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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:

› The Phenomenological Nature of Quasar-type Blazars (BZQ). I. Revisiting the Flat-Spectrum Paradigm
› Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective
› Detecting Gravitational-Wave Anisotropies with Simulation-Based Inference
› Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants
› A formation scenario of black hole-envelope systems --viscous hydrodynamics simulation in general relativity--
› Discovery and Analysis of a Type II Supernova Candidate at z = 3.19 from JWST's COSMOS-Web Survey
› Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes
› FASTAR -- I. Continuous and differentiable evolutionary stellar population models
› Fast and Flexible Characterisation of Astronomical Light Curves Using Multi-Time Attention
› The AGORA High-resolution Galaxy Simulations Comparison Project. XI: Solving the Non-Spherical Morphology and Evolution of Dark Matter Halos with Haskap Pie
› Dark matter-deficient twins: FCC 224 and FCC 240 as possible analogues of NGC 1052-DF2 and DF4
› Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE
› On the maximum neutrino flux of blazars in the one-zone leptohadronic model
› The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $z\geq 3$
› Pitch-Angle Scattering of Cosmic Rays: Confronting Theory with Observations
› The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation
› Hubble Astrometry for the Local Group and Beyond in the 2030s
› Orbital Parameters of the Unusual WR + O Binary System LS III +44 21
› JWST and Gemini Observations of the Active Centaur 450P/LONEOS: Nucleus and Coma Characterizations
› A Redshift-based Red Selection of Dusty Star-forming Galaxies
› Pushing the Limit of Asteroseismic Detection for Cool Dwarfs using TESS and Deep Learning
› Evidence for mass-dependent spin subpopulations in GWTC-4
› Near UV Stellar Activity and Brightness Fluctuations of the Alpha Centauri AB Star System from Weeks to Decades -- Inputs for Reflected Light Spectroscopy with HWO
› Constraining the Potential Index $n$ of the Early Dark Energy Model Using Cosmic Birefringence from Planck and ACT
› The 3D Structure and Kinematics of the Local Disk-Halo Interface: Intermediate-velocity Clouds are the Minority of High-altitude Clouds in the Solar Neighborhood
› Evolution of a long-period Cataclysmic Variable from the viewpoint of the donor star: the case of SDSS J085210.48+783246.6
› Radiative MHD Studies of Solar Spicules: Driving Mechanisms and the Role of Background Magnetic Field
› Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Survey
› FASTAR -- II. Semi-resolved evolutionary stellar population models
› Observational Technological Innovations and Future Development of the Lijiang Coronagraph
› Timing and Spectral Studies of PSR J2022+3842 with NICER and NuSTAR
› New galaxy cluster in the Zone of Avoidance SRGe CL0512.7+3712. Discovery and multi-wavelength characterization
› The XRISM measurements of the black-hole spin in Cyg X-1 are highly model-dependent
› Gravitational Waves from Post-Inflationary Magnetism: Direct and Scalar-Induced Contributions
› A Three-Decade VLBI Study of the Nucleus in the Lobe-Dominated Quasar 3C207
› Deep Learning-Enabled Prediction of Geoeffective CMEs Using SOHO and SDO Observations
› SN~2018erx: A fast-evolving, dust-reddened Type Icn supernova with broad C II emission lines
› The Evolution of Cataclysmic Variables Under Various Magnetic
› High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars
› Preliminary cosmological results using extreme accretors Quasar formalism
› Pulse Modulation as a Signature of the Asteroid-Neutron Star Collision Model for High-Energy Transients
› QPEs from Warped Disk Collisions with EMRIs: Brightness-Recurrence Diagram and Gravitational-Wave Follow-up
› Mass distribution of neutron stars in binary systems
› Puzzling Ultra-Diffuse Galaxy Evolution (PUDGE). II. A transformation pathway from UDGs to compact dwarfs (CDs) in galaxy clusters
› Radio Study of G76.9+1.0 Pulsar Wind Nebula
› Small and Complex II: Characterizing the Disk and Stellar Envelope of Edge-on $z \sim 0$ Massive Compact Galaxies
› Cyclotron breaking: a mechanism for parallel ion cyclotron waves to heat the fast solar wind
› Exploring biases in derived stellar parameters and the ionizing photon production efficiency
› Shear Particle Acceleration in Structured Gamma-Ray Burst Jets: IV. Thermal {\em vs.} Non-thermal Emission of the Jet Cocoon
› Kepler Discovery of GW Vir Pulsations of the Central Star of Planetary Nebula Kn 61
› The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios
› Discovery of Short-Term {\gamma}-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449
› Inverse Compton scattering occurring in a reverse-shock scenario involving a kilonova: A channel of TeV gamma-ray photons
› Signs of Sulphur fractionation under high magnetic field strength
› A Unified [CII] Morpho-Kinematic Corpus for 31 Star-Forming Galaxies at z = 4.26-5.68: The High-z Kinematic Corpus Z1
› Compact dusty starbursts at cosmic noon linked to high-energy neutrinos
› Discovery of Molecular and Atomic Gas associated with HESS J1646-458 (Westerlund 1): Spatial TeV Gamma-Ray and Interstellar Proton Correspondence
› Constraining the Inclination of Binary System Orbits with the Astrometric Excess Noise from Gaia DR3
› Long-Term Clustering Pattern of Solar Active Regions and Their Potential Connection with Magneto-Rossby Waves
› The Gas-Phase Mass-Metallicity Relation of Dwarf Galaxies Across Large-Scale Environments Using the CAVITY Parent Sample
› Legacy analysis of Milky Way dwarf spheroidal satellite galaxies: an update
› Superfluid fraction and effective ion mass in the crystalline crust of a neutron star: role of interband response
› Machine Learning-based Separation of the He I 10830{\AA} Chromospheric Signal: Quantitative Analysis of Chromosphere-Corona Intensity in the Quiet Sun
› Reassessing high-energy emission correlations in gamma-ray bursts using a large, homogeneous sample of X-ray afterglows
› Extreme color-magnitude variability: connection to changing-look AGNs
› Beyond the [OIII]$\lambda$4363 auroral line: [NeIII]$\lambda$3868 as a direct tracer of electron temperature
› Lithium-rich M-dwarfs at the ZAMS: Evidence for planetary engulfment?
