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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Zdjecie: Suhora w nocy
Suhora w nocy
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10.9 °C

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1016.6 hPa

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› Towards a Foundation Model for the Martian Atmosphere
› The energy conditions and model selection in the local Universe
› First head-to-head comparison of agentic AI applied to the analysis of simulated data of the Einstein Telescope
› The incidence and star-formation properties of X-ray active galactic nuclei across the star-forming main sequence in DESI-eRASS1: the role of host-galaxy morphology
› Photometry is all you need: supernova classification as a mixing problem
› Assessing Ariel's capabilities to observe free-floating brown dwarfs
› Delayed Radio Flares in Tidal Disruption Events from Star-Disk Collision Outflows
› Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe
› A 1% distance to the Large Magellanic Cloud measured by population-II pulsating stars using Gaia Data Release 3
› Dominated-Convergence Failure in Cosmological Perturbation Theory and a Numerical Foundation for BBGKY+ZA
› Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability
› Dust grain chemistry in the diffuse ISM towards the black hole transient GX 339-4
› Closing the UV Gap: Rest-frame EUV science from high-redshift QSOs as a legacy-defining capability
› Supermassive black holes in six triaxial galaxies: Insights from SINFONI and MUSE observations
› Massive Stars in the Thirties: awaiting new Hubble discoveries
› A Deep Study of the Spiral Galaxy W2246f
› Three-dimensional Conditional Diffusion Models for Cosmological 21 cm Lightcone Emulation
› JWST's Dusty Blue BOAT -- GRB 221009A
› Nebular Fingerprints of a Violent White Dwarf Merger: 3D NLTE Modelling of Type Ia Supernovae
› Kolmogorov--Arnold Networks as Implicit Regularizers: Noise Robustness and Interpretability for Stellar Classification
› Multi epoch spectroscopic variability of the B supergiant HD75149
› Ejected Surface Regolith as a Potential Source Material for Centaur Rings
› Using GALEX UV Excess to Search for Metal-poor Halo Stars
› Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole
› Next-generation Exo-REM atmospheric models: application to VHS 1256 b to emulate patchy clouds
› The MeerKAT Thousand-Pulsar Polarization Array I: Properties of the Polarization and Rotation Measure Time Series Data
› Compact near infrared sources in the center of the extraordinary galaxy IC 860
› Shock wave formation in the thermosphere by an earthgrazing fireball: Empirical evidence for volatile-enhanced hydrodynamic shielding
› Assessing the Relative Importance of Neutrino Matter Interaction Channels in Post-Merger Remnant of Binary Neutron Stars
› Constraints on the Atmospheric Composition of 2002 XV$_{93}$ from JWST Spectroscopy
› A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages
› Recoil-regulated extreme mass-ratio inspirals in AGN disks
› Modeling the Effect of the Heliospheric Magnetic Field on Cosmic Ray Muon Shadows
› Development and demonstration of a Modular Astrobiological Experiments (MAEx) payload for autonomous biological monitoring in Low Earth Orbit (LEO)
› Modeling Solitonic Cores, Stabilization of Bar, and Suppression of Bar Dissolution in DDO 168 via GPP Formalism: A Detailed Analysis of Bose--Einstein Condensate/Fuzzy Dark Matter Halo Structure and Bar Dynamics in the Dwarf Galaxy DDO 168
› ODIN: Rest-frame Optical Morphologies and Star Formation Activity of Ly{\alpha} Emitters at z=2.4, 3.1, and 4.5
› Sub-luminous Type IIP SN 2024abfl as a result of a significantly low energy Fe-core collapse
› The Impact of the New $^{59}$Fe Decay Rates on $^{60}$Fe and $^{26}$Al Nucleosynthesis in Massive Stars
› A Note on QPE Timing: False Alarms in O-C
› DELOS: Detecting Shallow Transits in Kepler Photometry Using a Contrastive-Learning Framework
› Optical transmission spectrum of HAT-P-47b: evidence for aerosols and tentative TiO absorption
› From reflection to scattering: polarimetric signatures of funnel-type outflows. Modeling obscured ultraluminous X-ray sources
› Multiple populations detection with the Chinese Space Station Survey Telescope main survey camera
› Time-Domain Deep Learning for Pairwise Identification of Strongly Lensed Gravitational-Wave Candidates
› Sub-surface structural changes associated with successive 11-yr solar activity cycles have been progressively more confined near the surface: new helioseismic results on Cycles 22 -- 25 from BiSON
› An Obscured Tidal Disruption Event Uncovered by Its Mid- and Near-Infrared Dust Echo in a Star-Forming Galaxy
› A New Cartwheel-like Collisional Ring Galaxy
› MAMMOTH-Grism: Gas-phase Metallicity Gradients of Star-forming Galaxies in Protocluster Environments at Cosmic Noon
› Enhanced All-Distance Equi-Zenith Angle Method for Cosmic-Ray Anisotropy Measurement
› Stellar Population Astrophysics (SPA) with the TNG. CNO abundances in 28 open clusters
› Model Independent Probe of Variation of Cosmic Opacity with Redshift
› The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects
› A Calibrated Bayesian Search for Potential Chemical Technosignatures in Polluted White Dwarf
› The asymmetric carbon-rich chemistry of the planet-forming disk of HD 142527 triggered by late infall
› Exploring the High-Redshift 21-cm Signal via Self-Consistent Simulations using Artificial Neural Network Emulation
› Transient Signatures of Star-Envelope Collisions in Little Red Dots
› Evidence of triggered star formation in the Pillars of Creation from JWST observations
› Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
› Modeling carbon outgassing from chondritic planetesimals
› Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
› High-S/N Quasar Observations with HST/COS: Deep Fields for Spectroscopy
› Dust dynamics in disk dust traps and late planetesimal formation
› Quantifying the effect of passband on observations in the Ca II K line
› Detection of unidentified molecular pure rotational lines in C-rich PNe I. The fullerene-containing PN IC 418
