Obserwatorium Astronomiczne na Suhorze Strona główna
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ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
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Obserwatorium Astronomiczne na Suhorze

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RSS  Najnowsze prace na astro-ph:

› The Impact of Computing Data Centres Orbiting Earth
› Mercury Craters Named after Tajik-Persian Poets: Planetary Nomenclature as a Form of Preserving Cultural Heritage
› From photometric surveys to HI intensity mapping: Improving constraints on magnification biases while testing gravity
› Declarative bespoke modelling: A new approach
› Gaia DR3 IDs for TESS Input Catalog Targets
› The CAVITY project. The spatially resolved SFR of galaxies in voids
› MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z \sim 1$ star-forming galaxies
› Numerical calculations of neutron star mountains supported by crustal lattice pressure
› Enhanced Multiphase Circumgalactic Medium and Gas Cycling in Galaxy Mergers
› Something Bright at the Edge of Everything: A Uniquely JWST-Dark Radio Source in COSMOS
› AGN Fueling and Radio Jet Evolution in the Galaxy Group NGC 5044 revealed by VLBA HI Absorption and Proper-Motion Radio Observations
› Large Dust Grains and a Possible Dust Trap in the Polar Circumbinary Disc of HD 98800B
› Formation and disruption of wide binaries in star clusters revealed by N-body simulations
› Where to Search For Life: Evidence from narrative sources with established predictive efficacy
› Survey of compact sources for pulsars and exotic objects -- I. Overview and initial discoveries
› Plan 9: Detecting Atmospheric Deterrence Against Interstellar Monsters
› From Detection to Host Galaxy Identification: Precision Continuous Gravitational Wave Localization with a Few Anchor Pulsars
› Sugar Rush: Improving Observing Productivity via Night Dessert
› JWST MIRI-MRS observations of the Red Rectangle: AIB class transformation in the outer nebula
› Hydrogen-helium immiscibility boundary in planets
› The Binary-Binary Hierarchical System XY Leo: A Laboratory for Stellar Activity and Concealed Companions
› New Paradigms in Pasta: Introducing $\mathtt{GF \ pastamarkers}$ for Enhanced Inclusivity and Productivity
› Reducing the Virgo site infrastructure noise in preparation of the O4 observing run
› On The Detection of Digiorno-like Objects in the Flavor Zone
› Protoplanetary Disk Evolution in a Low-Metallicity Environment: JWST's First Mid-Infrared Census of Low-Mass Stars
› Introducing PxP: A Population Synthesis Framework for Predicting YSO Properties
› Eccentricity constraints disfavor single-single capture in nuclear star clusters as the origin of all LIGO-Virgo-KAGRA binary black holes
› The Evolution of the Spin Alignments of Dark Matter Halos in the Cosmic Web
› AI Cosplaying as Astrophysicists: A Controlled Synthetic-Agent Study of AI-Assisted Astrophysical Research Workflows
› Late-Time HST UV Detections Reveal Eruptive Mass Loss and Circumstellar Interaction in a Quarter of Stripped-Envelope Supernovae
› AGN Disks as Supernova Mufflers I: 3D Local Hydrodynamic Models
› Pervasive Cavity-Ring Structure for Star Formation in Dwarf Irregular Galaxies
› Data-driven discovery of dynamo cycle equations
› Schr\"odinger's Seed: Purr-fect Initialization for an Impurr-fect Universe
› Nonthermal Velocity Dispersion in the Outer Disk of HL Tau
› The Evolving Faber-Jackson Relation: A Unifying Framework for Galaxy Ages and the Baryonic Tully-Fisher Connection
› Ripples of Stellar Enrichment (RoSE) -- simulating element production and mixing in the Milky Way star-by-star
› The Actinide-Boost Star LAMOST J122216.85-063345.2: A Detailed R-process Abundance Study with Gemini-S/GHOST
› Synthesis imaging with a lunar orbit array: II. Impacts of instrument-induced phase errors
› Spectroscopic orbits for three SB2s and one hierarchical triple using SALT data
› A Lower Bound on the Number of Fundamental Constants
› Spectroscopic study of the broad component of [O III]{\lambda}5007 profile in type 1 AGNs
› The Universe Favors Primes: A Study in the Primality of Cosmic Structures
