Development of the new multi-beam receiver and telescope control system for NASCO
Atsushi Nishimura, Akio Ohama, Kimihiro Kimura, Daichi Tsutsumi, Yudai, Matsue, Rin Yamada, Mariko Sakamoto, Kenta Matsunaga, Yutaka Hasegawa, Taisei, Minami, Takeru Matsumoto, Kazuki Shiotani, So Okuda, Kakeru Fujishiro,, Keisuke Sakasai, Masahiro Suzuki, Shun Saeki

TL;DR
This paper describes the development and current status of a new multi-beam receiver and a flexible, ROS-based control system for the NANTEN2 telescope, aimed at creating an all-sky CO data cube of the southern hemisphere.
Contribution
It introduces a novel 5-beam receiver with dual-band SIS detectors and a reconstructed ROS-based control system for improved flexibility and reliability in telescope operations.
Findings
Receiver and control system installed in December 2019
Commissioning and verification are ongoing
Science operations planned for early 2021
Abstract
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…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Atmospheric Ozone and Climate · Astrophysics and Star Formation Studies
