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1. A 1.46–2.48 μm spectroscopic atlas of a T6 dwarf (1060 K) atmosphere with IGRINS: first detections of H2S and H2, and verification of H2O, CH4, and NH3 line lists. Issue 3 (30th May 2022)

2. A 1.46–2.48 μm spectroscopic atlas of a T6 dwarf (1060 K) atmosphere with IGRINS: first detections of H2S and H2, and verification of H2O, CH4, and NH3 line lists. Issue 3 (30th May 2022)

3. A 1.46–2.48 μm spectroscopic atlas of a T6 dwarf (1060 K) atmosphere with IGRINS: first detections of H2S and H2, and verification of H2O, CH4, and NH3 line lists. Issue 3 (30th May 2022)

4. A 1.46–2.48 μm spectroscopic atlas of a T6 dwarf (1060 K) atmosphere with IGRINS: first detections of H2S and H2, and verification of H2O, CH4, and NH3 line lists. Issue 3 (30th May 2022)

5. A 1.46–2.48 μm spectroscopic atlas of a T6 dwarf (1060 K) atmosphere with IGRINS: first detections of H2S and H2, and verification of H2O, CH4, and NH3 line lists. Issue 3 (30th May 2022)

6. A search for variability in exoplanet analogues and low-gravity brown dwarfs. Issue 1 (22nd November 2018)

7. Debris Disk Science with the Palomar ExAO System: First Results. Issue Volume 8:Issue S299(2013) (6th January 2014)

9. Low-gravity L Dwarfs Are Likely More Variable. Issue Volume 10:Issue S314(2015) (November 2015)