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1. A newly identified emission-line region around P Cygni. Issue 1 (18th August 2018)

2. Correction of Near-infrared High-resolution Spectra for Telluric Absorption at 0.90–1.35 μm. (21st May 2018)

3. Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97-1.32μm. Issue 3 (28th February 2020)

4. Erratum: Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97–1.32 μm. Issue 2 (29th March 2022)

5. Fast optical flares from M dwarfs detected by a one-second-cadence survey with Tomo-e Gozen. (8th August 2022)

6. Highly Sensitive, Non-cryogenic NIR High-resolution Spectrograph, WINERED. (11th January 2022)

7. Method to estimate the effective temperatures of late-type giants using line-depth ratios in the wavelength range 0.97–1.32 μm. Issue 4 (23rd November 2017)

8. The effect of surface gravity on line-depth ratios in the wavelength range 0.97–1.32 µm. Issue 2 (3rd April 2020)

9. Video observations of tiny near-Earth objects with Tomo-e Gozen. (12th July 2022)