› Cow-culation: Reentry Impact Risk to Livestock in the Satellite Megaconstellation Era
› Optical spectroscopy of high redshift BL Lac objects
› PAC in DESI. II. Galaxy-halo connection into the $10^{6}{\rm M}_{\odot}$ frontier
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› Constraining the Galactic bar and spiral pattern speeds with the Hyades tidal stream
› Distribution function-based modelling of discrete kinematic datasets, in application to the Milky Way nuclear star cluster
› Milky Way evolution on a human timescale
› Anomaly detection in Fink. I. Discovery, follow-up, and classification of unusual sources
› Simulating the jittering-jets explosion mechanism: circum-jet rings account for observed core-collapse supernova remnant morphologies
› Brightness, Colour, Polarisation: A Multi-Instrument Observation Campaign of the Gorizont-6 Satellite
› StarHash: unique, memorable, and deterministic names for astronomical objects
› Antimatter Propulsion for Interstellar Travel via Positron Production from Potassium-40 Rich Biological Matter
› Multi-hierarchy simulation of Riemann problem for reconnection exhausts
› Constraints on the host galaxy and AGN properties of three z > 6 JWST AGN from NOEMA observations
› Direct N-body simulations of rotating and extremely massive Population III star clusters
› STRADAViT: Towards a Foundational Model for Radio Astronomy through Self-Supervised Transfer
› First Detection of Exoplanetary Cannabinoids: Evidence for THC and CBD in the Atmosphere of K2-18b
› Robustness of cosmic void statistics: insights from SDSS DR7 and the ELUCID simulation
› New Constraints on the M Dwarf Cosmic Shoreline from a Galaxy Far, Far Away
› Accurate Determination of Chemical Abundances near a Supermassive Black Hole
› Your Outie Is a Wonderful Astronomer: Macrodata Refinement of the Astro-ph ArXiv Feed at Phermon Industries
› Dark radiation from Kerr primordial black holes: the role of superradiance
› Early intrafamily collisions in newly formed asteroid families
› Homogeneous stellar parameters for 717,807 TESS FGK stars using Gaia DR3
› The SPHEREx Instrument: Calibration, testing and performance measurements of the NIR 2 spectroscopic surveyor from the laboratory to in-orbit commissioning
› Seeding grain nucleation and dust growth: Ionisation, epoxidation and charge disproportionation effects
› CROCS Data Release I: Constraints on the Hubble Constant
› Cloudy With a Chance of Meatballs
› A multi-scale molecular and atomic gas view on the HII region N113 in the Large Magellanic Cloud:Evidence for high-mass star formation triggered by supersonically-colliding HI flows
› Galactic Constellations in DESI DR1 and the Scales of Cosmological Homogeneity
› Do Papers with Titles Ending in a Question Mark Usually Have the Answer "No"?
› Constraining Lyman-Werner Feedback from Velocity Acoustic Oscillations in the Cosmic Dawn 21 cm Signal
› A Therapy Session with Sgr A*
› The Hollyfeld Gambit in Astrophysics
› Enabling fundamental understanding of Nature with novel binning methods for 2D histograms
› An inverted infall profile for the collapse of the massive star-forming IRDC SDC335.579-0.292
› The WEAVE acquisition and guiding software: pattern recognition-based acquisition and multi-fibre guiding
› Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run
› Filippov Sliding Dynamics of Cosmic Dust Atmospheric Entry: Survival Boundaries, Asymptotic Mass Loss, and Inverse Problem Limits
› Rotation of the polarization plane in axion fields: application to neutron star polar cap regions
› Boltzmann Equation Solver for Thermalization
› Quasi-linear theory of fast flavor instabilities in homogeneous environments
› Neutrinos as Dark Matter
› The Depletion of Collisionless Dark Matter Spikes
› Misalignment from kicks: the impact of particle interactions on ultra-light dark matter
› Constraining The Neutrino-Nucleon Cross Section with the Ultrahigh-Energy KM3NeT Event
› Fermion scattering in a Bose-Einstein condensate
› Baryogenesis from Exploding Primordial Black Holes
› No hair but plenty of feathers: are birds black holes?
