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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 Wiadomości z astronet.pl

› Liczba czarnych dziur we wszechświecie może być mniejsza niż wcześniej zakładaliśmy
› Sterowanie lotem za pomocą balonów – projekt DracoSat
› Katalog Caldwella: C13
› Misje Kosmiczne XX wieku: Endeavour
› Katalog Caldwella: C103
› Ćwierćwiecze działalności AstroNETu. Pierwsze papierowe wydanie
› Katalog Caldwella: C86
› AstroNET finalistą konkursu Popularyzator Nauki 2025
› Katalog Caldwella: C108
› Nowe informacje o gwiazdach Galaktyki – teleskop Nancy Grace Roman
RSS  Najnowsze prace na astro-ph:

› Evolving the Loeb Scale
› The next frontier in exoplanet science: Imaging our neighbouring planetary systems
› Direct imaging characterization of cool gaseous planets
› Hot Jupiters in Old Wide-Binary Systems
› Resolving dust and Ly{\alpha} emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS
› Hydrodynamical mass-loss rates for Very Massive Stars. I. Investigating the wind kink
› Confirming membership in Local Group galaxies with the Dark Energy Spectroscopic Instrument Data Release 1
› A minimalist approach to BL Lacertae: explaining gamma-ray spectral and temporal variability with a single physical parameter
› The chemical DNA of the Magellanic Clouds V. R-process dominates neutron capture elements production in the oldest SMC stars
› Exploring the origins of high-velocity features in SNe Ia with the spectral synthesis code TARDIS
› Halo Lightcones with Optimised Orientation and Interpolation in Cosmological Simulations -- an application to mock H$\alpha$ selected galaxies
› How Mass Flows Through Accretion Discs: A Spectral-Timing Vision for the 2040s
› Buried but not destroyed: the evolution from prompt cusps to NFW haloes
› Millimeter-Wavelength Observations of the Active Sun: Unveiling the Origins of Space Weather
› Spirals and Vertical Motions in the Planet-Forming Disk around HD 100546. A multi-line study of its gas kinematics
› A high-dynamic-range view of the growth of structure and the warm/hot Universe
› Connection between galaxy morphology and dark-matter halo structure II: predicting disk structure from dark-matter halo properties
› Searching for Intermediate-Mass Black Holes in Milky Way satellites
› Local Group dwarf galaxies as dark matter probes
› Convective Core Evolution of Main-Sequence Stars in Rapid Population Synthesis I: Framework and Implementation
› A wide-field X-ray search for the Geminga pulsar halo with SRG/ART-XC
› The search for dark matter axions from neutron stars in the inner parsecs of the Milky Way with AtLAST
› The molecular diversity of the ISM in galaxies across cosmic time
› ExoMol line lists -- LXIII: ExoMol line lists for 12 isotopologues of CO$_2$
› AtLAST -- Cosmology with submillimetre galaxies magnification bias
› AtLAST -- Determination of Halo Mass Density Profiles at kpc Scales through Magnification Bias
› AtLAST -- A five fold increase in the number of identified Strongly Lensed Galaxies in the sub-millimetre and its consequences
› A wide-field, multi-line survey of CO in the Magellanic Clouds at parsec-scale resolution: characterising the molecular gas content with a 50-m single-dish submillimeter telescope
› Atangana-Baleanu Regularized Wavelet Compression For Astronomical Time-Series
› Detection and characterisation of submm transient sources with a large single-dish telescope
› Cold Gas Infall onto A Brightest Group Galaxy via A Gas-Rich Minor Merger
› Doomed Worlds II: Reassessing Suggestions of Orbital Decay for TrES-5 b
› Investigating the Reionization Epoch through 21\,cm and Line Intensity Mapping Experiments
› Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
› From ASTRID to BRAHMA -- The role of overmassive black holes in little red dots in cosmological simulations
› The multiple facets of millisecond pulsar binaries
› Primordial Black Holes as Seeds for Extremely Overmassive AGN Observed by JWST
› How is Cold Gas Loaded into Galactic Nuclear Outflows?
› Vertically resolved minimal-set k-distribution for thermal infrared absorption in the Venus atmosphere
› The role of supernova remnants for the emergence of pre-biotic chemistry in molecular clouds
› Can dwarf spheroidal galaxies host a central black hole ?
