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Astronomia w Krakowie
Photo: Halo, moon dogs and parhelic circle around the Moon
Halo, moon dogs and parhelic circle around the Moon
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 News from astronomynow.com

› 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
› Astronomy Now under new ownership
› Binoculars to boost your night-sky viewing
RSS  Latest preprints on astro-ph:

› UNAGI: A Conceptual Electrodynamic Tethered Spacecraft Demonstration Mission for Propellantless Landing on Io
› Plasma lens with frequency-dependent dispersion measure effects on fast radio bursts
› Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
› Not All Sub-Neptune Exoplanets Have Magma Oceans
› pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
› Dwarf galaxy halo masses from spectroscopic and photometric lensing in DESI and DES
› Constraints on an optical counterpart for the long-period radio transient GPM J1839-10
› Massive Star Formation at Supersolar Metallicities: Constraints on the Initial Mass Function
› A roadmap to cosmological parameter analysis with third-order shear statistics IV. Analytic cross-covariance between second- and third-order aperture masses
› SAGAbg III: Environmental Stellar Mass Functions, Self-Quenching, and the Stellar-to-Halo Mass Relation in the Dwarf Galaxy Regime
› Star Formation under a Cosmic Microscope: Highly magnified z = 11 galaxy behind the Bullet Cluster
› Neural Networks as Surrogate Solvers for Time-Dependent Accretion Disk Dynamics
› A GLIMPSE of Intermediate Mass Black holes in the epoch of reionization: Witnessing the Descendants of Direct Collapse?
› On the Fate of Little Red Dots
› BlackTHUNDER: Shedding light on a dormant and extreme little red dot at z=8.50
› A DECADE of dwarfs: first detection of weak lensing around spectroscopically confirmed low-mass galaxies
› How two-dimensional are planet-disc interactions? II. Radiation hydrodynamics and suitable cooling prescriptions
› Technical Memo: The impact of Nancy Grace Roman Telescope's default image processing on the detectability of moving Solar system objects
› The elusive chase for the first RR Lyr star in a binary system: the case of KIC 2831097
› Separating Photospheric and Starspot Magnetic Fields in Pre-Main-Sequence Stars Using IGRINS Spectroscopy
› Multiwavelength study of Galactic PeVatron LHAASO J0341+5258
› Measuring the Central Dark Mass in NGC 4258 with JWST/NIRSpec Stellar Kinematics
› The interstellar heritage of comets
› Blue Stragglers and Friends: Initial Evolutionary Pathways in Close Low-Mass Binaries: Literature Review
› Gaussian Planck Relics are Ruled-Out as Dark Matter by LIGO
› Characterizing Nanoflare Energy and Frequency through Field Line Analysis
› HWO Target Stars and Systems: A Prioritized Community List of Potential Stellar Targets for the Habitable Worlds Observatory's ExoEarth Survey
› Under the glare of a luminous quasar, the FIR continuum is still an excellent tracer of the ISM down to the central kiloparsec
› The SOMA Atomic Outflow Survey. I. An Atomic OI and Highly Ionized OIII Outflow from Massive Protostar G11.94-00.62
› Why do solar wind models get it wrong: understanding the capabilities of time-dependent solar wind simulations
› Probing the Parameter Space of Axion-Like Particles Using Simulation-Based Inference
› von K\'arm\'an--Howarth Similarity of Spatial Correlations and the Distribution of Correlation Lengths in Solar Photospheric Turbulence
› The X-ray Emission of NGC 5005: An Unobscured Low-Luminosity AGN with a Weakly Accreting Broad-Line Region
› The First 4 Years of SN 1993J Revisited: Geometric $m$-ring Modeling of the Radio Shell with Closure Quantities Only
› Discovery of Two Highly Scattered Pulsars from Image-Based Circular Polarization Searches with the Australian SKA Pathfinder
› The impact of the point spread function fitting radius on photometric uncertainty based on the Fisher information matrix
› Millisecond Pulsar Discoveries in an Image-based MeerKAT Survey of the Galactic Bulge
