Solar & stellar physics
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- What visibility-graph curvature measures in Forbush decreases: a calibration on the two largest events of solar cycle 25
- The Best Guess: Testing new and old formalisms for the common envelope against observations
- Stellar Population Spectra Incorporating Detailed Binary Evolution using POSYDON
- A measurement-based approach to equivalent power flux density calculation, to quantify the impact of satellite mega-constellations on low-frequency radio astronomy
- Extended J-band spectroscopy of red supergiants: Parameter identifiability and metallicity robustness
- What powers the most energetic flares in the field? Kepler. Revisiting the superflaring star KIC 2852961
- A deep learning algorithm for black hole spin estimation using hot spot secondary images
- FastSpec : Fast and versatile stellar spectrum synthesis code
- Spectral classification of OB-type stars using tree-based ensemble methods and evaluation of their explainability
- Global solar compressible convection simulations on non-Cartesian mappings
- Magnetic conditions governing the transition to penumbral magneto-convection
- Frequency-dependent time delays in Sgr A* from a broadband VLA observation
- Sulphur-bearing molecule survey towards prestellar and starless cores in the Perseus molecular cloud
- Data-driven characterisation of variable source light curves with multimodal representation learning
- eROSITA all-sky survey - stars and optical loading
- 21cmEMUv3: A hybrid diffusion and long short-term memory emulator of 21cmFAST summary observables
- Measuring the Milky Way potential with the phase snail shape curves
- Sea Ice as an Origin of Life Location for Hycean and Ocean Worlds
- Non-Axisymmetric Pillar Structures due to Embedded Stars in AGN Accretion Discs
- Alien Skies: Visibility of Planetary Retrograde Motion from Rocky Habitable-Zone Worlds
- Dust-seeding Molecules in a Massive Protostar—Detection of TiO in Orion Source I
- Reconnection-driven Plasma Loading for Prompt Emission in Tidal Disruption Event Jets
- Assessing Accumulation and Erosion of Interplanetary Coronal Mass Ejections Using Lined-up Spacecraft
- Improved Constraints on the Surface of LHS 3844 b from Its Mid-infrared Spectrum
- Transonic Solutions for Recombination-driven Stellar Winds