in EnglishObserwatorium Astronomiczne na Suhorze
Zdjęcie mgławicy w Orionie (M42) zrobione z Suhory
Kamerka S
Kamerka N
Niebo
Temperatura
2.3 °C
Wilgotność
94%
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0.0 km/h
Ciśnienie
1011.3 hPa
Księżyc
Zdjęcie mgławicy w Orionie (M42) zrobione z Suhory
Wiadomości z 
Najnowsze prace na astro-ph:› Undetected past contacts with technological species: implications for technosignature science
› Relativistic Magnetohydrodynamic Simulations of Giant Magnetar Bursts
› Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge
› Addressing the Impact of Solar Modulation Systematic Uncertainties on Cosmic-Ray Propagation Models
› Identifying Exoplanets with Deep Learning VI. Enhancing neural network mitigation of stellar activity RV signals with additional metrics
› Teen TITANS simulations -- I. Inefficient intermediate-mass black hole seeding via stellar collisions in young massive clusters
› Bonnor-Ebert sphere collapse in filamentary structures
› Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE
› There and back again? Neutral outflows in z~3.5 quiescent galaxies
› Possible stratospheric emission in the warm Neptune GJ 436 b from high-resolution spectroscopy
› On the Origin of Coronal Picoflare Jets
› Long-term eclipse time variations in white dwarf binaries
› Improved Identification of Satellite Trails in ACS/WFC Imaging Using a Modified Radon Transform
› Ly{\alpha} forest bounds on sterile neutrino production via neutrino self-interactions
› The SB9 catalogue: status, comparison with non-single stars from Gaia DR3 and evolution to SBX
› Scaling Relations across Galaxy Classification Schemes: I. Star Formation Rate-Stellar Mass Plane of CALIFA Nearby Galaxies
› dfcosmic: A Python package for cosmic ray removal
› A Bayesian Exploration of the Mass of Ursa Major III: Kinematics, Rotation and their influence on the Mass to Light Ratio
› A Comprehensive Catalog of Radio Sources and Rotation Measures in the Perseus Molecular Cloud from Very Large Array Observations
› MATLAS-42, A Globular Cluster-Rich Ultra-Diffuse Galaxy That Diverges from the "Failed Galaxy'' Formation Pathway
› Probabilistic Methods for Initial Orbit Determination and Orbit Determination in Cislunar Space
› Investigating the role of mergers in galaxy assembly in the early Universe (z > 5)
› Modeling brightness temperature of sunspots using ALMA single-dish observations
› The attempted polarity reversal and evolving magnetic environment of AD Leo
› 3D radiative transfer modeling of scattering polarization with partial frequency redistribution I. Verification and disk-center results for the solar Ca I 4227 {\AA} line
› Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows
› TROYE: Modeling Dynamic Phase Transitions in Gravitational Waves from Neutron Star-Black Hole Mergers
› The GAPS Programme at the TNG: LXX. TOI-5734b: A hot sub-Neptune orbiting a relatively young K dwarf with an Earth-like density
› Testing the Icy Pebble Accretion Hypothesis with Primordial Main Belt Asteroids
› Updated Air-Shower $X_{\rm max}$ Moment Parametrizations for UHECR Composition with Latest Hadronic Interaction Models
› A Photometric and Spectroscopic investigation of 11 TESS eclipsing contact binaries
› MIGHTEE HI observations of low surface brightness and ultra-diffuse galaxies in the XMM-LSS field
› Power-law Indices of EUV Intensity Power Spectrum in Flaring Coronal Active Regions
› Euclid: An automated system to match Rubin transient alerts to Euclid observations
› A geometric physics-informed machine learning inference for the neutron star maximum mass and the inverse problem
› The Dispersed Matter Planet Project Sample -- Detection limits, Occurrence Rates and New Planets
› The GUAPOS project -- VII: Physical structure and molecular environment of the G31.41+0.31 HII region
› First Dark Photon Search Results from the Dandelion Experiment
› Mathematical derivation and verification of the amplitude of LISA's interferometric signals on an ultra-stable interferometer testbed
› CMB anisotropies from cosmic (super)strings in light of ACT DR6
› Chromaticity-Optimized Antenna Design and Bayesian Foreground Validation for the CANTAR Global 21 cm Experiment
› Single and double headed ORCs in the LOFAR surveys
› Cosmological Constraints on Temperature-Dependent Interaction between Dark Matter and Neutrinos
› Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8
› A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks
› Numerical simulations of cold clumps in the hot accretion flows around black holes
