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Astronomia w Krakowie
Photo: View over the dome at night
View over the dome at night
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1018.7 hPa

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RSS  Latest preprints on astro-ph:

› The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons
› CHRONOS Science Program
› A test of the Dedalus software for exoplanet atmospheric dynamics
› A Kiloparsec-Scale Stellar Cavity in the Center of Abell402-BCG May be Caused by Dynamic Interactions with an Ultramassive Black Hole
› The Cosmological Simulation Code OpenGadget3 -- Implementation of Self-Interacting Dark Matter
› Right round: onset and long-term evolution of rotation in star clusters
› XMM-Newton Observations of Flares and a Possible Pulse Dropout in the Supergiant X-ray binary 4U 1909+07
› Steeling Weak Lensing Source Galaxy Samples against Systematics using Wide Field Spectroscopy
› A Statistical Framework to Identify Kinematically Outlying LMC Globular Clusters and Implications for the LMC's Dark Matter Profile
› On the angular localization of gravitational-wave signals by pulsar timing arrays
› The baryon content of magnetically arrested black hole disks and jets
› Quantifying the impact of relativistic precession on tidal disruption event light curves
› Three Hundred Quasars from the Couch: A first look at high-redshift quasar discovery with SPHEREx
› Accreting White Dwarfs: An Unreview
› Relativistic \(^{56}\text{Ni}\) Decay Lines in GRB 221009A
› Thermal enhancement of inflationary magnetic fields
› The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes
› Neutrinos from extreme astrophysical sources
› Kick matters: The impact of a new recoil model on the retention of hierarchical black-hole remnants in globular clusters
› Radio selection of heavily obscured AGN in the J1030 field: unraveling a missing Compton-thick population
› A modern halo streaming model for redshift space distortions
› Attaining Spectral Energy Distributions With Sub-Percent Uncertainties: All-Sky DA White Dwarf Spectrophotometric Standard Stars For Large Telescopes And Surveys
› Cosmological simulation of radio synchrotron bridge between pre-merging galaxy clusters
› The Geometric Crisis in Cygnus~X-3: Limitations of Wind-Fed Accretion and the Case for Roche-Lobe Overflow
› Unexpectedly Weak General Relativistic Effects in Strongly Relativistic Tidal Disruption Events
› Linear Mode Conversion in Ultramagnetized Pair Plasmas: Single-Parameter Scaling
› At the stellar noise frontier: a transit survey of 121 TESS M3--M6 dwarfs
› The fine dynamics in homologous and recurrent jets induced by persistent rising loops and mini-filaments
› A variable ADAF disk model for X-ray binary systems
› New classification method for the dynamical state of galaxy clusters with a Gaussian mixture model
› On the dual nature of atmospheric escape
› A candidate proton cyclotron feature in the ultraluminous X-ray source NGC 4656 ULX-1
› Full Dynamical Model (SOCOL:14C-Ex) of 14C Atmospheric Production and Transport in Application to Miyake Events
› The FAST Discovery of a binary millisecond pulsar PSR~J1647-0156B (M12B) with a candidate cross matching algorithm
› Interstellar Object 3I/ATLAS Observed from Mars by China's Tianwen-1 Spacecraft
› Evaluating the spatial intra-pixel sensitivity variations and influence based on space observation
› Magnetic field strength constraints on $\gamma$-ray flaring regions in the flat spectrum radio quasar PKS 1222+216
› CSST-PSFNet: A Point Spread Function Reconstruction Model for the CSST Based on Deep Learning
› White Dwarfs with Infrared Excess from LAMOST Data Release 11
› Detection of periodic transit timing variations in warm sub-Saturn HD 332231 b
› Novae breves from magnetar giant flares: Potential probes of neutron star crusts
› Newly discovered Luminous blue variable candidates in M31 & M33
› Spectral Decomposition Reveals Surface Processes on Europa
› Kinematics and Untwisting Motion of an Intriguing Jet-like Prominence Eruption
› Multi-wavelength emission modelling of PSR~J0437$-$4715
› Chromospheric and photospheric properties of sunspots as inferred from Stokes inversions under magneto-hydrostatic and non-local-thermodynamic equilibrium
› Neural Differential Equations for the Solar Dynamo
› The Rayleigh Taylor instability in partially ionized plasmas: ambipolar diffusion effects in the non linear phase
› Extended Radio Galaxies in EMU: A Comparative Look at Source-Finding Techniques
› The in-situ growth of stellar-mass "light" seed black holes in nuclear star clusters
› The Asteroid Framing Cameras on ESA's Hera mission
› Star formation in the circumgalactic high-velocity cloud Complex H
› Interacting dark sector from intrinsic entropy couplings
› Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
› Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Solar Flare Loops
› Euclid: The linear-construction covariance and cosmology
› Design and performance of the coded mask for the Lunar Electromagnetic Monitor in X-rays (LEM-X)
› A Python-Based Peeling Framework for Radio Interferometry: Application to uGMRT 650MHz Imaging
› The Desert Fireball Network Clear-Sky Survey
› Measuring neutrino mass in light of ACT DR6 and DESI DR2
› Mass measurements of the double neutron star system PSR J0641+0448
› Identifying and Measuring Satellite Streaks in DECam Images
› Electromagnetic Signatures of Supermassive Binary Black Holes. I. Thermal Synchrotron, Self-Lensing Flares, and Jet Precession
› Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins
› Spectroscopic galaxy redshifts in the Peanut cluster - a massive nearly head-on cluster merger shortly after pericenter passage
