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- Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields
- The clumpy fraction of galaxies at z=1−9 with JADES: evidence for a mass-dependent transition in clump origin
- Resonant three-mode coupling in asteroseismology I: Bifurcations, chaos, and DAV white-dwarf outbursts
- Tight asteroseismic upper limits on hot subdwarf magnetism
- Identifying a jet-shaped point-symmetric morphology in the supernova remnant HB9
- Exponential Growth of Turbulent Cross Helicity in Shear-Flow-Driven Turbulence
- Hybrid Stars with Different Amount of Quark Matter
- KMOS Spectroscopic Follow-up of 16 Star Cluster Candidates of the Sagittarius Dwarf Galaxy
- Photometric variability of blue supergiants: Constraints on stellar masses and evolutionary stages
- Revisiting the Unknown Unknowns in Transient Astrophysics with the SKA Telescopes
- Data-Driven Ages from Asteroseismology for FGK Dwarfs
- Coevolution of Dust Growth and Gravitational Instability in Massive Protostellar Disks
- Real-Time 24-hour Ahead Forecasting of Solar Energetic Particle Events with SEPNET-PRISM-R
- The Effect of Field Line Tracing Height on Wang-Sheeley-Arge Solar Wind Predictions at Earth
- Orbital Parameters for 65 Wide Binary Systems: no evidence for gravitational anomaly at low acceleration
- Hidden engines in tidal disruption events: multimessenger signatures in a lepto-hadronic framework
- On the Stability of Tolman Oppenheimer Volkoff Fireholes
- Deriving Interplanetary Sector Boundary Crossings using Potential Field Source Surface Modeling
- The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres
- Pulsar J1909+0749 and Supernova Remnant G42.1-0.2: A case of a pulsar that has exited the shell of its associated supernova remnant
- Constraints on Dark Matter Annihilation from Starlight-Induced Inverse Compton Emission in Omega Centauri
- On the superbursts as photodisintegrators of ashes from the rp-process -- Numerical simulations of superbursts with MESA II
- Rapid Variability of Radiative Signatures from Driven Relativistic Reconnection
- Direct Urca process facilitated by non-Fermi-liquid quantum criticality
- Two-Component Dark Matter and Strongly First-Order Electroweak Phase Transition via a Two-Step Mechanism in the Inert Doublet plus Real Singlet Model