Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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RSS  Najnowsze prace na astro-ph:

› Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with HMG
› Time-resolved XRISM spectroscopy reveals the evolution and structure of the corona in MCG-6-30-15
› High-energy neutrino constraints on primordial black holes as dark matter
› A first empirical derivation of the average dust attenuation law at 2
› Eccentricities of millisecond pulsars with intermediate-mass progenitors
› Gaia astrometry disfavors a binary origin for long secondary periods
› Magnetic field alignment with dense cores in the transition between cloud and core scales
› Repopulating the pair-instability mass gap without sustained growth to massive IMBHs: the case of 47\,Tuc
› JWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia Supernova
› Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk
› Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics
› Even a precessing clock is right twice per orbit -- The super-periods of eRO-QPE2 and challenges for quasi-periodic eruption orbital models
› Observational and Dynamical Constraints on an Unseen Outer Perturber in the GJ 436 Hot Neptune
› High Resolution X-ray Spectroscopy of the Nova-Like Cataclysmic Variable BZ Cam using Chandra HETG: Diagnosis of the ADAF-like (Advective) Hot Flow
› Spectroscopic Characterization of WD J000801.25-350450 and its Two Co-Moving Companions
› Kozai-driven mass loss of the circumbinary disk in D9 in orbit around the supermassive black hole Sgr A*
› PEACC -- Precision Emitter for 21 cm Array Coherent Calibration
› Galactic Archaeology with the Subaru `\=Onohi`ula Prime Focus Spectrograph Strategic Program
› A Study of HH 270 with the James Webb Space Telescope
› Near-critical magnetic fields in Kepler red giants
› Impacts of Multidimensional Progenitor Perturbations on Core-Collapse Supernova Explosions
› Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation
› Spectroscopic Survey of Faint Planetary-Nebula Nuclei. VIII. The Dwarf Barium Central Star of Kohoutek 1-9
› Secular Light Curve of Exocomet 3I/ATLAS, and its Location on a Comet Evolutionary Diagram
› Environmental Dependence of Galaxy properties: A study of 341 Ring Galaxies in Cosmic Voids
› To understand the radiative processes of pulsars and fast radio bursts with the FAST
› Estimating the Luminosities of Protostars with Limited Infrared Photometry
› Possible Supermassive Dark Object Composed of Light Fermionic Gas with an Embedded Neutron Star Core
› Predicting Associations between Solar Flares and Coronal Mass Ejections Using SDO/HMI Magnetograms and a Hybrid Neural Network
› Ring formation around giant planets by tidal disruption of a single passing large Kuiper belt object II: The dynamical fate of tidal fragments
› Daily Predictions of F10.7 and F30 Solar Indices with Deep Learning
› A Multi-modal Fusion Network for Star-Galaxy Classification from CSST Simulated Datasets
› Impact of Observational and Modelling Assumptions on Intergalactic Magnetic Field Constraints from TeV Gamma-Ray Bursts with the Cherenkov Telescope Array Observatory
› Starbursts at Cosmic Dawn: Formation of Globular Clusters, Ultra-Faint Dwarfs, and Population III star clusters at z > 6
› Joint Observation of SGR J1935+2154 with \textit{Insight}-HXMT and KM40m during the active episode of October 2022
› A seeing measurement device for the PoET solar telescope
› Inflationary magnetogenesis from non-minimal coupling in large- and small-field potentials
› Uncovering the Dominant Spatial Scales of the Sun's Magnetic Field in Solar Cycle 24
› An Analytic Formalism of Inflation for Derivative Coupled Scalar Field and Validating its predictions for Some Inflationary Potentials
› A Theoretical Investigation of He I Line Profiles for the Spectroscopic Analysis of DB White Dwarfs
› Lorentz invariance violation search with flaring active galactic nuclei observations of the first Large-Sized Telescope of CTAO
› A Fast Direct Solver for Mutual Coupling Analysis of Large Arrays of Reflector Antennas
› The Milky Way Tomography with Subaru Hyper Suprime-Cam. II. Global halo structure
› The Milky Way Tomography with Subaru Hyper Suprime-Cam: Implications for the past orbit of the Large Magellanic Cloud
› Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign
› Miscibility and Transport Properties in Hydrogen-Neon Mixtures
› Multi-TeV $\gamma$-ray candidates from GRB 221009A: a downturn in the intrinsic $\gamma$-ray spectrum, an echo of the prompt emission phase, and intergalactic electromagnetic cascades
