My project examining the ISM properties and kinematics in A1689-zD1 has been highlighted in a press release with the National Radio Astronomy Observatory! The full press release can be found here.

This artist’s conception illustrates the complexity of the interstellar medium in A1689-zD1. Reaching far beyond the center of the galaxy, shown here in pink, is an abundant halo of cold carbon gas, fueled by outflows of hot, ionized gas pushing outward from the center. Credit: ALMA (ESO/NAOJ/NRAO), B. Saxton (NRAO/AUI/NSF), IAU/Sky & Telescope.