Extra-solar planets exploration using frequency comb: Infrared Doppler instrument for the Subaru telescope (IRD)

被引：0

作者：

Tamura, Motohide ^{[1
]}

Kotani, Takayuki ^{[1
]}

Nishikawa, Jun ^{[1
,2
]}

Kurokawa, Takashi ^{[1
,4
]}

Kashiwagi, Ken ^{[4
]}

Suto, Hiroshi ^{[1
]}

Sato, Bun'ei ^{[3
]}

Aoki, Wak ^{[1
,2
]}

Usuda, Tomonori ^{[1
,2
]}

Nishiyama, Shogo ^{[5
]}

Ikeda, Yuji ^{[6
]}

Hall, Donald B. ^{[7
]}

Hodapp, Klaus W. ^{[7
]}

Jacobson, Shane ^{[7
]}

Morino, Jun-Ichi

Okuyama, Yasushi ^{[4
]}

Tanaka, Yoichi ^{[4
]}

Suzuki, Shoya ^{[4
]}

Inoue, Sadahiro ^{[4
]}

Kwon, Jungmi

Oh, Dehyun ^{[2
]}

Baba, Haruka ^{[1
,2
]}

Hashimoto, Jun ^{[8
]}

Kudo, Tomoyuki ^{[9
]}

Kusakabe, Nobuhiko ^{[1
]}

Omiya, Masashi ^{[1
]}

Yamamuro, Tomoyasu ^{[10
]}

机构：

[1] Univ Tokyo, Tokyo 1130033, Japan

[2] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[3] GUAS, Mitaka, Tokyo 1818588, Japan

[4] Tokyo Inst Technol, Meguro Ku, Tokyo 1528550, Japan

[5] Tokyo Univ Agr & Technol, Koganei, Tokyo 1848588, Japan

[6] Miyagi Univ Educ, Aoba Ku, Sendai, Miyagi 9800845, Japan

[7] Photocoding, Sakyo Ku, Kyoto 6060025, Japan

[8] Univ Hawaii, Inst Astron, Hilo, HI 96720 USA

[9] Univ Oklahoma, Norman, OK 73019 USA

[10] Subaru Telescope, Hilo, HI 96720 USA

来源：

2015 OPTICAL FIBER COMMUNICATIONS CONFERENCE AND EXHIBITION (OFC) | 2015年

关键词：

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

Because of their large numbers, red dwarfs may be the most abundant planet hosts in our Galaxy. In order to detect Earth-like planets around nearby red dwarfs (in particular late-M stars), it is crucial to conduct the precise radial velocity (RV) measurements at near-infrared wavelengths where these stars emit most of light. We report the development of the Infrared Doppler (IRD) spectrometer for the Subaru telescope. IRD is a fiber-fed, high-precision, near infrared spectrometer with a spectral resolution of R similar to 70,000 covering from 0.97 to 1.75 mu m. To achieve 1m/s RV measurement precision, we employ our original laser frequency comb of a wide wavelength coverage as an extremely stable wavelength standard in the near-infrared. The spectrometer optics is composed of a new wide-pitch Echelle-grating and Volume-Phase Holographic gratings. To achieve ultimate thermal stability, very low thermal expansion ceramic is used for most of the optical components including the optical bench. The spectrometer will utilize a 4096x4096-pixel HgCdTe array,

引用

页数：3

共 21 条

[21] Doppler-free spectroscopy using a mid-infrared optical parametric oscillator linked to a frequency comb generator
Vainio, Markku
Merimaa, Mikko
Halonen, Lauri
2011 JOINT CONFERENCE OF THE IEEE INTERNATIONAL FREQUENCY CONTROL SYMPOSIUM/EUROPEAN FREQUENCY AND TIME FORUM PROCEEDINGS, 2011, : 701 - 705

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