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- Gas-phase chemistry of C3H3+: a key building block for carbon mass growth in space
- Probing Massive Star Formation with Intrinsic Multiplicity Constraints from TESS Eclipsing Binaries
- Gravitational Microlensing
- Measuring radial flows in disc galaxies
- Isotopic ratios as probes of star formation and the origin of molecular gas in the Central Molecular Zone
- Two Low-Mass-Ratio Microlensing Planets from High-Magnification Events: KMT-2021-BLG-0247 and MOA-2023-BLG-169
- Convergence of Roberts flow dynamos in Eulerian and Lagrangian codes
- Relaxation of a Vlasov gas to an inhomogeneous state due to phase space mixing in an axisymmetric potential: A Newtonian analogy of the Kerr orbital motion
- Discovery of thermal radio recombination line emission toward the high-mass protostar IRAS18162−2048
- N/O-enhanced chemical enrichment by massive stars: the interplay of optically-thick winds and rotation
- Characterizing the hierarchical structure of filaments I. On the origin of the length-mass (L-M) scaling relation
- The age of the Universe from a large sample of the oldest Galactic stars
- From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?
- GA-NIFS: The interplay between feedback and star formation at 3 < z < 9 probed by JWST/NIRSpec IFU
- Evolution of the morphology-density and morphology-mass relations of quiescent galaxies at 0.5 {2}lt;z<$ 2.5 in the COSMOS-Web survey
- A search for periodic active galactic nucleus variability in Gaia Data Release 3
- Scatter, bias, and chaos of satellite orbits in triaxial dark matter haloes
- Breaking the blend: a multitracer kinematic decomposition method for IFS data applied to disentangling the AGN outflow and circumnuclear ring in NGC 5728 with JWST
- Cold stream penetration of virial shocks: fragmentation, coagulation, and disruption in the hot circumgalactic medium
- Morphology Classification for Galaxies in the Kilo Degree Survey Using a Label-efficient Self-supervised Learning Framework
- Reconstructing the Projected Dark Matter Field across 0.1–100 Mpc Scales from the SDSS Survey*
- Multiband Structural Analysis of KiDS-selected Low Surface Brightness Galaxies with Hyper Suprime-Cam Imaging
- Population III Host Candidates at z ∼ 2: Strong He II λ 1640 and Absent Ultraviolet Metal Lines in HETDEX Ly α Emitters
- Atacama Large Millimeter/submillimeter Array (ALMA) ¹² CO(2–1) Gas Dynamics in NGC 315: A Multimethod Benchmark for Supermassive Black Hole Mass Measurement
- The Galaxy Luminosity Functions in ASTRID: Predictions for LSST