› A Path to Constraints on Common Envelope Ejection in Massive Binaries: Full Evolutionary Reconstruction of Three Black Hole X-ray Binaries
› Probing the Origin of Magnetar X-ray Polarization Diversity: A Multi-wavelength Geometrical Study of 1E 1547.0-5408 and 1E 2259+586
› Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations
› Searching for Gamma Ray Bursts associated with CHIME Fast Radio bursts
› Ages and masses of asymptotic giant branch stars from the period--luminosity diagram
› Vertical Structure of Local Disk Galaxies revealed by DESI Imaging Data
› Magnetic Reconnection at Hyperbolic Flux Tube associated with a Confined Flare in NOAA Active Region 12268
› Spatio-temporal analysis of helioseismic quasi-biennial oscillations
› Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
› Thermal Segregation and Reddening in Europa's Double Ridges
› Reionization Topology as a Probe of Self-Interacting Dark Matter
› The demise of the synchronous moon that gave Mars its triaxiality. The role of solar tides and a palaeo ocean
› Inferring Unreported Measurement Uncertainties via Information Geometry in Astrophysics
› A consistent MOND modelling of the Bullet Cluster
› Improving Solar Flare Soft X-ray Classification With FOXES: A Framework For Operational X-ray Emission Synthesis
› Systematic census of RR Lyrae stars in Milky Way stellar streams
› A Turbulence-Driven Magnetic Reconnection Model for the High-Energy Neutrino Emission from NGC 1068
› Plasma lensing modeling of substructures on pulsar scintillation screens
› Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b
› Seasonal Variability of Pluto's Haze Formation Revealed by Laboratory Simulations
› On the origin of the BAOtr-DESI tension
› Lunar nutation effect defines the sign of the Earth rotation rate for now, but this may change soon
› White Dwarfs with Infrared Excess from DESI EDR
› From Fragments to Flares: Migration, Tidal Disruption, and Observable Bursts in Massive Protostellar Disks
› Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid
› Space-Clock Elevator: Multi-Stage Orbital Transport via Rotating Tethers and Elliptical Nodes
› Observations of highly inclined disks with ALMA. Results from 12CO gas and continuum observations
› First observational constraints on cosmic backreaction over an extended redshift range
› Streaming instabilities in weakly ionized protoplanetary discs: the Ambipolar Streaming Instability (AmSI)
› A Comparative Study of TeV Gamma-Ray Sources with Various Objects
› Statistical Study of Balmer Continuum Enhancement in Solar Flares
› Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948
› The high-altitude, inner-disc, and chemically peculiar open cluster UBC 1052
› Compact CO emission and no evidence of radial drift. ALMA observations of the faintest planet-forming disks in Lupus
› GeV gamma-ray emission in the field of the shell-type supernova remnant Vela Jr revisited
› A Ring of Fire Orphan {\gamma}-Ray Flare in the Neutrino Candidate 3C 120
› A Falsifiable Timing Test for the Double-White-Dwarf Model of Long-Period Transients
› Ultra-fast simulations of the solar dipole and open flux
› Extragalactic microlensing through Ultra Diffuse Galaxies
› From Dust to Planets -- A Chemical Perspective
› Compact Hydrogen Sulfide Emission Indicates Sulfur-bearing Ice Sublimation in the Inner Disk of HD 163296
› The environmental imprint on molecular layering in the dusty streamer of M512
› Emergence of Complex Structures
› Scale-dependent surface and volume density properties of filaments in molecular clouds
› The RoPES project with HARPS and HARPS-N III. Two candidate planets orbiting the G-type star HD 161098
› Global m=1 slow mode in near-Keplerian self-gravitating torus: applications to stellar nuclear disks and AGN molecular tori
› Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal
› The magnetic sensitivity of the Ca II H and K lines
› Galactic Diffuse Gamma-Ray and Neutrino Emission from Cosmic-Ray Interactions in Stellar Atmospheres
› Combining the Mass--Radius Posteriors of J0030+0451 Allowing for Unknown Model Systematics
› Investigation of gravitational stability of protoplanetary disks based on statistical analysis of their masses
› Multi-fluid multi-species models for inverse FIP-effect
› Prominence signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics
› Do little red dots really form a distinct class of astronomical objects?
