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Astronomia w Krakowie
Photo: Sunset as seen from the Observatory
Sunset as seen from the Observatory
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1011.8 hPa

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Moon

 News from astronomynow.com
› 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
› Dark matter may come in multiple forms, new model suggests
› Witness to history: Artemis II, lunar exploration and hope
RSS  Latest preprints on astro-ph:
› Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole?
› CHARA Array Observations of the Evolved Components in Symbiotic Star Systems
› A first-principles binary neutron star merger model of GW170817, GRB170817A, and AT2017gfo
› Discovering Substellar Dark Matter Halos with Astrometric Weak Lensing of Multiply Imaged Quasars
› Resolved Dust in $z\approx1$ Galaxies with JWST/MIRI MRS: Survey Description and First View on PAHs, Mid-IR Atomic Emission, and Warm H$_2$
› TDCOSMO. XXVII. JWST-based Lens Models and H$_0$ Measurement of WFI2033, HE0435, and PG1115
› Exploring the capabilities of combined modelling strategies for supernova with relativistic jets using Redback
› Dust and PAHs in late-stage galaxy evolution: Imprints of TP-AGB dust injection, grain growth and AGN feedback in high-z quiescent galaxies with JWST and ALMA
› Stellar Flares Rather than High $T_{int}$ As Possible Cause for the Missing Methane in Young Exoplanets: The Case Study of V1298~Tau\,b
› Measuring Extragalactic Microlens Masses and Motions in Strongly Lensed Quasar Systems with Intensity Interferometry
› The Limited Lifetime of Self-Gravitating Accretion Disks In Galactic Centers
› Dynamical formation of high-eccentricity compact binaries through BH--BH*/TZO collisions
› Formation of black hole stars via star--black hole collisions
› BSN-VIII: Detailed Photometric Modeling of Ten W UMa Contact Binaries and a Revised Empirical Period-Mass Relationship
› Why is there cold gas inside the Local Bubble?
› Cluster Ages to Reconstruct the Milky Way Assembly (CARMA). V. The chronological merger tree of the Milky Way
› Spectral Synthesis for Classical Ae Stars: H${\alpha}$ and CaII
› Toward a realistic test of black-hole movie correlations as a probe of extreme lensing
› A 500 pc volume-limited sample of hot subluminous stars III. The short-period binary population
› Spin-disc misalignment drives periodic accretion and pulse profile asymmetry in X-ray pulsars
› Magnetospheric birefringence breaks the rotating-vector model and depolarises X-ray pulsars
› Overmassive supermassive black holes in SDSS close galaxy pairs
› The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation
› Near-Infrared Spectroscopy of Low-Redshift Palomar-Green Quasars and Composite Spectra
› PolPy: A universal tool for X-ray/gamma-ray polarimetry using common data format standards
› High Dispersion Measure Fast Radio Bursts from Young, Dust-Poor H II Regions
› JUG: JAX-based Unified pulsar timinG
› Low-energy antinuclei measurements for background-free indirect dark matter searches and PBH signatures
› Quiescent and Interacting Compact Remnant Binary Populations in the Space Telescope Era
› A Unified Tracer Analysis of DESI DR2 Baryon Acoustic Oscillations
› Dynamically driven collapse of a thermally stable accretion disk in a nova-like system
› Modeling Carbon-Based Planets with MAGRATHEA
› Dense Cores in the Vicinity of an HII Region
› Rapid Variability and Broadband Spectral Modeling in the Flaring Activity of BL Lacertae
› Learning the averaged history of an inhomogeneous universe from its present day density field
› From Inspiral to Expansion: The Wake-Driven Torque on Binary Black Holes in Gaseous Medium
› Hyperon bulk viscosity effects in neutron-star inspirals
› Cooling-regulated gas accretion onto gap-opening planets
› The Geometry of Ultra-Fast Outflows Probed by Soft X-ray Variability in PDS 456
› A decade of radial-velocity monitoring of rho Leo: moment analysis and periodic variability
› Spherical Accretion onto Konoplya Zhidenko Black Holes: Sonic Point Analysis and Fluid Dynamics