› NIKA2 Cosmological Legacy Survey. First measurement of the confusion noise at the IRAM 30 m telescope
› Fermi-LAT detections of novae V1723 Sco and V6598 Sgr
› The Alignment of High-resolution Solar Prominence Images Observed by the New Vacuum Solar Telescope
› Mass Assembly and Chemical Complexity in the Milky Way
› Exploring Cosmic Dawn with PANORAMIC II: Cosmic Variance and Galaxy Clustering at $z\sim10$
› Revealing the baryon cycle in Galaxy Clusters: connecting galaxy dynamics and gas thermodynamics using (sub-)mm-wave and optical IFU surveys
› A Possible Indication of Metallic Iron in White Dwarf Dusty Disks from their "Dirtiness"
› The ORCA-TWIN qCMOS Project I. Commissioning at Calar Alto Observatory
› Connecting galaxies with their haloes -- from parsec to Mpc scales
› New Bulgarian-Austrian project 'Joint observations and investigations of solar chromospheric and coronal activity'
› A Bridge between Young Stars Formed by Gravitational Interaction
› Comparative study between low and high energy SOHO/ERNE protons in solar cycle 23
› Invisible gravitons and large-scale magnetism
› Development of a Central Trigger Processor board for the Advanced SiPM based camera of the CTA Large-Sized Telescopes
› Formation of a Magnetic Flux Rope Prior to the Eruption: Insight from a Radiative MHD Simulation of Active Region Emergence
› INTEGRAL IBIS catalog of magnetar bursts
› Surveying Galaxy Clusters (in formation) in the Distant Universe
› The Role of Self-Gravity in Debris Disk Warp Formation: The Case of HD 110058
› QUIJOTE-TFGI polarization calibration -- Ground characterization and on-sky validation with Tau A and the Moon
› A sub-ppm upper limit on the cosmological variations of the fine structure constant alpha
› Coexistence of coagulation and streaming instabilities in protoplanetary discs
› Primordial features and low-$\ell$ suppression from isocurvature modes in multi-field Higgs-$R^2$ inflation
› Bowshocks driven by the pole-on molecular jet of outbursting protostar SVS 13
› The quest for Magrathea planets. II. Orbital stability of exoplanets formed around double white dwarfs
› Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Time-domain astronomy
› A one-parameter two-zone leptonic model for the blazar sequence
› A first systematic study of [OIII] 88$\mu$m at $z>8$: two luminous oxygen lines and a powerful ionized outflow in the first 600 million years
› Orbits of Twelve Multiple Stars
› Geminids are initially cracked by atmospheric thermal stress
› The stellar activity-rotation-age relationship under the lens of asteroseismology
› Interfacing adaptive optics simulations with the optical model: a powerful tool for MORFEO
› Multi-messenger and time-domain astronomy in the 2040s
› A network for solar optical observations in Bulgaria
› Kinematic Reconstruction of $\Lambda(t)$CDM Models
› Probing hadronic interactions at the 100 TeV scale with the Pierre Auger Observatory
› Selection and characterisation of the M-dwarf targets in the PLATO Input Catalogue
› The role of mergers and rejuvenation in the buildup of the quiescent population at cosmic noon
› The Dynamics of the Milky Way: Unveiling the 6D Skeleton of Star Formation in the 2040s
› kSZ for everyone: the pseudo-Cl approach to stacking
› Cluster properties as a function of dynamical state in the DESI Legacy x UNIONS surveys
› Attention-Based Preprocessing Framework for Improving Rare Transient Classification
› Radio emission in star-forming galaxies: connection to restarted or relic AGN activity
› NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
› From the Solar System to cosmological distances: a complete formalism for gravitational wave astrometry
› 1D stellar mergers: entropy sorting and PyMMAMS
› A universal scaling law for gravitational waves induced during inflation
› Clustering with Light (but Massive) Relics
› Cosmic Strings Gravitational Wave Probe of Leptogenesis: Thermal, Non-thermal, Near-resonant and Flavourful
› JWST Observations of the Double Nucleus in NGC 4486B: Possible Evidence for a Recent Binary SMBH Merger and Recoil
› XID+PRIMA, II: Stepping Through Hyperspectral Imaging to Deblend PRIMAger Beyond the Extragalactic Confusion Limit