› X-ray polarization in the soft state of Cyg X-1
› Catalogue and statistics of greater than 100 MeV solar proton events during solar cycles 23-25 from SOHO-ERNE observations
› TOI-4616 b: a benchmark Earth-sized planet transiting a nearby M4 dwarf
› Gaia-GIC-1: An Evolving Catastrophic Planetesimal Collision Candidate
› Universal behaviour of $\alpha$-viscosity in black hole accretion discs
› Searching for Magnetic White Dwarfs in LAMOST DR10
› Gravitational Anomaly Measurement in Wide Binaries is Sensitive to Orbital Modeling
› Oxygenated False Positive Biosignatures in Mars-like Exoplanet Atmospheres
› Blind mitigation of foreground-induced biases on primordial $B$ modes for ground-based CMB experiments
› XMM-Newton Observation and Optical Monitoring of the Candidate Redback Millisecond Pulsar 1FGL J0523.5$-$2529
› Stodolsky effect in the framework of Generalised Neutrino Interactions
› Searching for axions with time resolved pulsar polarimetry
› The phenomenon of the axion kinetic misalignment with a generic PQ-breaking operator
› Holographic dark energy from a new two-parameter entropic functional
› Interpretable and physics-informed emulator for the linear matter power spectrum from machine learning
› A spinodal decomposition model for the large-scale structure of the universe
› Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5
› Constructing Four-Body Ballistic Lunar Transfers via Analytical Energy Conditions
› Search for Quasar Pairs with ${\it Gaia}$ Astrometric Data. I. Method and Candidates
› Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
› Sensitivity of the Global 21-cm Signal to Dark Matter-Baryon Scattering
› Barycenter kinematics in Local Group analogues
› The analytical general solutions of power-law inflation
› An Ultra-Faint, Chemically Primitive Galaxy Forming in the Reionization Era
› Application of a modified commercial laser mass spectrometer as a science analog of the Mars Organic Molecule Analyzer (MOMA)
› Identifying Anomalous DESI Galaxy Spectra with a Variational Autoencoder
› The BoRG-$JWST$ Survey: Analogs at $z\sim8$ to the UV-luminous Galaxy Population at $z\gtrsim10$
› Before its time: a remarkably evolved protocluster core at z=7.88
› Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
› Modeling of AR 12760 with GX Simulator and Evidence for the Extended Transition Region in Peripheral Active Region Loops
› Bulk viscosity from early-time thermalization of cosmic fluids in light of DESI DR2 data
› Magnetic, thermal and rotational evolution of isolated neutron stars
› The Non Parametric Reconstruction of Binary Black Hole Mass Evolution from GWTC-4.0 Gravitational Wave Catalog
› Measuring the Temperature of Extremely Hot Shock-Heated Gas in the Major Merger MACS J0717.5+3745 With Relativistic Corrections to the Sunyaev-Zel'dovich Effect
› The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
› First detection of ultra-high energy emission from gamma-ray binary LS I +61 303
› Dents in the Mirror: A Novel Probe of Dark Matter Substructure in Galaxy Clusters from the Astrometric Asymmetry of Lensed Arcs
› Covariance spectrum of MAXI J1820+070: On the nature of the Comptonizing flow
› Analytical Emulator for the Baryon Density Distribution inside the Fuzzy Dark Matter Soliton from Machine Learning
› Impact of Nuclear Reaction Rate Uncertainties on Type I X-ray Burst Nucleosynthesis: A Monte Carlo Study
› The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis
› Pre-training vision models for the classification of alerts from wide-field time-domain surveys
› Hunting for the First Explosions at the High-Redshift Frontier
› Simulation-Based Inference for Probabilistic Galaxy Detection and Deblending
› Broad line regions behind haze: Intrinsic shape of Br$\gamma$ line and its origin in a type-1 Seyfert galaxy
› sponchpop: Population synthesis to investigate volatile sulfur as a fingerprint of gas giant formation histories
› Non-adiabatic Effect on Convective Mode
› Calibration-independent consistency test of BAO and SNIa data: update
› Calibrating redshift distributions at $z>2$ with Lyman-$\alpha$ forest cross-correlations
› Disk Wind Feedback from High-mass Protostars. V. Application of Multi-Modal Machine Learning to Characterize Outflow Properties
› Searching for the Shortest-wavelength Aromatic Infrared Bands: No Evidence for the Predicted 1.05 $\mu$m Polycyclic Aromatic Hydrocarbon Feature
› The eruptive young star IRAS 21204+4913
› Ground-based Atmospheric Characterization of Super-Earth L 98-59 d at High Spectral Resolution
› The Evolution of X-ray Spectra in Tidal Disruption Events
› A Catalogue of Orbital Periods of Cataclysmic Variables and Candidates from TESS Observations
› Geometric masking in AGN jets and its implications for unification and blazar physics
› Broadband SETI: a New Strategy To Find Nearby Alien Civilizations
› Evolution and formation of ultramassive white dwarf stars: The case for a 9Msun progenitor
› ODIN: Confirmation and 3D Reconstruction of Six Massive Protoclusters at Cosmic Noon
› Superradiance in acoustic black hole
› Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study
› Addressing the Hubble Tension: Insights from Reversible and Irreversible Thermodynamic Processes
› Gravitational memory meets astrophysical environments: exploring a new frontier through osculations
› Vector dark matter production during inflation in the gradient-expansion formalism
› Effects of dark dipole radiation on eccentric supermassive black hole binary inspirals
› Impact of Anisotropy on Neutron Star Structure and Curvature

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