Obserwatorium Astronomiczne na Suhorze Strona główna
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 Wiadomości z astronet.pl

› Pixinsight cz.VI – Łączenie zdjęć monochromatycznych w kolorowy obraz
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› Katalog Caldwella: C75
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› Przełomowe odkrycie! Pierwsza planeta swobodna odkryta i ,,zważona” przez polskich naukowców
› Rozsiewanie nasion za pomocą satelity – projekt Greenstar
› Katalog Caldwella: C98
› Niebo w styczniu 2026 roku
› Podsumowanie roku 2025 w astronomii i astronautyce
› Katalog Caldwella: C19
RSS  Najnowsze prace na astro-ph:

› AT2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole
› Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes
› Early thin-disc assembly revealed by JWST edge-on galaxies
› Non-thermal particle acceleration in multi-species kinetic plasmas: universal power-law distribution functions and temperature inversion in the solar corona
› Mind the peak: improving cosmological constraints from GWTC-4.0 spectral sirens using semiparametric mass models
› Simulation-Based Prediction of Black Hole Spectra: From $10M_\odot$ to $10^8 M_\odot$
› The SOL $\textit{(Solar Origin and Life)}$ Project: Detailed characterization of candidates for the ZAMS and Subgiant stages
› Extreme-ultraviolet synthesis of nanojet-like ejections due to coalescing flux ropes
› Multiwavelength Modeling of the Luminous Fast Blue Optical Transient AT2024wpp
› Late-Time Infrared Cooling in Magnetar-Driven Supernovae
› Estimation of the tidal heating in the TRAPPIST-1 planets. Influence of the internal structure
› Integral field spectroscopy and numerical simulations of the NGC 2207/IC 2163 system
› Simulation-Based Inference for Probabilistic Galaxy Detection and Deblending
› MARVEL: A Multi Agent-based Research Validator and Enabler using Large Language Models
› Time-dependent chemical evolution during cloud formation: H$_2$-regulated chemistry in diffuse molecular cloud
› The steep redshift evolution of the hierarchical merger rate may cause the $z$-$\chi_{\rm eff}$ correlation
› The maximum mass ratio of hierarchical mergers may cause the $q$-$\chi_{\rm eff}$ correlation
› Jet-torus interaction revealed by sub-parsec SO absorption in NGC 1052
› Perhaps there is no brown dwarf desert? A study of sub-stellar companions with Gaia DR3
› Electron Cyclotron Maser Emission from Ejected Stellar Prominences on V374 Peg
› Particle Acceleration and Depolarization in the Protostellar jet knots HH 80 and HH 81
› An Enhanced Sample of Galactic Red Supergiants Reveals Spiral Structures
› Investigating the Center-to-Limb Effects in Helioseismic Data Using 3D Radiative Hydrodynamic Simulations
› Protonic thermoelectric effect of Superionic H2O and magnetic field generation in Uranus and Neptune
› Predicting dust temperature from molecular line data using machine learning
› Characteristics of the High-frequency Humps in the Black hole X-ray Binary Swift J1727.8--1613
› Identification of solid N2O in interstellar ices using open JWST data
› A Multiband Photometric Study of RR Lyrae Stars in M53 (NGC 5024)
› The massive hot subdwarf binary LAMOST J065816.72+094343.1
› Modelling spacecraft-emitted electrons measured by SWA-EAS experiment on board Solar Orbiter mission
› Disc fragmentation. II. Ejection of low mass Free Floating Planets from growing binary systems
› Short gamma-ray burst progenitors have short delay times
› First detection of VHE gamma-ray signal from the FSRQ TON 0599
› Filtering interlopers with photometry and diagnostic features: A machine learning framework validated with CSST slitless spectroscopy
› Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
› HST+IGRINS synergy to characterise the newly discovered metal-rich bulge globular cluster Patchick 126
› Science with a large field-of-view polarization survey: The Large Array Survey Telescope Polarization Node (LAST-P)
› Polarization rotation through differential transmission in refractive CMB telescopes identified using a hybrid physical optics method
› The uncertainty in water mass fraction of wet planets
› Search for gamma-ray variability around Fermi-LAT pulsar glitches
› Evidence for a Damped Millisecond Quasi-Periodic Structure in a Fast Radio Burst
› Broadband spectroscopy of astrophysical ice analogues: IV. Optical constants of N$_2$ ice in the terahertz and mid-infrared ranges
› Exploring the potential for ultra-relativistic jets in Scorpius X-1 with low angular resolution radio observations
› Formation of multi-planetary systems via pebble accretion in externally photoevaporating discs in stellar clusters
› Can Dynamic Spectrum Sharing Protect Passive Radio Sciences?
› The Gaia All-Sky Stellar Parameters Service (GASPS)
› Investigation of the dynamics and origin of the NEA pair 2021 PH27 and 2025 GN1
› Stellar-mass black holes on the millimetre fundamental plane of black hole accretion
› HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
› Two-source terrestrial planet formation with a sweeping secular resonance
› Cosmological constraints on viable $f(R)$ models using weak lensing
› Spiral galaxies with flat radial abundance gradients at large radii
› Dissecting the dust distribution and polarization around two B213 young stellar objects with ALMA
› Modeling the Effect of C/O Ratio on Complex Carbon Chemistry in Cold Molecular Clouds
› Characterizing the physical and chemical properties of the Class I protostellar system Oph-IRS 44. Binarity, infalling streamers, and accretion shocks
› Satellite-borne {\gamma}-ray astrophysics from coherent interactions in oriented crystals
› A census of star-formation and gas mass tracers in two lensed $z \sim 4$ dusty star-forming galaxies
› Secular Excitation of Polar Neptune Orbits in Pure Disk-Planet Systems
