Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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RSS  Najnowsze prace na astro-ph:

› You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA
› Satellite Metallicity Enhancement I: Suppressed Star Formation, Stellar Mass Loss, and Enriched Inflow of DESI and EAGLE Galaxies around Massive Clusters
› An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos
› Empirical estimates of how massive galaxies can be in {\Lambda}CDM
› Identification of Compact Groups of Galaxies in IllustrisTNG300
› The Peculiar Velocity of Messier~87 from Microarcsecond Geodetic VLBI Astrometry
› Discovery of 30 Repeating Fast Radio Burst Sources and Uniform Population Statistics of 80 Repeating Sources from CHIME/FRB
› How to augment cosmic shear measurements with radio polarimetry of galaxies?
› Thirty Circumbinary Disk Occultation Systems (KH 15D-like stars) from the OGLE Project
› Wideband RFI Monitor Requirements, Design, and Commissioning at DRAO
› Unmasking Stellar Feedback-Driven Bubbles: Identification and Properties Analysis
› Specific Star Formation Rate Enhancement across the Galaxy Merger Sequence: Insights from Citizen Science Classifications
› Bayesian Doppler Imaging: Simultaneous Inference of Surface Maps and Geometric Parameters
› Cosmological test of a length-preserving biconnection gravity
› Non-Parametric Equation of State Reveals Non-Conformal Behavior Beyond Neutron Star Densities
› Gravitational-wave standard sirens and application in cosmology
› Coupling magma-ocean and atmospheres in spectral retrievals of sub-Neptunes
› The Stellar Abundances and Galactic Evolution Survey (SAGES). V. The First Data Release of the DDO51 Band
› Chasing the neutrino blazar candidates II: SED modeling with hadronic model
› The evolution of C4H and c-C3H2 in molecular cores
› When Magnetic Fields Sculpt the Sky: The Riegel-Crutcher cloud in optical polarization
› Observations of the 2023 February 27 fireball in northern Sweden using the auroral imaging system ALIS_4D
› Beyond power spectrum to unveil systematics on HI intensity maps
› The Status of Gravitational Vector Perturbations with Recent CMB Data
› BOCOSUR: An all sky network for fireball detection in Uruguay
› Reionisation time field reconstruction from 21-cm Maps: Investigating predictor coherence in WDM cosmology
› The MaNGA Low-mass disks HUnt for CO (MaLHUCO) Survey
› Interstellar X-ray Absorption and Scattering
› Complexity and Multifractal Variability in Multi-Band Emission of Seyfert AGN
› Separate Universe Super-Resolution Emulator
› Plato's view on supermassive black hole binaries: Exploring the faint limit of ESA's Plato space mission
› Exploring Enceladus's Interior Structure Using Electromagnetic Induction
› JWST observations and a model for the extremely luminous obscured quasar W2246-0526 at z=4.6
› How to count clustered galaxies
› Characterizing the Scale Height and Filamentary Structure of Radiatively Cooled MADs
› GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate
› High-Spin BBH Subpopulation from AGN Accretion
› Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way
› Physical characterization and modeling of candidate Hyper-Compact HII Regions
› Search for quasar pairs with Gaia astrometric data. II. Photometric redshift prediction with machine learning for the MGQPC catalogue
› Consistency between dynamical modeling and photometrically derived masses of fireballs
› A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287
› Bayesian Analysis of Massive Boson Star Models for Sagittarius A* Using Near-Infrared Astrometry Data
› Accelerating 3D Non-LTE Synthesis with Graph Neural Networks