› Cosmological inference with halo clustering reconstructed from the redshift-space galaxy distribution
› A bright flare in the obscured state of GRS 1915+105 as seen by NICER and Swift
› The GAPS Programme at TNG. LXXIII. Confirmation of the hot sub-Neptune TOI-4602 b (HD 25295 b), a key target for future atmospheric characterization
› NGC 1647: A young open cluster with a broad main sequence observed with LAMOST
› Origin and characterization of super-Earths and sub-Neptunes
› The nature of tilted supercritical accretion discs
› Effective Stability of Near-Rectilinear Halo Orbits in the Earth-Moon System
› Exact Gravastar Solution
› Generalized Kolmogorov systems with applications to astrophysics and biology
› Toward Neutrino and Dark Matter Detection with Ancient Minerals: TEM Study of Heavy-Ion Tracks in Olivine
› Spin-($0$, $1$, $\frac{1}{2}$) Field Perturbations, Quasinormal Modes, Overtones, Greybody Factors and Strong Cosmic Censorship of Einstein-Skyrme Black Holes
› Testing the Kerr hypothesis beyond the quadrupole with GW241011
› Induced Multi-phase Inflation with Reheating: Leptogenesis and Dark Matter Production in Metric versus Palatini
› Ion pickup and velocity space thermalization at outer planet moons
› Geometrically Significant Surfaces of Black Holes from a Single Scalar
› Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity
› Discussion on the equivalence of two relativistic point-particle Lagrangians
› Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals
› Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models
› Radiatively Corrected Hybrid Inflation: Parameter Scans and Machine Learning with ACT and Future CMB Experiments
› Probing Yukawa Gravity with Modulated Newtonian Cancellation in the CHRONOS Detector
› Emulator-Assisted Nuclear DFT Inference and Its Consequences for the Structure of Neutron Stars
› Helicity-supported stationary spacetimes: A class of finite-energy, horizonless, axisymmetric solutions
› Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas
› JWST reveals the diversity of nuclear obscuring dust in nearby AGN: nuclear isolation of MIRI/MRS datacubes and continuum spectral fitting
› Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order
› The Quintom theory of dark energy after DESI DR2
› Euclid preparation. LXXXIX. Accurate and precise data-driven angular power spectrum covariances
› Non-relativistic effective theories for fields with general potentials and their implications for cosmology
› Comparative Study of Early-Universe Epochs in an $f(R,L_m)$ Gravity Model with Effective Curvature--Matter Interaction and $\Lambda$CDM Cosmology
› Population III star formation near high-redshift active galactic nuclei
› Prototyping of 6.2-mm-Pitch Fiber Positioner Modules for Stage-V Telescope Instrumentation
› JWST Spectroscopic Insights Into the Diversity of Galaxies in the First 500 Myr: Short-Lived Snapshots Along a Common Evolutionary Pathway
› A fast machine learning tool to predict the composition of astronomical ices from infrared absorption spectra
› Gravitational waves reveal the pair-instability mass gap and constrain nuclear burning in massive stars
› Parity Violation in Galaxy Shapes: Primordial Non-Gaussianity
› Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints
› On Atomic Line Opacities for Modeling Astrophysical Radiative Transfer
› Graph-based Summary Statistics for Revealing the Stochastic Gravitational Wave Background in Pulsar Timing Arrays
› The Colors of Ices: Measuring ice column density through photometry
› Low-noise Fourier Transform Spectroscopy Enabled by Superconducting On-Chip Filterbank Spectrometers
› Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference
› Magnetized Shocks Mediated by Radiation from Leptonic and Hadronic Processes
