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Astronomia w Krakowie
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Temperature
2.6 °C

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 94%

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3.2 km/h

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1013.8 hPa

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RSS  Latest preprints on astro-ph:

› SGNL: Scalable Low-Latency Gravitational Wave Detection Pipeline for Compact Binary Mergers
› Combining CMB datasets with consistent foreground modelling
› Large-Scale Structure Probes of the Post-Inflationary Axiverse
› Heavy black hole seed survivors in dwarf galaxies: a case study of Leo I
› SRGt 062340.2-265751 confirmed as a nova-like cataclysmic variable with a possible magnetic nature
› Micrometeoroid Impact Rate Analysis for an Artemis-Era Lunar Base
› Sub-Gyr variability around the SFMS and its contribution to the scatter
› Dents in the Mirror: A Novel Probe of Dark Matter Substructure in Galaxy Clusters from the Astrometric Asymmetry of Lensed Arcs
› The essential elements of dust evolution: a-C(:H) nanoparticle sub-structures and photo-fragmentation
› HiSAXy: A fast methodology for solar wind structure identification in millions of time series
› Secondary small-scale dynamics of a Rayleigh-Taylor unstable solar prominence
› Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth $\tau$
› ALMA Sub-parsec Resolution Dense Molecular Line Observations of the NGC 1068 Nucleus
› Kinematic and extinction analysis of a potential spiral arm beyond the Galactic bar
› Synthetic JWST galaxy images in the TNG50 simulation - I. Model validation and comparison to observations
› How Low Can You Go: Constraining the Effects of Catalog Incompleteness on Dark Siren Cosmology
› Comprehensive Listing of 208 Nova White Dwarf Masses As the Primary Determinant of Spectral-Class and Light-Curve-Class
› Blind Strong Gravitational Lensing Inversion: Joint Inference of Source and Lens Mass with Score-Based Models
› Comparative Analysis of 10 - 50 MeV Solar Proton Events at Lagrange Point 1 and the Geostationary Orbit
› FermiPhased: A tool for phase-resolved likelihood analysis of Fermi-LAT data
› Using ML-based Regression Techniques to Mitigate GOES Energetic Proton Flux Data Contamination and Magnetospheric Effects
› Empirical measures of the largest amounts of magnetically-induced radius inflation in low-mass stars
› JWST provides a new view of cosmic dawn: latest developments in studies of early galaxies
› The Dual Nature of Solar Wind Structuring: Resonant Standing Waves and Laval Nozzle Dynamics in Coronal Streamers
› SCATTER Common Envelope Formalism for Triples
› Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties
› On the Energetic Role of Forward Neutrino Scattering in Core-Collapse Supernovae
› Investigation on the Predictive Potentiality of Photospheric Magnetic Parameters for Distinguishing Confined from Eruptive Solar Flares
› Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction
› Precise Measurement of Cosmic Ray Light and Helium Spectra above 0.1 Peta-electron-Volt
› LHAASO Detection of Ultra-High-Energy Gamma-Ray Emission toward the Giant Molecular Clouds
› Unveiling the Nature of Superorbital Modulation of SMC X-1 using NinjaSat
› Discovery of an X-ray Luminous Radio-Loud Quasar at $z=3.4$: A Possible Transitional Super-Eddington Phase
› A deep X-ray look to the most obscured quasar at z~3.6 and its environment
› Quokka-based understanding of outflows (QED) - IV. Limitations of H$\alpha$ as an outflow diagnostic
› Probing Lorentz Invariance Violation at High Energies Using LHAASO Observations of GRB221009A via DisCan Algorithm
› NGC 6860, Mrk 915, and MCG -01-24-012. II. Inflowing and outflowing cold molecular gas and the connection with ionized gas in Seyfert galaxies
› Formation of millisecond pulsar-helium star binaries
› Sym-EFT: Accelerating Effective Field Theory of Large Scale Structure with Symbolic Regression
› Spatially-resolved PAH_3.3 emission and stellar ages in ram pressure stripped clumps at z~0.3
› Stellar Population Astrophysics (SPA) with the TNG 23 IR elemental abundances of 114 giant stars in 41 Open Clusters
› The most distant optically polarised GRB afterglow: GRB 240419A at z = 5.178
› Searching for Electromagnetic Counterpart Candidates to GW231123
› Mass determination of the three long-period Neptune- and sub-Neptune-sized planets transiting TOI-282
› Upper limits on atmospheric abundances of KELT-11b and WASP-69b from a retrieval approach
› High-spectral Resolution, Multi-wavelength Center-to-limb Observations of the Sun
› On the possibility of using decayless kink oscillations of coronal loops to forecast powerful solar flares and coronal mass ejections
› Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars
› Multiplicity of stellar systems in the solar neighbourhood, wide binaries, and planet-hosting stars
› The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
› A Mass-Independent Damping Timescale in Black Hole Accretion Systems
› Focus Point on Tensions in Cosmology from Early to Late Universe: Part II: New Directions in the Light of Observations from the Most Modern Astronomical Facilities
› Spectrum of PeV Cosmic-Ray Protons and Helium Nuclei with IceCube
› Optimizing broadband microwave absorbers for applications in the 70-200 GHz range
› Near-degeneracy effects in Quadrupolar Mixed Modes. From an Asymptotic Description to Data Fitting
› A subpopulation of low-mass, spinning black holes: signatures of dynamical assembly
› EMPEROR I. Exoplanet MCMC parallel tempering for RV orbit retrieval
