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- Nine new eclipsing accreting ultracompact white dwarf binaries from the Zwicky Transient Facility
- Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. IV. Heavy Element Enhanced Stars
- Identifying narrow-band mutual coupling resonances in SKA-low stations using frequency-independent current basis functions
- Analysis of Multi-Wavelength Data for 30 Galactic Emission-Line Stars with Dusty Envelopes
- Channelled versus Isotropic Accretion of Galaxy Groups onto Clusters: Kinematics, Spin Alignment, and Assembly Bias
- Diamonds in the sky: the shape of gravitational waves from cosmic string cusps
- Benchmarking Quantum Neural Networks Developed for MBHB Coalescence in the Context of LISA Space Mission
- Mapping cluster angular momentum with the rotational kinetic Sunyaev-Zel'dovich effect
- Recent advances in numerical modeling of solar inertial modes
- Preparation of a celestial field for precise VLBI observations of the JUICE spacecraft: a test case of the Venus flyby
- A MUSE and MeerKAT study of dynamics and star formation in HCG 16
- Sequince: a modular sequential Monte Carlo toolkit
- Looking for gravitational waves with orbital dynamics: GUEST mission and the μHz band of Gravitational Waves
- Energy-Dependent Hard X-Ray QPP Modulation in M- and X-Class Solar Flares Observed by Aditya-L1/HEL1OS
- VERITAS Limits on Dark Matter Annihilation in the Galactic Center Halo
- Tidal disruption or plunge: the role of neutron star internal structure in black hole-neutron star mergers
- The first mass peak of merging black holes from core binding energies and jet-driven explosions
- RAKI: High-Order Alternative Finite Differences for General Relativistic Magnetohydrodynamics
- The stellar orbit distribution of 24 late-type galaxies observed by MUSE
- Robust statistical significance for Gravitational Wave inference
- Dwarf Galaxy Reticulum II's MeerKAT L-Band Observation: Constraining WIMP Dark Matter
- The Radio Neutrino Observatory in Greenland (RNO-G) - System Design and Instrumentation
- Search for Cosmic Rays in GRANDProto300
- Feeding or Fleeing: The Impact of Enhanced Early Black Hole Growth on Circumgalactic Clumps at z > 6
- Dust growth in the early Universe: insight from the NewCluster spin-off simulation