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Obserwatorium Astronomiczne na Suhorze

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Księżyc
Najnowsze prace na astro-ph:
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Particle acceleration to PeV energies in Pulsar Wind Nebula: a two zone model ›
Stellar engines and Dyson bubbles can be stable ›
Spacetime in motion: an evolving relativistic binary black hole metric for GIZMO ›
Quasi-periodic Eruptions from Stellar-mass Black Holes Impacting Accretion Disks in Galactic Nuclei ›
Long-term Spectroscopic Survey of the Hyades Cluster: The Binary Population ›
The Baryon Budget of Galaxies across the First Billion Years -- Theoretical Predictions for Gas Phases, Depletion Times, and Stellar Return Fractions ›
Calibrating Eruptive Mass Loss in Red Supergiants with Local Group Data ›
GA-NIFS: Dissecting The Alchemised: NIRSpec/IFU reveals turbulent gas inflows in a complex system at $z=10.17$ ›
Constraining the synchrotron peak and estimating the VHE brightness of a sample of extreme high synchrotron peak blazars ›
Variance of gravitational-wave populations ›
Spectroscopic follow-up of hot subdwarf variables found in ZTF -- Atmospheric and fundamental properties of radial-mode sdB pulsators ›
Small hosts, big appetites: unveiling rapid and early low-mass black hole growth in cosmological zoom-in simulations of dwarf galaxies ›
The Star Formation History of WLM from Asymptotic Giant Branch Stars and The Discovery of a Possible Accreted System in its Outer Disk ›
Halving and Doubling: Boosting the Detection of Relativistic Effects in the Galaxy Bispectrum with Optimal Subsample Selection ›
SIMPLIFI-Study of Interstellar Magnetic Polarization: A Legacy Investigation of Filaments. II. Enhancement of grain alignment near embedded protostars in the DR21 Ridge ›
HST view of NGC 5044: Constraints on Filament Widths, Magnetic Support, Multiphase Structure, and Comparison with Cluster Environments ›
${}^{12}$CO Ro-vibrational Spectroscopy of AB Aurigae -- A Potential Point Source is Present ›
A dynamical attractor in the evolution of dwarf spheroidal galaxies ›
AT 2024ahzi: A Type IIP Supernova Discovered by the LSST Commissioning Camera ›
EMBERS I: Low redshift post-starburst galaxies are frequently depleted in molecular gas relative to star forming progenitors ›
Upper Limits on Pulsed Radio Emission from Unseen Compact Objects in Six Galactic Stellar Binaries ›
Giant radio pulses in the magnetar XTE J1810-197 detected with the IAR's telescopes ›
Comprehensive MHD modelling of ten successive CMEs driving a historic geomagnetic storm -- The 2024 Mothers Day event ›
FRB scattering statistics through the CGM are sensitive to morphology and intermittency ›
A Comprehensive Diffuse Neutrino Search Using the Full Askaryan Radio Array ›
Fast Radio Bursts in the Era of the Vera C. Rubin Observatory's Legacy Survey of Space and Time ›
Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience ›
TOI-1080 b: a temperate, rocky planet orbiting a quiet M4V host ›
Rotation Period of C/2006 P1 (McNaught) Through Morphological Analysis with Narrowband Imaging ›
Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin-Velocity Alignment ›
Terraforming Mars: Mass, Forcing, and Industrial Throughput Constraints ›
A Particle Detector Array deployed to the Murchison Widefield Array in the Murchison Radio-astronomy Observatory ›
Accretion history dependence of the halo depletion radius ›
Identifying and distinguishing quenching galaxies with spatially resolved star formation in TNG50 ›
2024 YR4: Identification of Possible Precoveries in 2016 IPTF Data ›
Detection and classification of astronomical sources with Astro-RetinaNet in crowded stellar fields ›
Parameterizations of the Hubble Constant: Logarithmic vs Power-Law Expansion from the Binned Master Sample of SNe Ia ›
Electron-positron Pair Production in Global GRMHD Simulations of Black Hole Accretion Flows ›
Constraining the neutral hydrogen fraction during reionization: Cross-simulation inference using power spectrum and bispectrum ›
Planetary Desert around Compact Binaries: Dynamical Instability Triggered by Resonance-Induced Eccentricity Excitation ›
First Sardinia Radio Telescope detection of the Sunyaev-Zel'dovich effect at 18.6 GHz ›
A generalized dipole-segment model for the gravitational field of elongated bodies ›
Deep learning-based astronomical multimodal data fusion: A comprehensive review ›
High-resolution observations of small-scale activity in coronal hole plumes ›
Systematic and Statistical Uncertainties in the Non-Gravitational Acceleration of 3I/ATLAS ›