› The transitional Type Ibn/IIn SN 2022pda, with pre-explosion outbursts and a double-peaked light curve
› skysurvey: a pure python package to simulate the transient sky
› Core-collape supernovae and supernova neutrinos
› Diversity of morphology of type II spicules in MURaM-ChE simulations
› Gaia FGK Benchmark Stars: Impact of Spectral Resolution on Stellar Abundances
› Chronos: Towards a self-consistent and absolute stellar age scale. I. A Bayesian hierarchical lithium-age model: Validation on the Pleiades cluster
› Building on SVOM : the CATCH satellite constellation for transient astronomy
› Reversible-jump MCMC reveals binary black hole subpopulations with distinct redshift evolution
› Compactness Peaks and Subpopulations: Probing Stellar Physics and Formation Channels of Merging Binary Black Holes
› Interstellar extinction, polarization efficiency, and grain alignment in the direction towards bright-rimmed clouds and cometary globules
› Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension
› X-ray Polarization Signatures from Comptonization by Magnetic Reconnection Plasmoids
› Understanding hydrodynamical wave-driven shear mixing in stellar radiation zones. Looking in the mirror of the dyapicnal oceanic mixing
› GRB 260310A / SN 2026fgk: A Multi-Wavelength Study of a Nearby Underluminous Long GRB and SN with a Complex Afterglow
› Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions
› The imprints of the instantaneous appearance of a conformal Killing vector field on the evolution of self-gravitating fluid spheres
› Quantification of atmospheric carbon dioxide from the Geostationary Operational Environmental Satellite (GOES East)
› Aurora Hunter: A Two-Stage Framework for Probabilistic Visibility Forecasting
› Production of Leptophilic Bosons in Ultradegenerate Relativistic Matter
› Neutron Star Bounds on Muonic Fifth Forces from Picometer to Kilometer Scales
› Solar Axions from Nuclear Transitions
› Inferring Neutron-Star Properties from Post-merger Gravitational-wave Spectra with Neural Networks
› Efficient Nonlinear Uncertainty Quantification for Spaceflight Leveraging Nonlinear Expansions
› Leptogenesis without on-shell right-handed neutrinos
› Wideband Balanced Photodetectors for Classical and Quantum Light Detection from Optical, EUV, to X-rays
› Thermal Spin Polarization Driven by Nuclear Spin-Orbit Coupling in Neutron Star Pasta
› Bayesian Estimation of Spectroscopic Parameters: Application to the Atomic Nitrogen Bound-Bound System
› Gravitational Wave Propagation in K-essence Cosmology: Theory and Observational Constraints
› Pulse magnet of 10 T for power laser experiments with x-ray free-electron laser diagnostics
› Polarized Anisotropic Stochastic Gravitational Wave Background Search with Ground-Based Detector Networks
› Exploring the ex-situ components within Gaia DR3
› Many-body atomic response functions of xenon and germanium for leading-order sub-GeV dark matter-electron interactions in effective field theory
› Turbulence in Magnetised Neutron Stars
› SDSO1 is a Shocked Ghost Planetary Nebula in Front of M 31
› A tunable Monte Carlo method for mixing correlated-k opacities. PRAS: polynomial reconstruction and sampling
› The Magnetic Origin of Primordial Black Holes: A Viable Dark Matter Scenario
› Multi-messengers from the radioactive decay of $r$-process nuclei
› Point-like and Narrow-lined: A Potentially New Population of Objects Discovered by JWST
› Systematic Effects of Chaotic Magnetic Fields on Neutron Star Tidal Deformability: Implications for Gravitational Wave Constraints on Dense Matter
› High five from ASTEP: Three validated planets and two eclipsing binaries in a diverse set of long-period candidates
› Infall Explains the Disk Kinematics of AB Aur Without Gravitational Instability
› Control variates from Eulerian and Lagrangian perturbation theory: Application to the bispectrum
› Gamma-Ray Spectra of $R$-Process Nuclei
› How precisely can we measure the ages of subgiant and giant stars?
