Obserwatorium Astronomiczne na Suhorze Strona główna
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Obserwatorium Astronomiczne na Suhorze

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 Wiadomości z astronet.pl

› CanSat sterowany sztuczną inteligencją – projekt WindRiders
› Katalog Caldwella: C54
› Misje kosmiczne XX wieku: Program Discovery
› Powrót po serii porażek. Ostatni lot rakiety Alpha Block 1
› Do 20 marca zapisy do konkursu Łowcy Cząstek 2026
› Katalog Caldwella: C64
› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
› Niebo w marcu 2026 roku
› Artemis III nie wyląduje na Księżycu. NASA ogłasza duże zmiany
› Startrails, czyli najprostszy astrokrajobraz
RSS  Najnowsze prace na astro-ph:

› \texttt{py5vec}: a modular Python package for the 5-vector method to search for continuous gravitational waves
› Formation and relaxation of halos in the context of wave DM particles evolving on a background of neutrino condensate
› AGILE: an end-to-end Rubin-LSST simulation of AGNs, galaxies, and stars I. Software description and first data release
› Field-Level Inference from Galaxies: BAO Reconstruction
› Inferring the mass and size of 3I/ATLAS from its non-gravitational acceleration
› Halo assembly bias in the early Universe: a clustering probe of the origin of the Little Red Dots
› Multi-phase AGN-driven outflow in the NLSy1 IRAS 17020+4544. Unveiling dual-feedback and an energy-conserving ionized outflow with MEGARA/GTC integral field spectroscopy
› Hankel low-rank matrix approximation for gravitational-wave data analysis
› Shocks from Exploding Primordial Black Holes in the Early Universe
› A 5kHz modulator for pyramid wavefront sensors
› BL Lac host galaxies: how to systematically characterise them in optical-NIR spectroscopy
› Magnetar counterparts, kinematics and birth sites with HST and JWST
› BASS. LI. Cool gas supply of HI-massive local Seyfert galaxies
› Single-source-class interpretation of the diffuse astrophysical neutrino flux
› Out of oxygen: Extremely metal-poor galaxy candidates identified at $2.5 < z < 6.5$ with deep JADES medium-band imaging
› Optimizing the Roman Space Telescope High-Latitude Wide Area Survey for mitigating chromatic PSF effects on shear measurement
› Self-Consistent Nonlinear Classical Cepheid Pulsations During Stellar Evolution with MESA
› NEATH V: the relationship between line emission from dense gas tracers and the star formation rate
› Confidently Wrong: Why Ignoring Binaries Biases IMF Inference at Large Sample Sizes
› Late-Onset Energy Injection in Type Ic SNe and W-Shaped O II Absorption in SLSNe-I
› Revisiting observational constraints on coupled exponential quintessence with energy and momentum transfers: degeneracy with massive neutrinos
› Experimental evidence for granular shear-flow instability in the Epstein regime
› First detailed optical spectroscopic observations of the supernova remnants G107.7-5.1 and G150.3+4.5
› ODIN: Searching for LyC emission from Lyman-$\alpha$ emitters at $z=4.5$ in the E-COSMOS and XMM-LSS fields
› Exploring memory-burdened primordial black holes with ultra-high-energy cosmic-rays
› Spectral Hierarchy of the Cosmic Web
› Gravitational-Wave Propagation Through the Axiverse
› EGS-z11-R0: a red, dust-rich galaxy at Cosmic Dawn
› A Third Galaxy Missing Dark Matter along a Trail of Galaxies in the NGC 1052 Field
› Dark Energy with Constant Inertial Mass Density: Updated Constraints and Curvature-Induced Sign Transitions in $\rho_{\rm DE}$ and $\rho_{\rm DE}+p_{\rm DE}$
› Analysis of spatially resolved stellar populations and emission line properties in nearby galaxies with J-PLUS data. II-Results for the M51 group and first comparison with the M101 group
› NEO Colors from The Mission Accessible Near-Earth Object Survey (MANOS)
› SN 2025adpq: A Type Ia supernova in a collisional ring formed during a major galaxy merger
› Measurements on the kinetic origin of streamer dynamics
› A chemical perspective on planet formation in reduced systems
› Cosmological prospects for multiband detection of intermediate-mass binary black holes with Taiji and ground-based detectors
› Emulation of SPHEREx Galaxy Power Spectra I: Neural Network Details and Optimization
› A Candidate Open Cluster Pulsar: Timing Analysis of PSR J1922+3745 in NGC 6791
› HESS J1832$-$085: evidence for a new gamma-ray binary candidate
› Evolution of fractality in centrally concentrated young clusters
