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:

› Effective Field Theory for a Baryon-Correlated Dark Matter Profile
› Cosmological perturbations with $f(R)$ gravity scalarons : Galaxy power spectra and the scalaron mass
› CMB Acoustic Power Spectra in STVG-MOG
› Simulation-Based Prediction of Black Hole Fe K$\alpha$ Line Profiles
› Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection
› Inferring Globular Cluster Initial Mass Function from Stellar Streams
› Suppression of Radiative Cooling in Galaxy Cluster Cores by the Combination of AGN Heating and Sloshing
› On the origin of anomalous dissipation in simulations of tidal disruption events
› Thermal Structure and Chemical Enrichment of the North and South Polar Spurs: Supersolar N/O and Ne/O in the X-ray Plasma
› Unraveling the Mystery of the Peculiar and Young Hot Jupiter CoRoT-2b. I. H$_2$O and CO Detection from Dayside Observations with Gemini-S/IGRINS
› Sensitivity of spectral lines to granulation: from the Sun to K-type stars
› On the correlation between globular clusters and the distribution of dark matter in galaxy clusters: the case of Abell 2744
› The Highly Variable Wind from WD J005311, the Stellar Remnant of the Peculiar Galactic Supernova of 1181
› Investigating the impact of Solar Fusion III reaction rates on helioseismic constraints and solar neutrino fluxes
› Formation of intermediate-mass black holes in young massive clusters detected with JWST: analytic mass estimates
› The Splashback Mass Function of Galaxy Clusters from Photometric Data
› Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns
› Dynamical Cluster Assembly Framework (D-CAF): The Link Between Star Cluster Formation and Expansion Rates
› JWST Observations of Asteroid 2024 YR4 Rule Out a 2032 Lunar Impact and Demonstrate a New Regime for Planetary Defense Follow-up
› The chemo-dynamical complexity of {\omega} Centauri: different kinematics for different populations
› Mapping Cosmological Signal Scales to Beam Calibration Requirements in 21cm Experiments and Implications for Near-Field Measurement
› Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
› Binary Neutron Star Merger Evolution and r-Process Enrichment in the Milky Way Disk
› The \emph{R}-process Alliance: A Bright, Strongly \emph{R}-process-enhanced Extremely Metal-poor Star Observed with GHOST
› Connecting CGM enrichment with Lyman alpha emitters at 2.9 < z < 6.7
› Multi-wavelength Emission for a Post-merger Magnetar: The Magnetar-Driven Poynting Jet and Its Associated Pulsar Wind Nebula
› Formation of extremely low-mass white dwarf binaries undergoing enhanced angular momentum loss
› A systematic study of CO/SiO absorption features in early-type galaxies using AKARI/IRC near-infrared spectra
› CO(7-6) and [C I](2-1) survey in z > 6 quasars
› Data Formats and Visualisation BoF
› Probing late-time deviations from $\Lambda$CDM with a quadratic dark energy expansion
› A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667
› Revisiting the mass metallicity relation and the fundamental metallicity relation of dwarf galaxies at cosmic noon with NIRISS
› Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions
› Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT
› Adaptive multi-line fitting for stable line-core intensity and Doppler velocity
› Robustness Analysis of USmorph: II. Optimizing Feature Extraction, Dimensionality Reduction, and Clustering for Unsupervised Galaxy Morphology Classification
› Down going muon rate monitoring in the ANTARES detector
› Relativistic Scattering in the Funnel of Cygnus X-3
› The TNG50-SKIRT Atlas: Multi-wavelength nonparametric galaxy morphology
› Difference Between Half-mass Radius and Half-light Radius of Galaxies at 0.2 $< z
› Interpretations of galaxy spectra at high redshift. \ The H_gamma/H_beta excess
› Superfluid fraction in the crystalline crust of a neutron star: role of quantum zero-point motion of ions
› Type-III solar radio bursts with spike-like toppings
› Dawn of the Milky Way disk: Determination of when a rotationally supported disk appears and dating the spin-up of the disk
› Lack of Significant Orbital-Phase Locking in the Active Phases of the Recurrent Nova T CrB
› Reconstruction of Reionization Histories from 21 cm Power-Spectrum Evolution with Artificial Neural Networks
› Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models
› The radio emission from radiative filaments of Cygnus Loop
› The Search for Technosignatures: a Review of Possibilities
› B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12
› Multi-diagnostic convergence: a single measurement in weakly collisional plasmas
› CosmoForge I: A unified framework for QML power spectrum estimation and pixel-based likelihood analysis
› The benefit of a multi-band high resolution spectroscopic monitoring for studying stellar transients: the NGC 300 OT2008-1 UVES spectrum as a test case
› Detection of a dark matter subhalo in the strongly lensed system PJ011646
› Solar Vortices: Catalysts of Magnetoacoustic Wave Dissipation and Atmospheric Heating
› The Beauty of k2: Probing Stellar Interiors Using Apsidal Motion. I. The Benchmark Massive Binary HD 152248
› Chandra X-ray Observations of the Pulsar Wind Nebula within CTA 1
› On the Possibility of an Extragalactic Positron Annihilation Signal
› Optical Super-orbital Modulation of SMC X-1: Disk Precession and a Revised Pulsar Mass
› HD 38973 b -- a cold Saturn orbiting a Sun-like star
› FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287
› Searching for links between energetic millisecond pulsars and repeating fast radio bursts
› Euclid: Early Release Observations -- The formation of peanutty dwarf galaxies in Perseus
› Compact Object Astrophysics with Frontline Astrometry
› Producing planetary debris exterior to white dwarf Roche radii through sublimative rotational fission
› Lithium Enrichment in a Subgiant Star with a Brown Dwarf Companion: A Planetary Engulfment Candidate
› Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum
› Negative neutrino mass or negative dark energy?
