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Obserwatorium Astronomiczne na Suhorze

Zachód Słońca

Kamerka S

Kamerka N

Niebo
Temperatura
14.7 °C
Wilgotność
70%
Wiatr
3.2 km/h
Ciśnienie
1015.0 hPa

Księżyc
Najnowsze prace na astro-ph:
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On the reconstruction of the Rotation Curve for Milky Way and its spacetime implications: a Machine Learning approach ›
Primordial tensor mode from the neutrino sector ›
Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys ›
Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters ›
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy ›
Forest without Trees is still Fruitful: Constraints on the thermal state of the neutral IGM at $z\approx5.6$ with the 21-cm forest power spectrum ›
Ultraviolet to Infrared Spectroscopy of the Type Ibn SN 2023tsz Suggests a Lower-mass Progenitor ›
The Azahar Project: Non-Thermal Physics Drives Star Formation Burstiness and the Evolution of the UV Luminosity Density at Cosmic Dawn ›
Polarization geometry of magnetohydrodynamic turbulence ›
The first three-dimensional map of thermal phases in the local interstellar medium ›
Tunnelling out of Starobinsky inflation: Raising the spectral tilt ›
Very Large Telescope observations of interstellar comet 3I/ATLAS III: High-resolution monitoring of CN and forbidden oxygen emission across the perihelion passage with ESPRESSO ›
Non-Thermal Physics Drives Compact, Self-Regulated Galaxy Morphologies at Cosmic Dawn ›
Observations of X-ray quasi-periodic eruptions ›
Multimessenger prospects of quasi-periodic eruptions ›
Stellar heavy-element slope index ›
Assembly, integration, and verification of MITESI: an optical testbed for simulating the ELT in the laboratory ›
Luminous Red Novae as shock-powered transients I: Electron-scattering wings and deviations from Case B ›
Ephemeris Refinement for Qatar-4 b, HAT-P-18 b, and CoRoT-1 b with Small Telescope and TESS Observations ›
Large-scale emission from gamma-ray binaries: the case of LS 5039 ›
Pre-main Sequence B Stars Surrounding the Orion Nebula ›
Uncovering Hierarchical Sub-Population of Binary Black Holes ›
A Multiwavelength Study of a Long-Duration VHE Flare from BL Lacertae with VERITAS ›
Two-component large-scale radio emission in Abell 2244 ›
Triple radio flares from tidal disruption events: jet-wind collisions and the discovery of a third radio flare from AT2020vwl ›
Assessing the waveform systematics from parameter estimation to population inference with eccentricity ›
Implications of the UV/optical Plateau of AT2018cow ›
A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins ›
Star formation, stellar evolution, and planets in high-resolution X-ray imaging ›
Gas-Phase Metallicity and Nitrogen Abundances in Low-Mass Galaxies Down to $M_\star\simeq10^{5.7}\,M_\odot$ at $z\simeq4.5$--$10.1$ from JWST Lensing Cluster Surveys ›
Silicate Clouds, SiO, and Molecular Trends across the L-T Sequence: A JWST/MIRI LRS Spectral Library of Brown Dwarfs ›
Investigation of projected rotational velocities of Be-type stars in LAMOST DR7 ›
22 Newly Identified Repeating Changing-look AGNs and Evidence for Extreme Broad-line Region Breathing ›
Morphological Bias: How Ellipticals and Spirals Trace the Cosmic Web Differently ›
High-Density Sound Speed and Post-Merger Dynamics ›
The FAST HI 21-cm Absorption Blind Survey. III. OH Absorption Search in the 21-cm Absorber Sample and Continued HI Absorption Search ›
Oscillation Period Properties of Sunspots in the 8-10 $\mu$m Infrared Band: A Multi-Dataset Analysis ›
Identifying and Distinguishing Quenching Galaxies with Spatially Resolved Star Formation in Mock CASTOR and NGRST Observations ›
Distant TNO Inclinations as a Constraint on Primordial Cluster Perturbations in the Presence of Planet Nine ›
Update on the Physics of the Cosmic Microwave Background (2015-2025) ›
Torsional-X Seismometer for Lunar Decihertz Gravitational-Wave Detection ›
Debris Evolution from Spacecraft Fragmentation in Earth-Moon Distant Retrograde Orbits ›
Explainable AI for Solar Flare Prediction: Quantitative Magnetic Field Analysis of Model-Focused Regions ›
Stable X-ray reverberation lags in the black hole X-ray binary Swift J1727.8-1613 ›
Testing various assumptions for radiolysis, non-diffusive chemistry, and chemical desorption in cold cores ›
Three-dimensional evolution of a solar filament with multipoint observations ›
Accuracy Analysis of VLBI Universal Time Measurement Based on a GNSS Single-Station Regional Ionospheric Model ›
Radial velocity and atmospheric parameter calculations for the GaiaNIR spectrograph ›
A cosmic-ray loaded nascent outflow driven by a massive star cluster ›
Chemical Evolution of Galaxies: Past, Present and Future ›
Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction ›
Solar Cycle Variation of the Distribution of Photospheric Magnetic Flux Features ›
Compressing radio interferometric visibility data into a probabilistic model using sparse Gaussian processes ›
The S-PLUS Fifth Data-Release: Over 4500 square degrees of the Southern Sky and a multicolor view of the Hydra and Antlia galaxy clusters ›
GW Microlensing: Degeneracy with Unlensed Precessing and Non-Spinning Gravitational-Wave Signals ›
Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals ›
Spectral features in the visible spectra of the Enceladus particle plume and E ring: Potential evidence of organic materials and/or missing sub-micron particles ›
Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 ›
Radio-detected Lya emitters at 1.88 < z < 3.52: AGN fraction and Lya emission ›
