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Obserwatorium Astronomiczne na Suhorze

Teleskop 60cm na Suhorze

Kamerka S

Kamerka N

Niebo
Temperatura
-0.7 °C
Wilgotność
81%
Wiatr
0.0 km/h
Ciśnienie
1005.7 hPa

Księżyc
Najnowsze prace na astro-ph:
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Delayed Wind Onset in Pa 30, the Remnant of Type Iax SN 1181 ›
V570 Per: Characterization of a Benchmark Eclipsing Binary ›
Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity? ›
Mixing between AGN winds and ISM clouds produces luminous X-ray emission ›
First Mid-infrared Detection and Modeling of a Flare from Sgr A*. II. Mid-IR Spectral Energy Distribution and Millimeter Polarimetry ›
Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE): a likely aligned orbit for the 3 Myr planet TIDYE-1 b ›
Variability-selected AGN in dwarf galaxies: the incidence of AGN in dwarf and massive galaxies is similar ›
Probing the influence of the protocluster environment on galaxy morphology at z = 2.23 ›
J-HERTz: J-PLUS Heritage Exploration of Radio Targets at z $ ›
Mid-infrared extinction toward the Galactic center ›
Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre ›
Large Language Model Driven Analysis of General Coordinates Network (GCN) Circulars ›
Radio properties of the quasi-periodic eruption source RXJ1301.9+2747 at parsec scales ›
Tidal Disruption Events ›
Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core Collapse ›
SN 2023taz: Implications for the UV Diversity of Superluminous Supernovae ›
Simulations of a Conducting Sphere Moving through Magnetized Plasma: Alfv\'en Wings, Slow Magnetosonic Wings, and Drag Force ›
Proton specific entropy as a proxy for the $O^{7+}/O^{6+}$ charge state ratio over heliocentric distance ›
Constraining the Jet Energetics of the Transient X-ray Binaries MAXI J1348-630 and MAXI J1820+070 through Calorimetry ›
Understanding the Origin and Dynamical Evolution of the Unique Open Star Cluster Berkeley 20 using FIRE Simulations ›
A Neural Network Approach to Preferred Event Selection for Low-Latency Gravitational-Wave Alerts ›
Toward Complete Merger Identification at Cosmic Noon with Deep Learning ›
Relative Strengths of Fundamental and Harmonic Emissions of Solar Radio Type II Bursts ›
Hyperaccretion-driven relativistic jets from massive collapsars in active galactic nucleus disks ›
Deep-learning mitigation of foregrounds and beam effects in 21-cm intensity mapping using hybrid frequency differencing and PCA ›
The ALMA-QUARKS survey: Evidence of a candidate high-mass prestellar core aside a bright-rimmed cloud IRAS 18290-0924 ›
Implications of the Two-Component Dark Energy Model for Hubble Tension ›
PHR~J1724-3859: A Bipolar Planetary Nebula in Open Cluster Trumpler 25 ›
Solar Periodic Companion and Random Stellar Flybys: Dynamical Perturbations of Highly Eccentric Comets in the Oort Cloud ›
Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter ›
Electron Cyclotron Maser Emission as the Driving Mechanism in Long-Period Radio Transients ›
Non-thermal processes in standard big bang nucleosynthesis: III. Reactions with slow nuclei and the overall effect ›
Gravitational Wave Phase shifts of black hole mergers in AGN Disks ›
Evolution of action-space coherence in a Milky Way-like simulation ›
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. IV. Broad Emission Line Evolution Sequence Among H{\alpha}, Mg II, and H{\beta} ›
The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking ›
Refractive indices of photochemical haze analogs for Solar System and exoplanet applications : a cross-laboratory comparative study between the PAMPRE and COSmIC experimental set-ups ›
A Method for Gamma-Ray Energy Spectrum Inversion and Correction ›
A JWST Transit of a Jupiter Analog: II. A Search for Exomoons ›
Origin of Galaxies ›
Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability ›
Type Iax supernovae as a source of iron-rich silicate dust ›
Galaxy-Multiplet Clustering from DESI DR2 ›
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. V. Dramatic Variability in High-Ionization Broad Emission Lines ›
Simple relations from complex outflows: How the $M-\sigma$ relation emerges in a multi-phase environment ›
Insights on Gas Distribution and Dynamics in Massive Proto-cluster G358.46$-$0.39: Possible Multiplicity in G358.46$-$0.39 MM1a ›
