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Astronomia w Krakowie
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Sunset from the kitchen window
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 News from astronomynow.com
› Europe’s planet hunting spacecraft complete and ready for final testing
› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
RSS  Latest preprints on astro-ph:
› Very High Precision Astrometry for Exoplanets and Dark Matter with the Habitable Worlds Observatory
› Living with Neighbors. VI. Unraveling the Dual Impact of Bars on Star Formation in Paired Galaxies Using DESI
› Warped Disk Galaxies. II. From the Cosmic Web to the Galactic Warp
› The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes
› Intruder Alert: Breaking Resonant Chains with Planetesimal Flybys
› Galaxy Activity, Torus and Outflow Survey (GATOS) X: Molecular gas clumpiness under the influence of AGN
› A spectral library and census of near-infrared stellar large-amplitude variables from Palomar Gattini-IR
› Dark Matter profiles of "in silico" galaxies: deep learning inference
› Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess
› A resistive MHD module in the GPU-accelerated GRMHD code GRaM-X
› Eccentric discs as a gateway to giant planets outward migration
› Accreted stars and stellar haloes of simulated galaxies in TNG50
› The Lensing Counter Narrative: An Effective Description of Small-Scale Clustering in Weak Lensing Power Spectra
› Resolving the Nuclear Environments of Tidal Disruption Event Host Galaxies within 45 pc
› Constraints on Axion-Like Particles from VERITAS Observations of a Flaring Radio Galaxy in the Perseus Cluster
› Modeling the Optical Colors of Galactic Cirrus Clouds in the Stripe 82 Region
› A very young and fast rotating shell star discovered in the eclipsing binary ZTF J200347.63+394429.8
› The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
› Hubble tension in an anisotropic Universe
› Modeling atmospheric phase corruptions in high-frequency VLBI using Gaussian processes
› The dynamics of S-stars and G-sources orbiting a supermassive compact object made of fermionic dark matter
› X-ray Observations of Nova Scorpii 2023 (V1716 Sco) in Outburst
› Linking Magnetic Field Diagnostics with 3D CME Speeds in Solar Active Regions
› Evidence of Energy Injection in the Short and Distant GRB 250221A
› Fast Radio Bursts
› $H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
› A Compact Multi-Planet System of Three Transiting Giant Planets Around TIC118798035
› Transfer Learning Beyond the Standard Model
› An XMM long look at the accretion disk plasma in the dipping neutron star LMXB 4U1624-490
› BaryonBridge: Stochastic Interpolant Model for Fast Hydrodynamical Simulations
› Nearly Monochromatic Primordial Black Holes as total Dark Matter from Bubble Collapse
› On the origins, growth, and radiative efficiency of J0529-4351, reportedly the fastest-growing known black hole
› Segmentation and Celestial Mapping of Unobservable Regions in Nighttime All-sky Images for the Mephisto Observations
› Anomalous scattering of pulsars towards the Gum Nebula
› Modeling Globular Cluster Counts with Bayesian Latent Models
› Application and development of advanced mathematical tools for population and time series analysis in pulsar astrophysics
› The impact of superradiance on the spin evolution of variably accreting massive black holes
› Interacting supernovae and where to find them
› WALLABY: an untargeted search for H I-bearing ultra-diffuse galaxies uncovers the first known ultra-diffuse galaxy pair
› Advances in detector response and background modelling in the ANAIS-112 experiment for annual modulation and other rare event searches
› Can we ignore the time dependence in matter neutrino resonance?
