Development of a new wideband heterodyne receiver system for the Osaka 1.85 m mm-submm telescope: Corrugated horn and optics covering the 210-375 GHz band
Development of a new wideband heterodyne receiver system for the Osaka 1.85 m mm-submm telescope: Corrugated horn and optics covering the 210-375 GHz band
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为大阪 1.85 m mm-submm 望远镜开发新型宽带外差接收器系统:覆盖 210-375 GHz 频段的波纹喇叭和光学器件
DOI:
10.1093/pasj/psab062
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发表时间:
2021
影响因子:
2.3
通讯作者:
Gonzalez A
中科院分区:
文献类型:
--
作者:
Yamasaki Y.;Masui S.;Ogawa H.;Kondo H.;Matsumoto T.;Okawa M.;Yokoyama K.;Minami T.;Konishi R.;Kawashita S.;Konishi A.;Nakao Y.;Nishimoto S.;Yoneyama S.;Ueda S.;Hasegawa Y.;Fujita S.;Nishimura A.;Kojima T.;Kaneko K.;Sakai R.;Gonzalez A
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 as they improve observation efficiency and allow 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 210–375 GHz 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 matched frequency-independent optics, and simultaneous observations of12CO,13CO, and C18O (J= 2–1, 3–2) were successfully made. We describe the new design of the corrugated horn and report the performance evaluation results including the optics.