Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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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:

› A practical guide to implementing zero-order-hold interplanetary trajectory legs
› Clustering constraints on super-early galaxy formation scenarios
› Spectroscopic Bolometric Corrections and Empirical Zero-point Constants of \textit{Gaia} Magnitudes, $G$, $G_{\rm BP}$, and $G_{\rm RP}$, from \textit{Gaia} XP Spectra
› A correlation predicting galaxies without dark matter
› Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722)
› A Uniform Determination of the Bulk Metallicities and Alpha Enrichments of Confirmed Exoplanet Systems with TRES
› The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6
› New Isocurvature Constraints from JWST UV Luminosity Function
› FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics
› A Quantum Gravitational Mechanism for Isotropization of de Sitter Cosmologies
› The $R$-Process Alliance: The $R$-Process Enhancement of Stars from Chemodynamically Tagged Groups in the Milky Way Halo
› Seasonal Insolation Variability on Early Venus: Implications for Energy Budget
› The Quadruply Lensed Supernova SN 2025wny: Implications for LSST
› Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
› Survey Footprint Explorer: A Browser-Based Interactive Tool for Visualizing and Cross-Matching Astronomical Survey Footprints
› Tracing Radio AGN-Driven Quenching in Post-Starburst Galaxies at Cosmic Noon
› A Cyclic Burst Rate Behavior of a Persistent X-ray Burster: Recent XMM-Newton and NuSTAR Observations of 4U 1323-62
› Detection and Characterization of the Temperate Super-Earth Ross 318 b
› An Outer Giant Planet or Brown Dwarf in the 51 Pegasi System?
› Quantifying the Reconstructability of Astrophysical Methods with Large Language Models and Information Theory: A Case Study in Spectral Reconstruction
› From raw data to neutrino candidates: a neural-network pipeline for Baikal-GVD
› The Extended Plane of the Local Supercluster
› Prospects for multi-messenger discovery of the gravitational-wave background anisotropies via cross-correlation with galaxies
› The applicability of the JAGB method for measuring the distance of galaxies subject to different metal enrichment rates
› Variable stars in the field of the Galactic globular cluster M71
› Black Hole Binary Detection Landscape for the Laser Interferometer Lunar Antenna (LILA): Signal-to-Noise Calculations & Science Cases
› Optical Design of OPTICAM-ARG: A Three-Channel High-Time-Resolution Camera for the Jorge Sahade Telescope
› Continuous mass ablation of planets engulfed in stellar envelopes
› Transonic accretion and the analogue gravity in multi-component elliptical galaxies hosting pseudo-Schwarzschild black holes
› The Internal Nebular Attenuation Curve of Three-Dimensional Turbulent HII regions
› An investigation of magnetic energy and helicity thresholds at the onset of solar eruptions based on numerical simulations
› Exploring the stellar streams and satellites around the giant low surface brightness galaxy Malin 1
› Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin
› Revisiting GW170817 at milliarcsecond scale: high-precision constraints on jet geometry and $H_0$
› A Nearly Constant Compton y-parameter for Mildly Relativistic Slab Coronae in AGN
› Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints
› A Hybrid Origin for the Multiple Ring-Gap Structures in the Large Protoplanetary Disk V1094 Sco: A Low-Mass Planet and Secular Gravitational Instability
› Black Hole Ringdown Seen in Photon Polarization Swings
› Are Single-Zone Emission models Sufficient to Explain GRB 220426A and GRB 230812B?
› A hierarchical Bayesian pipeline for soliton-plus-NFW inference on SPARC rotation curves: diagnostics and prior-boundary behaviour
› Interacting Binary Stars as Progenitors for Interacting Supernovae
› Metal Enrichment by the First Stars Exploding at the Lower Energy Limit of Pair-Instability Supernovae
› GI BAO as a cosmological consistency check
› Evidence for Multiple Orbiting Hotspots in the 340 GHz Variability of Sgr A*
› Starspot activity and surface differential rotation on UX Arietis
› Synergy between the Cherenkov Telescope Array Observatory and the Vera C. Rubin Observatory
› A New Timing Signature of Black Hole Spin: Time-Delay Asymmetry in Kerr Accretion Flows
› Measurements and predictions of H2 pressure-broadening coefficients of CO2 absorption lines for exoplanet atmosphere studies
› Simulation of the spin evolution of some selected exoplanets and inferences on their climate
› Reaccumulation process after a catastrophic disruption event on a differentiated asteroid
› Real-time detection of solar flares from ground-based VLF data
› High-energy Multi-messenger Emission from Galaxy Clusters in the Local Universe
› High-energy Neutrino and Gamma Ray Emission from Clusters-like Perseus
› Inferring host environment properties and gravitational-wave decay time from the eccentricity measurement of dynamically captured binaries
› Limit on high energy neutrino emission from Abell 119 using IceCube 10-year muon track data
› Marginal multi-object multi-frame blind deconvolution
› A phenomenological model of the magnetic field re-emergence in magnetars and discrepancy between the kinematic and characteristic ages
› An eclipsing CEMP candidate discovered in a search for dwarf carbon stars in post-common envelope binaries
› Ultra-light axion constraints from Planck and ACT: the role of nonlinear modelling
› Effect of Solar Flares on Decayless Kink Oscillations in Nearby Coronal Loops
› Catching UHE Neutrinos with HERON
› Periodic Emission Frequency Modulation in a Hyperactive Fast Radio Burst
› Discriminating Planck Reionisation Histories with the kSZ Effect
› Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects
› Proximate damped Lyman-$\alpha$ systems as tracers of quasar feedback
› A tool of Hierarchical cOre ideNtification and Kinematic property AssIgnment (HONKAI) for Dense Cores
› An Ultra-Short Period Super-Earth and a Sub-Neptune Orbiting the K dwarf TOI-4311
› How plasma coupling and convective-zone depth shape the rotation of solar-mass stars
› Simulating the jittering-jets explosion mechanism: Supernova remnant G11.2-0.3