› XRISM mock observations of simulated AGN jets in the core of a galaxy cluster
› Probing Accretion Disk Winds of Stratified Nature with Fe XXVI Doublet in Black Hole X-ray Binaries
› Singular Value-based Atmospheric Tomography with Fourier Domain Regularization (SAFR)
› The Regulated GeAs Cycles with the New $^{63}$Ga(p,$\gamma$)$^{64}$Ge and $^{64}$Ge(p,$\gamma$)$^{65}$As Reaction Rates and Their Impact on the GS 1826$-$24 Clocked Bursts and SAX J1808.4$-$3658 Photospheric Radius Expansion Bursts
› Accretion with two-phase gas supply and its application in black hole X-ray binaries
› Exploring Synergies between Twinkle and Ariel: a Pilot Study
› Revisiting the Radio Lateral Distribution Function: An amplitude dependence on $X_{\rm max}$ and primary composition
› Distortions in Periodicity Analysis of Blazars II: The Impact of Gaps
› Beyond Standard Model equation of state and primordial black holes
› FAUST. XXVIII. High-Resolution ALMA Observations of Class 0/I Disks: Structure, Optical Depths, and Temperatures
› The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth
› On the origin of ~ 100 TeV neutrinos from the Seyfert galaxy NGC 7469
› Beyond single tracers: CNN-based inference of galaxy mass profiles from combined gas and stellar kinematics
› Collisional Excitation in Space: Recent Advances and Future Challenges in the JWST Era
› Compositional characterisation of asteroid (84) Klio with JWST
› The magnetic sensitivity of the Ca II resonance and subordinate lines in the solar atmosphere
› Coupling of neutrino beam-driven MHD waves and resonant instabilities in rotating magnetoplasmas with neutrino two-flavor oscillations
› Exoplanetary radio emission predictions and detectability in the SKA era
› Detecting gravitational lensing by matter currents
› Chromospherically active stars: Lithium and CNO abundances in northern RS CVn stars
› The richest clusters in the Coma and Leo superclusters: Properties and evolution
› A Census of Chemically Peculiar Stars in Stellar Associations
› Supermassive Black Hole Growth in Massive Galaxies at Cosmic Dawn
› MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars
› Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots
› Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
› Axion Production and Detection Using a Dual NMR-type Experiment
› Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons
› Global time-frequency search for stellar-mass binary black holes in LISA
› Charge distribution of the gauge-mediation type Q ball
› Implications of $f(R)$ gravity on late-time cosmic structure growth through a complete description of density perturbations
› Effects of Dynamical Capture on two equal-mass non-spinning black holes
› Galactic Positrons from Thermonuclear Supernovae
› A smooth filament origin for distant prolate galaxies seen by JWST and HST
› Forcing Planets to Evolve: Interactions Between Uranus and Neptune at Late Stages of Dynamical Evolution
› Gas-induced perturbations on the gravitational wave in-spiral of live post-Newtonian LISA massive black hole binaries
› Prospects for Observing Astrophysical Transients with GeV Neutrinos
› Spectro-temporal analysis of ultra-fast radio bursts using per-channel arrival times
› Using LSDB to enable large-scale catalog distribution, cross-matching, and analytics
› Cool dark gas in Cygnus X: The first large-scale mapping of low-frequency carbon recombination lines
› FIP Bias Evolution in an Emerging Active Region as observed in SPICE Synoptic Observations
› TOPz: Photometric redshifts using template fitting applied to the GAMA survey
› Primordial black holes with mass ratio-modulated initial clustering: merger suppression and projected constraints
› The Evolution of Jupiter and Saturn as a function of the Parameter R$_{\rho}$
› Proto-neutron Stars with Dark Matter Admixture: A Single-Fluid Approach
› Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
› Bimetric gravity improves the fit to DESI BAO and eases the Hubble tension
› The Effects of Linear Matter Power Spectrum Enhancement on Dark Matter Substructure
› JWST Observations of SN 2023ixf I: Completing the Early Multi-Wavelength Picture with Plateau-phase Spectroscopy
› New Radio Data on Sources of the Big Trio Program for Searching for Distant Radio Galaxies
› Clustering of DESI galaxies split by thermal Sunyaev-Zeldovich effect
› One-Loop Nonlinear Matter Power Spectrum from Unified Lagrangian Perturbation Theory: Fast Computation and Comparison with Emulators
› Renormalization-Free Galaxy Bias in Unified Lagrangian Perturbation Theory
› Extensive Analysis of gamma-Ray Periodicity in Jetted AGN from the 4FGL Catalog Using Fermi-LAT Observations
› WALLABY Pilot Survey: A gas-rich diffuse dwarf on the baryonic Tully Fisher relation
› Re-accretion of Giant Impact Ejecta Can Drive Significant Atmospheric Erosion on Terrestrial Planets
› M3DIS -- A grid of 3D radiation-hydrodynamics stellar atmosphere models for stellar surveys. II. Carbon-enhanced metal-poor stars
› A fast powerful X-ray transient from possible tidal disruption of a white dwarf
› Revealing evolution of Dark Energy density from observations
› 84 Second and 169 Second Rotation of Two Isolated, Ultramassive, Strongly Magnetic White Dwarfs
› Inflationary Gravitational Waves as a probe of the unknown post-inflationary primordial Universe
› Uniqueness of gravitational constant at low energies from the connection between spin-2 and spin-0 sectors
› Gravitational atoms beyond the test field limit: The case of Sgr A* and ultralight dark matter
› Cosmological Origin of the KM3-230213A event and associated Gravitational Waves
› Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
› Search for high energy 5.5 MeV solar axions with the complete Borexino dataset
› Naturally resonant two-mediator model of self-interacting dark matter with decoupled relic abundance
› Low-temperature Performance of $\mathrm{Gd_3(Ga, Al)_5O_{12}}$:Ce Scintillators
› Superconducting Strings in $E_6$

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