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Astronomia w Krakowie
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view from north-east
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Temperature
12.0 °C

Humidity
 59%

Wind
3.2 km/h

Pressure
1014.6 hPa

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 News from astronomynow.com

› Happy New Year, Mars! The Red Planet is turning 39
› 3I/ATLAS was born in the deep freeze
› Roman Space Telescope launches on mission to survey the Universe
› JWST’s ‘impossible’ early galaxies may be even more massive than we thought
› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
RSS  Latest preprints on astro-ph:

› Supermassive Black Hole Winds in X-rays -- SUBWAYS. VI. Interplay between the soft X-ray excess and ultra-fast outflows
› On the Nature of the BeWD System Nova FQ Circinus
› Inferring the shapes of low-mass galaxies at $z>6$ from FIREbox$^{HR}$. Where are the disks?
› Euclid Bypass end-to-end simulations for spectroscopic galaxy clustering performance assessment
› PSR~B0355+54: An Unexpected Compendium of Nearly All Scintillation Arc Morphologies
› Gamma-ray Bursts as Cosmological Probes Calibrated with Strongly Lensed Quasars and Neural Networks
› The science case for an in-situ measurement platform in the Venus clouds
› Graph Neural Networks for Astrophysics and Cosmology
› The ALMA REBELS Survey: The [C II] Luminosity Function of UV-Selected Galaxies at $z\sim7$
› Planets surviving common envelope evolution should be rare, massive, and orbit very close to their host star
› How does a galaxy's quenching probability depend on its black hole's mass?
› Metal-poor molecular clouds in dwarf galaxies at parsec-scale resolution
› Small Collisions, Big Impact: The Sensitivity of Atmospheric Temperatures to Collision-Induced Absorption
› ASTROLABE: A 3D Particle-Level Surrogate for Cosmology Simulation with Physical Flow Matching
› Beyond static torques: Self-consistent migration and dynamical trapping of low-mass planets in dusty disks
› Optical and Ultraviolet Emission from the Gas Photoionized by Gaia BH3: Archival Constraints and Predictions for the 2029 Periastron
› Balmer breaks in accreting super-massive black hole binaries
› Localizing binary neutron stars with the Einstein Telescope: a full Bayesian comparison of the triangular and 2L configurations
› Dual and lensed AGN at sub-arcsecond separations uncovered by ERIS
› DDELenS: Tomographic Weak Lensing Simulations with Dynamical Dark Energy
› The SIMPLIFI Survey: Polarization of Dense Filaments with SOFIA III. Relative orientations of antenna temperature gradients with the magnetic field in the DR21 molecular cloud
› Leviathan: a very massive, extended sub-millimetre galaxy spectroscopically confirmed at $\rm z = 4.05$
› Slowly Rotating Fully Convective Stars at $\lesssim$ 1 Gyr: Evidence from the Hyades and Praesepe
› 20,000 Rotation Periods in Nearby Open Clusters and Moving Groups from ZTF and ASAS-SN
› Twenty-five years of XMM-Newton EPIC-MOS2 Unfocused Particle Background: Solar Cycle Modulation, Galactic Cosmic-Ray Correlation, and Implications for NewAthena
› Ammonia-Hydrogen Phase Equilibria in Planetary Envelopes from First-Principles-Based Machine-Learning Molecular Dynamics
› Numerical shock broadening and supernova neutrino conversion: implications for DUNE
› A MUSE Study of Stellar and Ionized-Gas Kinematics in Central Group Galaxies
› The GLEAM 4-Jy (G4Jy) Sample: V. Broadband spectral analysis
› The Imprint of Core-collapse Asymmetries on Supernova Shock Breakout
› Evolution of Massive Main-Sequence Stars in Binary Population Synthesis. II. Consequences for Black Hole High-Mass X-ray Binaries and Binary Black Holes
› Analytical Chemistry at the Planetary Frontier
› Ionized Gas Kinematics and Star-forming Clumps in Extremely Metal-poor Galaxies
› Are Dynamical Dark-Energy Cosmologies Old Enough?
