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Astronomia w Krakowie
Photo: Międzynarodowa Stacja Kosmiczna i Księżyc z halo
Międzynarodowa Stacja Kosmiczna i Księżyc z halo
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RSS  Latest preprints on astro-ph:
› The Material Point Method (MPM) for simulating hypervelocity impact on asteroids
› Secular Brightness Trends of Starlink and OneWeb Satellites
› Persephone's Torch: A 15th Magnitude Quadruply-Lensed Quasar From the Couch Discovered with SPHEREx and the LBT
› From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas
› A Dynamical Test for Cooling-Induced Entrainment in a Runaway Supermassive Black Hole Tail
› Resolving circumgalactic gas flows around a z$\approx$3.6 quasar using MUSE and ALMA
› Investigating the Circumgalactic Medium through Mg II absorption coincidence
› Solar photospheric spectrum microvariability III. Radial velocities and line profiles in magnetic active-region granulation
› The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
› Euclid: Quick Data Release (Q1) -- Dual AGN in low-mass galaxies
› Targeted search for eccentric supermassive binary black holes in OJ 287 and nearby galaxy clusters with PPTA DR3
› Chromospheric dynamics and turbulence regulate the solar FIP effect
› 4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < $z$ < 7) selected with SED fitting
› The NuSTAR view of Ultra-Compact X-ray Binaries
› Galactic Rain: Cool Gas Inflows in Red Geyser Galaxies and Their Connection to AGN Activity and Interactions
› Radiation hydrodynamic simulations for the origin of quasi-periodic oscillations for accretion onto supermassive black holes
› Are Thalassa and Despina in Resonance Lock with Neptune's Oscillations?
› An Information-Theoretic Metric for Transient Classification and Novelty Detection
› Sparks: The Magellan/FIRE survey from starburst to post-starburst
› Sparks II: Panchromatic SED modeling and galaxy physical properties across the starburst to post-starburst sequence
› A spatial and kinematical reinterpretation of Gould's Belt in light of Gaia
› Rings Around Non-Spherical Worlds: Sub-mm Dust Retention Around Triaxial Small Bodies in the Solar System
› The Great Escape of ionizing photons during Cosmic Morning
› The steady-state population of Earth's co-orbitals of lunar provenance
› CII fine-structure line observations of the Sagittarius C Region in the Galaxy's Central Molecular Zone
› The DECam MAGIC Survey: Investigating the Jet Stellar Stream with Photometric Metallicities
› ALESS--JWST: Dust-driven Morphologies and Hidden Stellar Mass in $z\sim3$ Sub-millimeter Galaxies
› Into the Gompverse: A robust Gompertzian reionization model for CMB analyses
› Substructures of the Milky Way's Retrograde Halo: Evidence for Multiple Accretion Events
› Site Quality Analysis for an Indian Submillimeter Telescope: A Reanalysis-Based Approach
› A Unified HI Rotation Curve Corpus for Computational Astrophysics: 438 Galaxies from SPARC, THINGS, LITTLE THINGS, and WALLABY DR2
› CHARA Interferometry and TESS Asteroseismology of the Core-Helium Burning Red Giant $\kappa$ Cyg
› Double the axions, half the tension: multi-field early dark energy eases the Hubble tension
› Reconstructing inflationary features on large scales using genetic algorithm
› Relaxation of magnetically-confined mountains on accreting neutron stars through cross-field mass transport
› Simulation of non X-ray background for the DIffuse X-ray Explorer (DIXE) mission
› Understanding mechanisms underlying solar cycle predictability with a general framework
› SJET: An Interactive Solar Jet Extraction Tool
› Irregularly Sampled Time Series Interpolation for Binary Evolution Simulations Using Dynamic Time Warping
› Fast Neutrino-Flavor Conversion with Attenuation and Global Lepton Gradient
› Fundamental effective temperature measurements for eclipsing binary stars -- VIII. NIRPS spectroscopy of CD-27 2812
› Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System
› Massive star clusters and clumps in the collisional ring galaxy Arp 147
› Probing Coronal Activity Using Radio Signals Based on the 2021 superior conjunction of Mars: the Downlink Data from Tianwen-1
› The ALMA-QUARKS Survey: Multipolar episodic molecular outflow associated with W49N, the most energetic water maser source in the Milky Way
› CHILES XII: The H I evolution of Luminous Compact Blue Galaxies
› JWST spectroscopy of SN 2010da/NGC 300 ULX-1: a surviving star hidden by dust
› Reanalysing large-scale structure using an updated gamma-ray burst spatial density approach
› Optical depth to reionization in a Universe with multiple inhomogeneous domains
› Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
› JOYS$+$: A JWST/MIRI survey of the evolution of H$_2$ winds and jets from low-mass protostars
› Denoising clustering covariance matrices with Rotational Invariant Estimators
› Witnessing the onset of stellar winds in Super-Luminous Supernova Hosts: implications for star-formation-driven outflows in low and high-redshift galaxies
› Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
› Correlation between Ultra-High-Energy Neutrino KM3-230213A and Gamma-Ray Bursts
› The 256-antenna Coherent All-Sky Monitor
› Large-scale Morphology of the Optical F-corona from a Total Solar Eclipse Observation During the Artemis II Lunar Flyby
› Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs
› Shock properties for solar energetic particle events with signatures of inverse velocity arrival
› Radial Velocity Evidence for a Post-Mass-Transfer Massive Binary System: NaSt1
