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Astronomia w Krakowie
Photo: Sunset view from dome
Sunset view from dome
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Temperature
2.7 °C

Humidity
 88%

Wind
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Pressure
1015.1 hPa

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 News from astronomynow.com

› Happy New Year, Mars! The Red Planet is turning 39
› 3I/ATLAS was born in the deep freeze
› Roman Space Telescope launches on mission to survey the Universe
› JWST’s ‘impossible’ early galaxies may be even more massive than we thought
› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
RSS  Latest preprints on astro-ph:

› A Burst of Reionization in the Dark Ages
› A Single Line-Emitter Identified in an Unbiased Search with JWST/NIRSpec: Multi-Object Coronagraphy for Slitless Spectroscopy
› The accretionally heated atmospheres of protoplanets and brown dwarfs
› The road to $H_0$, $\Omega_m$, and $w$ with a global neutrino-telescope network
› When dust growth takes over: the origin of dust in post-reionization galaxies
› Nailing down the Hubble constant value through time delay cosmography: A 3% measurement from SN Refsdal
› "Mega-Earths" are likely an artifact of stellar activity
› The Fast & Fourier: Using neural operators to speed up radiative modeling of protoplanetary disks
› Dust-driven vertical shear instability in an isothermal shearing box: I. Turbulence and gas dynamics without dust feedback
› The GAPS programme at TNG LXXXII. The first atmospheric investigation of the gas giant WASP-13b at high resolution with GIARPS
› Exploring Case B I: The Footprints of Hidden Radiation Fields in H I Balmer Decrements
› Bridging Theory and Observation: Synthetic Far-infrared Insights into Star Formation Efficiency
› Predicted state-to-state collisional rate coefficients from neural networks
› Decomposing the Kinematics of SNR G180.0-01.7 with Medium-Resolution Spectra
› In-flight Timing Calibration of the Follow-up X-Ray Telescope on Board the Einstein Probe
› Global analysis of tensor mode helicity
› The Neptunian Final Parsec Problem: How Inertial Waves Enable Neptunes and Gas Giants to Survive Tidal Migration
› An Ultraviolet Instrument on the Habitable Worlds Observatory: Considerations and Capability Trades on the Multi-Object, Integral-field, and High-resolution modes of a potential UVI
› ASKAP Monitoring of the Rubin Deep Drilling Fields
› Redshifted Cool Gas in the Disturbed HI Disk of the Starburst Dwarf NGC 4214
› A Relationship Between Fast Radio Burst Dispersion Measure and Host Galaxy Inclination
› Star Cluster Ecology VIII. -- Dynamically Forming S-Type and $\alpha$Centauri-like Systems
› Formation Dynamics of a Rotating Solar Spicule-like Event and Associated Energy-Mass Transport
› Flux Evolution of PSR B0540--69 and the Spectral Energy Distribution of its Pulsar Wind Nebula
› Simulation Study of Reconstruction of Cosmic Ray Extensive Air Shower with Thermal Neutron Detected by ENDA
› Detailed study of HD 219134: a benchmark K-dwarf with a compact planetary system
› The Population of Type~1 Active Galactic Nuclei in Dark Energy Spectroscopic Instrument. I. Profile-dependent Measurements of the Low-redshift Sample
› Combination of multi-observatory photometry to determine asteroid rotation periods
› Towards a coupled activity-fallback model for comets I) 67P/Churyumov-Gerasimenko's water activity from a microphysics model with dynamic dust-depth
› Resistive alignment of a black-hole magnetosphere
› Extreme mass ratio inspirals from the Hills mechanism, The eccentricity distribution of Hills EMRIs in LISA
› The Silk Nebula: A Newly Discovered Giant [OIII] Emission Filament
› Flip-Flop Shocks and Tori in Bondi-Hoyle-Lyttleton Accretion onto Rotating Kerr-Weyl Black Holes and Their Quasi-Periodic Variability
› Detecting redshift space distortions with forthcoming 21cm intensity maps from MeerKLASS
› Fermentation heterotrophy can reproduce Enceladus's H2 and CH4 under limited serpentiniaztion
› An empirical calibration of the spectral resolution of JWST NIRSpec PRISM
› The Hydrological Cycle and Circulation of Tidally-Locked Planets with a Finite Moisture Inventory
› First Experimental Results of Space Object Detection Using the InteRFeX Array
› X-Shooter view of planetary nebulae microstructures I: The case of NGC 7009 knots
› Magnetic connectivity from the Sun to the Earth with MHD models II. Impact of input magnetic maps
› How long could volcanic plumes persist in the Venus atmosphere?
› Assessing PLATO's Discovery Potential across Different Observing Strategies
› High Resolution Spectro-Polarimetric Observations of the Optical Filaments surrounding NGC 1275 with ESPaDOnS
› Turbulence modes in molecular clouds in M33: a challenging test of the Brunt-Federrath framework
› Relaxation Dark Energy: Compositional Dynamics and the Future of Cosmic Acceleration
› A strategy for astrometric quasar selection with Gaia DR3 and its application to discover new luminous $z>2$ quasars
› A dust-reddened quasar in a [C II]-luminous host at z=6.55
› The origin of the large heavy element contents of warm Jupiters
› TeV Gamma-Ray Emission in the DA 495 Region from HAWC Observations of J1952+2924, J1954+2837, and J1958+2848
› Insights from the stability of methanol maser flare properties I: G9.62+0.20E
› Perpendicular transport in isotropic magnetic turbulence. The role of stochastic drifts
› The Redshift-Space Galaxy Power Spectrum at Two-Loop Order
› A Comprehensive JWST Slitless Spectroscopic Census of $\sim$12,000 Emission-Line Galaxies at Redshift $0\sim9$ in COSMOS
› Adiabatic evolution of hadronic neutron stars
