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- Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider
- Even central galaxies feel their environment: cosmic siphoning of cool gas accretion
- 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
- UCLCHEM 4.0: An open source gas-grain astrochemistry simulation framework
- Stellar Population Spectra Incorporating Detailed Binary Evolution using POSYDON
- Toward Bayesian photometric cosmic chronometers: Application to VIPERS
- 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
- Link between the properties of circumgalactic outflows and the recent star formation history of their host galaxies
- 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
- Euclid Quick Data Release (Q1). XLIII. The Strong Lensing Discovery Engine F -- Bright and low-redshift strong lenses
- Measuring the Milky Way potential with the phase snail shape curves
- Uncertainty-Aware Deep Learning for the Lyα Forest: CNN-Based Absorber Detection and Characterization
- On what scales does strong lensing robustly constrain the mass profile of low-mass perturbers?