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:

› GALFITools: A Python library to enhance GALFIT usage in galaxy image modeling
› Interaction of the central jet with the surrounding gas in the protostellar outflow from IRAS 04166+2706
› Overestimated Pressure Broadening Misleads Model Spectra in Cool M Dwarf Stars
› Modeling the Milky Way wind: Supernova-driven outflows accelerate HI clouds near the Galactic center
› Revised AGN Spectral Model Reveals a More Significant Role in Cosmic Reionization
› The fate of the failed supernova candidate M31-2014-DS1
› Accretion disc winds in X-ray binaries
› Probing General Relativity on Cosmological Scales in the 2040s
› On the gravitational stratification of multi-fluid-multi-species plasma
› Kinematic lensing with high-resolution spectroscopic surveys. A unique opportunity for transformative cosmology at high redshifts in the 2040s
› Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at $z>7$
› Featureless stars: Flux Calibration for Extremely Large Telescopes
› Dispersive Properties of MHD Waves in the Expanding Solar Wind for a Parker Spiral Geometry
› The Column Density Probability Density Function of Cygnus-X
› Superluminous supernovae: diverse rise times explain diverse spectra
› Rotational Kinematics in the Globular Cluster System of M31: Insights from Bayesian Inference
› Paving the Road to the Habitable Worlds Observatory with High-Resolution Imaging I: New and Archival Speckle Observations of Potential HWO Target Stars
› Detection of the 2021 Arid Meteor Shower on Maunakea, Hawai'i
› The Nucleated Atomistic Grain Growth Simulator (NAGGS): application to the size-dependent structural and physical properties of nanosilicate dust
› The Cosmic-ray Knee as a Local Signature of Nearby PeVatrons
› Structural Tilting and Depth-Dependent Behavior of Equatorial Rossby Waves
› Stellar control on atmospheric carbon chemistry, CO runaway, and organic synthesis on lifeless Earth-like planets
› A Large and Precise All-Sky Photometric Standard Star Dataset Across More Than 200 Passbands
› I can see your halo: Constraining the Milky Way halo DM with FRB population studies
› Backlighting young stellar objects in the Central Molecular Zone: an ensemble-averaged abundance structure of methanol ices
› Empirical study of the Pantheon SNeIa Catalog within power-law cosmology and varying speed of light
› Analysis of Solar Flare and Sunspots on 4th Jan 2025 and Their Effects on Space Weather
› Data post-processing gain resulting from the patchy nature of speckles
› Dust-obscured radio-emitting tidal disruption event coincident with a high-energy neutrino event
› A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections
› Impact of Newly Measured Nuclear Reaction Rates on $^{26}$Al Ejected Yields from Massive Stars
› Impact of newly measured 26Al(n, p)26Mg and 26Al(n, {\alpha})23Na reaction rates on the nucleosynthesis of 26Al in stars
› Energy Bounds from Relative Magnetic Helicity in Spherical Shells
› The NuGrid AGB Evolution and Nucleosynthesis Data Set
› Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4
› Methanol Formation via the Radical-radical Reaction of OH and CH3 Radicals Undergoing Transient Diffusion on Ice at 10 to 60 K
› Probing the CME Core--Prominence Relation Using Inner Coronal Observations
› Fading into darkness: A weak mass ejection and low-efficiency fallback accompanying black hole formation in M31-2014-DS1
› A Catalog of 45,206 H{\alpha} Emission-line Stars from LAMOST MRS DR7
› Probing the morphology of the Gum Nebula through pulsar observables and a novel distance estimation method
› Two temperate Earth- and Neptune-sized planets orbiting fully convective M dwarfs
› A Minimalist Merger Interpretation of XRISM's Gas Velocity Measurements in the Coma Cluster
› A Phenomenological Study of the Accretion Disk in the Super-Eddington AGN I Zw 1
› Extragalactic archaeology through high-resolution integrated-light spectroscopy of globular clusters
› Evaluating star formation rates at z = 5
› On the orbital evolution of binaries with polar circumbinary disks
› Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
› Ultra Diffuse Galaxies in clusters : the peculiar gas loss of VCC 1964
› The Linear Point Standard Ruler with DESI DR1 and DR2 Data
› Feasibility of event-by-event primary mass discrimination using radio observables and supervised machine learning
› Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
› Radial differential rotation leading to dipole collapse in pre-main-sequence stars
› An Improved UV-Optical Diagnostic for Rejuvenating Galaxies in the Local Universe and Implications for Galaxy Evolution
