BH

2405.14843

• Accretion onto supermassive black hole binaries

AGN

2405.14809

• Increasing AGN sample completeness using long-term near-infrared variability

2405.14764

• Multi-Messenger Emission Characteristics of Blazars

2405.13479

• The origin of the soft excess in the luminous quasar HE 1029-1401

2405.14269

• The time-variable ultraviolet sky: Active Galactic Nuclei, Stars and White Dwarfs

2405.13148

• Ensemble Variability Properties of Active Galactic Nuclei in the SDSS DR17

2405.13906

• Direct estimates of nitrogen abundance for Seyfert 2 nuclei

  
  
  image.png

2405.13887

• Multi-Zone Modeling of Black Hole Accretion and Feedback in 3D GRMHD: Bridging Vast Spatial and Temporal Scales

SF-Galaxy

2405.13284

• Sub-kiloparsec scaling relations between hot gas, dense gas and star formation rate in five nearby star-forming galaxies

2405.13122

• Ly Halo Properties and Dust in the Circumgalactic Medium of Star-forming Galaxies

Galaxy winds

2405.13121

• Why are thermally- and cosmic ray-driven galactic winds fundamentally different?

Galaxy

2405.13116

• Low CI/CO Abundance Ratio Revealed by HST UV Spectroscopy of CO-rich Debris Disks

CGM

2405.13113

• MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Ly Nebulae at Cosmic Noon

2405.13110

• Host-galaxy stars can dominate the ionizing radiation field of the circumgalactic medium in galaxies at Cosmic Noon