› Challenges to the cosmological constant model following results from the Dark Energy Survey
› X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission
› Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis
› Optical Appearance of the Kerr-Bertotti-Robinson Black Hole with a Magnetically Driven Synchrotron Emissivity Model
› Image Processing Framework for Eclipse Shadow Band Analysis
› A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588
› Cooling of Isolated Neutron Stars with Hyperon-mixed Kaon-Condensation Matter
› Small and Complex I: The Three Component Structure of $z \sim 0$ Massive Compact Quiescent Galaxies
› Stardust Galaxies at z>9: A Dust-Origin Transition Behind the Excess of UV-Bright Galaxies
› Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations
› Validating Coronal Magnetic Field Models Using Gaussian Separation
› Numerical estimation of the capture ability of Neptunian mean motion resonances
› RAYTHEIA: A high-performance ray-tracing algorithm for three-dimensional direction-dependent equations in astronomical simulations
› Lunar ejecta as the missing piece to resolve the lunar cratering asymmetry
› On the Problem of Prognostication of Bright Kreutz Sungrazers
› On the residual missing mass of the Bullet Cluster
› Hydrodynamical simulation of wind production from hot accretion flows in tidal disruption events
› The Influence of Aliphatic Components on the Aromatic Emission Characteristics of Polycyclic Aromatic Hydrocarbons
› Tracing the kinematic perturbations of the Milky Way spiral arms with APOGEE DR17 and Gaia DR3
› From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
› Cyclotron Line Variability and Accretion Dynamics in Vela X-1
› Application of Machine Learning to 21 cm Cosmology
› Reionization History and Neutrino Mass
› CosmoDRAGoN III: Shaping the Afterlife -- How Progenitors and Environments Sculpt Radio Galaxy Remnants
› Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-Duration Magnetic Field Sector Transition
› Isolating Broadband Radio Technosignatures (BRaTs): A Framework for Detecting Planetary-Scale Leakage
› Astrophysical signatures of Kerr-Bertotti-Robinson black holes in a cloud of strings: ISCO, microquasar QPOs, and Bondi-Hoyle-Lyttleton accretion
› Stellar Age Compression Reshapes Interpretations of the Milky Way Thick-Disk Formation History
› Thermal Deformation Reduction in High-Power Interferometry with Higher-Order Laser Modes
› Design and in-orbit calibration of the MXT optics
› Transition region-induced kinetic Alfven wave conversion. Electric displacement field
› Wolf-Rayet stars as tracers of gamma-ray emission: Isolated stars and stellar clusters/associations
› STEPSIC: Initial condition generator for stereographic cosmological simulations
› Energy-resolved pulse profiles of Vela X-1: cross-calibrating XMM-Newton and NuSTAR to trace spectral features
› Quantum and Structural Effects Captured via a Statistical Method: the SACM Applied to HCN and HNC Colliding with CO
› The dispersal of compact protoplanetary discs
› High-speed single-photoelectron detection for Cherenkov astronomy
› SAPLE: Swift Analysis Pipeline for Lightcurve Extraction
› Comparing Results from Two Uniform Phase Curve Surveys
› Dynamic Competition of Fast and Collisional Neutrino Flavor Instabilities with Collisional Damping in Spatially Inhomogeneous Systems
› Breaking Free from the Swampland of Impossible Universes through the DESI Portal
› HI absorption in MHONGOOSE -- Spin temperatures and cold neutral medium in nearby disk galaxies
› Observational Properties of Nonthermal Emission from Relativistic Jets Escaping Active Galactic Nucleus Disks
› Can magnetic reconnection power neutrino emission from AGN coronae?
