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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Astronomia w Krakowie
Zdjecie: Zachód Słońca
Zachód Słońca
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
14.7 °C

Wilgotność
 70%

Wiatr
3.2 km/h

Ciśnienie
1015.0 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› 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

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