Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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Zdjecie: Teleskop 60cm na Suhorze
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RSS  Najnowsze prace na astro-ph:

› The Amplitude-Growth Degeneracy and Implied $A_s$ Diagnostic for Background-Inert Modified Gravity
› Spherical collapse and cluster number counts in DHOST theories that pass the constraints from gravitational waves
› The Hunt for Red Dual AGNs I: Spatially-Resolved Mid-IR Dual AGNs in the DeCam Legacy Survey
› Improved recipes for peculiar velocity power spectra using Evolution Mapping
› Spin Demographics of Active Supermassive Black Holes: Updated Estimates from X-ray reflection and Future opportunities
› Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves
› The Demographics of Sagittarius A* X-ray Flares over 25 Years with Chandra
› Massive Galaxies Form Early and Gray: Stellar Assembly and Dust Attenuation at $\mathbf{z>3.5}$ from CAPERS
› When galaxies burst: enhanced shot-noise for line-intensity mapping in the JWST era
› Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes
› Determining star formation histories and age-metallicity relations with convolutional neural networks
› Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn
› Rapid and robust simulation-based inference for kilonovae
› Infrared Line Diagnostics Fail to Constrain Sgr A*'s UV Output
› Ionization Structure and Metal Enrichment of the Galactic Center Minispiral Observed with JWST
› The Homogeneous MeerKAT and Swift/XRT X-ray Binary Radio:X-ray Plane
› Analysis of DQZ White Dwarf Evolution through Procyon
› Constraining the Galactic Center Dark Cluster with ELT/MICADO Observations
› Spectral Disentangling Reveals Deep CNO-cycle Exposure in ET Cru
› The Magnetic Origin of Primordial Black Holes: Ultralight PBHs and Secondary GWs
› Planets in Pulsar Winds
› SN2023ixf: ultraviolet-to-infrared radiative-transfer modeling of the nebular-phase evolution until 1000 days
› Single field matter bounce with dark energy era: comparison with CMB Planck 2018 data and best fit parameters
› Coupled Photochemical-Climate Modeling of Plausible Tenuous Outgassed Atmospheres on the TRAPPIST-1 Planets
› Direct Evidence of Non-Ideal Dissipative Dynamics in Solar Wind Magnetic Switchbacks
› Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
› Scattered light noise at LIGO Livingston Observatory during O4
› CIAO: Chandra's Data Analysis System for X-Ray Astronomy and Beyond
› The Distribution of Blue Straggler Stars in the Color-Magnitude Diagrams of Old Open Clusters
› The Close Binary V486 Carinae
› A new sample of Little Red Dots at $z
› Dynamical Evolution of V-Shaped Collision Debris
› The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius
› Opportunities for Gravitational Wave Physics at the South Pole
› Reconstructing the Stripping History of the Sagittarius Stream with Neural Networks
› An Updated Characterization of Luminous Ly{\alpha} emitters at the End of Reionization
› A $Z_1^2$ framework for rotational-parameter estimation and uncertainty quantification in high-energy pulsars
› Observation of spontaneous N-bearing PAH formation using ion trap: a new formation pathway in the interstellar medium
› Where Do Hot Jupiters Come From? Revisiting Tidal Disruption and Ejection in High-Eccentricity Migration
› Not All Who Wander Are Lost: Early Excess Demographics in the Volume-limited ZTF DR2 SN Ia Sample
› GeV emission around SS 433 with 17 years Fermi-LAT observation
› A new hot core in the outer Galaxy: Impact of metallicity on the formation of complex organic molecules
› Discovery of a Compact Hub-Filament System in G286.21+0.17 with JWST and ALMA: Insights into Protocluster Formation and Competitive Accretion
› Luminaries in the Sky: The TESS LEGACY Sample of Bright Stars. II. In-depth seismic characterisation of 32 naked-eye stars in the PLATO LOP fields
› Boundary-supported radial layering in Hoag-like ring galaxies
› Beyond AI as Assistants: Toward Autonomous Discovery in Cosmology
› Tidal coplanarization of circumbinary planetary systems through stellar Cassini states
› Resonant Networks of Spin-Orbit Coupling in Ellipsoid-Ellipsoid Binary Asteroid Systems
› Self-confinement of ultra-high-energy nuclei in cosmic filaments: implications for the UHECR spectrum and composition
› Self-Interacting Dark Matter in Brown Dwarfs
› DREAMS. JWST Spectroscopy of a $z=8.3$ Galaxy with an ALMA Dust Continuum Detection: Early Dust, Very High $T_{\rm dust}$, and a Multi-wavelength [OIII] Ratio Discrepancy
› Identifying group galaxies merging with massive clusters using machine learning
› Denoising Interferometric Observations Using Visibilities-Informed Neural Networks
› Pulsar scintillation arcs formed from branched flow
› A Climate-Constrained Bayesian Inverse Method for JWST Rocky Exoplanet Eclipse Spectra: A Case Study of LTT 1445A b
› JWST COMPASS Program: The 3--5$\mu$m transmission spectrum of LTT 1445 A b
› Imaging without visibilities: FAST-Effelsberg scintillometry of PSR B1508+55
› Millimeter dust continuum and polarization in protoplanetary disks with scattering: A slab model
› The DESIRED electron temperature relations in star-forming regions of the local Universe
› The Role of Magnetic Reconnection in Energizing Protons and Heavier Ions at the Heliospheric Current Sheet
› Probing the IMF in the Early Universe -- Direct measurements in the Bo\"otes I UFD with JWST/NIRCam
› KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions
› Impact of stellar population models on the estimated physical properties of galaxies
› Analysing the highly irregular boundaries of solar pores
› Significant or Not? The Impact of Randomisation During Data Reduction on Confirming a New Pulsating Ultraluminous X-ray Source Candidate in Centaurus A
› Eclipses of Nearby Radio-Loud Galactic Nuclei by Stars in Nuclear Star Clusters
› Polarization Signatures from GRMHD Simulations of Black Hole Accretion
› The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
› Detecting the Axion-Photon Conversion Background
› Strong Gravitational Lensing with the James Webb Space Telescope
› Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus
› Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls
› Gravitational collapse of matter fields in de Sitter spacetimes
› Unique Gravitational-Wave Signals from Negative-Mass Binaries
› Stochastic Resonance in a Thermally Driven Low-Dimensional Geodynamo Model
› Analytic thin disks and rings in a class of nonasymptotically flat static spacetimes
› On the impossibility of observational confirmation of black holes
› Exploring neutrino loss with diffuse astrophysical neutrino fluxes
› Baryoid Dark Matter from $\mathbb{Z}_N$ Domain Walls: The $(N-1):1$ origin of the dark matter-baryon coincidence
› Boris and Exponential Integrators in the Theory of Particles Interacting with Magnetic Turbulence
› The simulation on neutron background reduction for InDEx at JUSL
› Parametrization of the primordial power spectrum in loop quantum cosmology
› How Much Can Gravitons Be Squeezed?
› Conservative and dissipative sectors in a nonlinear scalar model for the gravitational self-force problem
› Exploring the CMB in Anisotropic Universes
› Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity
› Can a late-time cosmological model based on baby universe absorption explain the z-variation of w?
› Effective Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies
› Axion magnetohydrodynamics and reconnection-driven axion bursts
› Inferring neutron star properties through gravitational waves from r-modes and their relativistic counterparts
› Super-Kamiokande Strongly Constrains Leptophilic Dark Matter Capture in the Sun
› Non-Perturbative Hamiltonian and Higher Loop Corrections in USR Inflation
› Hamiltonians to all Orders in Perturbation Theory and Higher Loop Corrections in Single Field Inflation with PBHs Formation
› The (Limited) Effect of Viscosity in Multiphase Turbulent Mixing
› The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions
› Thermochemical models of outer core convection with heterogeneous core-mantle boundary heat flux
› SuNeRF-CME: Physics-Informed Neural Radiance Fields for Tomographic Reconstruction of Coronal Mass Ejections
› Search for synchrotron pair echo emission following KM3-230213A
› Solving the cooling flow problem with combined jet-wind AGN feedback
› Changing-Look Active Galactic Nuclei in SDSS-V: Host-Galaxy Properties and Black-Hole Scaling Relations
› Age and metallicity of low-mass galaxies: from their centres to their stellar halos
› GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars
› Tachyonic gravitational dark matter production after inflation
› High-fidelity stellar extinction with Gaia and APOGEE -- I. The method and a new extinction curve
› Constraining FRB Microstructure with Polarised Shot Noise
› Population Properties of Binary Black Holes with Eccentricity
› Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations
› A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN
› Calibrating Eruptive Mass Loss in Red Supergiants with Local Group Data
› Energetics and Emission in a Simulated Solar Flare Initialised by a Non-Force Free Magnetic Field
› Weighing gas-rich starless halos: dark matter parameters inference from their gas distributions
› Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance
› Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
› Deriving volume density profiles of filaments from observed surface densities
› A Cosmological Uncertainty Relation and Late-Universe Acceleration
› Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation
› Ellipsoidal modulation and multi-wavelength activity in the pre-cataclysmic binary RX J1553.0+4457
› Mitigating stellar radial velocity jitter using orthogonal activity indices and a time-aware neural network
› Results of ten years of UCLA SETI searches with the Green Bank Telescope
› Exploring the stellar streams and satellites around the giant low surface brightness galaxy Malin 1
› Magnetar-powered long gamma-ray bursts and connection to superluminous supernovae and fast radio bursts
› A New PSF Deconvolution Algorithm: Simultaneous Spatial Resolution Enhancement and Point Source Removal for Morphological Analysis of AGN Host Galaxies
› Photometric metallicity of Galactic RR Lyrae stars in the Gaia DR3 era
› Primordial black holes and magnetic fields in conformal neutrino mass models
› Detecting dark matter using optically trapped Rydberg atom tweezer arrays
› A Robust and Efficient F-statistic-based Framework for Consistent Bayesian Inference of Compact Binary Coalescences
› Finite parts of inflationary loops II: A streamlined UV in-in algorithm and distinguishable signatures
› Near-Resonant Thermal Leptogenesis
› Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6
› Gravitational edge mode powers galaxy flat rotation curves
› Phase-resolved field-space distance bounds in ekpyrotic, bouncing and cyclic cosmologies

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