› Cosmological hydrodynamical simulations of clustering dark energy with Nefertiti
› Resonant scattering at the center of the galaxy cluster PKS 0745-191 with XRISM
› Time-Lag properties associated with LFQPO in X-ray variability classes of GRS 1915+105: Findings from AstroSat
› Optimising the FRB Search Pipeline for the Northern Cross Radio Telescope
› Explainable machine learning workflows for radio astronomical data processing
› High-Precision Photometry with a scientific CMOS Camera: II On-Sky Testing of the Marana camera at the NGTS facility
› Detectability of Nearby Binary Neutron Stars with Future sub-mHz Gravitational Wave Missions
› The role of ambipolar heating in the energy balance of solar prominences
› Correlations Between kHz QPOs and Spectral Parameters from Time-Resolved Spectro-Temporal Analysis of 4U 1728-34
› Perturbative Effects of Dark Matter Environments on Black Hole Shadows
› Unveiling an Hourglass-Shaped Magnetic Field toward IRDC G351.77-0.53
› LenghuSky-8: An 8-Year All-Sky Cloud Dataset with Star-Aware Masks and Alt-Az Calibration for Segmentation and Nowcasting
› GEMS JWST: A sub-Solar metallicity atmosphere for giant planet TOI-5293Ab orbiting a rapidly changing M-dwarf
› Diversity of Type Ia supernova optical light curves among different spectroscopic subclasses
› Color and Size Distributions of Small Jupiter Trojans
› Geometric Search for Hawking Radiation from Nearby Primordial Black Holes
› Stellar Wind of Components of Detached Binary Systems
› Singular Templates of Imaging Cherenkov Shower distribution (STOICS): A background estimation method for Very-High-Energy $\gamma$-ray observations
› Laplace-Legendre expansion of the planar planetary Hamiltonian
› Testing the Coexistence of Dark Energy and Dark Matter with Late-time Observational Data
› Observational Constraints on WIMP Mini-Spikes Around Stellar-Mass Primordial Black Holes with 17 Years of Fermi-LAT Data
› A Search for the Lost Comet P/2010 H2 (Vales)
› The sensitivity and behaviour of the curvature in the \'echelle diagram of red-giant stars
› Particle acceleration at recollimation shocks in sub-relativistic jets A model for jets in Seyfert Galaxies, Microquasars and Protostellar Systems
› Stars with Plumbing Issues: The Formation of Collimated Outflows on Common-Envelope Simulations and Comparison to Water Fountains Observations
› The shape and spin state of (275677) 2000 RS11 from ground-based radar and optical observations
› Novel insights on the Coma Cluster kinematics with DESI. I. Linking mass profile, orbital anisotropy and galaxy populations
› The long-term accretion luminosity of V4641 Sgr through binary evolution simulations: implications for its ultrahigh-energy gamma-ray emission
› Cosmic Dipole as a Symmetry Response: From the Ellis--Baldwin Formula to Correlation Function Dipoles
› A Unified Origin of Faraday Rotation toward 3C 84: The Circumnuclear Ambient Medium within the Parsec-Scale Bondi Radius of the Host Galaxy NGC 1275
› Type Ia supernovae interacting with a close circumstellar material (SNe Ia-CSM) are SNe Ia inside planetary nebulae (SNIPs)
› Beyond $\Lambda$CDM with a Logistic RG-like Flow of the Low Redshift Cosmic Evolution
› Optical Magnus effect on gravitational lensing
› Cosmological Collider Searches beyond the Hubble Scale with Planck Data
› Crowdsourcing Gravitational Waves from Superradiant Axions
› Observing Micro Black Hole Dark Matter
› Quasi-pole quintessential inflation in metric-affine gravity
› Probing keV mass QCD axions with the SACLA X-ray free electron laser
› Twin-peaked gravitational wave signal from a dark sector phase transition
› Sensitivity of neutron star observables to microscopic nuclear parameters of realistic equations of state
› Nuclear pasta in hot neutron-star matter and proto-neutron stars
› Energy Conditions in Gauss-Bonnet Gravity
› Advances in the Fabrication of On-chip Superconducting Integral Field Units for CMB and Line-Intensity Astronomy
› On the survival of strong nuggets in the early Universe
› New benchmarks for direct detection of freeze-in dark matter in vector portal models
› Probing hadronic gamma-ray and high-energy neutrino emission from Gaia DR2 star clusters
› Orbital eccentricity in a neutron star - black hole merger
› Can a Breakdown of Hawking Evaporation Open a New Mass Window for Primordial Black Holes as Dark Matter?