› Primary gravitational waves at high frequencies I: Origin of suppression in the power spectrum
› Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network
› Phase-space perturbation theory for cosmic large-scale structure
› Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
› Effects of the radiative interior on solar inertial modes
› Cygnus X-3: A variable petaelectronvolt gamma-ray source
› Early thin-disc assembly revealed by JWST edge-on galaxies
› BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion
› Twenty-four thousand hours of GREENBURST observations with the GBT
› Extreme-Value Distribution Analysis of the Second CHIME/FRB Catalog: Assessing the Rarity of the One-off FRB 20250316A
› SN 2017ati: A luminous type IIb explosion from a massive progenitor
› A Minimal Interpretation of the Galactic Cosmic-Ray Proton and Helium Spectra from GeV to PeV Energies
› Stone Skipping Black Holes in Ultralight Dark Matter Solitons
› Predicting New Concept-Object Associations in Astronomy by Mining the Literature
› The Physical Properties of PS1-12sk and the implications for its Progenitor System
› Spectral Universality of Turbulent Fluctuations in Relativistic Flows
› Outflow from unmagnetized shocked radiative transonic accretion disk around a black hole
› Characterizing the Instrumental Profile of LAMOST
› Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments
› Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity
› Reconnection-driven State Transitions in Flat Spectrum Radio Quasars
› Mass Inventory of the Solar System Beyond the Sun: A Systematic Compilation with Uncertainty Budget
› TESS light curves of two new magnetic cataclysmic variables: an asynchronous polar at the period minimum, and an eclipsing system with a large spin-to-orbit ratio
› Measurement of the Orbital Parameters, Spin and Spectral Evolution During the Main High State of Her X-1 with Insight-HXMT
› Direct N-body simulations of rotating and extremely massive Population III star clusters
› An inverted infall profile for the collapse of the massive star-forming IRDC SDC335.579-0.292
› Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters
› Monitoring Volatile Evolution in Disrupting Comet D/2021 A1 (Leonard) with NOEMA and APEX
› Beyond $f(\phi)\mathcal{G}$: Gauss--Bonnet inflation with $\mu(\phi,X)$
› UMI: GPU-Accelerated Asymmetric Robust Estimator for Photometric Detrending in Exoplanet Transit Searches
› The Way We Tally Becomes the Tale: the Impact of Selection Strategies on the Inferred Evolution of Little Red Dots Across Cosmic Time
› Optical images of Kerr-Sen black hole illuminated by thick accretion disks
› Validating Prior-informed Fisher-matrix Analyses against GWTC Data
› Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory
› Supernova production of axion-like particles coupling to electrons, reloaded
› Exploring Leptogenesis in the Era of First Order Electroweak Phase Transition
› Possible evidences for physics beyond $\Lambda$CDM from DESI DR2 data
› Studying Ionospheric Phase Structure Functions Using Wide-Band uGMRT (Band-4) Interferometric Data
› Comparing astrophysical models to gravitational-wave data in the observable space
› Completing Axion Double Level Crossings
› Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair
› Scattering of massive particles from black holes and naked singularities
› False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE
› A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
› Quasi-pole inflation in metric-affine gravity
› Reheating in geometric Weyl-invariant Einstein-Cartan gravity
› The global structure of the time delay likelihood
› Accelerated Time-domain Analysis for Gravitational Wave Astronomy
› Probing soft signals of gravitational-wave memory with space-based interferometers

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