› Setting up the physical principles of resilience in a model of the Earth System
› Investigating Active Galactic Nuclei variability with the Cherenkov Telescope Array Observatory
› Simulations of collision and sloshing in the galaxy group NGC 5098/5096
› VENUS: Two Faint Little Red Dots Separated by $\sim70\,\mathrm{pc}$ Hidden in a Single Lensed Galaxy at $z\sim7$
› Probing Cosmic Expansion and Early Universe with Einstein Telescope
› Weak lensing of bright standard sirens: prospects for $\sigma_8$
› Primordial black holes: constraints, potential evidence and prospects
› Parity-violating Dark Photon Halos
› Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection
› Dipole Radiation and Kinetic Mixing from Dark Photon Solitons
› Robust Bilinear-Noise-Optimal Control for Gravitational-Wave Detectors: A Mixed LQG/$H_\infty$ Approach
› Condensate Dark Stars beyond the Mean-Field Approximation: The Lee-Huang-Yang correction
› A nonlinear voice from GW250114 ringdown
› Gravitational waves and small-field astrometry
› Towards Accurate Gravitational Wave Predictions: Gauge-Invariant Nucleation in the Electroweak Phase Transition
› GlueNN: gluing patchwise analytic solutions with neural networks
› Naturally small Dirac neutrino mass and $B-L$ dark matter
› Mimetic Dark Matter from Inflation
› Gravitational Ionization by Schwarzschild Primordial Black Holes
› Skyrme-Hartree-Fock-Bogoliubov mass models on a 3D mesh: V. The N2LO extension of the Skyrme EDF
› Constraining Hamiltonians from chiral effective field theory with neutron-star data
› Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
› Modeling the Solar System I: Characterization Limits from Analytic Timing Variations
› Genesis-Metallicity: Universal Non-Parametric Gas-Phase Metallicity Estimation
› A solution to the S8 tension through neutrino-dark matter interactions
› Cosmology with second and third-order shear statistics for the Dark Energy Survey: Methods and simulated analysis
› Testing the Shock-cooling Emission Model from Star-disk Collisions for Quasi-periodic Eruptions
› DESI Data Release 1: Stellar Catalogue
› Imaging systematics induced by galaxy sub-sample fluctuation: new systematics at second order
› Close-in planet induces flares on its host star
› On the origins of oxygen: ALMA and JWST characterise the multi-phase, metal-enriched, star-bursting medium within a 'normal' $z > 11$ galaxy
› Dark Energy Survey Year 3 Results: Cosmological constraints from second and third-order shear statistics
› Cascading from the winds to the disk: the universality of supernovae-driven turbulence in different galactic interstellar media
› Protohalos and their connection to halo assembly, shape and structure
› Merger-induced disturbance and temporal signatures in galaxy clusters: a combined phase space and photometric analysis
› Is Chevallier-Polarski-Linder dark energy a mirage?
› Violent mergers revisited: The origin of the fastest stars in the Galaxy
› ALMAGAL VIII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk
› First detection of ultra-high energy emission from gamma-ray binary LS I +61 303
› First Results from the PanRadio Gamma-Ray Burst Collaboration: The 400-day Afterglow of GRB 230815A
› Looking at infrared background radiation anisotropies with Spitzer II. Small scale anisotropies and their implications for new and upcoming space surveys
› High-energy astrochemistry in the molecular interstellar medium
› The AIDA-TNG project: 3D halo shapes
› On the Cooling of Compact Stars in Light of the HESS J1731-347 Remnant
› Predicting dust temperature from molecular line data using machine learning
› Dual AGNs on 100 kpc Scales from the Million Quasar Catalog
› A universal bound on the duration of a kination era
› New Source for QCD Axion Dark Matter Production: Curvature Induced
› Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
› Realistic assessment of a single gravitational wave source localization taking into account precise pulsar distances with pulsar timing arrays
› Adaptive Online Emulation for Accelerating Complex Physical Simulations
› Phased-Array Laser Power Beaming from Cislunar Space to the Lunar Surface
› Gravitational baryogenesis in $f(T,L_m)$ gravity
› A relativistic treatment of accretion disk torques on extreme mass-ratio inspirals around non-spinning black holes
› $\mathbb Z_2$-Stable Dark Matter via Broken $\text{SU}(5)$ Gauge Bosons
› Astrophysical Reaction Rates for Charged-Particle Induced Reactions on Proton-Rich Nuclides
› Pivot-Only Azimuthal Control and Attitude Estimation of Balloon-borne Payloads
› Graviton-Photon Mixing by a Kerr-Newman Black Hole with Worldline EFT

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