› Trajectory-Agnostic Asteroid Detection in TESS with Deep Learning
› Impact of Calibration Systematics on Dark Energy Constraints from LSST Type Ia Supernovae
› Late-time reconstruction of non-minimally coupled gravity with a smoothness prior
› Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets
› Self-consistent dynamical modelling of the Milky Way bar with orbital frequency analysis
› Precessing Black Hole Jets and Galactic Fossils
› Elemental Abundances in the Binary Star V505 Per
› Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles
› Photometric determination of the mass accretion rates of pre-main sequence stars. IX. Recent star formation in the periphery of NGC 346
› Measuring cosmic bulk flow with kinetic Sunyaev-Zel'dovich velocity reconstruction
› Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data
› Big Mysteries Survey: Physicists' Views on Cosmology, Black Holes, Quantum Mechanics, and Quantum Gravity
› Neutrino mixing and gravitational production via inflation
› CMB Birefringence from Vacuum Interfaces
› An ultra-broadband axion dark matter experiment
› Stochastic inflation from a non-equilibrium renormalization group
› The mean-field theory of superfluid-superconducting vortex states in the outer core of neutron stars
› gwBenchmarks: Stress-Testing LLM Agents on High-Precision Gravitational Wave Astronomy
› End-to-End Population Inference from Gravitational-Wave Strain using Transformers
› Detection of Gravitons: Graviton Absorption and Excess of Photon Luminosity from Interstellar Hydrogen
› Discovery of Interpretable Surrogates via Agentic AI: Application to Gravitational Waves
› Closing the Cosmographic Hierarchy: Dynamical Attractors from Inflation to Reheating
› Dynamic Alignment: A Fragile Survival Effect
› Reviving primordial black hole formation in slow first-order phase transitions
› Causality and Scientific Inquiry: Lessons from Space Physics and Medical Sciences
› GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors
› A self-adjoint Fourier-type model for the iQuad wavefront sensor
› Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating
› The choice of variables in cosmological dynamical systems
› Power Studies For Two-Sample and Goodness-of-Fit Methods For Multivariate Data
› Hyperfine-Resolved Rovibrational and Rotational Spectroscopy of OH$^+$ ($X ^3\Sigma^-$)
› Basilisk and Docker for Reproducible GN&C Simulation: A Workflow Reference
› Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM
› Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A
› Denoising weak lensing mass maps with diffusion model: systematic comparison with generative adversarial network
› A search for periodic AGN variability in $\textit{Gaia}$ Data Release 3
› Quantifying biases in stellar masses of JWST high-z quasar host galaxies caused by quasar subtraction
› Optical Flares in the Luminous Fast Blue Optical Transient AT2022tsd ("Tasmanian Devil")
› Exploring Jet Structure and Dynamics in Short Gamma Ray Bursts: A Case Study on GRB 090510
› Dark Matter and the Early Formation of Supermassive Black Holes
› Correcting the fiber-aperture bias affecting galaxy stellar populations in the Sloan Digital Sky Survey. Aperture corrections to absorption indices based on CALIFA integral field observations
› Probing Evolution of Long Gamma-Ray Burst Properties through Their Cosmic Formation History
› Probing evolution of Long GRB properties through their cosmic formation history aided by Machine Learning predicted redshifts
› Dark Matter from Holography
› A Bayesian Perspective on Evidence for Evolving Dark Energy
› The Impact of Supermassive Black Holes on Exoplanet Habitability. I. Spanning the Natural Mass Range
› Probing the Nature of Dark Matter Self-Interactions Through Observations of Massive Black Hole Mergers
› Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems
› Core-halo scaling relations in self-interacting scalar field dark matter
› Evolving and interacting dark energy: photometric and spectroscopic synergy with DES Y3 and DESI DR2
› Sensitivity of Weak Lensing Surveys to Gravitational Waves from Inspiraling Supermassive Black Hole Binaries
› Comprehensive study of solar type II radio bursts and the properties of the associated shock waves
› The JWST EXCELS survey: Outflows in 1.5 < z < 5 quiescent and recently quenched galaxies are likely relics from episodic AGN activity
› Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
› Possible evidence for a pair-instability supernova nature of ultra-early JWST sources
› Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
› An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A*
› Cosmological Averaging in Nonminimally Coupled Gravity
› Cylindrical cosmological simulations with StePS
› Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4
› X-SORTER (X-ray Survey Of meRging clusTErs in Redmapper): X-ray and Spectroscopic Characterization of 12 Optically Selected Galaxy Cluster Merger Candidates
› JWST's PEARLS: A clumpy ring galaxy at $z = 4.0148$
› The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4 < z < 6$
› Dust characterization of halos: The extended emission in protoplanetary disks
› Other red dots: A possible GLIMPSE of normal AGB stars at Cosmic Noon through extreme lensing
› IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament
› A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model
› Moving-Mesh Simulations of Mini-Common Envelope Ejection in Classical Novae
› Jet-driven shocks and turbulence in radio-loud Active Galactic Nuclei observed with JWST MIRI/MRS
› Challenges to the cosmological constant model following results from the Dark Energy Survey
› Application of Machine Learning to 21 cm Cosmology
› Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
› Theoretical Detailed Analyses for DC readout and a Fabri-P\'erot gravitational-wave detector
› Biased parameter inference of eccentric, spin-precessing binary black holes
› APRIL: Auxiliary Physically-Redundant Information in Loss -- A physics-informed framework for parameter estimation with a gravitational-wave case study
› Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties
› Covariant interpretation of proper infall times in Kerr spacetime
› Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity

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