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- Black hole spin-mass correlation and vector resonant relaxation in gaseous star clusters: the origin of GW231123?
- Setting requirements on out-of-band rejection for next-generation CMB experiments. Application to the LiteBIRD instrument
- Wave Optics Effects from Gravitational Wave Propagation Through Dark Matter Halos
- TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates
- Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies
- Detection and characterization of the temperate super-earth Gliese 48 b
- Revisiting predictions for cosmic-ray antinucleon fluxes from Galactic Dark Matter
- Operating the Fabry-Pérot systems of the European Solar Telescope in multi-aperture mode
- Two successive solar energetic electron events on 24 December 2022
- Unveiling the nonthermal environments of NGC,3411 and NGC,5903 through new MeerKAT observations
- Atmosphere mitigation in cosmic microwave background observations using multifrequency time-domain component separation
- Rotation and outburst-like brightenings in ZZ Ceti stars observed by TESS
- Metal-poor molecular clouds in dwarf galaxies at parsec-scale resolution
- Mass-dependent multiplicity fraction in low-mass stars revealed by astrometry Gaia
- MAXI J1820+070: A rapidly rotating black hole with a mildly truncated disk and warm corona layers in the soft state
- Ion-scale current sheets embedded in the reconnection-jet shear layer of the near-Sun heliospheric current sheet
- UX Men: Detached eclipsing binary as a benchmark candidate
- Phakoseismology: Asteroseismology of gravitationally microlensed stars
- Collisional excitation of E - and Z -ethanimine to model cold molecular clouds
- Forecast for the detectability of patchy hydrogen reionization in WEAVE-QSO measurements of the Lyman-α forest power spectrum at redshift z ≥ 4
- Pulsar glitches due to triggered vortex traps
- The host halo masses of AGNs and quasars at z ∼ 3 − 7 with TNG-Cluster, FLAMINGO and other cosmological galaxy simulations
- Fast Outflow Driven from the Magnetically Arrested Disc
- Channelled versus Isotropic Accretion of Galaxy Groups onto Clusters: Kinematics, Spin Alignment, and Assembly Bias
- Kinematic methods of spiral nature identification: limitations and applicability