› Spatio-Spectroscopic Representation Learning using Unsupervised Convolutional Long-Short Term Memory Networks
› Chandra Proper Motions and Milliarcsecond Astrometry of Nineteen Pulsars
› A response-matrix-centred approach to presenting cross-section measurements
› Hypothesis tests and model parameter estimation on data sets with missing correlation information
› Covering Unknown Correlations in Bayesian Priors by Inflating Uncertainties
› Plotting correlated data
› Spectral Homogenization of the Radiative Transfer Equation via Low-Rank Tensor Train Decomposition
› Scaling Laws for Template-Free Detection of Environmental Phase Modulation in Gravitational-Wave Signals
› Minimal Dark Matter: Generalized Framework and Direct-Detection Sensitivity
› Decay of a multi-axionic SU(N) symmetric color aether in the early Universe as an origin of emergence of a many-component dark matter
› Dark Photon mediated Inelastic Dark Matter in Cosmology, Astrophysics and Colliders
› GR-Athena++: Binary Neutron Star Merger Simulations with Neutrino Transport
› Constraining the $\Lambda\Lambda$ interaction with terrestrial and astronomical data
› Detection prospects of solar $g$-modes with LISA
› The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
› Deep Generative model that uses physical quantities to generate and retrieve solar magnetic active regions
› Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production
› Unveiling Electron Density Profile in Nearby Galaxies using SDSS MaNGA
› AstroMLab 4: Benchmark-Topping Performance in Astronomy Q&A with a 70B-Parameter Domain-Specialized Reasoning Model
› The Cosmic Owl: Twin Active Collisional Ring Galaxies with Starburst Merging Front at $z=1.14$
› A solution to the tension of burning on neutron stars and nuclear physics
› TasVisAn and InsPy -- Python Packages for Triple-Axis Spectrometer Data Visualization, Analysis, Instrument Resolution Calculation, and Convolution
› HOLISMOKES XVII: Detecting strongly lensed SNe Ia from time series of multi-band LSST-like imaging data
› No evidence for Keplerian taper of far-out galactic rotation
› Quantum estimation of cosmological parameters
› A spherical hydrodynamical model of cosmic voids in {\Lambda}CDM and beyond
› $r$-process Heating Feedback on Disk Outflows from Neutron Star Mergers
› New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
› The Impact of Baryonic Effects on the Dynamical Masses Inferred Using Satellite Kinematics
› Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models
› Joint Bayesian calibration and map-making for intensity mapping experiments
› The Galaxy Activity, Torus, and Outflow Survey (GATOS): N. Unveiling physical processes in local active galaxies. Unsupervised hierarchical clustering of JWST MIRI/MRS observations
› Quantifying the Effects of Parameters in Widespread SEP Events with EPREM
› Stochastic analysis of ultra-high energy cosmic ray interactions
› Ultra-long Gamma-ray Bursts from Micro-Tidal Disruption Events: The Case of GRB 250702B
› MEGATRON: Disentangling Physical Processes and Observational Bias in the Multi-Phase ISM of High-Redshift Galaxies
› The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape
› Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
› Rethinking mass transfer: a unified semianalytical framework for circular and eccentric binaries. II. Orbital evolution due to nonconservative mass transfer
› The PAU Survey: The $i$-band galaxy luminosity function from the present-day to $z = 2$
› Simulating Disky Broad Line Region Reverberation
› Joint Constraints on Fuzzy and Warm Dark Matter from Satellite Populations of the Milky Way and Andromeda
› DRAGNs in the Forest: Identifying Artifacts with Random Forest Models in the VLASS DRAGNs Catalog
› Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events
› NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period
› A simple mechanism for the enhancement of the inflationary power spectrum
› Supermassive black holes swallow stellar objects at high rates: from Little Red Dots to Black Hole Stars
› PDRs4All XXI. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
› Gravitational-wave signatures of nonviolent nonlocality
› Primordial black hole ringdown: The irreducible stochastic gravitational wave background
› Fast and Fewrious: Stochastic binary perturbations from fast compact objects
› Towards an anomaly detection pipeline for gravitational waves at the Einstein Telescope
› Gravitational Ionization by Schwarzschild Primordial Black Holes