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Obserwatorium Astronomiczne na Suhorze

Suhora w nocy

Kamerka S

Kamerka N

Niebo
Temperatura
1.4 °C
Wilgotność
82%
Wiatr
0.0 km/h
Ciśnienie
1028.2 hPa

Księżyc
Najnowsze prace na astro-ph:
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CNN+FoF: application of deep learning to the identification of dark matter haloes ›
A Path to an All-Sky Survey with Roman ›
The DECam MAGIC Survey: Uncovering the Tidal Tails of the Crater II Dwarf Galaxy ›
NOCTURNE. III. Unidentified variable emission in the nuclear regions of PKS 2153-69 ›
Testing models for fully and partially stripped low-mass stars with Gaia: Implications for hot subdwarfs, binary RR Lyrae, and black hole impostors ›
Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres ›
Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal ›
Evolution of Cosmic Voids: Structure, Galaxies, and Dynamics ›
Shock-induced chiral magnetic effect ›
Implications for PBH Dark Matter from a single Sub-Solar$\unicode{x2013}$GW Detection in LVK O1$\unicode{x2013}$O4 ›
Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations ›
FRESCO: Constraining Dust Attenuation and Star-Formation Rates of $z\sim 2$ Star-Forming Galaxies with JWST Paschen and Ground-Based Balmer Emission Line Observations ›
Probing the magnetic fields and dust properties in the young embedded star-forming region AFGL 6366S using Near Infrared and Optical linear polarimetry ›
Rattle-and-Break: the Impact of Planetesimal Scattering on Super-Earth Resonant Chains ›
The MeerKAT 1.3 GHz Survey of the Large Magellanic Cloud ›
Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines ›
The turbulence driving mode in NGC7793 and NGC1313 ›
Complex Analysis of Askaryan Radiation: UHE-$\nu$ Identification and Reconstruction using the Hilbert Envelope of Observed Signals ›
Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission ›
On the Importance of the Convective Urca Process in 3D Simulations of a Simmering White Dwarf ›
Intracluster Medium Fluctuations on Scales up to 1 Mpc: A Combined eROSITA and SPT/Planck Analysis of Abell 3266 ›
Resurgence and Hyperasymptotics in Wave Optics Astronomy ›
Revisiting the Origin of the Star-Forming Main Sequence Based on a Volume-Limited Sample of ~25,000 Galaxies ›
A Decade-Long Increasing Mid-Infrared Luminosity in Galaxy NGC6447: a Turning-On Candidate of Active Galactic Nucleus ›
Conditional Image Diffusion with Interferometric Closure Invariants: Independent EHT Imaging of Centaurus~A and 3C~279 ›
Short-duration GRB 250221A Afterglow Driven by Two-Component Jets from merger of compact star ›
Constraints on neutrino emission and hadronic flux from 1LHAASO catalog $\gamma$-ray sources ›
Performance assessment of the gPLUTO code for the numerical modeling of radio galaxy evolution ›
Bulk and turbulent gas motions in the interacting galaxy cluster Abell 3395 South observed with XRISM ›
HATPI Pre-Perihelion Time-series Photometry of the Interstellar Comet 3I/ATLAS ›
AT2024lhc and AT2024kmq in the landscape of featureless tidal disruption events ›
$r$-mode stabilization in rotating hyperon-rich neutron stars and its implications for GW190814 ›
Spectral and photometric variability of SS 433 observed with XRISM and simultaneous optical and near-infrared telescopes ›
AVID: A Near-Major Post-Merger of Late-Type Dwarfs beneath a Regularly Rotating HI Disk (VCC 693) ›
Retarded Stellar Dynamo in Tidally Deformed M Dwarfs ›
Is Mira B a low mass white dwarf? ›
Sub-second cadence structure of optical flares on AD Leo ›
A sound horizon independent measurement of $H_0$ from BOSS, DESI and DES Y3 ›
A Robust Analysis of QU-fitting Behavior for 800-1088 MHz and 1296-1440 MHz ›
Formation timescales for stellar bars in diverse galactic discs ›
Linear Perturbations and Multi-Probe Diagnostics in Dark-Sector Selective $f(R,T_{\chi})$ Gravity ›
CALIMA: On-the-fly dust and PAH evolution for radiation-hydrodynamics galaxy formation simulations ›
Classical, large scale 3D MHD simulations of interacting pulsar wind nebulae ›
The supersonic nature of jellyfish galaxies ›
pythonradex: a fast Python re-implementation of RADEX with extended functionality ›
The accretion discs in WZ Sge-type stars in deep quiescence. How do they outburst? ›
Impact and interplay of $\Lambda$CDM analysis choices for LSST cosmic shear ›
The Dawes Review: A Decade of Ultra-Diffuse Galaxies ›
A deep HST view of the open cluster NGC2158: binaries, mass functions, and M-dwarf discontinuity ›
The impact of cosmic filaments on starburst galaxies across cosmic times ›
Tidal disruptions of rubble piles: The case of Phobos ›
Probing Dark Photon Dark Matter with CTAO ›
How does a MOND cosmology fare on Gpc scales? - Collisionless $N$-body simulations of $\nu$HDM ›
Probing Large-scale Structure and the Multi-Phase IGM at the Cosmic Noon -- Insights from a Joint Survey with Euclid, CSST, JPCam, and JUST ›
Spectroscopic study of five Mira stars ›
MESA Isochrones and Stellar Tracks. II. Models with alpha-enhanced chemical composition ›
Optical Spectroscopy of Dwarf Galaxies at $z\sim 0.15$ in the COSMOS Field: Star Formation and Dust Properties ›
IGR J12580+0134: A Candidate for Repeating Partial Tidal Disruption Events Supported by Multi-Wavelength Observations ›
Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion ›
Survival of Protoplanetary Disks in Upper Scorpius from Population Synthesis Models with External Photoevaporation ›
Overlap Zoo Beta: A Catalogue of ~800 Occulting Pairs in the DESI Legacy Survey using Citizen Science ›