› An Excited Dark Matter Solution to the MeV Galactic Center Excesses
› Neutrino Constraints on Scalar-Tensor Gravity
› A Cosmic Higgs Collider
› Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media
› Quantum Walks and Exact RG in de Sitter Space
› The Role of Microstate Degeneracy in Phase Transitions: Gravitational Waves from Bubble Entanglement
› Any Light Particle Searches with ALPS II: first science results
› Inspiral-Transition-Plunge Gravitational Waveforms Beyond Kerr: A Kerr-Newman Case Study
› Cosmological Bounds on Scotogenic Model with Asymmetric Mediator
› NASA/NOAA MOU Annex Final Report: Evaluating Model Advancements for Predicting CME Arrival Time
› Demonstrating sub-picometer non-reciprocity levels in the Three-Backlink Experiment for LISA
› Construction techniques and commissioning of the Three-Backlink Experiment for the LISA mission
› Gravitational Waves from Confinement in $SU(N)$ Yang-Mills Theory
› Stochastic Inflation in Numerical Relativity
› Search for Gravitational Wave Memory in PPTA and EPTA Data: A Complete Signal Model
› Astrophysical Tests of Dark Matter Self-Interactions
› CMB delensing with deep learning
› Genuine Retrieval of the AGN Host Stellar Population (GRAHSP)
› Constraints on the interaction strength in the model of interacting dynamical dark energy with linear and non-linear interacting terms
› Variability of the UV luminosity function with SPICE
› Is gamma-ray burst polarization from photosphere emission?
› Hints of Primordial Magnetic Fields at Recombination and Implications for the Hubble Tension
› Bar ages derived for the first time in nearby galaxies: Insights on secular evolution from the TIMER sample
› Evidence of Time-Dependent Diffusive Shock Acceleration in the 2022 September 5 Solar Energetic Particle Event
› The dynamical lineage of ultra-diffuse galaxies from TNG50-1
› The spin-orbit alignment hypothesis in millisecond pulsars
› Detection of CO$_2$, CO, and H$_2$O in the atmosphere of the warm sub-Saturn HAT-P-12b
› Lord of LRDs: Insights into a "Little Red Dot" with a low-ionization spectrum at z = 0.1
› Can Big Black Holes Merge with the Smallest Black Holes?
› The Impact of Spectroscopic Redshift Errors on Cosmological Measurements
› Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds
› Particle acceleration up to the synchrotron burn-off limit in relativistic magnetized turbulence
› An improved model for the effect of correlated Si-III absorption on the one-dimensional Lyman-$\alpha$ forest power spectrum
› Dwarf galaxies in the MATLAS Survey: Hubble Space Telescope observations of nuclear star clusters
› Gravitational lensing of 21 cm HI signal: detection prospects at z ~ 1 with uGMRT in galaxy cluster lenses
› JWST-TST High Contrast: Medium-resolution spectroscopy reveals a carbon-rich circumplanetary disk around the young accreting exoplanet Delorme 1 AB b
› Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
› SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope
› Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum
› A search for transit timing variations in the transiting hot Jupiter systems HIP 65, NGTS-6, NGTS-10 and WASP-173
› The HITRAN2024 methane update
› Supervised Classification of LEO Debris Families Using Multi-Set Proper Elements
› The AURORA Survey: Constraining Chemical Enrichment Pathways at Cosmic Noon with Argon Abundances
› The magnetic origin of the outer boundary of sunspots
› Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach
› Multiband neural network classification of ZTF light curves as LSST proxies
› Primordial black holes as cosmic expansion accelerators
› Modeling Relative Peak Times of Gravitational Wave Harmonics
› A Common Origin of Asymmetric Self-interacting Dark Matter and Dirac Leptogenesis
› Maximum mass limit of strange stars in quadratic curvature-matter coupled gravity
› Precision gravity constraints on large dark sectors
› Misspecification-robust amortised simulation-based inference using variational methods
› General Framework for the Spontaneous Scalarization of Regular Black Holes
› Extreme mass ratio inspirals in the cold vector dark matter environment

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