› Large-scale Vortices in the Solar Photosphere: Statistical Properties and the Reliability of Local Correlation Tracking
› Searching for Dense Perturbers in Cold Dark Matter Simulations
› AI and The Enclosure of the Scientific Commons
› J-PLUS: Identifying Outlier Spectral Energy Distributions in the Fourth Data Release Using Unsupervised Machine Learning
› The Future of Gamma-Ray Bursts as Probes of the Epoch of Reionization in the Era of JWST and the Extremely Large Telescope
› The presence and order of QCD phase transitions from gravitational-wave observations of neutron star mergers
› Globular Clusters GMRT Pulsar Survey (GCGPS) III: ORION - a multi-beam acceleration search pipeline
› Source velocities of fast radio bursts constrained by their dispersion measure variations
› SN 2023iop: An Extreme 1987A-like Supernova and the Death of Very Massive Stars
› Core-Collapse Supernova Rates in the Dark Energy Survey
› Size, Albedo, and Taxonomy of Asteroid (1201) Strenua from Stellar Occultation and ATLAS Photometry
› Exomoonlight Sonata: On the Fate of Exomoons Around Migrating White Dwarf Planets
› Constraining the FRB Central Engine from Flux Variations of Persistent Radio Sources: FRB 20240114A as the First Attempt
› A $\wedge$-like metallicity profile in the disk of the Sagittarius dwarf galaxy
› A Radiation-Hardened, Fault-Aware Quantized Neural Network That Self-Heals
› Probing Nearby Electron Sources and Local Diffusion with the TeV All-Electron Spectrum
› Short-timescale X-ray variability of the blazar 1ES 1959+650 observed with AstroSat/SXT
› Gaussian process-based Bayesian imaging of bolometric (sub-)millimetre data
› Estimator Precision and Selection for Up-the-Ramp Sampling with a High-Read-Noise InGaAs Camera
› An improved self-gravity treatment in general relativistic smoothed particle hydrodynamics
› Cosmic-ray melt windows in interstellar ice make a four-carbon ketose but not the sugar pattern of G+0.693-0.027
› When the core ate the atmosphere
› Probing the Optical/UV Continuum Variability of Active Galactic Nuclei with the Damped Random Walk Model
› What Shapes the Ultraviolet Spectra of Type Ia Supernovae?
› The chemical evolution of the LMC from APOGEE abundances: a hybrid two-infall OMEGA+ analysis
› Single-Parameter Exponential Model Outperforms Standard Dark Matter and Modified Newtonian Frameworks in Predicting Galactic Rotation Curves
› A bright X-ray flaring event from the intermediate supergiant fast X-ray transient IGR J00370+6122 observed with NuSTAR
› The environments of type Ibn supernovae: evidence for a strong Wolf-Rayet star component
› Probing Minihalos in the Late Dark Ages through Velocity Acoustic Oscillations in the 21-cm Power Spectrum
› Constraining Solid HNCO and Its Environment in Open JWST Data with Laboratory Spectra
› VVV CL001: A strong candidate for the most ancient star cluster in the Galaxy
› Understanding the formation of alpha-Fe bimodality in the Milky Way using constrained cosmological simulations of the Local Group
› Phakoseismology: Asteroseismology of gravitationally microlensed stars
› An improvement to the spatial discretisation in the Astrophysical Weighted Particle Hydrodynamics method
› Kinematically isolating intracluster light in AS1063: a distinct stellar population tracing the dark matter core
› Rapid Variability of Radiative Signatures from Driven Relativistic Reconnection
› On the superbursts as photodisintegrators of ashes from the rp-process -- Numerical simulations of superbursts with MESA II
› Constraints on Dark Matter Annihilation from Starlight-Induced Inverse Compton Emission in Omega Centauri
› Pulsar J1909+0749 and Supernova Remnant G42.1-0.2: A case of a pulsar that has exited the shell of its associated supernova remnant
› The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres
› Deriving Interplanetary Sector Boundary Crossings using Potential Field Source Surface Modeling
