasing cosmological parameters from large-scale foreground contamination in Cosmic Microwave Background data ›
Doubling the Number of Blue Large-Amplitude Pulsators: Final Results of Searches for BLAPs in the OGLE Inner Galactic Bulge Fields ›
Covariant diagonalization of the perfect fluid stress-energy tensor ›
Superradiant scattering of electromagnetic fields from ringing black holes ›
Primordial Non-Gaussianity from Light Compact Scalars ›
Phase transitions in the inner crust of neutron stars within the superfluid band theory: Competition between $^1\text{S}_0$ pairing and spin polarization under finite temperature and magnetic field ›
Entanglement between pair-created twin universes with opposite time arrows should leave a birthmark on CMB spectrum ›
Constraining the Coexistence of Freeze-in Dark Matter and Primordial Black Holes ›
Can local White Dwarfs constrain Dark Matter interactions? ›
On the Present Status of Inflationary Cosmology ›
Avoidance of Big Crunch Singularity in the Q-SC-CDM model via nonminimal coupling: Theory and Data Analyses ›
Smooth hybrid inflation in light of ACT DR6 data ›
Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries ›
A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario ›
Imprints of screened dark energy on nonlocal quantum correlations ›
GWKokab: An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources ›
Ghost-free, gauge invariant SVT generalizations of Horndeski theory ›
Gravitomagnetic-Hydrodynamics and Turbulence in Early Universe ›
Axion Perturbations: A General Analytical Treatment ↓↑