› The giant pulse population of PSR B0355+54
› Velocityformer: Broken-Symmetry-Matched Equivariant Graph Transformers for Cosmological Velocity Reconstruction
› The Era of Extremely Large Optical Telescopes The ELT
› The third wheel: ringdown and lensing of triple systems
› Cosmological History of Flavour Deconstruction Models: Constraints from Monopole Production
› Indirect Parametric Resonance of the Electromagnetic Field Driven by an Oscillating SU(2) Dark Matter Condensate
› Benchmarking Cylindrical Blast Wave Theory Against the OSIRIS-REx Sample Return Capsule Reentry
› Compensator-Based Inference for Signal Detection Under Unknown Background
› Audible Axion Magnetogenesis: Linking Intergalactic Magnetic Fields and Gravitational Waves
› Self-Consistent Parker Bound on Magnetic Monopoles
› Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection
› Cosmological Collider Signatures from Right-Handed Neutrino Loop
› Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component
› Opening the Window of Ultra-Light PBHs by Exorcising the Poltergeist
› Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
› Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations
› Chemical decoding of kinematic substructures in the Galactic halo
› Recalibration of the H$\alpha$ surface brightness-radius relation for planetary nebulae using Gaia DR3: new distances and the Milky Way oxygen radial gradient
› Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates
› JADES: An Abundance of Ultra-Distant T- and Y-Dwarfs in Deep Extragalactic Data
› Growth of Structure in Multi-species Wave Dark Matter
› Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations
› An Extreme Scattering Event Toward PSR J2313+4253
› Radiation-mediated shocks in gamma-ray bursts: spectral evolution
› High-energy radiation from the pulsar Equatorial Current Sheet
› Can accreting isolated neutron stars be detected?
› JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8
› Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
› ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior
› The Nysa family as the main source of unequilibrated LL ordinary chondrites
› Cosmic-Ray Spectra and Metal Budget Regulated by the Galactic Wind
› The MeerKAT 1.3 GHz Survey of the Large Magellanic Cloud
› Cosmic Environment as the Primary Driver of Dwarf Satellite Statistics
› Observational constraints on Luciano-Saridakis entropic cosmology
› Resolving diffusion signatures in distant pulsar halos with current and future experiments
› Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
› The Hubble Missing Globular Cluster Survey. III. Astro-photometric catalogs, artificial-star tests, and improved absolute proper motions
› The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
› Kardashev's Conundrum: Statistical Falsification of the Standard Kardashev Model and the Kardashev--Sagan--Nakamoto Resolution
› Generalizing the CPL Parametrization through Dark Sector Interaction
› Effects on vsini determinations of O stars from 3D model atmospheres with high turbulent velocities
› No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison
› Isocurvature-Free QCD Axion Dark Matter from Inflaton-Driven Early QCD: the Necessity of Inflationary Plateaus
› The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky
› Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion
› Mare versus highland lunar impact flash light curve dichotomy
› COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0
› Reconstructing slow-roll Scalar-Tensor Gauss-Bonnet single field inflation from running spectral data
› Significant noise improvement in a Kinetic Inductance Phonon-Mediated detector by use of a wideband parametric amplifier
› Connecting Early Dark Energy to Late Dark Energy by the Diluting Matter Potential
› Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
› Bayesian analysis of the complex singlet model with phase transition gravitational waves
› Particle Production by Time-Varying Dark Energy and the End of Cosmic Expansion
› Temperature-Dependent CPT Violation: Constraints from Big Bang Nucleosynthesis
› Dark matter in classically conformal theories: WIMP and supercooling
› Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies
› The impact of seasonality over the sensitivity of Einstein Telescope and the SNR of CBC signals at the Sardinia candidate site

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