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:

› Enhancement of the Rate of Tidal Disruption Events in Active Galactic Nuclei due to the Sweeping Secular Resonance Mechanism
› Probing heartbeat oscillations from the black hole X-ray binary GRS 1915+105 using spectral-timing analysis
› Visual Characteristics of a Rotating Black Hole in $4$D Einstein-Gauss-Bonnet Gravity with Thin Accretion Disk Under EHT Constraints
› Asteroid Mining to Sustain a Mars Colony: A Logistics Point of View
› GOALS-JWST: Resolved multi-phase molecular gas in IRAS 20551-4250 using JWST and ALMA
› Binary Evolution Can Mimic the Pair-Instability Mass Gap in Black Hole Mergers
› The KM3NeT event: a primordial high energy neutrino?
› Coupled orbital and interior structure evolution of lava planets
› Galaxies at z > 10: {\Lambda}CDM predicts increased Star Formation Efficiency
› White dwarf + M dwarf Detached Binaries in Long Period Radio Transients: Observed Binary Parameters, Evolution, and Population Constraints
› Other red dots: A possible GLIMPSE of normal AGB stars at Cosmic Noon through extreme lensing
› Extending the ALMA survey of the SCUBA-2 CLS UDS field: Tracing the obscured formation of spheroids across z~1-4
› SAETASS: Solver for Astroparticle Equation of Transport Analysis in Spherical Symmetry
› Investigating the formation channel of GW231123: Population III stars or hierarchical mergers?
› Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics
› New constraints on stellar feedback through [O III] emission: interpreting ALMA and JWST observations with SPICE simulations
› Stellar feedback SPICEs up [C II] emission in the first galaxies
› Magnetic properties of the Abell 3391-3395 system revealed using wide-field MeerKAT polarimetry
› Laser-based mass spectrometry for the detection of signatures of life within our Solar System
› Linking System of Jets to the Non-Gravitational Acceleration of 3I/ATLAS
› Machine Learning Supports Existence of Previously Unrecognized Transient Astronomical Phenomena in Historical Observatory Images
› Analysis of synthetic OVI absorption associated with galaxy groups in SIMBA and TNG50 simulations
› SAGUI: SED-based Segmentation of Multi-band Galaxy Images -- Application to JADES in GOODS-South
› Design of a mission to measure the shape and substructure of the 511 keV gamma-ray line from the center of the Milky Way
› Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
› Pulsar Selection Criteria and Performance Evaluation of Autonomous X-ray Pulsar Navigation Systems
› Testing $\Lambda$CDM versus dynamical dark energy in one year: A DESI spectroscopic follow-up program for Rubin supernovae
› Cosmic Ray Electron Evolution in Supernova Remnants: Log-Parabola Distribution
› Predicting Redshift in Seyfert Galaxies Using Machine Learning
› Stellar separation shapes spin-orbit alignment in visual binaries
› Revisiting the distance and the globular cluster system of the remarkable galaxy UDG1 in the NGC 5846 group
› Very Long Baseline Interferometry Search for Nuclear Radio Continuum Emission in the Barred Spiral Galaxy NGC 7479
› The Gamma-Ray Monitor onboard the SVOM satellite
› Estimating galactic foreground with the population of resolved galactic binaries
› Seeing at Timau National Observatory Based on ERA5 Dataset
› A comprehensive framework for phase-coherent mapping of the gravitational-wave sky with pulsar timing arrays
› What is Powering the Enigmatic He II Emitter Hebe: The First Stars or Black Holes?
› Investigation of Hourglass-shaped Magnetic fields in the G35.20-0.74 Star-Forming Complex
› A General Framework for Radial Velocity Calibration in Low-Resolution Spectroscopic Surveys: Correcting Wavelength-Dependent and Global Systematics with Application to LAMOST DR9
› A tidally detached super Neptune on a strongly misaligned retrograde orbit
› Identifying Merger-Driven and Collapsar-Driven Gamma-Ray Bursts with Precursor based Solely on Prompt Emission
› Cosmological constraints on TeV-scale dark matter subcomponents decaying between recombination and reionisation
› VLTI-GRAVITY observations of blazars
› Conceptual Design and Analysis of a NanoTug Swarm for Active Debris Removal
› Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
› The Ophiuchus DIsc Survey Employing ALMA (ODISEA). Substructures as a function of SED Class and disc mass in 100 systems
› Rapidly oscillating Ap stars observed with TESS. The LAMOST Ap sample and 49 Cam
› Merger rate of initially clustered primordial black holes for the two-body channel
› Physical Analysis of Bennu Samples Reveals Regolith Production by Collisional Disruption on Near-Earth Asteroids
› HOTDISK. Finding Massive Protostellar Disks with Water and Refractory Molecular Species
› Exploring the central region of SNR 0540-69.3 with JWST I: 3D morphology
› Model-independent consistency tests of DESI DR2 BAO and SN Ia
› IZ Tel and UW Vir: Southern oscillating eclipsing Algol systems with active mass transfer
› Oort Cloud Ecology - IV. Exchanging Asteroids
› SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy
› Do Solar Energetic Electrons cross the Heliospheric Current Sheet? - A Statistical Study
› Cosmological constraints from the small scale clustering of Emission Line Galaxies
› On combining estimated and analytic covariance matrices
› ALMA Observations of Acetone in Hot Cores
› Design and preliminary performance study of the broad-band spectrometer detector for POLAR-2
› Cosmic evolution of the [CII]-to-molecular gas relation
› The swept-back multipolar magnetic field of neutron stars: Application to NICER MSP J0030+0451
› Dynamically cold discs in high-redshift galaxies: comparison between ALMA observations and TNG50
› Characterizing and spectrally modeling embedded FUor eruptions in the near-infrared
› Nonlinear Programming of Low-Thrust Multi-Rendezvous Trajectories Using Analytical Hessian
› Are X-ray Atmospheres Heated by Turbulent Dissipation? XRISM Constraints
