Instruments | Telescope | Wavelength Range | Slit Width (x Length) | Resolution | Limiting Magnitude (mag) | Remarks | In Charge |
---|---|---|---|---|---|---|---|
SuSanoo | 0.55m SaCRA | 0.37-1.0 | Various (up to 10.0″) | 2400@0.66μm with 2.0” slit | 10.5 (approx.) | Limiting magnitude depends on slit viewer. Approximately 10.5 based on experience. | Oasa |
KOOLS-IFU | 3.8m Seimei | N/A | N/A | N/A | N/A | Refer to the link below the table | Nogami |
MALLS | 2.0m Nayuta | 0.38-0.8 | 0.8″,1.2″, 1.6″, 5.0″ x 5′ | 9000@0.66 | 13@0.66μm | Resolution and limiting magnitude are when using 1800l/mm diffraction grating and 0.8″ slit. There’s also a 150l/mm diffraction grating. | Takahashi Hayabusa |
HOWPol | 1.5m Kanata | 0.45-1.1 | 2.3 x 15′ | 500-2300 | 15.2@0.66μm(mid) 16.1@0.66μm(low) | 420g/mm, 1579g/mm | Nakaoka |
HONIR | 1.5m Kanata | Various Ranges | Various Sizes | Various Resolutions | N/A | Simultaneous visible and near-infrared in two colors. The resolution is experimental, and the actual might be slightly lower. | Nakaoka |
High-speed Imaging Spectrometer (Out of Order) | 1.5m Kanata | N/A | 2.3 x 15′ | 150, 9-73 | N/A | Max readout = 35.8 fr./s | Nakaoka |
For more details on the KOOLS-IFU of the Seimei Telescope, please refer to: Device details and ETC.
You can check the person in charge of the telescope here.