Comparing dynamical effects of the central bar and the spiral arms in the solar neighborhood ›
High-Energy Shock Breakout from Supernovae and Gamma-ray Bursts ›
Third order correlations and skewness in convection. I. A new approach suitable for three-equation non-local models ›
Accretion Geometry of Black Hole X-ray Binaries: Insights from X-ray Observations ›
ALMA Central molecular zone Exploration Survey (ACES) V: CS(2-1), SO(2_3-1_2), CH3CHO(5_1,4-4_1,3), HC3N(11-10), and H40a lines data ›
New axion bounds derived from the 100-parsec Gaia DR3 white dwarf luminosity function ›
Stability and wave dynamics in polytropic Eddington-inspired Born-Infeld gravitating solar plasmas ›
Rotational Doppler Cartography of Technosignatures on Unresolved Planets ›
oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph ›
Kinematic and dynamics of the galaxy ESO 358-60 ›
Accretion in Binary Systems with Slow Stellar Winds ›
X-ray and H{\alpha} superflare on an RS CVn-type star, UX Arietis: Constraint on the flare location from radial velocity change during the flare ›
The effect of photon re-scattering due to cosmic reionization on 21-cm images and power spectra ›
Outflow from unmagnetized shocked radiative transonic accretion disk around a black hole ›
The UTR-2 decametre pulsar and transient survey I. Transient detection ›
TESS Hunt for Young and Maturing Exoplanets (THYME) XIV: A Comoving-Based Age Constraint for KELT-20 ›
The impact of strong lensing on Hubble constant measurements with gravitational-wave dark sirens ›
Protostellar Outflows Shed Light on the Dominant Close Companion Star Formation Pathways ›
ALMA High-J CO Spectroscopy of High-Redshift Galaxies. II. 0.03" Resolution CO Kinematics Reveal Super-Eddington Accretion in a Dust-Obscured Galaxy at z=3.111 ›
Everything Every Band All at Once II: The Relationship Between Optical Size and Stellar Mass Over Eight Billion Years of Cosmic History ›
Time-Domain Photometry and Activity Evolution of Interstellar Comet 3I/ATLAS with BHTOM ›
Identifying Compton-thick AGNs in the COSMOS II. Among mid-infrared selected AGNs ›
PhysFormer: A Physics-Embedded Generative Model for Physically Self-Consistent Spectral Synthesis ›
Two Lyman Continuum Escape Mechanisms at Play in $z\sim0.3$ galaxies Revealed by Infrared Observations ›
Local Analogs of Little Red Dots: Optical Variability and Evidence for an AGN Origin ›
LCEz4-M1: A Lyman Continuum Emitter Candidate at z = 4.444 in the MUSE Hubble Ultra Deep Field ›
CosmicWeb-21cm array: A New Radio Observation Array Design for 21cm Cosmology ›
Role of Domain Walls in the Early Universe in the Context of Mode Matching ›
The Intrinsic Multiplicity Distribution of Exoplanets Revealed from the Radial Velocity Method. II. Constraints on Giant Planet Multiplicity from Different Surveys ›
Modelling the long-term impacts of artificial warming on the Martian water cycle and surface ice distribution ›
Superfluid Vortex Lines-Magnetic Flux Tubes Interaction and Braking Indices of Pulsars ›
SPACE-Timers -- A Stack-Based Hierarchical Timing System for C++ ›
Episode-wise spectro-polarimetry of GRB 220107A: Testing the hypothesis of evolving radiation mechanisms ›
A Unified Explanation for JWST Little Red Dots and High-Redshift Low-Mass Disk-like Galaxies: Prolate Galaxies Viewed End-on vs Side-on ›
Planet-forming disks and their environment across regions and time from the full NIR census ›
The Galaxy Stellar Mass-SFR-Size Relation in EAGLE, TNG100, and Observations ›
KMT-2025-BLG-1314 and KMT-2025-BLG-1392: two microlensing planetary/brown-dwarf candidates analyzed with differentiable code ›
Testing the isothermal Jeans model for self-interacting dark matter halos in the collapse phase ›
Quantification of Tides in Giant Planets from Observations ›
A universal brown dwarf desert formed between planets and stars ›
Triaxial Schwarzschild Models of Brightest Cluster Galaxies with Long-Slit LBT Data ›
Observational insights into Sr I 4607 \AA\ scattering polarization with DKIST/ViSP ›
Predicting the Peak Energy of Swift Gamma-Ray Bursts Using Supervised Machine Learning ›
A z$\sim$1 galactic-scale outflow transversally mapped to $\sim$50 kpc through gravitational-arc tomography ›
A data-driven estimate of the protosolar helium mass fraction ›
B-fields And dust in interstelLar fiLAments using Dust POLarization (BALLAD-POL): VI. Grain alignment mechanisms in the massive quiescent filament G16.96+0.27 using dust polarization observations from JCMT/POL-2 ›
A New Identification Method and Sample of Counter-Rotating Disk Galaxies in SDSS-IV MaNGA DR17 ›