› Analysis of Lyman-beta and Lyman-gamma Lines in a Pre-Eruptive and Eruptive Prominence with Solar Orbiter SPICE Observations
› Non-LTE Analysis of Pre-eruptive Prominence Plasma Parameters Effects on the Lyman-beta and Lyman-gamma Lines with Solar Orbiter SPICE Observations
› Prominence Plasma Parameters Maps Inferred From Lyman $\beta$ and Lyman $\gamma$ Observations and Non-LTE Modelling
› Analysis of Eruptive Prominence Plasma Parameters' Effects on the \ion{He}{2} 304~\AA\ Line with Solar Orbiter EUI Observations
› BROOM: a python package for model-independent analysis of microwave astronomical data
› Radial Distribution of Star Formation and Gas-phase Metallicity in Spiral-Elliptical Galaxy Pairs
› A Salpeter-like filament linear density function across nearby molecular clouds
› Search for CBCs with SSM Components in Data from The First Part of LVK Fourth Observing Run
› Icy Volatile Enhancements in Evolving Protoplanetary Disks
› The Radial and Vertical Structure of Molecular Gas in the Edge-On Galaxy NGC 4565
› TDCOSMO XXV: A "soup-to-nuts" 6.5% $H_0$ measurement $-$ strong lensing and dynamics with a maximally flexible mass sheet
› Visplot: A visibility plot and observation scheduling tool for astronomical observatories
› SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations
› Potentials of axisymmetric razor-thin disks
› Searching for axions with quantum interferometry
› Observational constraints on nonlocal black holes via gravitational lensing
› Investigating the effect of sensitivity of KAGRA on sky localization of gravitational-wave sources from compact binary coalescences
› Axion Inflation from Heavy-Fermion One-Loop Effects
› VIGILant: an automatic classification pipeline for glitches in the Virgo detector
› Projections of Earth's Technosphere: Civilization Collapse-Recovery Dynamics and Detectability
› Basilic: An end-to-end pipeline for Bayesian burst inference and model classification in gravitational-wave data
› Robust parameter inference for Taiji via time-frequency contrastive learning and normalizing flows
› Interferometer observations of pulse pairs in an interstellar communication experiment
› Gravitational Sommerfeld Effects: Formalism, Renormalization, and Perturbation to $O(G^{10})$
› Pulsar Population Synthesis with Magnetorotational Evolution: Constraining the Decay of Magnetic field
› Chern-Simons gravitational term coupled to a spectator field
› A High Resolution Search for Dual AGN Candidates in Mergers: A Pre-Selection Strategy using Keck AO
› Precision spectral estimation at sub-Hz frequencies: closed-form posteriors and Bayesian noise projection
› Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation
› Primordial Black Holes (PBHs) and The Signatures of Cosmic Non-Gaussianity
› Gravitational waves from axion inflation in the gradient expansion formalism. Part II. Fermionic axion inflation
› On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference
› Accretion-Driven Turbulence in the Circumgalactic Medium
› Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach
› Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4
› The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
› SIMLA: The Spitzer Infrared Spectrograph Mapping Legacy Archive
› Machine learning for the early classification of broad-lined Ic supernovae
› Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
› Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
› The $\gamma$-ray-emitting blazar B3 1239+376 at $z$ = 3.82 identified in a multi-wavelength context
› The Quasar Proximity Effect as an Alternative Probe of Quasar Pair Distances
› Global magnetohydrodynamic simulations of the inner regions of protoplanetary discs. II. Vertical-net-flux regime
› The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Constraints on disk turbulence, fragmentation velocity, and inner pebble fluxes
› Water D/H in 3I/ATLAS as a Probe of Formation Conditions in Another Planetary System
› Redshift Dipoles from Non-Geodesic Observer Congruences in Covariant Cosmology
› Traces of Helium Detected in Type Ic Supernova 2014L
› Cosmological zoom-in perturbation theory as a consistent beyond point-particle approximation framework
› Replacing Gaussian Processes with Neural Networks in Pulsar Timing Array Inference of the Gravitational-Wave Background
› Enhancing astrometric registration of Chinese historical Astronomical Digital Plates with deep learning
› Developing Pre-Supernova Neutrino Support for sntools
› Extended coronal line emission and new clues to a possible dual AGN in the merger J1356+1026
› Galactic Archaeology with the Subaru `\=Onohi`ula Prime Focus Spectrograph Strategic Program
› The demise of the synchronous moon that gave Mars its triaxiality. The role of solar tides and a palaeo ocean
› Dark Matter's influence on Evolution of MBHB in Dwarf Galaxies: A Case Study of Leo I dSph
› Probing Cosmic Ray Composition and Muon-philic Dark Matter via Muon Tomography
› Unitary and Analytic Renormalisation of Cosmological Correlators
› Direct Collapse Black Hole Candidates from Decaying Dark Matter
› Every Wrinkle Carries A Memory: An Integro-differential Bootstrap for Features in Cosmological Correlators
› Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production
› Approximations and modifications of celestial dynamics tested on the three-body system
› Black Holes as Catalysts for Cosmic String Detection and Axion Dark Matter Genesis
› An efficient finite element formulation for Newtonian noise analysis

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