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1. Connecting black holes and galaxies in faint radio populations at cosmic noon. Issue Volume 15:Issue S352(2019) (June 2019)

2. Measuring the total infrared light from galaxy clusters at z = 0.5–1.6: connecting stellar populations to dusty star formation. Issue 2 (31st October 2020)

3. The Quantum Efficiency and Diffractive Image Artifacts of Si:As IBC mid-IR Detector Arrays at 5–10 μm: Implications for the JWST/MIRI Detectors. (23rd December 2020)

4. The Science Performance of JWST as Characterized in Commissioning. (1st April 2023)