› Implications of Non-equatorial Relativistic Accretion Flows for Ultra-Fast Inflows in AGNs
› A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
› Radio Activity from the Rapidly Rotating T dwarf 2MASS 2228-4310
› GRB 180728A and SN 2018fip: the nearest high-energy cosmological gamma-ray burst with an associated supernova
› Local simulations of common-envelope dynamical inspiral. Impact of rotation, accretion, and stratification
› Fast frequency-domain phenomenological modeling of eccentric aligned-spin binary black holes
› Cavity Multimodes as an Array for High-Frequency Gravitational Waves
› Sterile Neutrino Dark Matter as a Probe of Inflationary Reheating
› Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations
› On flying through the base of a pseudo-streamer
› Real-time Gravitational Wave Response in Thermal Spinning fields
› Limits on the mass of compact objects in Ho\v{r}ava-Lifshitz gravity
› Combining simulation-based inference and universal relations for precise and accurate neutron star science
› A constrained-transport embedded boundary method for compressible resistive magnetohydrodynamics
› Symmetries of cosmological perturbations: The residual low multipole ambiguity
› Properties of Magnetic Switchbacks in the Near-Sun Solar Wind
› A framework for LISA population inference
› Evolution of proto-neutron stars to pulsars, magnetars and central compact objects
› Machian Gravity: Modeling Rotation Curves and Radial Acceleration in the SPARC Galaxy Sample
› PySCo: A fast Particle-Mesh $N$-body code for modified gravity simulations in Python
› Unveiling the nature of SN 2022jli: The first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late times
› Measurement of Very-high-energy Diffuse Gamma-ray Emissions from the Galactic Plane with LHAASO-WCDA
› Pulsar Polarization Array Limits on Ultralight Axion-like Dark Matter
› Towards Galactic Archaeology with Inferred Ages of Giant Stars From Gaia Spectra
› DESI Dark Secrets
› The dynamical and thermodynamic effects of turbulence on the cosmic baryonic fluid
› AliCPT Sensitivity to Cosmic Reheating
› On the effects of radiation on mass transfer in binary stars
› Disentangling the Halo: Joint Model for Measurements of the Kinetic Sunyaev-Zeldovich Effect and Galaxy-Galaxy Lensing
› The dynamics of background evolution and structure formation in phase space: a semi-cosmographic reconstruction
› The first phase of mass transfer in low-mass binaries: neither stable nor a common envelope
› Scalar-induced gravitational waves from coherent initial states
› Measuring the muon content of inclined air showers using AERA and the water-Cherenkov detectors of the Pierre Auger Observatory
› Magnetized Proto-Neutron Stars: Structure and Stability
› Convection-Driven Multi-Scale Magnetic Fields Determine the Observed Solar-Disk Gamma Rays
› Revisiting the Radial Metallicity Gradient-Age Relation in the Milky Way's Thin and Thick Disks
› The Open mulTiwavelength Transient Event Repository (OTTER): Infrastructure Release and Tidal Disruption Event Catalog
› Revisiting thermodynamics at the outskirts of the Perseus cluster with Suzaku: importance of modeling the Hot Galactic gas
› A simple, flexible method for timing cross-calibration of space missions
› The lower mass limit for circumbinary disc fragmentation
› Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow
› XRISM-Subaru views of Abell 754: an off-axis, near-line-of-sight merging cluster
› When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps
› Probing cosmic isotropy with Gamma-ray bursts: A dipole and quadrupole analysis of BATSE and Fermi GBM data
› Spatially resolved PAH$_{3.3}$ emission and stellar ages in ram pressure stripped clumps at $z\sim0.3$
› Upper Limits on Radio Emission from the K2-18 System
› Analytical Solutions for Planet-Scattering Small Bodies
› Peculiar SN Ic 2022esa: An explosion of a massive Wolf-Rayet star in a binary as a precursor to a BH-BH binary?
› Water vapor emission at the warm cavity wall of the HD 100546 disk as revealed by ALMA
› The impact of non-Gaussianity when searching for Primordial Black Holes with LISA
› Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
› VERITAS contributions to the 39th International Cosmic Ray Conference
› Not Just Gas: How Solid-Driven Torques Shaped the Migration of the Galilean Moons
› When the Shadow Meets Its Measure: Assessing the Feasibility of Submillimeter Black Hole Shadow Imaging in Megamaser Disk AGN
› Physical Vetting of the Ultra-Short-Period Sub-Earth TOI 864.01
› CHANG-ES XXXVII. Effects of spectral aging on radio scale heights
› Where does the simplified Stellar Contamination Model fail in Exoplanet Transmission Spectroscopy?
› Deflection angle in the strong deflection limit for static and axisymmetric spacetimes: local curvature, matter fields, and quasinormal modes
› Gravitational Equilibrium with Steady Flow and Relativistic Local Thermodynamics
› The Dark Matter Diffused Supernova Neutrino Background
› Scalar parity-odd trispectrum from gravitational Chern-Simons interaction vertices
› Optical appearance of Schwarzschild black holes with optically thin and thick accretion disks at various inclination angles
› Ultralight boson constraints from gravitational wave observations of spinning binary black holes
› Illuminating Scalar Dark Matter Co-Scattering in EFT with Monophoton Signatures
› GW200105: A detailed study of eccentricity in the neutron star-black hole binary
› Gravitational Waves from $\textit{Type-I}$ Strings in a Neutrino Mass Model
› Leptogenesis from Dark Matter Coannihilation
› Exotic compact objects in Einstein-scalar-Maxwell theories
› Photon Accelerator in Magnetized Plasma
› Taxonomy of periodic orbits and gravitational waves in a deformed Schwarzschild black hole spacetime

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