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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Astronomia w Krakowie
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Temperatura
-6.1 °C

Wilgotność
 92%

Wiatr
3.2 km/h

Ciśnienie
1026.6 hPa

Moon

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› Breakthrough Listen Observations of 3I/ATLAS with the Green Bank Telescope at 1-12 GHz
› SN 2025ogs: A Spectroscopically-Normal Type Ia Supernova at z = 2 as a Benchmark for Redshift Evolution
› K-DRIFT Science Theme: Illuminating the Next Era of Galaxy Cluster Science
› A multiwavelength study of an early galaxy group merger in COSMOS revealed by two tailed radio galaxies at z = 0.35
› New and updated timing models for seven young energetic X-ray pulsars, including the Big Glitcher PSR J0537-6910
› Obtaining Magnetization of Super-Alfv\'enic Turbulence with the Structure Functions of Gradient Directions
› VERITAS contributions to the 39th International Cosmic Ray Conference
› The EUV Late-Phase: Statistical Results from 15 Years of Solar Dynamics Observatory Observations
› Unfolding the Energy Spectrum of Ultra-High-Energy Cosmic Rays Using Pierre Auger Open Data
› Double-hump spectrum, pulse profile dip, and pulsed fraction spectra from the low-accretion regime in the X-ray pulsar MAXI J0655-013
› Detecting Strongly-Lensed Supernovae in Wide-field Space Telescope Imaging via Deep Learning
› Observational constraints on early time non-phantom behaviour of dynamical dark energy
› Superluminal Wave Activation at Relativistic Magnetized Shocks
› Astrophysical constraints on the cold equation of state of the strongly interacting matter
› Observation of Large-Scale Kelvin-Helmholtz Instability Wave Driven by a Coronal Mass Ejection
› Lyman Continuum escaping from in-situ formed stars in a tidal bridge at z = 3
› Microlensing Black Hole Shadows-II: Constraining Primordial Black Hole Dark Matter using the photon rings of M87 and Sgr A*
› Stable mass transfer in massive binaries leading to merging black holes
› Unveiling the Dual Nature of V1180 Cas: UXor-like Dips and EXor-like Bursts Across a Decade
› Detection of dark companions via the combination of eclipse timing variation, Hipparcos and/or Gaia astrometry: the cases of V Puppis and CY Ari
› Alfv\'enic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigation
› The Solirad (So) as a Convenient Unit for Quoting Astronomical Irradiances for Planetary Insolations and Exoplanetary Instellations
› Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample
› Abundance of cosmic voids in EFT of dark energy
› Formation of an optically thick shocked shell in the very fast nova V1674 Herculis: the origin of superbrightness
› Deep learning-driven atmospheric parameter prediction for hot subdwarf stars with synthetic and observed spectra
› Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
› How Mergers and Flybys Shape Azimuthal Age Patterns in Spiral Galaxies
› The AI Scaling Wall of Diminishing Returns: Of LLMs, Electric Dogs, and General Relativity
› Super-Eddington Accretion through a Multiwavelength Lens: Searching for Counterparts of Ultraluminous X-ray Sources
› Presence of solar inner F-corona and coronal heating
› The impact of selection criteria on the properties of green valley galaxies
› A Spectrum of Cosmological Rips and Their Observational Signatures
› From Cosmology to Cosmonomy
› The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget
› Machine Learning vs. SED-Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
› Revisiting the near infrared Calcium triplet as metallicity indicator
› The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios
› Dynamical Dark Energy models in light of the latest observations
› Kinetic theory an the speed of sound in dense matter
› $N_{\textrm{eff}}$ Constraint on Pseudo-Dirac Neutrinos
› Time-dependent flux backgrounds in type IIB supergravity
› On the Stability of Anisotropic Neutron Stars
› Dissipative cosmology with $\Lambda$ from the first law of thermodynamics
› A non-compact QCD axion
› Novel Light Dark Matter Detection with Quantum Parity Detector Using Qubit Arrays
