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- The white dwarf binary pathways survey – XI. The Gaia - GALEX UV excess sample for systems within 350 pc
- A combined HST and JWST analysis of the stellar population in Draco II
- Modelling stellar convective transport with plumes – II. Transport properties of locally and non-locally driven convection
- Impact of Stochastic Pop III X-ray Binaries on the Cosmological 21-cm Signal
- An Efficient Galaxy Morphology Classification Framework updated with Two-Stage Feature Extraction with AlexNet Encoding and UMAP
- The impact of recombination during tidal disruption events
- PSR B0355+54: An Unexpected Compendium of Nearly All Scintillation Arc Morphologies
- JWST observations of the planetary nebula NGC 6302 IV: PAH spectral characteristics, formation and evolution
- Core-dominated non-Gaussian photometric redshifts in the COSMOS field: a normality test analysis
- A unified cosmographic reconstruction of the Hubble expansion: Bayesian constraints on dark energy and modified-gravity diagnostics
- A Framework for Analysing Nebular-Phase JWST Supernova Spectra with Application to Type Ic SN 2024aecx
- New insights into the Martian ozone deficit problem from an uncertainty propagation study
- The Solar Neighborhood. LVI. The RMSTAR Catalog of the Nearest 3352 M Dwarf Systems and 305 of Their Wide Companions
- The Sensitivity of TESS to Transiting Planets in TOIs with Close-in Stellar Companions
- Evidence for an Extended Hydrogen Outflow on WASP-12 b
- A Forest of Emission Lines Observed by Sunrise III/SUSI above the Solar Limb
- A Possible Complication of Using the 4.14 μ m Band to Assess D/H Ratios on Icy Bodies
- Wave-growth-limited Particle Confinement in a Near-parallel Interplanetary Shock Observed by Parker Solar Probe
- Chandra X-Ray Imaging and an Inverse Compton/Cosmic Microwave Background Model for the Inner Jet of PKS 0637–752
- Sharpening the Mass Measurement of PSR J1048+2339 via High-cadence Photometry
- Asteroseismology of the High-amplitude δ Scuti Star EH Librae
- Synchrotron Emission from Cooled Particle Distributions
- Dynamic Accretion Disk–Corona Connection and Broad Fe K α Variability in Mrk 766 Revealed by Time-resolved High-resolution X-Ray Spectroscopic Analysis
- Markov Chain Monte Carlo for Bayesian Parametric Galaxy Modeling in LSST
- Sublimation of H ₂ O Molecules from Interstellar and Dynamically New Comets: Case Study of 3I/ATLAS