› Constraints on the Orbit of the Young Substellar Companion GQ Lup B from High-Resolution Spectroscopy and VLTI/GRAVITY Astrometry
› Merger-Induced Disturbance and Temporal Signatures in Galaxy Clusters: A Combined Phase Space and Photometric Analysis
› Cosmic Multipoles in Galaxy Surveys II: Comparing Different Methods in Assessing the Cosmic Dipole
› Stochastic Heating in the Sub-Alfv\'enic Solar Wind
› Reconciling the Tension Between Light Curve Modeling of Type II Supernovae and Neutrino-Driven Core-Collapse Supernovae Models with Late-Phase Spectroscopy
› Performance of LACT Array: Instrument Response Functions and Source Prospects
› First Radio Neutrino & Cosmic Rays Astronomy Workshop in India
› Episodic Feedback in Triple AGN Candidate SDSS J0849+1114 Revealed by Extended ionized gas
› Hybrid Strategy for Coordinated Interstellar Signaling: Linking the Galactic Center and Extragalactic Bursts
› Formation Of Sub-Structure In Luminous Submillimeter galaxies (FOSSILS): Initial sample and the discovery of a dusty spiral at Cosmic Noon
› Tidal features around simulated groups and cluster galaxies: Enhancement and suppression of merger events through environment in LSST-like mock observations
› Techniques for Continuous Wave Identification and Filtering in the Askaryan Radio Array
› Assessing the Power-Law Emissivity Assumption in X-ray Reflection Spectroscopy: A Simulation-Based Evaluation of Different Coronal Geometries
› A New Precise Measurement of the Cosmic Microwave Background Radiation Temperature at $z=0.89$ Toward PKS1830-211
› Exciting Stellar Eccentricity in Gaia BH3 via a Hidden Black Hole Binary
› Galactic Contrail in NGC 3627 caused by Dwarf Galaxy Candidate or Massive Black Hole Flyby
› Probing redshift-dependent systematics in the Hubble tension: Model-independent $H_0$ constraints from DESI R2
› The Extended Stellar Distribution in the Outskirts of the Ursa Minor Dwarf Spheroidal Galaxy
› Galactic chemical evolution of short-lived radioactive isotopes produced by explosive nucleosynthesis: $^{60}$Fe and $^{53}$Mn
› Vacuum Ultraviolet Photoabsorption Spectra of Icy Isoprene and its Oligomers
› High energy gammas and neutrinos from the Sun, Jupiter and Earth
› A sample of 3403 galaxy clusters identified in XMM-Newton X-ray images
› VERITAS Observations of the Microquasar SS 433
› PENELLOPE VIII: Revisiting empirical relations to measure accretion luminosity
› A statistical study of type II outbursts of XRPs: Brighter accreting pulsars rotate faster
› A new era for multi-wavelength studies of blazars with Rubin and the CTAO
› Resistive Scaling in the Magnetic Helicity-Driven Inverse Cascade
› A LOFAR search for coherent radio emission accompanying prompt engine activity in gamma-ray bursts
› Unveiling Central ortho-H2D+ Depletion at Sub-kau Scales in Prestellar Core G205.46-14.56M3: The First Interferometric Evidence and Implications for Deuterium Chemistry
› A Two-Stage Kick Scenario for the Peculiar LMXB GX 1+4
› The depletion of the asteroid belt and the impact history of the Earth
› The NANOGrav 15-Year Data Set: Improved Timing Precision With VLBI Astrometric Priors
› RadioSED II: discovering the peaked spectrum radio sources in Stripe 82
› Limitations on Morphological Fitting for JWST "Little Red Dots"
› Polycyclic aromatic hydrocarbon (PAH) abundances in the disk around T Chamaeleontis (T Cha): PAH sizes, ionization fraction, and mass during JWST observations
› Modelling the effect of stellar metallicity on the XUV evolution of low-mass stars and its impact on exoplanet atmospheres/habitability
› Emission line tracers of galactic outflows driven by stellar feedback in simulations of isolated disk galaxies
› Outflow-cloud interaction as the possible origin of the peculiar radio emission in the tidal disruption event AT2018cqh
› J-PLUS: Understanding outlier white dwarfs in the third data release via dimensionality reduction
› Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes
› Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
› Explaining the Origin of TeV Gamma Rays from M87 During High and Low States
› Dark matter: red or blue?
› Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized/Resonant Hair
› A relativistic treatment of accretion disk torques on extreme mass-ratio inspirals around non-spinning black holes
› Collider probes of baryogenesis with maximal CP asymmetry
› A Passive UV-Based System for Discharging the Test Masses of Ground Based Gravitational Wave Detectors
› Anderson self-localization of light in pair plasmas
› Regression of Suspension Violin Modes in KAGRA O3GK Data with Kalman Filters
› Scalaron dark matter dynamics: effects of Higgs non-minimal coupling to gravity
› Gravitational waves from two scalar fields unifying the dark sector with inflation
› Probing Light Dark Matter with Cosmic Gravitational Focusing
› Primordial black holes formation in inflationary $F(R)$ models with scalar fields
› Probing the mass relation between supermassive black holes and dark matter halos at high redshifts by gravitational wave experiments
› The Local Volume Database: a library of the observed properties of nearby dwarf galaxies and star clusters
› Resolved mass assembly and star formation in Milky Way Progenitors since $z = 5$ from JWST/CANUCS: From clumps and mergers to well-ordered disks
› PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). III. Composition and winds in the atmosphere of TOI-1518 b
› Eclipse Timing Variations of Circumbinary Substellar Objects in TESS Data
› Magnetic Webs in Stellar Radiative Zones
› Matter Dipole and Hubble Tension due to Large Wavelength Perturbations
› First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
› The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. II. Hydrogen Recombination Lines Toward High-Mass Protostars
› Search for GeV-PeV neutrinos from nova T Coronae Borealis with IceCube
› The JWST Weather Report: retrieving temperature variations, auroral heating, and static cloud coverage on SIMP-0136
› AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
› Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers
› STRRINGS: STReams in Residual Images of Nearby GalaxieS
› PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
› Role of CME clusters and CME-CME interactions in producing sustained $\gamma$-ray emission
› Constraining Common Envelope Evolution in Binary Neutron Star Formation with Combined Galactic and Gravitational-Wave Observations
› Lithium evolution in the Galactic thin disc from Main-Sequence and early Red-Giant-Branch stars
› Quintessential dark energy crossing the phantom divide
› Road map for the tuning of hadronic interaction models with accelerator-based and astroparticle data
› Tidal disruption events in active galactic nuclei: on orbital inclination and Schwarzschild apsidal precession
› Cosmic Ray Spatial Distribution and the Galactic/Extragalactic Transition
› Probing Hernquist dark matter with black hole shadows: A comprehensive study of various accretions
› Expected Constraints on the Intergalactic Magnetic Field using Gamma-Ray Bursts with the Cherenkov Telescope Array Observatory
› Are X-Ray Detected Active Galactic Nuclei in Dwarf Galaxies Gamma-Ray Bright?
› Solar and Stellar Activity
› Supernova axions convert to gamma-rays in magnetic fields of progenitor stars
› Constraining matter-bounce scenario from scalar-induced vector perturbations
› Hybrid Summary Statistics
› Limits on New Lorentz-violating Bosons
› Symmetry energy expansion and the peak value of the bulk viscosity
› Primordial magnetogenesis from a supercooled dynamical electroweak phase transition
› A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
› Exact Taub-NUT-like Black Holes in Einstein-bumblebee gravity: their thermodynamics and thermodynamic topology
› StrCGAN: A Generative Framework for Stellar Image Restoration

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