› An archival summary: 15 years of ALMA observations on disks and planet formation
› Long-Duration GRB 211211A: Internal Energy Dissipation Driven by a Long-Lived Magnetar
› Extending Hubble into the 2030s to Resolve the Physics of LyC Escape
› The outer rings of SN 1987A from year 1994 to 2024: morphology, light curves, and optical to mid-infrared spectra
› The Shape of (486958) Arrokoth
› The evolution and internal structure of Neptunes and sub-Neptunes II. Convective mixing and thermal conductivity
› Cosmo-PINN: A Physics-Informed Neural Network for Cosmological Reconstruction
› Determining the incidence rate of magnetic $\delta$ Scuti candidates with CoRoT
› A new completely parameter-free clustering algorithm for unsupervised classification of BATSE gamma-ray bursts
› The Architecture of the 14 Herculis System Suggests Primordial Ejection of a Massive Planet
› The Northern Cross Fast Radio Burst project: VI. The INCART public database
› Signals from the early Universe: a comprehensive search for primordial features in Planck CMB datasets
› Efficient computation of the galaxy angular bispectrum in redshift space
› From Images to Orbits: A Hubble 2030s Astrometric Legacy for the M31-M33 Star Cluster Systems
› Late-time Quantum Vacuum Decay and its Cosmological Implications
› Augmented Correlation Functions for Spectroscopic Galaxy Surveys
› Effective chemical potential and its phenomenological implications for the Hubble parameter
› A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino
› When the Ringing Stops: Purely Imaginary Modes in the Ringdown Spectrum of Dynamical Black Holes
› Signatures of loop quantum gravity in primordial black hole cosmologies
› Visible inelasticity as a probe of tau flavor content of astrophysical neutrinos
› Dynamical Tsallis WIMP Freeze-Out and Residual Memory Channels in the Radiation Sector
› Statistical study of energy dissipation in magnetic structures during turbulent reconnection in the Earth's magnetotail
› Quantum transitions of vector vortex light in gravitational waves
› Problems of cosmology on small scales of the Universe
› Black Hole Photon Rings Saturate the Quantum Chaos Bound
› Propagation of waves in weakly ionized two-fluid plasmas. II. Nonlinear Alfv\'enic waves
› Supermassive black hole seeds from direct collapse of CDM-curvature peaks
› Characterization of Spurious Charge in SENSEI Skipper-CCDs
› Physics Is All You Need? A Case Study in Physicist-Supervised AI Development of Scientific Software
› Modeling spectra of MN112
› Evidence for a sign change of the ISW effect in the very recent universe? hot voids and cold overdensities at $z
› Long-Lived Isomers of C$_{11}$H$_9^+$: New Experimental Insights from the PIRENEA Setup
› Observed Timescales of Stellar Feedback in Star-Forming, Low-Mass Galaxies
› Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections
› Spin Precession Signatures as an Indicator of Microlensing in Strongly Lensed Gravitational Waves
› Gravitational lensing by a spiral galaxy I: the influence from bar's structure to the flux ratio anomaly
› 3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae
› Quokka-based understanding of outflows (QED) -- IV. Limitations of H$\alpha$ as an outflow diagnostic
› The Sesquinary Catastrophe on Deimos can reconcile its excited past with its dynamically cool present
› Considering lensing effect on gravitational wave signals from black holes in mass gap
› Spectral State Switching in Mrk 421: Results from the AstroSat LAXPC/SXT Observations
› Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots
› A multi-technique search for year-scale $\gamma$-ray quasi-periodic modulation in the high-redshift FSRQ PKS~2052$-$47
› Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys
› Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS
› An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics
› Inspectorch: Efficient rare event exploration in solar observations
› Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance
› Path Measures for Stochastic Galaxy Formation on Layered Halo Graphs
› The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
› A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
› Circular polarization images of Sgr A* for different magnetic field geometries
› Oort Cloud Ecology -- IV. Exchanging Asteroids
› The POKEMON Speckle Survey of Nearby M dwarfs. IV. Distance-Limited Catalog (POKEMON-DLC)
› Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks
› The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
› Orbital motion and dynamical mass of the complex periodic variable binary system 2MASS J05082729-2101444
› Mars as an Exoplanet: Lessons from a Planet at the Edge of Habitability
› CMB Acoustic Power Spectra in STVG-MOG
› Formation of intermediate-mass black holes in young massive clusters detected with JWST: analytic mass estimates
› Scattered light signatures of flyby-induced warps in protoplanetary discs
› A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum
› Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction
› The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios
› Bar-halo interaction: the role of orbital anisotropy
› Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena
› Fermi-LAT View on Three Ultra-high-energy 1LHAASO Sources in the $52^{\circ}
› FARSim: a fast RF-chain-aware trigger-screening surrogate for radio detection of ultra-high-energy cosmic rays
› Microcanonical Hamiltonian Monte Carlo
› Neutrino Physics and Astrophysics at Colliders
› Gravitational Wave Signatures of $\mathrm{U(1)_X}$ Breaking and Right-Handed Neutrino Dynamics
› Effective matter sectors from modified entropies
› Massive boson stars: Stability and GW emission in head-on mergers
› Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
› The reason peculiar velocities grow faster in general relativity than in Newtonian gravity
› Isentropic hybrid stars in the Nambu-Jona-Lasinio model: effects of neutrino trapping
› GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
› Inflation with vector fields revisited: non-Gaussianities

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