› Calibration Method of Spacecraft-Inertial Sensor Center-of-Mass Offset for the Taiji Gravitational Wave Detection Mission under Science Mode
› Cosmological consequences of spontaneous symmetry breaking
› Non-equilibrium Quantum Field Theory and Axion Electrodynamics in curved spacetimes
› Signatures of High-Frequency Gravitational Waves in Electromagnetic Cavities
› The Hot Jupiter Radius Anomaly and Stellar Connections
› A Young Supernova Selection Pipeline For The LSST Era
› Full-sky Models of Galactic Microwave Emission and Polarization at Sub-arcminute Scales for the Python Sky Model
› Kinetic model and numerical method for multispecies radiation hydrodynamic system with multiscale nonequilibrium transport
› Is Dynamical Dark Energy Necessary? DESI BAO and Modified Recombination
› Scalar-Induced Gravitational Waves from self-resonant preheating in $\alpha$-attractor models
› A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
› Quantifying the Fermi paradox via passive SETI: a general framework
› Lense-Thirring Precession Modulates Repeated Lensing of Continues Gravitational Wave Source from AGN Disks
› X-ray and Radio Analysis of Abell 1644: Constraints on Cluster Dynamics
› The Bispectrum of Intrinsic Alignments: II. Precision Comparison Against Dark Matter Simulations
› Investigating FRB 20240114A with FAST: Morphological Classification and Drifting Rate Measurements in a Burst-Cluster Framework
› Impact of 3D macro physics and nuclear physics on the p nuclei in O-C shell mergers
› The explosion jets of the core-collapse supernova remnant Circinus X-1
› Hurst Index of Gamma-Ray Burst Light Curves and Its Statistical Study
› 200,000+ Deep Learning-inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae
› Cosmographic Footprints of Dynamical Dark Energy
› 3D Macro Physics and Light Odd-Z Element Production in O-C Shell Mergers: Implications for $^{40}\mathrm{K}$ production and radiogenic heating inventories of rocky exoplanets
› Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes
› How clear are the skies of WASP-80b?: 3D Cloud feedback on the atmosphere and spectra of the warm Jupiter
› A fast powerful X-ray transient from possible tidal disruption of a white dwarf
› JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the Explosion
› Primordial Black Holes from Primordial Voids
› Very Massive Stars and High N/O: A Tale of the Nitrogen-enriched Super Star Cluster in the Sunburst Arc
› Emergence of streamers in simulations of late infall
› Fast far-sidelobe modeling for centimeter to sub-millimeter astrophysical observations
› Tracing Quenching in Nearby Galaxies Through Inner Surface Mass Density and Cold Gas Content
› Real-time RFI Mitigation Techniques in Radio Astronomy and Their Practical Limitations
› Tachyonic dark energy- Constraints from current observations
› Deuterium fractionation and CO depletion in Barnard 5
› Towards an Agnostic Algorithm for Sampling Empirical Structure Models: The case of Uranus and Neptune
› SatTrack: Software for Evaluating Satellite Interference and Rim-Based Interference Mitigation Using a Reconfigurable Parabolic Antenna
› Pre-supernova O-C shell mergers could produce more $^{44}\mathrm{Ti}$ than the explosion
› Selected topics on: 1) proposal of interpreting the Crab supernova with a GRB 2) progress in identifying the seven GRBs episodes 3) the role of Sagittarius A in identifying the dark matter component (the X fermion)
› Linear Analyses of Thermal Instability in Stratified Medium
› Relativistic magnetohydrodynamics in the early Universe
› Effective field theory reproducing the MOND phenomenology based on a non-Abelian Yang-Mills graviphoton
› Quantum-enabled optical large-baseline interferometry: applications, protocols and feasibility
› Multifaceted Supercooling: From PTA to LIGO
› Decay and lifetime of oscillons coupled to an external scalar field: Insights from instability band analysis
› Vacuum breakdown around a Kerr black hole surrounded by a magnetic field
› A Framework for Lorentz-Dirac Dynamics and Post-Newtonian Interaction of Radiating Point Charges

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