› MG-NECOLA: A Field-Level Emulator for $f(R)$ Gravity and Massive Neutrino Cosmologies
› A Possible Protocluster of Galaxies Serendipitously Discovered in the Field of an Intermediate-Redshift Post-starburst Galaxy
› Resolved UV-Optical HST Imaging and Spectral Energy Distribution Modeling of Nearby BAT Active Galactic Nuclei
› Is the `Known' Enough? An Integrated Machine Learning Framework for Eclipsing Binary Classification and Parameter Estimation Based on Well-Characterized Systems
› QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole
› A practical theorem on gravitational-wave background statistics
› Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology
› Viscously Stirring Particle Disks into Lorentzians and Gaussians to Infer Dynamical and Collisional Masses (ARKS XIII)
› Precision Kinematic Sunyaev--Zel'dovich Measurements Across Halo Mass and Redshift with DESI DR2 and ACT DR6: Part I. Luminous Red Galaxies
› Precision Kinematic Sunyaev--Zel'dovich Measurements Across Halo Mass and Redshift with DESI DR2 and ACT DR6: Part II. Bright Galaxy Survey and Emission-Line Galaxies
› Calibration-Induced Systematics in SALT3 Training and Their Impact on Dark Energy Constraints from Stage IV Supernova Surveys
› Inflation from a Weyl-flat null origin
› Hunting Sterile Neutrino Dark Matter in the MeV Gap
› Flavomon ray tracing in matter gradients
› System Size Dependence of Collisionless Reconnection Rate
› String-inspired Gauss-Bonnet Gravity Inflation and ACT
› Three-dimensional recoil-electron reconstruction using combined optical imaging and waveform readout for electron-tracking Compton cameras
› Understanding supernova gravitational waves with protoneutron star asteroseismology
› Mass ratio estimates for overcontact binaries using the derivatives of light curves
› Observable CMB B-modes from Cosmological Phase Transitions
› Euclid: Galaxy morphology and photometry from bulge-disc decomposition of Early Release Observations
› Sifting for a Stream: The Morphology of the $300S$ Stellar Stream
› Inflationary Fossils Beyond Perturbation Theory
› A massive and evolved slow-rotating galaxy in the early Universe
› Color dichotomy and gradients in the bulges and disks of EFIGI galaxies along the Hubble sequence
› The HST-Hyperion Survey: Environmental Imprints on the Stellar-Mass Function at z~2.5
› Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE
› Conditioning halos on the tidal environment for fast and accurate HI power spectra during reionization
› pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
› Computational advances and challenges in simulations of turbulence and star formation
› Simulating the late stages of WD-BH/NS mergers: an origin for fast X-ray transients and GRBs with periodic modulations
› Massive neutrinos and interacting dark matter look alike through the lens of lensing
› Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
› The 12CO Gas Structures of Protoplanetary Disks in the Upper Scorpius Region
› Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars
› "SNe Ia twins" in the Hubble flow, and the determination of H0
› A Robust Launching Mechanism for Freely-Floating Planets from Host Stars with Close-in Planets
› On the role of gravity, turbulence, and the magnetic field in angular momentum transfer within molecular clouds
› IRMaGiC: Extending Luminous Red Galaxy Selection into the Infrared with Joint Rubin Observatory's Large Survey of Space Time and Roman's High Latitude Imaging Survey
› Spectral response of SPHEREx
› Evolution of the transitional millisecond pulsar PSR J1023+0038 from Aqueye+ and NICER observations
› Full-Spectrum Machine Learning Diagnostics for Interstellar PAHs
› The nearby He-rich superluminous supernova SN 2021bnw at photospheric phases
› Chemo-dynamical reconstruction of Milky Way globular cluster progenitors: Age-metallicity relations and the universality of multiple stellar populations
› The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. VII. Molecular Mapping Performance with JWST/MIRI MRS: VHS 1256 b as a case study
› The demise of the synchronous moon that gave Mars its triaxiality. The role of solar tides and a palaeo ocean
› On the origin of the BAOtr-DESI tension
› Constraints on Coupled Dark Energy in the DESI Era
› The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
› Uniform Reinterpretation of Rocky Exoplanet Secondary Eclipse Observations and the Impact of Stellar and Orbital Uncertainties
› ExoNet: Multimodal Deep Learning for TESS Exoplanet Candidate Identification via Phase-Folded Light Curves, Stellar Parameters, and Multi-Head Attention Fusion
› Missing pairs in open cluster catalogs
› High-Frequency Gravitational Waves from the Galactic Pulsar Population
› Plate Sensitivity Is Invariant Across Geomagnetic Storm Intensity at Harvard and Palomar: A Protocol for Artifact Control in Historical Plate Archive Studies
› Vaulting the barrier: An intrinsic mechanism to fuel the gas beyond the nuclear ring into the central region of barred galaxies
› Two Potential Exoplanets around A-type Stars Selected from 18 Planetary Candidates
› NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations
› Collective excitations in magnetic topological insulators and axion dark matter search
› Symmetry Energy Expansion with Strange Dense Matter
› GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed
› Leptogenesis and neutrino mass with one right-handed neutrino and Higgs inflaton
› Revisiting constraints on magnetogenesis from baryon asymmetry
› Extracting Properties of Dark Dense Environments around Black Holes from Gravitational Waves
› Linking Leptogenesis and Asymmetric Dark Matter: A Testable Framework for Neutrino Mass and the Matter-Antimatter Asymmetry
› Bipartite Solution to the Lithium Problem
› Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment

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