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Obserwatorium Astronomiczne na Suhorze

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Kamerka N

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65%
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Księżyc
Najnowsze prace na astro-ph:
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Mosaic: Area-Closed Spherical Surface Mosaics Induced by Cartesian Grids ›
Polarization Birefringence and Waveform Systematics in GW231123 ›
Expected redshift drift for tilted observers ›
The limits of feedback from active galactic nuclei ›
Halo-driven Origin and Suppression of Over-massive Black Holes and Little Red Dots ›
The pair-instability origin of supernova 2023vbw ›
Thermostats, Not Engines: A New Picture of Halo Gas Regulation ›
The interaction phase of engine-driven explosions and high-energy winds ›
Spinning out of focus: The challenge of rotational line broadening in exoplanet reflection spectroscopy ›
Hot DQs, magnetic and metal-polluted white dwarfs: spectroscopic insights from a Gaia machine-learning-selected 500 pc sample ›
A 14-year-old Mystery: The Peculiar Case of the Engine-driven SN 2012ap ›
Stellar encounters in the solar neighbourhood and the special case of GJ~710 ›
Searching for the Third Wheel: High-Contrast Imaging Constraints on Tertiaries to Black Hole and Neutron Star Binaries ›
A Revised Mass and Period for the Habitable Zone super-Earth GJ 3378b: A Planet Straddling the Cosmic Shoreline ›
Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31 ›
Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae ›
Feedback driven interactions between dark and luminous matter to explain tight galaxy scaling relations ›
Is the Binary Black Hole Population Inference from Gravitational-Wave Data Robust? ›
Modeling the probability distribution for cosmological analysis with photometrically classified samples ›
SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints ›
Probing the Mass-loss Histories of Type IIn and II-L Supernovae with Late-time Radio Observations ›
The EDGES Analysis Pipeline: Description and Validation ›
The bound origin of low-mass stellar binaries ›
The Torques Acting on Accreting Millisecond X-Ray Pulsars in the Outburst and Quiescent States, and During the Long-Term Evolution ›
The First Remotely Detected Biosignature May Not Be the Most Common: Implications for JWST and HWO ›
Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures ›
A Rare Population of Intermediate-mass Helium Stars Between Hot Subdwarfs and Wolf-Rayet Stars ›
Extracting redshifts from 2D slitless spectroscopic images using deep learning for the CSST galaxy survey ›
XRISM detection of the 6.4 keV Fe K$\alpha$ line in the radio galaxy Cygnus A ›
Simulation study of the cosmic ray Sun shadow with a time-dependent solar magnetic field model ›
SN 2023dbc in M108: Optical and Near-Infrared Observations of a Highly-Obscured, Moderately Energetic Stripped-Envelope Supernova ›
The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky ›
Magnetised CGM Gas at z~1 revealed by SPICE-RACS ›
Circular polarization of the cosmic microwave background induced by the optical Magnus effect on gravitational lensing ›
Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison ›
Red novae, their progenitors, and remnants ›
The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud ›
PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes ›
Nonlinear electrodynamics in magnetars: systematic effects on radius constraints and timing analysis ›
Systematic KMTNet Planetary Anomaly Search. XIII. Complete Sample of 2021 Prime Field Planets ›
Jet-Structure Imprint on the Curvature Tail of Gamma-Ray Burst Prompt Emission ›
A Framework for Applying the Loeb-Turner $\alpha$-Slope Test to Archival Photometry of Trans-Neptunian Objects ›
On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows ›
Constraints on Self-Interacting Fuzzy Dark Matter from the Stellar Kinematics of the Dwarf Galaxy Leo II ›
Identifying observable MeV lines from the decays of weak and main $r$-process isotopes in mergers ›
HI Observations of Baryon-Dominated Dwarf Galaxy Candidates ›
A growth of early superhump: Multi color observation of the WZ Sge star TCP J23580961+5502508 ›
Radio Emission from Fast Blue Optical Transients Powered by Trans-relativistic Shocks in Confined Circumstellar Material ›
Understanding corona and disk evolution in black hole X-ray binaries through a comprehensive study of their broadband variability and QPO characteristics ›
The Deep Learning-Based Dual-Branch Multimodal Fusion Model for Solar Flare Prediction ›
From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system ›
Precise and Rapid Parameter Inference of Kilonova with Conditional Variational Autoencoder ›
Exploring the Transitional Parameter Space of Blazars using Gamma-ray and X-ray Population Diagnostics ›
Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO ›
Stellar Density Classification and Regression for CSST Multi-color Imaging Using Deep Learning ›
Accretion geometry and spectral evolution in 1A 1118-61: a comparison of the 2009 and 2026 outbursts ›
GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States ›
Accelerating Redshift-Conditioned Galaxy Image Synthesis with One-step Generative Modeling ›
Population synthesis of active galactic nuclei based on the radiation-regulated unification model ›
Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers ›
Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87 ›
Four-Body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source ›
'Unacceptable to our people': Diverse cultural beliefs, Indigenous rights, and the future of human activities on the Moon ›
BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW ›
Classification of IGR J20084+3221 as an Intermediate Polar using X-ray and Optical Observations ›
Coupled quintessence with a potential from supergravity exhibits sign-changing interaction ›
The First Insights into an Ultraluminous X-ray Pulsar with XRISM: Phase-Resolved High-Resolution Spectroscopy of the Fe K-shell Band of M82 X-2 ›
A Hycean Interpretation of K2-18b Supported by Photochemical Atmospheric Compositional ›
Assessing the Impact of Source Confusion for GREX-PLUS based on Deep JWST NIRCam Imaging ›
Impact of Satellite Constellations on Observations with the 80-cm Telescope and the Mini-SiTian at the Xinglong Observatory, NAOC ›
Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries ›
Nuclear Activity and Host Galaxy Properties of Low-Luminosity AGN Identified from VLA Observations ›
Search for the Highest-energy Quasiperiodic Oscillation in the Black Hole X-Ray Binary Candidate Swift J1727.8-1613 ›
Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties ›
Spectral energy-loss bump and $\gamma$-ray pulsar halos ›
Anisotropic Ejecta from Binary Neutron Star Mergers: Self-Consistent Main Thermal and Late-Time Radio Emission of NS-Powered Kilonovae ›
Inferring stellar metallicity and elemental abundances from kinematic and spectroscopic data using machine learning -- Implications for exoplanet host stars ›
Testing the reliability of magnetic field strength measurements for M dwarfs ›
SDSS-V: Revealing a weak accretion state in X-ray selected red quasars ›
Gravitational lensing time delay beyond the Shapiro/geometry split ›
Photometric classification of quasars from DES and photo-$z$ estimation with Machine Learning ›
Wolf-Rayet stellar evolution models with improved treatment of the atmosphere ›
Quadratic Dark Energy Phase-Space Dynamics and Analysis ›
Sub-stellar Strange Quark Matter Objects: Predicting a New Class of Highly-Compact Candidates ›
FastChem 4: New chemical elements and improved convergence behaviour ›
Two kinds of Galactic source populations could explain the cosmic-ray observation up to the "knee" region ›
Polarization Observations of a Sample of 6.7 GHz Methanol Masers ›
Sungrazer comets as analogs of star-planet magnetic interactions ›
Constraining the magnetic field strength of a flaring radio core in the compact steep spectrum source 3C 138 ›
Primary gravitational waves at high frequencies II: Emergence of the exponential cut-off in the power spectrum ›
Discovery of variable polarization in H$\alpha$ profile of symbiotic star Y Gem: A case for orbital-phase dependent variation of Raman-scattered Ly$\beta$ emission ›
Probing Reionization up to the Mark: The Marked Power Spectrum to unveil the HI 21-cm signal from the EoR ›
A Three-Dimensional Exploration of Magnetic Fields, Rotation, and Shock Revival in a $39 M_\odot$ Core-Collapse Supernova Progenitor ›
A fast tree algorithm for multi-component coagulation equation ›
7DT Insight: Variability in Young Stellar Objects ›
Iron line diagnostics of the stellar wind in X1908+075 ›
Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH line mapping along the Orion BN/KL explosive outflow and irradiated shocks ›
(An)Isotropy in Pantheon+ and Type Ia supernova samples: intrinsic limits of directional tests ›
Datacubes of H$\alpha$, CaII K, CaII H and H$\epsilon$ line profiles of the full solar disk recorded daily at Meudon observatory since 2017 and some typical profiles of solar features ›
A 4200-hour HyperFlash and \'ECLAT campaign on the hyperactive FRB 20240114A: constraining energetics with the most brilliant bursts ›
Towards the Deployment of the First NectarCAM, a Medium-Sized-Telescope Camera for the Cherenkov Telescope Array Observatory ›
Primordial power spectrum reconstructions from BOSS + eBOSS ›
Faster CMB lensing with control variates ›
CCD () photometry of the open cluster NGC 6793 and its dynamical evolution ›
The Wide Field Imager (WFI) Instruments for the Polarimeter to Unify the Corona and Helliosphere (PUNCH) ›
Recoupled Dark Radiation reconciling CMB and DESI BAO measurements ›
WaveDriver: a Laser Guide Star AO System for HWO ›
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 ›
A universal framework to identify eccentric binary mergers: GW200105 case study ›
Modifications of CMB Temperature and Polarization Quadrupole Signals in Thurston Spacetimes ›
Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems ›
Particle Dynamics, Shadow and Hawking Sparsity of a Kalb-Ramond Black Hole Coupled to Nonlinear Electrodynamics ›
Freeze-in Warm Dark Matter via Dimension-6 Operators in 3-3-1 Models ›
StAD: Stein Amortized Divergence for Fast Likelihoods with Diffusion and Flow ›
Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories ›
Bidirectional Internal Squeezing for Gravitational-Wave Detectors ›
Constraints on non-canonical chaotic inflation from ACT DR6 and BICEP/Keck data ›
Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds ›
Warm inflation in Weyl geometric gravity ›
Direct On-Wafer Measurements of Noise Parameters in C- and X-bands at $T=4$ K ›