› Lots of Shade on Satellite Constellations
› Revisiting the Coprecessing Frame in the Presence of Orbital Eccentricity
› Mexican Burrowing Toads as gravitational wave detectors
› Gravitational waves from gaps of neutron stars
› Tidal deformations of general-relativistic multifluid compact stars
› Revisiting QCD-induced little inflation with chiral density wave state and its implications on pulsar timing array gravitational-wave signals
› Conventional and Unitarity-Conserving Pecci-Quinn Inflation Models and ACT
› Warm Warped Throats
› The Instrumented Baffle at the Input Mode Cleaner of Advanced Virgo Plus: Four years of Successful Operation as a Monitor of Stray Light
› What does the Universe sound like?
› The Hubble Constant from Blue Type Ia Supernovae
› A 44-minute periodic radio transient in a supernova remnant
› Origin of the lunar inclination from tidal interaction of multiple-moon system
› Euclid Quick Data Release (Q1). The first Euclid view of Planck galaxy protocluster candidates at cosmic noon
› The Growth of Dust in Galaxies in the First Billion Years with Applications to Blue Monsters
› Probing spectral variability in NGC 4490 ULX-8 over 24 years of XMM-Newton, Chandra and Swift-XRT observations
› Simulation budgeting for hybrid effective field theories
› Conversion and Damping of Nonaxisymmetric Internal Gravity Waves in Magnetized Stellar Cores
› Event types in H.E.S.S.: a combined analysis for different telescope types and energy ranges
› Exploring Ultra-Slow-Roll Inflation in Composite Pseudo-Nambu-Goldstone Boson Models: Implications for Primordial Black Holes and Gravitational Waves
› Explodability matters: how realistic neutrino-driven explosions change explosive nucleosynthesis yields
› CAZ catalog and optical light curves of 7918 blazar-selected active galactic nuclei
› Association of the IceCube neutrinos with CAZ blazar light curves
› Exploring the Co-SIMP dark matter model using the 21-cm signal from the dark ages
› Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
› Dynamics of Streamers and Pseudostreamers and Implications for the Solar Wind
› Trapped fireshell (halo) of photons and pairs around black-hole horizon: source for ultra-high-energy particles
› The influence of Parker spiral on the reflection-driven turbulence
› Tracing nitrogen enrichment across cosmic time with JWST
› Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
› New CDM Crisis Revealed by Multi-Scale Cluster Lensing
› Simultaneous determination of Hubble constant and cosmic baryon density: Forecasts for the synergy between FRBs and emerging probes
› Rate of Repeating Tidal Disruption Events with 5--19 years interval
› Discovery of an Extremely Metal-Poor Galaxy at $z=3.654$ Using JWST Infrared Spectroscopy
› X-Ray Analysis of an Off-Axis Merger Stage Binary Galaxy Cluster: PSZ2 G279.79+39.09
› Gravitational-Wave Signals for Supernova Explosions of Three-Dimensional Progenitors
› An updated constraint for the Gravitational Wave Background from the Gamma-ray Pulsar Timing Array
› Optical Spectroscopy of Dwarf Galaxies at $z\sim 0.15$ in the COSMOS Field: Star Formation and Dust Properties
› Are supernovae driving turbulence in the solar neighborhood?
› Pulsar timing arrays: the emerging gravitational-wave landscape
› Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant
› Evolution of the early-type fraction in massive galaxies at $z
› Derivation of the injection spectrum of positrons and electrons from Geminga and Monogem
› ROLLIN': Rotating globular cluster simulations. I. The kinematic evolution of realistic direct N-body models
› Turning JWST/MIRI backgrounds into a survey of diffuse molecular hydrogen
› Avoiding recollapse in an open-AdS Universe via a self-tuning-like mechanism
› Supermassive black hole formation in the initial collapse of axion dark matter
› Earliest Structures in the Universe can be explained by a Relativistic Cosmological Perturbation Theory
› NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration
› Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model
› Dark graviton sensing with magnetically levitated superconductors

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