Explosions in the Empty: A Survey of Transients in Local Void Galaxies ›
Elemental abundance ratios for the bulge of M31 ›
Viscous Dark Energy and Mass-Varying Dark Matter in Lyra Manifold: Cosmological Dynamics and Observational Constraints ›
21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter ›
Advancing Identification method of Gamma-Ray Bursts with Data and Feature Enhancement ›
Optical gains measurement with a gain scheduling camera: On-sky demonstration with PAPYRUS and perspectives ›
Challenging the $\omega_0\omega_a$CDM parametrization through rational expansions in view of DESI data release ›
LCS: A Learnlet-Based Sparse Framework for Blind Source Separation ›
Probing the disk-jet coupling in M87 ›
Efficient Exoplanet Imaging Simulations of the Habitable Worlds Observatory ›
Identification of periodic density structures in Solar Orbiter data: Radial evolution ›
Using Light Curve Derivatives to Estimate the Fill-out Factor of Overcontact Binaries ›
The VVVX quest for satellites around the Circinus galaxy ›
Is There New Physics Beyond 30 TeV in the BOAT? ›
Quadruple system HD 135160 in a unique 2+2 configuration ›
Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data ›
Catching the 2021 {\gamma}-ray flare in the blazar TXS 2013+370 ›
Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break ›
Reporting a Deficit of Intrinsic NV Absorbers in Core-dominated, Radio-loud Quasars ›
The Cherenkov Camera for the PBR mission ›
The data processing system of the POEMMA-Balloon with Radio mission ›
The JWST weather report from the nearest brown dwarfs III: Heterogeneous clouds and Thermochemical instabilities as possible drivers of WISE 1049AB's spectroscopic variability ›
Impact of cosmic expansion on gravitational wave spectra from strongly supercooled first-order phase transitions ›
The Relationship Between Emission Line and Continuum Luminosity and the Baldwin Effect in Blazars. I. The Case of the Mg II {\lambda}2798 {\AA} Emission Line ›
The Atacama Cosmology Telescope: Cross-correlation of kSZ and continuity equation velocity reconstruction with photometric DESI LRGs ›
Detection of a highly stable orbital-period signal in GRACE-FO one-way intersatellite ranging using a synchronization-free differential observable (origin currently unidentified) ›
On the Theory of Bulk Viscosity of Cold Plasmas ›
The significance of Halley's Comet in the Bayeux Tapestry ›
The Physics of Black Holes and Their Environments: Consequences for Gravitational Wave Science ›
Low-frequency radio telescopes sensitivity to light dark matter ›
511 keV Gamma Ray Echo from Particle Decays in Supernovae ›
Improved cosmological constraints on axion-lepton interactions ›
Computational and Experimental Comparison of CLF5605 and roamx-0201 Martian Helicopter Rotor Airfoils ›
IonCast: A Deep Learning Framework for Forecasting Ionospheric Dynamics ›
The effects of dark energy on the matter-gravity coupling ›
Power-law Bianchi type I inflation with multiple vector fields ›
Divergence in tracing the flavors of astrophysical neutrinos: can JUNO help IceCube? ›
Gravitational Bound State Perturbations Inside Black Holes and Isospectrality ›
Dynamical Evolution and Graceful Exit in Quartic Warm Inflation ›
A New Definition of Horndeski Theory and the Possibility of Multiple Scalar Field Extensions ›
Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors ›
Wavelengths and Energy Levels of Neutral Manganese (Mn I) Determined Using High-Resolution Fourier Transform and Grating Spectroscopy ›
Turbulence in the terrestrial magnetosheath: space-time correlation using the Magnetospheric Multiscale mission ›
Relativistic mean-field model with density- and isospin-density-dependent couplings ›
Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation ›
Formation of neutron stars inside planetary nebulae via accretion-induced collapse and core-merger-induced collapse from white dwarf binaries ›
A Novel Density Profile for Isothermal Cores of Dark Matter Halos ›
Isolated Binary Black Hole Formation and Merger Rates from Galaxy Evolution ›
Halo spin and orientation in Interacting Dark Matter Dark Energy Cosmology ›
UHECR deflections in the coherent Galactic magnetic field ›
Structure Formation with Warm White Noise: Effects of Finite Number Density and Velocity Dispersion in Particle and Wave Dark Matter ›
Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network ›
Detection of a Type-C QPO during the soft-to-hard transition in Swift J1727.8-1613 ›
Smoking gun signature from axion and the constraints with radio telescopes ›
Spectroscopic Characterization of redMaPPer Galaxy Clusters with DESI ›
Analytical Transit Light Curves for Arbitrary Power-Law Limb Darkening: A Unified Framework ›
Understanding the Drag Torque in Common Envelope Evolution ›
Cool Gas in the Circumgalactic Medium of Massive Post Starburst Galaxies ›
JWST's PEARLS: A Candidate Massive Binary Star System in a Lensed Galaxy at Redshift 0.94 ›
Investigating the Growth of Little Red Dot Descendants at z ›
DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry ›
Globular Clusters in the Galaxy Cluster MACS0416 at z = 0.397 ›
Dance to Demise -- How Massive Stars May Form Dense Circumstellar Shells Before Explosion ›
MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components ›
The source of the cosmic-ray excess in the Centaurus region -- constraints on possible candidates, mass composition and cosmic magnetic fields ›
Unlocking 21cm Cosmology with SBI: A Beginner friendly NRE for Inference of Astrophysical Parameters ›
Detecting Local and Integrated Relativistic Effects by Multi-Tracing a Single Galaxy Population in Harmonic Space ›
Gravitational Recoil and Suppression of Super Massive Black Hole Seeds in the Early Universe ›
Dust Attenuation of Lyman-Werner Feedback: Reassessing Early Super Massive Black Holes Seed Formation ›
A simple, flexible method for timing cross-calibration of space missions ›
Kinematics of Stellar Streams from Globular Clusters Depend on Black Hole Retention and Star Mass: A Selection Effect for Dark Matter Inference ›
Bayesian Gaussian Methods for Robust Background Modeling in CALorimetric Electron Telescope (CALET) Gravitational-Wave Searches ›
Cosmological constraints on nonphantom dynamical dark energy with DESI Data Release 2 Baryon Acoustic Oscillations: A 3$\sigma$+ lensing anomaly ›
Orbital decay candidates reconsidered: WASP-4 b is not decaying and Kepler-1658 b is not a planet ›
The ALPINE-CRISTAL-JWST Survey: Stellar and nebular dust attenuation of main-sequence galaxies at z~4-6 ›
Efficient analytic approximation for small-scale non-cold relic perturbations ›
XRISM Spectroscopy of the Stellar-mass Black Hole GRS 1915+105 ›
An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise ›
The interstellar flux gap: From dust to kilometer-scale objects ›
Kerr Black Hole Shadows in Dispersive Plasma: Frequency-Dependent Geodesics and Shadow Distortions ›
JWST/NIRCam observations of HD~92945 debris disk: An asymmetric disk with a gap ›
Conservation laws in non-inertial frames and non-conservation of energy of relative motion in two-body problem ›
Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections ›
Recalibrating Inflation: Insights from Starobinsky Gravity ›
Foreground removal in HI 21 cm intensity mapping under frequency-dependent beam distortions ›
JWST observes the assembly of a massive galaxy at z~4 ›
Stellar Flares in the TESS Light Curves of Planet-hosting M dwarfs ›
Asteroseismic Imprints of Mass Transfer in Binary Stars: Probing the Interiors of Donors and Accretors with Gravity and Acoustic Modes ›
Magnetic Fields in the Shapley Supercluster Core with POSSUM: Challenging Model Predictions ›
Detector Response to Gravitational Wave Polarizations in Gravitational Quantum Field Theory ›
Understanding large-scale dynamos in unstratified rotating shear flows ›
Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology ›
A waveform and time digitization mainboard prototype for the hybrid digital optical module of TRIDENT neutrino experiment ›
Primordial regular black holes as all the dark matter. III. Covariant canonical quantum gravity models ›
Using tunable coherence for reaching micrometer coherence lengths and suppressing stray light in a power-recycled Michelson interferometer ›
Constraints on the Variation of the QCD Interaction Scale $\Lambda_{\text{QCD}}$ ›
Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network ›
A General Framework for the Spontaneous Scalarization of Regular Black Holes ›
Large-Scale Calculations of $\beta$-Decay Rates and Implications for $r$-Process Nucleosynthesis ›
Generating optimal Gravitational-Wave template banks with metric-preserving autoencoders ↓↑