› An agentic framework for gravitational-wave counterpart association in the multi-messenger era
› Astrons: Reissner-Nordstr\"om Primordial Naked Singularities
› Co-evolution of the Milky Way high- and low-{\alpha} sequences with chemical evolution models
› On the origin of variability in $\alpha$ Cygni variable $\epsilon$ Ori (HD 37128) using TESS observations and modelling
› Mineral False Positives in the Search for Exoplanet Surface Biosignatures
› Photonic integrated circuits for astronomy: A formal description of an integrated photonics-based wavefront sensor (IP-WFS)
› Multifield stochastic inflation: Relevance of number of fields in statistical moments
› Gas Phase Distribution in the Neutral ISM: A Comparison between Observation and Numerical Simulation
› Machine Learning Techniques for Astrophysics and Cosmology: Simulation-Based Inference
› Numerical Study of Some Generalizations of the Starobinsky Inflationary Model
› Joint probabilistic inference of galaxy redshifts and rest-frame spectra from photometric fluxes with latent diffusion
› Revisiting the greenhouse effect of non-greenhouse gases in the atmospheres of Earth-like planets
› Search for long-term variability of HESS J1745-290
› Milky Way Dynamics Favor Dark Matter over Modified Gravity Models
› Characterizing Pulsar Distances Using HI Kinematics
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› Magnetic Evolution of Highly-Sheared Region in Active Region 13842 Producing Large X9.0 Flare
› Mitigating residual foregrounds and systematic errors in SKA1-Low AA* EoR observations via Bayesian Gaussian Process Regression
› Demonstrating the Use of the Spherical Fourier Bessel Basis for Large Scale Clustering Systematics Discovery and Mitigation with eBOSS
› Electromagnetic Follow-up of the Sub-Solar Mass Gravitational Wave Candidate S251112cm: Kilonova Constraints and a Coincident IIb Supernova
› Designing a low-loss high reflectivity mirror for gravitational waves detectors by combining a dielectric metasurface and a multilayer stack
› Producing the GeV Galactic Center Excess via Cosmic Ray-Dark Matter Scattering
› Neural Posterior Estimation of Terrain Parameters from Radar Sounder Data
› Primordial Black Hole Hotspots Beyond Flat Spacetime
› Revisiting predictions for cosmic-ray antinucleon fluxes from Galactic Dark Matter
› The Good, the Bad, and the Subtle: Relativistic mode sums for neutron-star tidal response
› Black hole mass and distance from accretion disk astrophysical observables
› Quasiparticle Quality Factors in Superconducting Resonators: Effects of Bath Temperature and Readout Power
› General Grad-Shafranov Equation
› Neutron stars in a conservative $f(R,T)$ gravity
› Asymmetric Reheating of Dark QED
› A study on Dusty Plasma Physics and the examination of Jeans Criteria for the Milky Way
› Controlled Penumbral Inflation from Monodromic Valleys
› Uncertainty in Physics and AI: Taxonomy, Quantification, and Validation
› Symfind: Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos
› Robust 1-norm periodograms for analysis of noisy non-Gaussian time series with irregular cadences: Application to VLBI astrometry of quasars
› Ultraheavy Ultrahigh-Energy Cosmic Rays
› Quantum coherence and the invisible Universe: Subradiance as a dark matter mechanism
› A Sample of Active Galactic Nuclei with Intermediate-mass Black Holes Extended to $z \approx$ 0.6
› The Two-component Model of the 'spokes' in Saturn's Rings
› Non-Gaussianity of Tensor Induced Density Perturbations
› LITMUS: Bayesian Lag Recovery in Reverberation Mapping with Fast Differentiable Models
› Ward Identity Constraints on Loop Corrections in Non-Attractor Inflation
› GW231123: A Possible Primordial Black Hole Origin
› Deep Learning for CMB Foreground Removal and Beam Deconvolution: A U-Net GAN Approach
› Evidence of the pair instability gap from black hole masses
› Observation of Galactic center in the sub-MeV gamma-ray band with electron-tracking Compton camera
› The Noise of Vacuum
› RX Gru: a short-period pre-main-sequence eclipsing binary with a distant circumbinary companion
› Jittering jets promote dust formation in core-collapse supernovae
› BGRem: A background noise remover for astronomical images based on a diffusion model
› DESI DR2 Galaxy Luminosity Functions
› Changing-Look AGN Powered By Disk Tearing
› A Fleeting GLIMPSE of N/O Enrichment at Cosmic Dawn: Evidence for Wolf Rayet N Stars in a z = 6.1 Galaxy
› Comparing galaxy merger orbits in hydrodynamical simulation and in dark-matter-only simulation
› Tracing the Trace Anomaly of Dense Matter inside Neutron Stars
› Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows
