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Astronomia w Krakowie
Photo: The Orion Nebula (M42) imaged from Mt. Suhora
The Orion Nebula (M42) imaged from Mt. Suhora
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RSS  Latest preprints on astro-ph:
› BASS.L. Near-infrared Data Release 3: A Spectral Atlas and Characterization of AGN
› Flux rope formation through flux cancellation of sheared coronal arcades in a 3D convectively-driven MHD simulation
› A Physics Informed Neural Network For Deriving MHD State Vectors From Global Active Regions Observations
› Simultaneous JWST, NuSTAR, and VLA Monitoring of Sgr A*: A Unified Picture of the Variable IR, X-ray and Radio Emission
› CORINOS IV: Quantifying Baseline-Fitting Uncertainties in SO$_2$ Ice Measurements with JWST/MIRI
› Thawing Quintessence: Priors, evidence, and likely trajectories
› Revisiting the Mass Step: Environmental Dependence of Type Ia Supernovae in Low-Metallicity Host Galaxies
› Universal relations between the quasinormal modes of neutron stars and magnetic tidal deformability
› On the Relationship Between Nanoflare Energy and Delay in the Closed Solar Corona
› Considering lensing effect on gravitational wave signals from black holes in mass gap
› Expanding Asteroseismic Studies in Star Clusters Using NASA's TESS and ESA's Gaia Missions
› Mid-IR luminosity functions: inferred dusty cosmic star-formation and black hole accretion histories from the JWST SMILES
› The polar IL Leo in a low accretion state
› GW241011 and GW241110: Hints of Hierarchical Mergers from the Merger Entropy Index
› IMPACTX: An X-ray Spectral Model for Polar Dust and Clumpy Torus
› DRAGNs in the Forest: Identifying Artifacts with Random Forest Models in the VLASS DRAGNs Catalog
› Quantum scattering of hot H/D on CO$_2$: Cross sections and rate coefficients for planetary atmospheres and their evolution
› The transport of angular momentum for massive stars I. Formation of slowly rotating WNE stars
› Asteroseismology and Dynamics Reveal Interior Structure and Coeval Evolution in the Triply Post-Main-Sequence system DG Leo
› Evolution of the 2021 Outburst of GX 339-4 with AstroSat
› The disc instability model: original recipe and additional ingredients
› Exploring the Role of Vector Potential and Plasma-$\beta$ in Jet Formation from Magnetized Accretion Flows
› Assessing systematic uncertainties from spectral re-analysis of Cyg X-1 with different coronal geometries
› Minijets and Broken Stationarity in a Blazar : Novel Insights into the Origin of $\gamma$-ray Variability in CTA 102
› ZTF SN Ia DR2 follow-up: Characterization of subluminous Type Ia supernovae in the ZTF DR2 full sample
› A Near-Infrared and Optical Study of NGC 5822: An Open Cluster Hosting Barium-stars and Lithium-Enriched Giant Stars
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› Changes in R Leonis over Two Centuries: Period evolution and dust shell development
› Bar Formation in Disc Galaxies: Internal Kinematics and Environmental Influence in MaNGA Galaxies
› A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
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› Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation
› Echoes of $R^3$ modification and Goldstone preheating in the CMB-BAO landscape
› Effects of External Magnetic Fields on the Multi-mode Rayleigh-Taylor Instability
› Black Hole Evaporation Driven by Non-Thermal Squeezing Through SNS and CSNS Dynamics
› Acetaldehyde as a molecule for testing variations of electron-to-proton mass ratio
› Axion-photon conversion in stochastic magnetic fields
› Large lepton asymmetry from axion inflation and helium abundance hinted by ACT
› Acoustic gravitational waves from primordial curvature perturbations
› (Lovelock)$^2$ inflation: explaining the ACT data and equivalence to Higgs-Gauss-Bonnet inflation
› Gravitational open effective field theory of inflation
› When Geometry Radiates Review: Gravitational Waves in Theory, Cosmology, and Observation
› Data-driven core collapse supernova multilateration with first neutrino events
› A Novel Technique for Long-term Timing of Redback Millisecond Pulsars
› Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XXII. Chandra observations of narrow-line quasar candidates at z>6
› Bayesian reconstruction of primordial perturbations from induced gravitational waves
› 21 cm Signal from the Thermal Evolution of Lyman-$\alpha$ during Cosmic Dawn
› Chromatic activity window of periodic FRBs: FRB 20121102A and FRB 20180916B
› Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
› From ANN to BNN: Inferring Reionization Parameters using Uncertainty-aware Emulators of 21-cm Summaries
› On the optical emission in the mini-outburst of the black hole X-ray binary MAXI J1348-630
› Unified $g$-mode and $r$-mode Analysis of Accreting White Dwarf Stars
› A Cold and Super-Puffy Planet on a Prograde Orbit
› The GAPS programme at TNG XYZ. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
› Polarization Dynamics of X-Ray Synchrotron Emission from a Multi-Zone Blazar Jet
› Testing the cosmic distance duality relation using model-independent approach
› Planet Across Space and Time (PAST). VII. The origin and tidal evolution of hot Jupiters constrained by a broken age-frequency relation
› Globular clusters of the Gaia Enceladus/Sausage -- I. Orbital and dynamical evolution on cosmological timescales
› Calcium versus silicon ejecta velocities and decline rates in supernovae Ia: The role of high-velocity features
› Improvements to the NSO Farside Mapping Pipeline: Noise Reduction Updates
› Is Dark Energy Dynamical in the DESI Era? A Critical Review
› AGN X-ray Reflection Spectroscopy with ML MYTORUS:Neural Posterior Estimation with Training on Observation-Driven Parameter Grids
› Constraints on light decaying dark matter candidates from 16 years of INTEGRAL/SPI observations
› Supernova Pointing Capabilities of DUNE
› A try for dark energy in quantum field theory: The vacuum energy of neutrino field
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› Singular $\alpha$-attractors
› Kinetic theory and the speed of sound in dense matter

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