› Detection and Statistics of large-scale Sector Boundary Crossings in the Solar Wind: The SBCross Catalog
› Hidden engines in tidal disruption events: multimessenger signatures in a lepto-hadronic framework
› Orbital Parameters for 65 Wide Binary Systems: no evidence for gravitational anomaly at low acceleration
› The Effect of Field Line Tracing Height on Wang-Sheeley-Arge Solar Wind Predictions at Earth
› Real-Time 24-hour Ahead Forecasting of Solar Energetic Particle Events with SEPNET-PRISM-R
› Coevolution of Dust Growth and Gravitational Instability in Massive Protostellar Disks
› Data-Driven Ages from Asteroseismology for FGK Dwarfs
› Revisiting the Unknown Unknowns in Transient Astrophysics with the SKA Telescopes
› Photometric variability of blue supergiants: Constraints on stellar masses and evolutionary stages
› KMOS Spectroscopic Follow-up of 16 Star Cluster Candidates of the Sagittarius Dwarf Galaxy
› Identifying a jet-shaped point-symmetric morphology in the supernova remnant HB9
› Tight asteroseismic upper limits on hot subdwarf magnetism
› The "Rubin 2036: Opportunities for Discovery" Workshop: A Community Roadmap for the Future of the Vera C. Rubin Observatory After the LSST
› A Solar Optical Clock
› Resonant three-mode coupling in asteroseismology I: Bifurcations, chaos, and DAV white-dwarf outbursts
› The clumpy fraction of galaxies at $z=1-9$ with JADES: evidence for a mass-dependent transition in clump origin
› Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields
› TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance
› A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274)
› Large fluctuations and cusp-core transformation in dwarf galaxies
› Resolving the extended interstellar medium of infrared galaxies II. Fine-structure line emission
› Resolving the extended interstellar medium of infrared galaxies I. Polycyclic aromatic hydrocarbon emission
› Automated optimization of solar energetic particle acceleration and transport parameters against five-spacecraft observations of the 9 October 2021 event
› Community Lessons from builders of infrared multi-object spectrographs
› Slow-Roll Inflation at Arbitrary Order
› Dynamical stability of Magnetic Supramassive Neutron Stars
› Constraints on Millimeter-wave Extragalactic Transient Populations from 4 Years of SPT-3G data
› Search for Compact Binary Coalescences with Sub-solar Mass Components in Data from the Second Part of LIGO-Virgo-KAGRA's Fourth Observing Run
› Adaptive Model-Switch Thermodynamic Integration: A Bayes Factor Estimator
› Ion Heating in Pair-loaded Relativistic Turbulence
› Floquet Instability of Photon-Axion Conversion
› Elementary-Symmetric Ricci Gravity: Metric Formulation
› Annihilation feedback on elastic scattering in self-interacting dark matter
› A Natural Dark Matter-Dark Energy Interaction from Axion-Monopole Dynamics
› Deglobalising the fit: how to search for physics beyond vacuum General Relativity in LISA catalogues
› Cosmic birefringence from a stiff axion field and its cosmological implications
› Modular Bayesian Inference for Partially Misspecified Mixtures with Uncertain Class Labels
› Self-interacting dark matter from radiative bound-state-formation feedback
› Illuminating Light Dark Matter with Fixed-Target Experiments
› A Multipole Technique for the Simulation and Analysis of Gravitational Waveforms from Extreme Mass Ratio Inspirals
› High-cadence GW astrometry in the $\mu$Hz gap
› P-ONE-1: the first detector line of the Pacific Ocean Neutrino Experiment
› Stability Analysis of Axion Dark Energy Model
› Untangling Extreme Mass Ratio Inspirals and Massive Black Hole Binaries in LISA Data
› Axion detection in the non-Markovian noise
› Two-Component Dark Matter and Strongly First-Order Electroweak Phase Transition via a Two-Step Mechanism in the Inert Doublet plus Real Singlet Model
› Direct Urca process facilitated by non-Fermi-liquid quantum criticality