Coherence differential imaging using gradient-boosted decision trees for the direct detection of exoplanets ›
Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band ›
OpenCosmo: Community Portal and Analysis Framework for Flagship Cosmological Simulations ›
Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect ›
Dynamics and geometry of the inner sub-parsec-scale jet in 3C 279 observed with the Event Horizon Telescope ›
Commissioning and on-sky performance of FiberPol: a fiber-fed spectropolarimetric system for the SAAO 1.9 m telescope ›
Discovery of $\gamma$-Ray Pulsations from the Extreme-Spin-Down Millisecond Pulsar PSR J0435+3233 ›
Impact of eccentricity and higher-modes on neutron star-black hole parameter estimation ›
Eccentricity as a Magnifying Glass: Precision Population Inference Enabled by Eccentric Neutron Star--Black Hole Mergers ›
X-ray polarization of Z-type neutron star low-mass X-ray binaries -- II. Spectropolarimetric analysis ›
Large deviations for halos and voids: beyond perturbative non-gaussianities ›
SEP-PRISM Data: A multi-source dataset for solar energetic particle forecasting ›
Constraining primordial non-Gaussianity and parity-violation through Scalar-Induced Gravitational Waves with next-generation ground-based interferometers ›
Euclid: Calibrating distances from surface brightness fluctuations with Early Release Observations of the Fornax cluster ›
Morphologies of SAGAbg low-mass galaxies in Legacy Survey multi-band imaging: dependence on stellar masses, star-formation rates and low-redshift evolution ›
Cosmological Evidence for Dark Axion-Dark Baryon Interactions from Apparent Phantom Crossing ›
A Momentum-Regulated Model For Star Formation Efficiency in Giant Molecular Clouds ›
Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae ›
PBH formation and Gravitational Waves as Multi-messenger Signals of First-order Phase Transitions ›
Relativistic Scaling and Magnetization-Current Feedback in Stern Gerlach-Modified Pair-Plasma Reconnection: SpinPIC2D Validation and Nonlinear Regimes ›
Hanbury-Brown Twiss effect, squeezed gravitons and the photon correlations ›
Localized Vector Modes on Local Cosmic Strings ›
Classifications for Exoplanet and Exoplanetary Systems -- Could it be developed? I. Exoplanet classification ›
Optical appearance of the Konoplya-Zhidenko rotating non-Kerr black hole surrounded by a thin accretion disk ›
Preliminary Analysis into the Feasibility of Missions to Asteroid 2024 YR$_4$ ›
Searching optimal scales for reconstructing cosmological initial conditions using convolutional neural networks ›
Nutation Damping from Core-Mantle Boundary Topography ›
Pad\'e Approximants for cosmic Dispersion Measures ›
Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments ›
Figuring Out Gas & Galaxies in Enzo (FOGGIE). XV. Examining the Spatial and Kinematic Relationship between Circumgalactic Mg II and O VI ›
FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters ›
Dynamics of magnetoviscous warped discs around compact objects ›
Excitation and Damping of Oscillation Modes in Gaseous Planets ›
Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model ›
Search for quasar pairs with Gaia astrometric data IV. Confirmation of 17 dual quasars and 143 projected quasars ›
Solar Cycle Prediction: Challenges, Progress, and Future Perspectives ›
Exploration of the inner region of the system HD 142527 ›
Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates ›
Towards Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions ›
Realtime forecasting of solar energetic particle event and proton flux using multi-source solar observations and multi-task deep learning ›
Impact of 21-cm foreground mitigation strategies on reionization power spectrum constraints ›
The Edge-on Galaxies in the DESI survey (EGIDE): sample building and photometry ›
TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS ›
Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group ›
The GAPS programme at TNG: LXXVI. TOI-1533: a compact system hosting a super-Neptune-mass pair with disparate radii ›
The Fleeting Laboratory: An Experimental Guide for Total Solar Eclipses ›
Gravitational Waves from Primordial Black Holes: Connecting Low-Frequency Scalar-Induced Signatures to High-Frequency Binary Mergers ›
Understanding Pulsar Magnetospheres with the SKAO ›
The coronal mass ejection productivity of solar active region 13664/8 ›
The VST ATLAS Survey IV: Galaxy, LRG and QSO bias and HODs via ACT CMB Lensing ›
Tracking electron capture processes in classical molecular dynamics simulations for spectral line broadening in plasmas ›
Unitary quantum matter-bounce in a universe with a positive cosmological constant ›
Naturally resonant two-mediator model of self-interacting dark matter with decoupled relic abundance ›
Constraining the axiverse with reionization ›
Dark Matter Capture in Supernovae Modifies Dark Photon Cooling Bounds ›
(Lovelock)$^2$ inflation: explaining the ACT data and equivalence to Higgs-Gauss-Bonnet inflation ›
Higgs-like inflation in scalar-torsion $f(T,\phi)$ gravity in light of ACT-SPT-DESI constraints ›
Spectrum of radiation from global strings and the relic axion density ›
Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models ›
Lyman-$\alpha$ Forest Constraint on Dark Matter from Dark Sector Decay ›
Gravitational-wave astronomy requires population-informed parameter estimation ›
Stern--Gerlach Spin Sorting and Dynamical Feedback in Relativistic Pair-Plasma Reconnection ›
Ringdown and lensing of triple systems ›
Newtonian Shirokov Effect: Epicyclic Frequency Splitting from Mass Multipoles ↓↑