Development of the new multi-beam receiver and telescope control system for NASCO

• Published in: arXiv.org 2020-12
• Main Authors: Nishimura, Atsushi, Ohama, Akio, Kimura, Kimihiro, Tsutsumi, Daichi, Matsue, Yudai, Yamada, Rin, Sakamoto, Mariko, Matsunaga, Kenta, Hasegawa, Yutaka, Minami, Taisei, Matsumoto, Takeru, Shiotani, Kazuki, Okuda, So, Fujishiro, Kakeru, Sakasai, Keisuke, Suzuki, Masahiro, Saeki, Shun, Satani, Kouki, Urushihara, Kousuke, Kato, Chiharu, Kondo, Takashi, Okawa, Kazuki, Kurita, Daiki, Inaba, Tetsuta, Maruyama, Shohei, Koga, Masako, Noda, Kenya, Kohno, Mikito, Iwamura, Hiroaki, Hyoto, Yuki, Hori, Yuichi, Nishikawa, Kaoru, Nishioka, Takeru, Pang, Thoqin, Sano, Hidetoshi, Enokiya, Rei, Yoshiike, Satoshi, Fujita, Shinji, Hayashi, Katsuhiro, Torii, Kazufumi, Hayakawa, Takahiro, Taniguchi, Akio, Tsuge, Kisetsu, Yamane, Yumiko, Hattori, Yusuke, Ohno, Takahiro, Ueda, Shota, Masui, Sho, Yamasaki, Yasumasa, Kondo, Hiroshi, Suzuki, Kazuji, Kobayashi, Kazuhiro, Fujii, Yasunori, Fujii, Yumi, Minamidani, Tetsuhiro, Okuda, Takeshi, Yamamoto, Hiroaki, Tachihara, Kengo, Onishi, Toshikazu, Mizuno, Akira, Ogawa, Hideo, Fukui, Yasuo
• Format: Article
• Language: English
• Subjects: Carbon monoxide; Control systems; Polarization; Robot control; Separation; Sky surveys (astronomy); Southern Hemisphere; Spectrometers; Telescopes
• ISSN: 2331-8422

We report the current status of the NASCO (NAnten2 Super CO survey as legacy) project which aims to provide all-sky CO data cube of southern hemisphere using the NANTEN2 4-m submillimeter telescope installed at the Atacama Desert through developing a new multi-beam receiver and a new telescope control system. The receiver consists of 5 beams. The four beams, located at the four corners of a square with the beam separation of 720\(''\), are installed with a 100 GHz band SIS receiver having 2-polarization sideband-separation filter. The other beam, located at the optical axis, is installed with a 200 GHz band SIS receiver having 2-polarization sideband-separation filter. The cooled component is modularized for each beam, and cooled mirrors are used. The IF bandwidths are 8 and 4 GHz for 100 and 200 GHz bands, respectively. Using XFFTS spectrometers with a bandwidth of 2 GHz, the lines of \(^{12}\)CO, \(^{13}\)CO, and C\(^{18}\)O of \(J\)=1\(-\)0 or \(J\)=2\(-\)1 can be observed simultaneously for each beam. The control system is reconstructed on the ROS architecture, which is an open source framework for robot control, to enable a flexible observation mode and to handle a large amount of data. The framework is commonly used and maintained in a robotic field, and thereby reliability, flexibility, expandability, and efficiency in development are improved as compared with the system previously used. The receiver and control system are installed on the NANTEN2 telescope in December 2019, and its commissioning and science verification are on-going. We are planning to start science operation in early 2021.