› X-ray Emission Signatures of Neutron Star Mergers
› Gravitational waves from strong first order phase transitions
› Primordial black holes save $R^2$ inflation
› Dayside Clouds and an Elevated C/O Ratio in the Atmosphere of the Ultra-hot Jupiter WASP-19b
› Unveiling the dark Universe with HI and EMBER-2
› Rotational Effects on Neutrino Emission in Core-collapse Supernovae
› Quantifying the Effects of Parameters in Widespread SEP Events with EPREM
› Directly Probing Neutrino Interactions through CMB Phase Shift Measurements
› Weakly model-independent determination of total expansion during inflation
› The Spatially Resolved Hot Gas Properties of NGC 1266's AGN-Driven Outflow
› Vision-Based CNN Prediction of Sunspot Numbers from SDO/HMI Images
› Ly{\alpha} Intensity Mapping in HETDEX: Galaxy-Ly{\alpha} Intensity Cross-Power Spectrum
› The Nephele ecosystem: stars, globular clusters, and stellar streams associated with the progenitor galaxy of $\omega$ Centauri
› Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope
› A TESS View of Post-Eruption Variability in the Novae V1405 Cas,V1716 Sco, and V1674 Her
› APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina
› Self-bound quark stars with a first-order two-to-three flavor phase transition
› Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars
› Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones
› Towards Unveiling the Origins of the Milky Way Bulge through Multi-band-Messenger Sky Surveys
› On the gravitational stratification of multi-fluid-multi-species plasma
› Weak lensing of bright standard sirens: prospects for $\sigma_8$
› The early r-process nucleosynthesis scenarios
› Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branch
› Spectral response of SPHEREx
› Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments
› Toward Black Hole Stars: supermassive black hole growth in nuclear clusters via stellar-object and gas accretion
› First Dark Photon Search Results from the Dandelion Experiment
› A steadily declining dispersion measure for the repeating fast radio burst FRB 20220529A: Evidence for an FRB engine embedded in an expanding supernova remnant
› PICASO 4.0: Clouds and Photochemistry in Climate Models of Brown Dwarfs and Exoplanets
› The Baryon Budget of Galaxies across the First Billion Years -- Theoretical Predictions for Gas Phases, Depletion Times, and Stellar Return Fractions
› Evidence for a Delayed UV Counterpart to X-ray Quasi-periodic Eruptions in Ansky
› Merger-driven buildup of the $M_{\rm BH}$ - $M_*$ relation bridging high-$z$ overmassive black holes with the local relation
› Robustness of Neural Networks for CMB Polarization Foreground Removal
› Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms
› Mass Production of 2023 KMTNet Microlensing Planets. II: Two Planets and A Brown Dwarf
› Spectral Variations of $\gamma$-rays in Mrk 421
› The Chandrasekhar's Conditions as Equilibrium and Stability of Stars in a Universal Three-Parameter Non-Maxwell Distribution
› Freeze-in gravitational waves and dark matter in warm inflation
› Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data
› Fermionic Love of Black Holes in General Relativity
› Dark matter: red or blue?
› Dark matter silences Cepheids in the Galactic Center
› Bubble Nucleation from Boson Star Collapse
› ANNA: a toolbox for Newtonian Noise Analysis

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