1. A Warm Near-Infrared High-Resolution Spectrograph with Very High Throughput (WINERED)
- Author
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Kondo, Sohei, Ikeda, Yuji, Kobayashi, Naoto, Yasui, Chikako, Mito, Hiroyuki, Fukue, Kei, Nakanishi, Kenshi, Kawanishi, Takafumi, Nakaoka, Tetsuya, Otsubo, Shogo, Kinoshita, Masaomi, Kitano, Ayaka, Hamano, Satoshi, Mizumoto, Misaki, Yamamoto, Ryo, Izumi, Natsuko, Matsunaga, Noriyuki, and Kawakita, Hideyo
- Subjects
Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
WINERED is a newly built high-efficiency (throughput$ > 25-30\%$) and high-resolution spectrograph customized for short NIR bands at 0.9-1.35 ${\rm \mu}$m. WINERED is equipped with ambient temperature optics and a cryogenic camera using a 1.7 ${\rm \mu}$m cut-off HgCdTe HAWAII-2RG array detector. WINERED has two grating modes: one with a conventional reflective echelle grating (R$\sim$28,300), which covers 0.9-1.35 $\mu$m simultaneously, the other with ZnSe or ZnS immersion grating (R$\sim$100,000). We have completed the development of WINERED except for the immersion grating, and started engineering and science observations at the Nasmyth platform of the 1.3 m Araki Telescope at Koyama Astronomical Observatory of Kyoto-Sangyo University in Japan. We confirmed that the spectral resolution ($R\sim$ 28,300) and the throughput ($>$ 40\% w/o telescope/atmosphere/array QE) meet our specifications. We measured ambient thermal backgrounds (e.g., 0.06 ${\rm [e^{-}/sec/pixel]}$ at 287 K), which are roughly consistent with that we expected. WINERED is a portable instrument that can be installed at any telescope with Nasmyth focus as a PI-type instrument. If WINERED is installed on a 10 meter telescope, the limiting magnitude is expected to be J=18-19, which can provide high-resolution spectra with high quality even for faint distant objects., Comment: 9 pages, 7 figures
- Published
- 2015