› CoBiToM project. III. Physical characterisation of the potential merger candidates AL Lep, ASAS J082243+1927.0, and ZZ PsA
› Extremely Low Mass Ratio Contact Binaries. III. Photometric and Spectroscopic Investigations of Eleven Systems
› Broadband heterodyne interferometry with a chirped femtosecond laser in the H-band
› Dissecting ultra-diffuse galaxies in the field
› On the theoretical instability strips of {\gamma}-Doradus stars including the effect of the metallicity and rotation
› The Canadian Galactic Emission Mapper: A New 8-10 GHz Telescope to Map the Polarization of the Northern Sky
› A High Velocity SiO Jet from S255N SMA3
› Design and implementation of an SLM-driven coherent differential imaging scheme
› The PLACID active coronagraphic imager instrument: commissioning status
› Search for magnetic fields in seven slowly rotating A stars
› Guide for the Hubble Tension: Mid-Time Solutions and Generalized PAge Parameterizations
› Development, Configuration and Performance Characterization of a Scalable BETA ASIC-Based Readout System for Multi-Channel SiPM Detectors
› Probing magnetic fields in stars: A 2D oscillation framework including rotation and magnetism
› Correction of the influence of rolling shutter detectors on determining the velocity of meteors from video recordings
› JWST telemetry combined with active coronagraphy: raw contrast predictions for exoplanet imaging with the Habitable Worlds Observatory
› Deep VISTA observations of the Magellanic Clouds (VMCDeep)
› Explicit gauge-invariant variables in multifield inflation beyond linear order and Hamiltonian dynamics
› On the Origin of a Dusty Circumstellar Medium around Red Supergiants
› Inversion Framework of Internal Mass Distribution Parameters of Asteroid Apophis from Dynamical Observations
› Three-dimensional Core-Collapse Supernova Simulations: From shell burning to shock revival
› A high-frequency type II radio burst associated with an X2.3 class flare
› PIFFLE: Characterizing the Foreground Contributions from 4 Decades in Halo Mass to the FRB20230907D Dispersion Measure
› Dynamical Modeling of Kinematically Decoupled Galaxies: Structural Components
› Astrophysical Sensitivity Projections for the IceCube Upgrade
› Follow-up of SN 2025wny I: Space-based Observations of the First Multiply-imaged Superluminous Supernova
› Follow-up of SN 2025wny II: Superluminous Supernova Physics at Cosmic Noon
› Follow-up of SN 2025wny III: Spectroscopic Time-delay Measurements of a Strongly Gravitationally Lensed Superluminous Supernova
› Follow-up of SN 2025wny IV: Photometric Time-delay Measurements of a Strongly Lensed Superluminous Supernova
› Follow-up of SN 2025wny V: Lens Modelling and Cosmography of a Strongly Lensed Superluminous Supernova at $z = 2.015$ using Space Data
› Characterising the Globular Cluster Systems of Three Local Group Dwarf Galaxies: NGC6822, NGC147 and NGC185
› Reassessing the contribution of long-GRB high-energy afterglows to the isotropic gamma-ray background after GRB 221009A
› pyEDITH: the coronagraphic exposure time calculator for the Habitable Worlds Observatory
› Enhancing Cosmological Constraints from Foreground-Cleaned CMB Maps Using Large-Scale Structure Surveys
› Relativistic outflows power a quasi-periodic eruption: constraints on energetics, mass loss, and emission mechanisms
› Fast and efficient nested sampling with BEST
› An All-Sky Catalog of 6.5 Million Primary Red Clump Stars from Gaia DR3 XP Spectra
› Distinct Modes of Pulsar Glitch Activity Revealed by the Waiting-Time--Amplitude Morphology
› Exploring the sensitivity of in-ice radio detectors to cosmic ray mass composition
› A Clearer View of HAT-P-1 b: JWST NIRSpec G395H Reveals Water, Carbon Dioxide, and Possibly Hydrogen Sulfide
› ExoMOD I. A Forward Model for the Orbital Architecture of Kepler Multi-Planet Systems
› ExoMOD II. A Statistical Model of Transit Timing Variations in Kepler Multi-Planet Systems
› A Similarity Theorem and Its Breakdown in Atomic Black Hole Accretion
› Detecting Axion-Like Particles With Coiled Optical Fibers I: Silica Fibers
