Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› 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

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