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Astronomia w Krakowie
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Sunset from the kitchen window
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 News from astronomynow.com
› Nova outburst in Centaurus
› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
› Binoculars to boost your night-sky viewing
RSS  Latest preprints on astro-ph:
› Advanced stereoscopy applied to CTAO
› Debris disks and their properties with the Habitable Worlds Observatory
› Upper Limit on the Non-Gravitational Acceleration and Lower Limits on the Nucleus Mass and Diameter of 3I/ATLAS
› The stability of propagating plane inertial waves in rotating fluids
› First Light for the GRAVITY+ Adaptive Optics: Extreme Adaptive Optics for the Very Large Telescope Interferometer
› Formation of multiple dynamical classes in the Kuiper belt via disk dissipation
› Dynamical Pathways to the Misalignment of the VHS 1256-1257 System
› Stochastic analysis of ultra-high energy cosmic ray interactions
› Radio Stars in the Era of New Observatories
› Constraining GREA, an alternative theory accounting for the present cosmic acceleration
› Characterizing Temperatures of Flares on the M Dwarf Wolf 359 from Simultaneous Multiband Optical Observations
› The EBLM project XVI. Spin-orbit alignment of the low mass eclipsing binary EBLM J0021-16
› HR6819: a puffed-up stripped star system challenging stable mass transfer theory
› Unveiling Obscured Accretion in the Local Universe
› Performance characterization of a new Structural and Thermal Architecture for a future spaceborne Closed-Cycle Dilution Refrigerator
› A Combined TESS and Ground-based Study of Transit Timing Variations in HAT-P-16, TOI-1516 and TOI-2046 Systems
› BlackTHUNDER: evidence for three massive black holes in a z~5 galaxy
› Limb Asymmetries on WASP-39b: A Multi-GCM Comparison of Chemistry, Clouds, and Hazes
› Visualizing the mass transfer flow in direct-impact accretion
› Extreme Geomagnetic Storm on Early Earth Induced by Corotating Interaction Regions from the Young Sun
› A nearly pristine star from the Large Magellanic Cloud
› BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season
› Adaptive Reconstruction of Cluster Halos (ARCH): Integrating Shear and Flexion for Substructure Detection
› A Disk-Originated 329-day Quasi-Periodic Oscillation in the Seyfert 1 Galaxy J1626+5120
› First results from ALPPS: a sub-Alfv\'enic streamer in SVS13A
› MESA Isochrones and Stellar Tracks (MIST) III. The White Dwarf Cooling Sequence
› FITrig: A High-Performance Detection Technique for Efficient Ultra-Long-Period Pulsars
› Multidisciplinary analysis of pit craters at Hale Crater, Mars
› Mapping CO Ice in a Star-Forming Filament in the 3 kpc Arm with JWST
› Helium-burning blue large-amplitude pulsators: A Population Study with BPASS
› The Draco Dwarf Spheroidal Galaxy in the First Year of DESI Data
› Weakly model-independent determination of total expansion during inflation
› The EDGE-CALIFA Survey: Influence of Mergers on Radial Profiles of Star-Formation Properties
› Baseline-Aware Dependence fitting for DAmping Timescales (BADDAT): A Nearly Unbiased Approach to Constraining Optical Variability Dependence on Physical Properties of Active Galactic Nuclei
› Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in Near Future
› Fermi detection of $\gamma$-rays from the radio-quiet Seyfert galaxy NGC 3281
› Origin of gas in the Magellanic Bridge: MeerKAT detection of HI 21-cm absorption
› Mass stratification in the globular cluster system revealing the assembly history of the nearest S0 galaxy NGC 3115
› Revisiting 3C 279 jet morphology with space VLBI at 26 microarcsecond resolution
› Exploring the Early Universe with Deep Learning
› Optimization procedure of the baffle of the GroundBIRD Telescope to mitigate stray light
› Next-day observation processing for the LST-1 and MAGIC
› High-redshift Merger-induced Bar-like Galaxies in IllustrisTNG
› Probing the Topology of the Early Universe using CMB Temperature and Polarization Anisotropies
› Low-mass companions to nine stars
› Photometric Redshift Forecast for 7-Dimensional Sky Survey
› The impact of cosmic filaments on the abundance of satellite galaxies
› Detection of HI filament: Pair Stacking vs. Filament Stacking
› Investigating solid-state CH3OH formation with chemical modelling
› Particle Acceleration and Transport in the Large-scale Current Sheet under an Erupting Magnetic Flux Rope
› Stairway to Axions: the cross-correlation of birefringence and galaxies from NPIPE and Quaia
› Starshades as technosignatures in direct imaging phase curves: Application to the Habitable Worlds Observatory targets
› Coupled non-canonical scalar field to neutrinos could alleviate the Hubble tension and cross the phantom barrier
› Galaxy Zoo: Cosmic Dawn -- morphological classifications for over 41,000 galaxies in the Euclid Deep Field North from the Hawaii Two-0 Cosmic Dawn survey
› Ion-neutral chemistry at icy moons: the case of Ganymede
› N+2 Mapmaking for Polarized CMB Experiments
› First direct detection of an RR Lyrae star conclusively associated with an intermediate-age cluster
› AGN spectral variability across activity states and searches for axion-like particles
› Searching for Corannulene with ALMA: Observations of the Red Rectangle Nebula
› The Simons Observatory: Characterization of the 220/280 GHz TES Detector Modules
› Choked jets in BSG/RSG as possible sources of high-energy neutrinos
› The Diamond Ring in Cygnus X: Advanced stage of an expanding bubble of ionised carbon
› Hyper-py: HYbrid Photometry and Extraction Routine in PYthon