› A microwave SQUID multiplexing concept for macro-cryogenic calorimeter arrays
› Creation of an inflationary epoch from an Emergent Universe through quantum tunneling
› Horizon-Dependent Tube MPC for Elliptical-Orbit Rendezvous Under Mass Uncertainty
› Future of Artificial Intelligence for Science in Japan 2024 Community Report
› Dynamical friction on black holes in scalar field environment
› Devoured by a Hairy Gargantua: Probing Massive Scalar Charges with Non-minimal Curvature Coupling with Extreme-Mass-Ratio Inspirals
› Editorial: Promoting Green Computing in High Energy Physics and Astrophysics
› Solar Magnetic Configuration Control over Radiation Belt Electrons
› Separate universe in multifield inflation: a phase-space approach
› DESI Data Release 1: Stellar Catalogue
› Reappraising the Elatina series: What if the Solar Interpretation Were Correct?
› One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters
› Renormalization group corrections to $\Lambda$CDM model and observational consequences for $H_0$ tension
› A Practical Study of Lightweight Neural Gravitational-Wave Detection in Real LIGO Noise: Models, Ablations, and Open Software
› Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy
› Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP
› The Binary Populations of Stellar Streams are Set by Cluster Dynamics
› Fast modelling of ionization balance in the intergalactic medium: I- implications for the IGM metallicity
› NOEMA3D: Extended CO, [C I] and dust in massive star-forming main-sequence galaxies at cosmic noon
› Probing the IMF in the Early Universe -- Direct measurements in the Bo\"otes I UFD with JWST/NIRCam
› Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31
› A Steep-Extinction Quasi-stellar Object at z=4.6: JWST Evidence for Abundant Small Dust Grains
› GATOS XV: A JWST/MIRI survey of extended circumnuclear dust emission in nearby Seyfert galaxies
› A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter
› The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy
› On the astrophysical origin of cosmic rays: Constraining the Ultra-High-Energy Cosmic Ray Horizon through Nearby Galaxy Distributions
› Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster
› A Systematic Trend in the Observed vs. Predicted Radii of Transiting Brown Dwarfs
› Distinct Jet Properties in the X-Ray-Obscured State of GRS 1915+105
› Qualification pathways for Photonic Integrated Circuits in Astrophotonic Space Missions
› A bestiary of low-level electrical artifacts in SPHEREx flight data
› Exact spherical-wave forward model for radio reflection from stratified media and implications for the anomalous-polarity events observed by ANITA
› Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates
› Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion
› Magnesium silicate condensation in sub-Neptune envelopes: the fundamental link between chemistry, structure, and observables
› Status of BICEP Array and Integration of the 220/270 GHz Receiver
› Distinguishing cold and self-interacting dark matter through topological analysis
› The MegaWave Radio Surveyor
› Primordial black holes from Q-balls produced in a first-order phase transition
› WimPyC: an extension module of WimPyDD for the calculation of WIMP capture in celestial bodies
› A parameterized equation of state for dark energy and Hubble Tension
› Assessing astrophysical foreground subtraction in DECIGO using compact binary populations inferred from the first part of the LIGO-Virgo-KAGRA's fourth observation run
› Can UV meet IR in the Swiss cheese?
› Optimized numerical evolution of perturbations across sharp background trajectory turns in multifield inflation
› An Asymptotically Causal Metamodel for Neutron Star Equations of State
› Irreducible Gravitational Wave Background as a Particle Detector
› Model-Building Implications from Light Magnetic Monopoles: A Case Study of Flavour Deconstruction
› Determination of the metric of a Schwarzschild black hole surrounded by a halo of dark matter
› Photon Acceleration in Magnetized Plasma: A Mechanism for Fast Radio Bursts

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