Imaging Observation Instruments:

Specifications and limiting magnitudes (60-second integration, equivalent to S/N=10 Vega magnitude) of imaging instruments.

InstrumentTelescopeFOV(‘x’)Pixel Scale(“)Limiting Magnitude(mag)RemarksPerson in Charge
MSI 1.6m Pirka 3.3 x 3.3 0.389 17.3U 20.0B 19.9V 19.8Rc 18.7Ic Narrow-band, Broad-band, liquid crystal tunable filter, EM CCD mode Saito
MuSaSHI 0.55m SaCRA 32.9 x 32.0 1.87@PF 0.73@Cas 16.8r 17.1i 17.2z Upper is the primary focus, lower is the Cassegrain focus. riz simultaenous, imaging, polarizationOasa
Tomo-e Gozen 1.05m Schmidt 9 deg Φ 1.17 19 no filter, 2-fps readout Takita
MITSuME 0.5m MITSuME Akeno 28 x 28 1.64 16.7g’ 16.6Rc 15.8Ic g’RcIc simultaneous Ichiro Takahashi
SIRIUS 1.4m IRSF 7.7 x 7.7 0.453 17.7J 17.1H 15.8K JHK simultaneous, Polarization mode, ND filter, Pa β, Br γ, [FeII], H2 filter Kusune
TriCCS 3.8m Seimei Refer to the link below the table Nogami
Visible CCD Kyoto University 0.4m 11.5 x 11.5 1.3 18.2C UBVRI filter Nogami
NIC 2.0m Nayuta 2.7 x 2.7 0.16 15.6J 15.7H 14.7K JHK simultaneous Jun Takahashi
WFGS2 2.0m Nayuta 6.8 x 6.8 0.20 18.2B 18.5V 18.5Rc 18.0Ic g’ r’, i’, with wide-Halpha filter Jun Takahashi
MITSuME 0.5m MITSuME Okayama 26 x 26 1.52 16.9g’ 17.0Rc 15.9Ic g’RcIc simultaneous Murata
HOWPol 1.5m Kanata 15 Φ 0.29 18.4B 19.2V 19.4R 19.1I z’,Hα filter, simultaneous polarization of 2 components Nakaoka
HONIR 1.5m Kanata 10×10 0.29 17.5B 18.6V 18.7R 18.5I 16.6J 15.6H 14.7Ks Visible and near-infrared simultaneous in two colors Nakaoka
kSIRIUS Kagoshima University 1.0m 3.7 x 2.9 0.69 16.3J 15.3H 14.5Ks (270-second integration, S/N=10) JHKs simultaneous Nagayama
MITSuME 1.05m Murikabushi 12.3 x 12.3 0.72 18.7g’ 19.0Rc 17.8Ic g’RcIc simultaneous Hanayama, Hayatsu

For details on the Seimei Telescope TriCCS, please refer to:

Instrument

Check here for the person in charge of the telescope.

ブックマーク パーマリンク.

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