A reversed solar illumination dependence of unintended emission from Starlink Direct-to-Cell satellites at 72-234 MHz with the EDA2 ›
An EFT Map of Axion Dark Radiation from Reheating ›
Impact of the axion-like self-interactions in gravitational atoms for LISA ›
Positive Running of the Spectral Index for Scalar Theory and Modified Gravity ›
Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies ›
Proton-to-Alpha Branching Ratio in the $^{12}$C+$^{12}$C fusion reaction at Astrophysical Energies ›
The impact of seasonality over the sensitivity of Einstein Telescope and the SNR of CBC signals at the Sardinia candidate site ›
Cosmological perturbations of TDiff fields ›
Probing (sub-)solar-mass black holes and superspinars with current and next-generation gravitational-wave observatories ›
Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties ›
Self-Supervised Conformal Prediction with Equivariant Bootstrapping for Image Uncertainty Quantification ›
Traditional statistical representations outperform generative AI in identifying expert peer reviewers ›
Modelling DSA, FAST and CRAFT surveys in a z-DM analysis and constraining a minimum FRB energy ›
Globular cluster distributions as a dynamical probe of dark matter ›
Constraints on primordial non-Gaussianity from Quaia ›
Method for testing diffusive shock acceleration and diffusion propagation of 1-100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula ›
SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI ›
Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe ›
Extracting latent representations from X-ray spectra. Classification, regression, and accretion signatures of Chandra sources ›
Multi-species Dark Matter with Warmth and Randomness ›
FLAMINGO: Tracing the co-evolution of hot gas and black holes in galaxy groups and clusters ›
A Census of Double-Peaked Lyman-alpha Emitters in MAGPI: Classification, Global Characteristics, and Spatially Resolved Properties ›
Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates ›
Observing Orbital Decay in the Ultracompact Hot Subdwarf Binary System ZTFJ213056.71+442046.5 ›
SE3D: Testing the recovery of stellar population, dust and structural properties on mock-observed toy model and simulated galaxies ›
SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars ›
Non-Gaussianity in SMICA ›
The Shear-to-Cosmology Paradigm I. Hybrid Field-Level and Simulation-Based Framework for Weak Lensing Surveys ›
Stellar feedback drives the baryon deficiency in low-mass galaxies ›
Measurements of quasar proximity zones with the Ly$\alpha$ forest of DESI Y1 quasars ›
The GRB Intrinsic Duration Distribution: Progenitor Insights Across Cosmic Time ›
The Contribution of Stars, Dust, Neutral Gas and SMBHs in Galaxies to the Cosmic Baryon Inventory ›
proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope ›
The Nulling Interferometry Cryogenic Experiment (NICE): Architecture, requirements, and preliminary warm precursor results ›
Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes ›
Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework ›
Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem ›
Pure Natural Inflation Passes the ACT ›
Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins ›
The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation ›
Variable ADAF disk as the origin of Changing-Look AGN ›
Solar Extreme Ultraviolet Spectrograph and High-energy Imager (SEUSHI): Design, Development, and Pre-Flight Calibration ›
Hot blue progenitors of stellar-mass black holes ›
Stellar Coronal Mass Ejections with HWO: A Science Case Concept ›
JWST Exoplanetary Worlds and Elemental Survey (JEWELS) II: Condensation Temperature Trends and Galactic Chemical Evolution in JWST Planet-Hosting Stars ›
Status of the COSmological Microwave Observations CALibrator ›
Ellipsoidal modulation and multi-wavelength activity in the pre-cataclysmic binary RX J1553.0+4457 ›
Chromosphere of the quiet sun: II. Atmospheric response to small-scale magnetic flux emergence ›
Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling ›
Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications ›
Exploring Enceladus's Interior Structure Using Electromagnetic Induction ›
On the residual missing mass of the Bullet Cluster ›
Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles ›
Photometric determination of the mass accretion rates of pre-main sequence stars. IX. Recent star formation in the periphery of NGC 346 ›
Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves ›
Dynamical Evolution of V-Shaped Collision Debris ›
Improving Slow-Roll Estimates in Starobinsky Inflation Using Analytic Hubble Parameter ›
Testing the consistency of gravitational waves and large scale structure constraints on dark energy ›
False Vacuum Decay across the Quantum-to-Thermal Crossover: A Comparison of Real-Time Observables ›
U-spin symmetry energy and hyperon puzzle ›
Low-frequency radio telescopes sensitivity to light dark matter ›
The effects of dark energy on the matter-gravity coupling ›
Cosmographic Connection Between Cosmological And Planck Scales: The Barrow-Tsallis Entropy ›
Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective ›
Time-of-Flight Constraints on Neutrino Millicharge from Supernova Neutrinos in Galactic Magnetic Fields ›
A study on Dusty Plasma Physics and the examination of Jeans Criteria for the Milky Way ↓↑