What is D-Shooter NINJA?†
Instrument Specifications†
Coming Soon
Target Science†
kilonova and supernova spectroscopy to uncover their nucleosynthesis and progenitors
high-redshift galaxy spectroscopy to uncover the galaxy formation process
metal-poor galaxy spectroscopy to uncover the first-generation galaxies in the Universe
high-redshift quasar spectroscopy to uncover the origin of supermassive black holes
metal-poor star spectroscopy to uncover the nucleosynthesis in the early Universe
and more! Team Members†
Principal Investigator : Michitoshi Yoshida (Subaru)
Project Manager : Chihiro Tokoku (NAOJ)
Project Scientist : Takashi Moriya (NAOJ)
Instrument Team
Shinobu Ozaki (NAOJ)
Kentaro Motohara (NAOJ)
Yoshito Ono (Subaru)
Yosuke Minowa (Subaru)
Yutaka Hayano (NAOJ)
Kenshi Yanagisawa (NAOJ)
Kosuke Kushibiki (U. Tokyo)
Shogo Homan (U. Tokyo)
Science Team
Yusei Koyama (Subaru)
Masaomi Tanaka (Tohoku U.)
Masami Ouchi (NAOJ/U. Tokyo)
Masayuki Akiyama (Tohoku U.)
Masayuki Tanaka (NAOJ)
Nozomu Tominaga (NAOJ)
Tohru Nagao (Ehime U.)
Yoshiki Matsuoka (Ehime U.)
![[PukiWiki]](image/pukiwiki.png "[PukiWiki]")
NINJA (formerly called D-Shooter) : "Near-INfrared and optical Joint spectrograph with Adaptive optics" is an Optical-to-NIR spectrograph optimized for the LTAO system at the Subaru telescope, realized by the Adaptive Secondary Mirror
It consists of at least two spectrograph units, one is in the optical(0.4-0.9um) and the other in the NIR(0.9-2.5micron).