› Reviving Quadratic Inflation: Minimal Deformation for CMB Compatibility and Reheating Consistency
› Intensive X-ray/UVOIR continuum reverberation mapping of the Seyfert AGN MCG+08-11-11
› Linking Warm Dark Matter to Merger Tree Histories via Deep Learning Networks
› A scaling relationship for non-thermal radio emission from ordered magnetospheres - II. Investigating the efficiency of relativistic electron production in magnetospheres of BA-type stars
› Modeling Solar Atmosphere Dynamics with MAGEC
› Charge-dependent spectral softenings of primary cosmic-rays from proton to iron below the knee
› Recovering Ion Distribution Functions: II. Gyrotropic Slepian Reconstruction of Solar Wind Electrostatic Analyzer Measurements
› Crossing the veil of the brightest radio relic in the sky MACS J0717.6+3745
› Investigating the imprints of tidal features on simulated galaxy outskirts in LSST-like mock observations
› Upper Limits on Radio Emission from the K2-18 System
› Unsupervised Discovery of High-Redshift Galaxy Populations with Variational Autoencoders
› $\texttt{unimpeded}$: A Public Nested Sampling Database for Bayesian Cosmology
› Chemical Evolution and Kilonova Implications of Post-Merger Accretion Disk Winds
› Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation
› Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST
› CATS: Empowering the next generation of rocket scientists through educational flight computers
› Higgs inflation in Weyl-invariant Einstein-Cartan gravity
› Effective Field Theories for Neutron Stars Physics
› Fast and Flexible Neutrino Decoupling Part I: The Standard Model
› Millicharged Particle Production in Pulsars via the Schwinger Effect
› Novel Solar System Probes for Primordial Black Holes
› Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production
› Exact Renormalisation Group Evolution of the Inflation Dynamics: Reconciling $\alpha$-Attractors with ACT
› Quantum Gravity, de Sitter Space, and Normalizability
› One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
› The distribution of ultra-high-energy cosmic rays along the supergalactic plane measured at the Pierre Auger Observatory
› Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis
› Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry
› The radio properties of the JWST-discovered AGN
› Constraining the potential of the Milky Way using stellar streams and the Inverse Time Integration method
› Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory
› Dynamics of $Z_N$ domain walls with bias directions
› Updated cosmological constraints on axion dark energy with DESI
› Testing the Shock-cooling Emission Model from Star-disk Collisions for Quasi-periodic Eruptions
› Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots
› Jet-environment interaction after delayed collapse in binary neutron star mergers
› One-loop kernels in scale-dependent Horndeski theory
› On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays
› A deep dive down the broad-line region: permitted OI, CaII and FeII emission in an AGN Little Red Dot at z=5.3
› On the Interpretation of Velocity Residuals in Protoplanetary Disks
› On the Efficiency of Producing Gamma-Ray Bursts from Isolated Population III Stars
› Constraints on the progenitor and explosion of SN 2024ggi in harmony with pre-explosion detection and hydrodynamic simulations
› Modelling the M68 stellar stream with realistic mass loss and frequency distributions in angle-action coordinates
› Renormalization-Free Galaxy Bias in Unified Lagrangian Perturbation Theory
› DiskMINT: Self-Consistent Thermochemical Disk Models with Radially Varying Gas and Dust -- Application to the Massive, CO-Rich Disk of IM Lup
› Role of sunspot latitude versus tilt in determining the polar field and amplitude of the next cycle: Cause of the weak Solar Cycle 20
› The Hubble Tension resolved by the DESI Baryon Acoustic Oscillations Measurements
› Not All Sub-Neptune Exoplanets Have Magma Oceans
› Solar limb faculae: intensity contrast from two vantage points
› Design and Scientific Prospects of the POLAR-2 Mission
› AppleCiDEr II: SpectraNet -- A Deep Learning Network for Spectroscopic Data
› Picoflares in the Quiet Solar Corona: Solar Orbiter Observations Halfway to the Sun
› Estimating Orbital Parameters of Direct Imaging Exoplanet Using Neural Network
› Evidence of Energy Injection in the Short and Distant GRB 250221A
› The Missing Mechanism: Picoflare Heating in the Solar Corona
› Wind-AE: A Fast, Open-source 1D Photoevaporation Code with Metal and Multi-frequency X-ray Capabilities
› The Physical Origin of Periodic Density Structures in the Solar Wind: Coronal Streamers as Magnetohydrodynamic Resonators
› Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
› On the Inner Crusts of Neo-Neutron Stars: exotic light nuclei, diffusional and thermodynamical stability
› Bright ring features and polarization structures in Kerr-Sen black hole images illuminated by radiatively inefficient accretion flows
› Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector
› Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies
› The importance of being non-minimally coupled: scalar Hawking radiation from regular black holes
› Gravitational waves from the sound shell model: direct and inverse phase transitions in the early Universe
› Cosmological and High Energy Physics implications from gravitational-wave background searches in LIGO-Virgo-KAGRA's O1-O4a runs
› Geometric acceleration in $f(Q,C)$ theories
› Conserved Quantities in Expanding G\"odel Cosmology
› Computing the Full Earth System at 1 km Resolution
› Observational tests of the conformal osculating Barthel-Kropina cosmological model

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