Forward hadron production in proton-air collisions above LHC energies through the fluctuations of extensive air showers ›
Fermi-LAT 16-year Source List ›
Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons ›
Uncovering the absorbed atomic Universe with the [OI]63um line ›
Whistler-Alfv\'en turbulence in a non-neutral ultrarelativistic pair plasma ›
Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole ›
Exocometary physics: material release and tails ›
Electrical coupling of a horizontal dipole antenna to a dielectric half-space: applications to radio astronomy from the lunar surface ›
Recovering 3D Magnetic Turbulence from Single-Frequency Faraday Screens ›
SIRIUS: The relation between the diversity of dwarf galaxies and their formation histories ›
INFLAVON: CMB as cosmic tracer of Flavor physics ›
Tests of general relativity in pseudo-Newtonian approach ›
Pseudo-Newtonian potential for accretion disks in a modified gravity spacetime around the black hole and underlying properties ›
Using thermodynamics to learn gravitational wave physics ›
Beam tube boundary effects in stray light modeling of long Fabry-Perot arm cavities for third-generation gravitational-wave detectors ›
Direction-of-arrival estimation of a gravitational wave by correlations between quadrupole moments of pulsar timings ›
On the Kalb-Ramond field with non-minimal coupling to gravity ›
Analytic force-free jet from disk-fed rotating black holes ›
Analysis of eigenvalue clustering leads to optimal scaling in numerical radiative transfer ›
Choice of Quantum Vacuum for Inflation Observables ›
ALP Dark Matter, Cosmological Magnetic Fields and the Direct Collapse Black Hole Formation Scenario ›
Improving Precision in Kinematic Weak Lensing with MIRoRS: Model-Independent Restoration of Reflection Symmetries ›
GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere ›
A deep X-ray and UV look into the reflaring stage of the accreting millisecond pulsar SAX J1808.4-3658 ›
New bounds on Axion-Like Particles in the Ultraviolet from Legacy Data ›
The Rise of Ionized Gas Filaments in Early-Type Galaxies ›
SKYSURF. X. A Novel Method for Measuring Integrated Galaxy Light ›
Effective bias expansion for circumventing 21 cm foregrounds ›
COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase ›
Efficient evaluation of the dark-matter two-loop power spectrum in the EFT of LSS ›
The possible accretion discs of GN-z11 at redshift z = 10.6, MoM-z14 at z = 14.44 and other high redshift objects ›
CMB component-separated power spectrum estimation by Spectral Internal Linear Combination (SpILC) ›
The HyLight model for hydrogen emission lines in simulated nebulae ›
From Dark Radiation to Dark Energy: Unified Cosmological Evolution in K-essence Models ›
Prolonged fallback and late-time rebrightening episodes in stellar tidal disruptions as imprints of a galactic environment ›
A Vertically Orientated Dark Matter Halo Marks a Flip of the Galactic Disk ›
Dark Energy Survey Year 6 Results: Clustering-redshifts and importance sampling of Self-Organised-Maps $n(z)$ realizations for $3\times2$pt samples ›
Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA ›
Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation features ›
The influence of AGN feedback on star formation in red spiral galaxies ›
Relationship Between Major Stellar Physical Parameters and Normal Mode Frequencies in Accreting White Dwarf Stars ›
A Test of Substellar Evolutionary Models with High-Precision Ages from Asteroseismology and Gyrochronology for the Benchmark System HR 7672AB ›
Hot, Photoionized X-ray Gas in Two Luminous Type 2 Quasars: Chandra-HST Evidence for a Wind-Driven Sequence ›
Varying core-envelope coupling efficiency identified from stellar rotation--activity relation ›
QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon ›
Simultaneous JWST, NuSTAR, and VLA Monitoring of Sgr A*: A Unified Picture of the Variable IR, X-ray and Radio Emission ›
Tidal capture and repeating partial tidal disruption events of giant stars ›
Probing Heavily Obscured AGN in Major Galaxy Mergers Using the mm-X-ray Correlation ›
XMM-Newton observations of ten high-redshift CAMIRA clusters of galaxies ›
The size-velocity dispersion relationship of Galactic HII regions ›
Observational imprints of tidal internal gravity wave dissipation in star-planet systems ›
Assessment of DKIST/VTF Capabilities for the Detection of Local Acoustic Source Wavefronts ›
Cold and eccentric: a high-spectral resolution view of 51 Eri b with VLT/HiRISE ›
AT 2025abao: the fourth luminous red nova in M 31 ›
Cosmology with galaxy clusters using machine learning. Application to eROSITA Data ›
AT 2024wpp: the most luminous fast-evolving optical transient linked to the merger explosion of a black-hole binary ›
Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections ›
The energy and momentum of the Universe ›
Supercool subtleties of cosmological phase transitions ›
Asteroid-mass soliton as the dark matter-baryon coincidence solution ›
Bright ring features and polarization structures in Kerr-Sen black hole images illuminated by radiatively inefficient accretion flows ›
Cosmology in warped massive gravity ›
Tidal disruption of a neutron star near naked singularity ›
When inverse seesaw meets inverse electroweak phase transition: a novel path to leptogenesis ›
A battle of designs: triangular vs. L-shaped detectors and parity violation in the gravitational-wave background ›
Probing a minimal dark gauge sector via microlensing of compact dark objects ↓↑