› OzDES Reverberation Mapping of Active Galactic Nuclei: Final Data Release, Black-Hole Mass Results, & Scaling Relations
› Reaching diffraction-limited localization with coherent PTAs
› The abundance of thin dwarf galaxies: a challenge for cosmological simulations
› KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature
› Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference
› Resolving the Core-Cusp and Diversity Problems with a Baryon-Correlated Dark Matter Profile
› Revisiting the Reported Period of FRB 20201124A Using MCMC Methods
› Possible evidence for a pair-instability supernova nature of ultra-early JWST sources
› New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
› Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics
› Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN
› The early r-process nucleosynthesis scenarios
› Impact of Rastall gravity on hydrostatic mass of galaxy clusters
› Rarity of rocket-driven Penrose extraction in Kerr spacetime
› Studying dark gaps in Ly-$\alpha$ forest transmission with large reionization simulations
› A Unified Framework for 10 TeV to EeV Diffuse Neutrino Sky and KM3-230213A
› Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
› Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts
› Large-scale and local environmental drivers of quenching: tracing H$\alpha$ concentration in X-ray and optical galaxy groups
› Inferring the population properties of galactic binaries from LISA's stochastic foreground
› Magnetic structure of coronal dark halos
› Variational views for self-supervised learning in radio astronomy
› Primordial Black Hole Formation in Rastall Gravity: Shifted Collapse Threshold and Exponential Abundance Sensitivity
› Inefficiency of chiral dynamos in protoneutron stars and the early universe
› Cosmological peculiar velocities in general relativity
› The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
› Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy
› Organosulfur Chemistry on sub-Neptunes: Implications for hazes and biosignatures
› Early emission characterization of TDE 2025aarm
› ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser
› Large-scale Morphology of the Optical F-corona from a Total Solar Eclipse Observation During the Artemis II Lunar Flyby
› Long-Term Dynamical Evolution and Ejection of Near-Earth Asteroids
› The apparent Large Magellanic Cloud star cluster age gap
› Sub-Neptunes Show a Stronger Correlation with Cold Jupiters than Super-Earths Especially in Metal-rich Systems
› A SPHEREx Pipeline and Spectral Library for Ultracool Dwarfs
› Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity
› A Multi-Survey Machine-Readable Corpus of Milky Way Globular Cluster Parameters for Retrieval-Augmented Generation Applications
› PySME v1.0: improved modelling of stellar spectra for survey-scale applications
› How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4
› On the origin of the environmental step: A BayeSN view of the ZTF SN Ia DR2
› String Thresholds, Dynamical Gauss--Bonnet Couplings, and Starobinsky Attractors
› Neutron Star Eclipses as Axion Laboratories
› Parameter inference of millilensed gravitational waves using neural spline flows
› How Many Times Should We Matched Filter Gravitational Wave Data? A Comparison of GstLAL's Online and Offline Performance
› New Methods for Offline GstLAL Analyses
› Inflation Model Based on Virasoro Squeezing
› Searching for dark photon dark matter from terrestrial magnetic fields
› Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
› Orbital dynamics and precession in magnetized Kerr spacetime
› Nucleosynthesis and CMB bounds on photophilic ALPs: a fresh look
› Boson Stars Hosting Black Holes
› Properties of Stable Massive Quark Stars in Holography
› Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model
› Curvaton-assisted hilltop inflation
› Cosmological long-wavelength solutions in non-adiabatic multi-fluid systems
› The new generation lunar gravitational wave detectors: sky map resolution and joint analysis
› An approximate Kappa generator for particle simulations
› Effects of isovector spin-orbit interaction on the charge-weak form factor difference in $^{48}$Ca, $^{208}$Pb, $^{90}$Zr and $^{62}$Ni
› Searching for axions with time resolved pulsar polarimetry
› Preliminary study on the impact of stress-energy tensor compared to scalar field in Nonminimal Derivative model
› Outer-Crust Equations of State for Neutron Stars
› Quantum Noise Fraction and the Thermal Frontier in High-Frequency Gravitational Wave Detection
› Hadronic lensing
› Adaptive ray tracing, image diagnostics, and photon ring signatures of rotating dark-matter-dressed black holes

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