› OGLE-2016-BLG-0523: A Low-mass Brown Dwarf or super-Jupiter in a $>100$ au Orbit
› General Spin-1 Dynamics During Inflation: Microcausality Constraints and Cosmological Collider Signals
› Galaxy Clustering Can Reveal Host-Galaxy Properties of Binary Black Hole Mergers
› Seeing in the Dark: Gravitational Waves from Resonant Production of Dark Photon Dark Matter
› Stochastic gravitational waves from narrow-band cosmological magnetic fields
› Phantom Zernike Wavefront Sensor: Phase Contrast with Engineered Focal Plane Reference Speckles
› Direct detection constraints on EFT operators for inelastic dark matter
› Binary Ellis-Bronnikov wormholes in 3+1 numerical relativity: mergers, fly-bys and gravitational waves
› The School on Gravity: from motion to commotion
› Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain
› Unifying spherical convolutions through lifting
› Cosmic rays density fluctuations with turbulence universal spectrum -8/3
› Cellular Dynamics of Helium-rich Detonation on sub-Chandrasekhar Mass White Dwarf
› Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis
› KSZ Velocity Reconstruction with ACT and DESI-LS using a Tomographic QML Power Spectrum Estimator
› Limb Asymmetries on WASP-39b: A Multi-GCM Comparison of Chemistry, Clouds, and Hazes
› A Star's Death by a Thousand Cuts: The Runaway Periodic Eruptions of AT2023uqm
› Radio streaks in the Lighthouse Nebula discovered with MeerKAT -- Particles escaping from the tail and illuminating the ambient magnetic field
› From cosmological simulations to binary black hole mergers: The impact of using analytical star formation history models on gravitational-wave source populations
› Search for Gamma-ray emission from Abell 119 galaxy cluster using INTEGRAL/ISGRI, COMPTEL, and DAMPE data
› The many boundaries of the stratified dark matter halo
› On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints
› Far-infrared Polarization Properties of Nearby Star-forming Regions: A New Compendium of SOFIA/HAWC+ Observations
› A Unified Scalar-Field Mechanism for the $H_0$, $S_8$ and Evolving Dark-Energy Tensions
› A possible detection of gas rotation in galaxy groups via the kinetic Sunyaev-Zeldovich effect
› Selection--Clustering Coupling and Pair-Midpoint Anisotropy from Observer Motion
› ID-MAGE II: The Star Forming Satellites of Low-Mass Hosts
› Primordial Black Hole interpretation of the subsolar merger event S251112cm
› Why Stellar Sequences Turn Over: Fixed Points, Instability, and Equation-of-State Universality
› The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
› Inpainting to search for premerger massive black hole binaries in realistic LISA datasets
› Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering
› Observing the Peculiar Acceleration of our Solar System with Quasar Proper Motions
› Hybrid neutron stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$
› Reduced incidence of little red dots at z < 3 based on number density and halo mass evolution
› Fast Astronomical Transients in Archival Photographic Plates: Using optical aberrations as a tool for discerning real images, from plate artifacts
› Statistical Field Theory for Weak Gravitational Lensing
› HAMCOR: A physics-driven Hamiltonian framework for inferring AGN coronal geometry from X-ray reverberation lags
› Search for double-line spectroscopic binaries in RAVE survey
› The FAST HI 21-cm Absorption Blind Survey. III. OH Absorption Search in the 21-cm Absorber Sample and Continued HI Absorption Search
› Infrared spectroscopy of gas-phase hydrogenated and methylated pyrenes: from laboratory spectra to the simulated 3.4 $\mu$m emission band
› The PSR J0435+3233 Triple System
› Carbon in J0815+4729: Casting a shadow of doubt on the interpretation of CH absorption in the most primitive stars
› Optical Depths from the Thermal Sunyaev-Zel'dovich Effect with ACT DR6 and DESI DR1 Spectroscopic Galaxies and Optically-Selected Clusters
› Reconstructing Early Primordial Black Hole Domination from Gravitational-Wave Backgrounds
› Breaking the Blend: A multi-tracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST
› An LSST-DESC Precursor Project: Hyper Suprime-Cam Year 1 $3\times2$pt in Harmonic Space
› The GAPS Programme at TNG. LXXX. Characterisation of the 400 Myr old multi-planet system K2-233
› Mass Proxy Quality of Halo Properties in IllustrisTNG and FLAMINGO Simulations: II. Galaxies, Stars, and Black Holes
› Investigating the nature of magnetic turbulence in Tycho's SNR using X-ray observation
› Rotation period of the O giant xi Persei: Coexistence of cyclic and periodic variability. A weakly magnetic candidate star
› Looking for WIMPs through the neutrino fogs
› Neutrino Telescope Event Classification on Quantum Computers
› Scalar nonstandard neutrino interactions in galactic supernovae
› Prominence: A discriminator of gravitational wave signals
› Metastable cosmic strings are broken at the start
› Fermion scattering in a Bose-Einstein condensate
› The Instrumented Baffle at the Input Mode Cleaner of Advanced Virgo Plus: Four years of Successful Operation as a Monitor of Stray Light
› Real versus Complex Fermion Bare Mass and Multi-Wall String Defect Annihilation
› Fire at the Tip of the Throat: Hagedorn Phase after brane-antibrane inflation?
› Particle production from bubble collisions
› Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity
› Color-Kinematics Duality and the Double Copy in Curved Spacetimes
› Joint Model-independent Constraints on the Post-Newtonian Parameter and Cosmic Curvature from Galaxy-scale Strong Lensing, SNe Ia, BAO, and Cosmic Chronometers

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