1. Development of a new wideband heterodyne receiver system for the Osaka 1.85-m mm-submm telescope -- Corrugated horn & Optics covering 210-375 GHz band
- Author
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Yamasaki, Yasumasa, Masui, Sho, Ogawa, Hideo, Kondo, Hiroshi, Matsumoto, Takeru, Okawa, Masanari, Yokoyama, Koki, Minami, Taisei, Konishi, Ryotaro, Kawashita, Sana, Konishi, Ayu, Nakao, Yuka, Nishimoto, Shimpei, Yoneyama, Sho, Ueda, Shota, Hasegawa, Yutaka, Fujita, Shinji, Nishimura, Atsushi, Kojima, Takafumi, Kaneko, Keiko, Sakai, Ryo, Gonzalez, Alvaro, Uzawa, Yoshinori, and Onishi, Toshikazu
- Subjects
Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
The corrugated horn is a high performance feed often used in radio telescopes. There has been a growing demand for wideband optics and corrugated horns in millimeter and submillimeter-wave receivers. It improves the observation efficiency and allows us to observe important emission lines such as CO in multiple excited states simultaneously. However, in the millimeter/submillimeter band, it has been challenging to create a conical corrugated horn with a fractional bandwidth of ~60% because the wavelength is very short, making it difficult to make narrow corrugations. In this study, we designed a conical corrugated horn with good return loss, low cross-polarization, and symmetric beam pattern in the 210-375GHz band (56% fractional bandwidth) by optimizing the dimensions of the corrugations. The corrugated horn was installed on the Osaka 1.85-m mm-submm telescope with the matched frequency-independent optics, and simultaneous observations of 12CO, 13CO, and C18O (J = 2-1, 3-2) were successfully made. In this paper, we describe the new design of the corrugated horn and report the performance evaluation results including the optics., Comment: 22 pages, 15 figures, Accepted for publication in PASJ
- Published
- 2021
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