› Extremely UV-bright starbursts at the end of cosmic reionization
› The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
› Evidence of dynamical dark energy found via the DESI DR2 Lyman$\alpha$ forest
› Multi Messenger Study of GRB 221009A with VHE Gamma-ray and Neutrino Afterglow from a Gaussian Structured Jet
› Accessing the homogeneity scale with 21 cm intensity mapping surveys
› Enhanced antineutrino emission from $\beta$ decay in core-collapse supernovae with self-consistent weak decay rates
› First detection of X-ray polarization from the long-period X-ray pulsar 4U 1954+319
› Identification of periodicities with arbitrary shapes in AGN light curves
› Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension
› The contribution of the color space in LSST-like photometry for the selection of extragalactic globular cluster candidates
› Joint constraints on $R_h=ct$ cosmology from DESI DR2 BAO, CC, and SN\textit{Ia} Pantheon$^+$ sample
› Exploring the Limits of Machine Learning Classification of Neutron Star Matter Models
› The Origin of Spin-Alignment of Dark Matter Subhalos
› A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements
› A Guided Unconditional Diffusion Model to Synthesize and Inpaint Radio Galaxies from FIRST, MGCLS and Radio Zoo
› MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$
› Origin of Coronal Extreme Ultraviolet Shockwaves without a Coronal Mass Ejection Event
› AMICO galaxy clusters in KiDS-1000: Splashback radius from weak lensing and cluster-galaxy correlation function
› Gravitational Baryogenesis in $f(R)$ Cosmologies
› BASS LV. Connecting X-ray variability with AGN physical properties and a new path to Cosmological distances
› Capture and Stability of Resonant Planet Pairs in Turbulent Disk
› IGR J12580+0134: A Possible Repeated Partial Tidal Disruption Event Inferred from Late-Time Radio Re-brightenin
› Stochastic Particle Acceleration during Pressure-Anisotropy-Driven Magnetogenesis in the Pre-Structure Universe
› Discovery of a Strong-lens Galaxy Pair with the Smallest Projected Separation
› Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS
› A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5 < z < 6.0$ at a Critical Stellar Mass of $10^{10}M_\odot$ Revealed by JWST
› Irregular Repeating Tidal Disruption Events due to Diffusive Tides
› A 4.5-s Quasiperiodic Spectral Oscillation in GRB 230307A: Evidence for Free Precession of a Post-Merger Magnetar?
› Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with hyperconical modified gravity
› Validating z > 7.5 Lyman Break Galaxy candidates in the COSMOS field with JWST/PASSAGE
› Foundations for Discovery: A Coordinated Fleet Approach to NASA Astrophysics
› Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks
› Peculiar velocities at low Galactic latitude
› Information Content of the Cosmic Web
› Statistical methods for partitioning ribbon and globally-distributed flux using data from the Interstellar Boundary Explorer
› Fundamental Physics and Cosmology with TianQin
› Search for primordial black holes from gravitational wave populations using deep learning
› About electroweak domain walls in Majoron models
› Cosmic-ray boosted inelastic dark matter from neutrino-emitting active galactic nuclei
› Theoretical Signatures of QCD Phase Transitions in Compact Astrophysical Systems
› Scalaron dark matter dynamics: effects of Higgs non-minimal coupling to gravity
› Vector Resonant Relaxation and Statistical Closure Theory. II. One-loop Closure
› GW250114 reveals black hole horizon signatures
› Quantum Damping of Cosmological Shear: A New Prediction from Loop Quantum Cosmologies
› Direct detection of solar chameleons with electron recoil data from XENONnT
› Klein Bottle Cosmology
› Constraining meV Axion Dark Matter with ALMA Observations of the Galactic Center Magnetar SGR 1745-2900
› Gravitational Foundations and Exact Solutions in $n$-Dimensional Fractional Cosmology
› Baryon-dark matter coincidence in Randall-Sundrum Model
› Infrared Spectral Gap in a Gluonic Dark Sector and the Galactic Acceleration Scale
› Gauge-independent approach to inflation in quadratic gravity
› Transport of electrons in tangled magnetic fields
› Detection of Gravitons by Measuring Excess of Photon Luminosities from Interstellar and Intergalactic Hydrogen
› Dynamic Alignment as a Statistical Survival Effect

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