› On the Stability of Tolman Oppenheimer Volkoff Fireholes
› Hybrid Stars with Different Amount of Quark Matter
› Exponential Growth of Turbulent Cross Helicity in Shear-Flow-Driven Turbulence
› MadStree: automated evaluation of tree-level de Sitter correlators
› Lagrangian perturbation theory for modified gravity
› Don't miss the forest for the trees: the Lyman alpha forest power spectrum in effective field theory
› Unveiling dark forces with measurements of the Large Scale Structure of the Universe
› Causality and perturbative-QCD constraints on first-order phase transitions in neutron stars
› Kratos-polrad: Novel GPU system for Monte-Carlo simulations with consistent polarization calculations
› MAMMOTH-LyC: Investigating the Role of Galaxy Mergers in a Strong Lyman Continuum Leaker at $z=2.39$
› Formation and Evolution of [Wolf-Rayet] Planetary Nebulae through a Late Thermal Pulse
› An empirical derivation of the average dust attenuation law at 2
› Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study
› The Life and Death of Stars That Capture Primordial Black Holes
› The Effect of Adiabatic Index on Radius Evolution and the Mass Loss
› A New Scaling of Neutron Star Tidal Deformability for Directly Probing the Central Equation of State Parameter
› Search for Diffuse Supernova Neutrino Background in the Full KamLAND Dataset with Neural-Network-Based Event Classification
› Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors
› Infrasound Newtonian Noise Estimation at the Einstein Telescope Candidate Site Sos Enattos
› Observational Evidence for Anisotropic Metal Excess around Galaxies
› VAPOLA - A multiyear, multiband polarization survey of AGNs and Sgr A* at millimeter wavelengths with ALMA II. Spectropolarimetric properties and their evolution from 2017 to 2023
› Periodic activity on the (sub)mm surface of the AGB star Mira A
› Wide Field Localization Using Fixed Modulation Collimators
› Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey
› Solar spicule population properties inferred from IRIS Mg II k off-limb spectra using likelihood-free Bayesian inference
› Galaxy Protoclusters as Drivers of Cosmic Reionization: II. Te-Based Metallicities of Lyman-{\alpha} Emitters
› Collisional excitation of SiC$_6$ by helium: cross sections, rate coefficients, and astrophysical implications
› A faint dust ring beyond the compact disk of Sz 76
› Structure and evolution of cosmic voids within DESI DR1
› Optical constraints on intranight variability in TeV HBLs from a two-year Asiago Schmidt monitoring campaign
› Consistently Reproducing Early Galaxy Observations and 21-cm Signal during the Epoch of Reionization
› Beyond the Disc--Spheroid Dichotomy at $0.6 < z < 8.0$: Evidence for a Morphological Indeterminacy Regime from JWST
› The DARWIN Project: Cosmological Simulations of Galaxy Formation down to Dwarf Scales in Diverse Environments
› The Central Molecular Zone of our Galaxy, a chemical complexity factory: first interstellar detections of molecules towards G+0.693
› New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis
› Inflationary Particle Production and the Swampland
› Probing freeze-in dark matter using Bose-Einstein condensate in neutron star
› Energy extraction from NED-deformed rotating black holes via the Comisso-Asenjo reconnection process
› Detecting Tidal Resonances in Binary Neutron Stars
› A dark-matter-sensitive orientation clock near rotating black holes
› Resonant lunar tides of Earth's core and basal magma ocean
› Gravitational-wave responses and noise correlations in geometric time-delay interferometry
› Exact 1D Nonlinear Solutions for Proton-Driven Plasma Wakefields
› Entropic Chaplygin-Gas cosmology and late-universe tension diagnostics
› Penrose process in radiating Kerr-Vaidya black holes: efficiency, energy transport, and the viability boundary

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