Current and future constraints on the expansion history of the GREA model ›
Large scale mapping of [CI] and the [CI]-to-CO transition in $\rho$ Ophiuchus molecular cloud ›
Cancellation of loop corrections to soft scalar power spectrum ›
Halo Occupation Distribution estimation performance for LSST data ›
Core-envelope coupling of gravito-inertial waves in pre-main-sequence solar-type stars ›
Systematic errors in spectral measurements with the Tenerife Microwave Spectrometer ›
Photometric Modulations on Intermediate Timescales in the Symbiotic Binaries ›
Radio Study of Vela X Cocoon ›
The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Constraints on disk turbulence, fragmentation velocity, and inner pebble fluxes ›
The statistical properties of the cross spectrum ›
A Template-Based Search for Large-Scale-Structure--Correlated Anisotropy in the Nanohertz Gravitational-Wave Background Using the Public NANOGrav 15-Year Data Set ›
Low-$T/|W|$ instabilities in differentially rotating neutron stars resembling merger remnants ›
Interpreting map-based $E$/$B$ spectral properties of CMB foregrounds ›
Predicting Gaia astrometry's ability to constrain the populations of circumbinary planets ›
Ground-based Atmospheric Characterization of Super-Earth L 98-59 d at High Spectral Resolution ›
Reconciling 3D Models for the Central 10 parsecs of the Milky Way ›
Flavor-changing axions and Dirac neutrino masses ›
Dark matter as the source of neutrino mass: theory overview and experimental prospects ›
SunBURST: Deterministic GPU-Accelerated Bayesian Evidence via Mode-Centric Laplace Integration ›
Cosmological and Astrophysical Constraints on Late First-Order Phase Transitions ›
A Unified Interpretation of Supernova, GRB, and QSO Time Dilation Signals in a Generalized Cosmological Time Framework ›
Minisuperspace Cosmology in Extended Geometric Trinity of Gravity ›
To Verify Frame-Dragging: The Asymmetric Response of LARES 2 and LAGEOS to Tidal Perturbations ›
Non-Minimal Dilaton Inflation from the Effective Gluodynamics ›
Evgeny P. Velikhov (1935-2024) ›
Turbulent Heating between 0.2 and 1 au: A Numerical Study ›
Rugged magneto-hydrodynamic invariants in weakly collisional plasma turbulence: Two-dimensional hybrid simulation results ›
A Hybrid Particle Gaussian Mixture Filtering Method for Cislunar Orbit Determination Under Extreme Uncertainty ›
Modified Teukolsky formalism: Null testing and numerical benchmarking ›
$\mathcal{H}$-EFTCAMB: A Cobaya-Integrated, Python-Wrapped Extension of EFTCAMB for Covariant Horndeski Gravity ›
ImpCresst -- A versatile simulation tool focusing on solid-state detectors at keV energies ›
Hadronic description of nuclear matter and neutron star properties ›
Inflation (2025) ›
An Agnostic Biosignature Based on Modeling Panspermia and Terraforming ›
Curvature Mapping Method: Mapping Lorentz Force in Orion A ›
Planetary Nebulae ›
ELLIPSECT: A surface brightness analysis tool for GALFIT 3 ›
Cloud-scale gas properties, depletion times, and star formation efficiency per free-fall time in PHANGS--ALMA ›
A possible wave-optical effect in lensed FRBs ›
The Quintom theory of dark energy after DESI DR2 ›
Probing Ultralight Axion-like Dark Matter: A Pulsar Timing Arrays-Pulsar Polarization Arrays Synergy ›
SpiralMap: A Python library of the Milky Way's spiral arms ›
Inflationary attractors and radiative corrections in light of ACT data ›
A Ground-Based Transit Observation of the Long-Period Extremely Low-Density Planet HIP 41378 f ›
The Double-Episode Jet Genesis of the eROSITA and Fermi Bubbles ›
Ultraviolet photon production rates of the first stars: Impact on the He II $\lambda$ 1640 \AA{} emission line from primordial star clusters and the 21-cm signal from cosmic dawn ›
Stringent constraint on the CCC+TL cosmology with $H(z)$ Measurements ›
Observational challenges to holographic and Ricci dark energy paradigms: Insights from ACT DR6 and DESI DR2 ›
The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions ›
A preliminary orbit for the satellite of dwarf planet (136472) Makemake ›
Extracting the Alcock-Paczynski signal from voids: A novel approach via reconstruction ›
Equilibrium Points and Surface Dynamics About Comet 67P/Churyumov-Gerasimenko ›
Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Lens model comparison and H0 measurement ›
Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6 ›
The 21cm-galaxy cross-correlation: Realistic forecast for 21cm signal detection and reionisation constraints ›
Evidence of magnetospheric vacuum birefringence in the polarized X-rays of a radio magnetar ›
CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy. V. Chemical composition gradients as a function of the galactocentric radius ›
4MOST Cosmology Redshift Survey (CRS): Clustering Properties of CRS Bright Galaxy and Luminous Red Galaxy Target Catalogues ›
Probing departures from $\Lambda$CDM by late-time datasets ›
Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization ›
Revisiting Very High Energy Gamma-Ray Absorption in Cosmic Propagation under the Combined Effects of Axion-Like Particles and Lorentz Invariance Violation ›
Eclipsed X-ray Bursts from Magnetar SGR J1935+2154 and the Fireball Measurements ›
Equation-of-state-informed pulse profile modeling ›
Gravitational wave standard sirens from GWTC-3 combined with DESI DR2 and DESY5: A late-universe probe of the Hubble constant and dark energy ›
How Bright in Gravitational Waves are Millisecond Pulsars for the Galactic Center GeV Gamma-Ray Excess? A Systematic Study and Implications for Dark Matter ›
How Primordial Black Holes Change BBN ›
Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data ›
GRB 230204B: GIT Discovery of a Fast Fading Afterglow Associated with an Energetic GRB from a Massive-Star Progenitor ›
The Nuclear Star Cluster of M 74: a fossil record of the very early stages of a star-forming galaxy ›
Hot Jupiters are Inflated Primarily by Shallow Heating ›
The excess of molecular hydrogen in chemical networks without oxygen ›
Validating the CROCODILE model within the AGORA galaxy simulation framework ›
Dynamical Dark Energy models in light of the latest observations ›
Simultaneous JWST, NuSTAR, and VLA Monitoring of Sgr A*: A Unified Picture of the Variable IR, X-ray and Radio Emission ›
Unveiling SN 2022eyw: A Bright Member of the Type Iax Supernova Subclass ›
Protonic thermoelectric effect of Superionic H2O and magnetic field generation in Uranus and Neptune ›
Jet launching from the Kerr black hole magnetosphere: An electrogeodesic approach ›
A COLIBRI Photometric Study of SN 2025bvm: A Normal, Slowly Declining Type Ia Supernova ›
Constraining the Fraction of LIGO/Virgo/KAGRA Binary Black Hole Merger Events Associated with Active Galactic Nucleus Flares ›
A new magnitude--redshift relation based on Type Ia supernovae ›
ALMA Polarization Study of the Magnetic Fields in Two Massive Clumps in the 20 km s$^{-1}$ Cloud of the Central Molecular Zone ›
Properties and Possible Physical Origins of $\gamma$-ray Emission in Extreme Synchrotron Blazars ›
Cosmological analysis of a viable $f(R)$ gravity model ›
Reversal of Spin: Comet 41P/Tuttle-Giacobini-Kresak ›
Reevaluating thermal instability in a uniform plasma: an extended analysis of instability domains ›
High significance detection at 4.8 GHz of the radio halo in the Coma galaxy cluster with the Sardinia Radio Telescope ›
Astrometric properties of reference frame sources as a function of redshift ›
Surface Properties, Orbital Dynamics, and Thermophysical Modeling of the Primitive Asteroid (269) Justitia ›
Short-duration GRB 250221A Afterglow Driven by Two-Component Jets from the merger of a compact star ›
pythonradex: a fast Python re-implementation of RADEX with extended functionality ›
Impact and interplay of $\Lambda$CDM analysis choices for LSST cosmic shear ›
Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz ›
Non-minimally coupled scalar field dark sector of the universe: in-depth (Einstein frame) case study ›
ARCANE -- Early Detection of Interplanetary Coronal Mass Ejections ›
Evaluating statistical significance for massive black hole binary mergers with space-based gravitational wave detectors ›
Towards Realistic Detection Pipelines of Taiji: New Challenges in Data Analysis and High-Fidelity Simulations of Space-Based Gravitational Wave Antenna ›
Asymgenesis ›
Examining the influence of anisotropy on the fundamental mode of nonradial oscillation in neutron stars on a complete general relativistic scheme ›
Rolling with modular symmetry: quintessence and de Sitter in heterotic orbifolds ›
Are heuristic switches necessary to control dissipation in modern smoothed particle hydrodynamics ? ›
Black Hole Cold Brew: Fermi Degeneracy Pressure ›
On the Theory of Bulk Viscosity of Cold Plasmas and Thermodynamics of Alkali-Noble Gas Cocktails ›
On the treatment of thermal effects in the equation of state on neutron star merger remnants ›
Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model ›
Physical Predictions in Closed Quantum Gravity ›
Light dark sector via thermal decays of Dark Matter: the case of a 17 MeV particle coupled to electrons ›
Leptophilic scalar dark matter in U(1)$_{L_\mu-L_\tau}$: Evading direct detection and prospective neutron star heating ↓↑