› halox: Dark matter halo properties and large-scale structure calculations using JAX
› SDSS-C4 3028: The Nearest Blue Galaxy Cluster Devoid of an Intracluster Medium
› The Origins & Reservoirs of Exocomets
› Tomographic Distance Measurements to the Smith Cloud with SDSS-V Milky Way Mapper3
› Small Near-Earth Objects in the Taurid Resonant Swarm
› High Proper Motion Discoveries from the UKIRT Hemisphere Survey
› Overview of the ESCAPE Dark Matter Test Science Project for Astronomers
› Black Hole Polarimetry II: The Connection Between Spin and Polarization
› The alignment between brightest cluster galaxies and host clusters
› Asymptotics of spherical dynamos exhibiting a small-scale MAC balance
› Forecasting Seismic Waveforms: A Deep Learning Approach for Einstein Telescope
› Electrostatic waves in astrophysical Druyvesteyn plasmas: I. Langmuir waves
› A Python Interface for Numerical Relativity Program AMSS-NCKU
› Automating Sensor Characterization with Bayesian Optimization
› No room for monopole dark matter
› Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector
› Vector Resonant Relaxation and Statistical Closure Theory. II. One-loop Closure
› When backgrounds become signals: neutrino interactions in xenon-based dark matter detectors
› Engaging and Educating Eclipse Observers Through Workshops, Media, Planetarium shows and Citizen Science
› Swift Memory Burden in Merging Black Holes: how information load affects black hole's classical dynamics
› Likelihood-free inference for gravitational-wave data analysis and public alerts
› Gravitational Waves from Magnetars
› First direct carbon abundance measured at $z>10$ in the lensed galaxy MACS0647$-$JD
› Outer Solar System spacecraft to probe the $\mu$Hz gravitational wave frontier
› Innovative SiC ultraviolet instrumentation development with potential applications for the Habitable Worlds Observatory
› Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run
› Probing inflationary gravitational waves with cross-correlations: improved forecasting and validation with simulations
› Constraints on AvERA Cosmologies from Cosmic Chronometers and Type Ia Supernovae
› High-energy gamma-ray emission from memory-burdened primordial black holes
› A $\nu$ look at the Sun: Probing the conditions of the solar core using $^8$B neutrinos
› Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z$\sim$1.3
› Hot Diggity Dog: Simultaneous CO and Dust Modeling of the Most Luminous WISE Hot Dust-Obscured Galaxy Unveils Extreme Molecular Gas Excitation
› Resolving Individual Signals in the Presence of Stochastic Background in Future Pulsar Timing Arrays
› The first direct imaging of the silhouette of a damped Lyman $\alpha$ system along the line-of-sight to a background galaxy
› Power law $\alpha$-Starobinsky inflation
› SN 2023gpw: exploring the diversity and power sources of hydrogen-rich superluminous supernovae
› Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the dynamical companion to $\alpha$ Orionis from HST
› Transfer learning for multifidelity simulation-based inference in cosmology
› GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
› A Fuzzy Situation Eased: Cold Dark Matter with Multipoles Can Explain The Double Radio Quad Lens HS 0810+2554
› Fast Rotators at Cosmic Noon: Stellar Kinematics for 15 Quiescent Galaxies from JWST-SUSPENSE
› JWST lens model for A370: A very low dark matter fraction for a brightest cluster galaxy and lensing properties for the Dragon arc
› Comparing the Architectures of Multiplanet Systems from Kepler, K2, and TESS Data
› Gravitational Redshift for Rapidly Rotating Neutron Stars
› Constraints on the diffuse flux of multi-PeV astrophysical neutrinos obtained with the Baikal Gigaton Volume Detector
› Eclipse timing variations in 7 post-common envelope binaries: an update on recent circumbinary models
› Effects of Lorentz invariance violation on charged particles and photon production in astrophysical sources
› Euclid preparation. Simulating thousands of Euclid spectroscopic skies
› Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
› GPI+SPHERE detection of a 6.1 $M_{\text{Jup}}$ circumbinary planet around HD 143811
› Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
› Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking
› Propeller effect in action: Unveiling quenched accretion in the transient X-ray pulsar 4U 0115+63
› CWT-LSTM Autoencoder: A Novel Approach for Gravitational Wave Detection in LIGO Data
› The Discovery of a Large Active Wind from the Milky Way's Central Black Hole
› Light curves of time-dependent accretion disk in tidal disruption events
› A Search for High-Energy Emission from the Remnant of Supernova 1181
› An Educational Guide for 2D Stellar Structure Calculations of Rapidly Rotating Stars using the ESTER code
› A GLIMPSE of Intermediate Mass Black holes in the epoch of reionization: Witnessing the Descendants of Direct Collapse?
› Outflow-cloud interaction as the possible origin of the peculiar radio emission in the tidal disruption event AT2018cqh
› Constraining the pseudo-Dirac nature of neutrinos using astrophysical neutrino flavor data
› Contemporaneous Appearances of Auroral Spiral and Transpolar Arc: Polar UVI Observations and Global MHD Simulations
› Biased domain walls: faster annihilation, weaker gravitational waves
› Induced Gravitational Waves as Cosmic Tracers of Leptogenesis
› Freeze-in gravitational waves and dark matter in warm inflation
› Magnetic Monopole Molecules
› Attention U-Net for all-sky continuous gravitational wave searches
› Regression of Suspension Violin Modes in KAGRA O3GK Data with Kalman Filters

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