We present the design and measurements of a 90GHz prototype of a millimeter-wave channelizing spectrometer realized in rectangular waveguide for astronomical instrumentation. The device was fabricated using conventional high-precision metal machining, and the spectrometer can be tiled into a 2D array to fill the focal plane of a telescope. Measurements of the fabricated five-channel device matched well with electromagnetic simulations using HFSS and a cascaded S-matrix approach. This motivated the design of a 54-channel R=200 spectrometer that fills the single-moded passband of rectangular waveguide in the 130-175 GHz and 190-250 GHz atmospheric windows for millimeter-wave spectroscopic mapping and multi-object spectroscopy.
A waveguide spectrometer for high-resolution millimeter-wave imaging
Boston University（波士顿大学）；Cardiff University（卡迪夫大学）；California Institute of Technology（加州理工学院）；Rutherford Appleton Laboratory Space, UKRI（鲁瑟福阿普尔顿实验室空间，英国研究理事会）
A 3D-Printed Millimeter-Wave Inline Waveguide-to-Coplanar-Waveguide Transition to Enable Dense Spectrometer Arrays for Intensity Mapping Surveys
University of Chicago（芝加哥大学）；Kavli Institute for Cosmological Physics, University of Chicago（芝加哥大学卡弗里宇宙物理学研究所）；Dept. of Physics, University of Chicago（芝加哥大学物理系）；Dept. of Astrophysics, University of Chicago（芝加哥大学天体物理学系）；Argonne National Laboratory（阿贡国家实验室）；Dept. of Aeronautics and Astronautics, Massachusetts Institute of Technology（麻省理工学院航空航天系）；NVIDIA Corporation（英伟达公司）
Data reduction pipeline for the SuMAC millimeter-wave spectrometer at the LMT
Boston University（波士顿大学）；Cardiff University（卡迪夫大学）；California Institute of Technology（加州理工学院）；Jet Propulsion Laboratory（喷气推进实验室）；Instituto Nacional de Astrofísica, Óptica y Electrónica（国家天文学、光学和电子学研究所）；The University of Chicago（芝加哥大学）；University of California Santa Barbara（加州大学圣塔芭芭拉分校）；Dalhousie University（达尔豪斯大学）
Spectral characterization and performance of SPT-SLIM on-chip filterbank spectrometers
University of Chicago（芝加哥大学）；Kavli Institute for Cosmological Physics, University of Chicago（芝加哥大学卡弗里宇宙物理研究所）；Cardiff University（卡迪夫大学）；McGill University（麦吉尔大学）；Fermi National Accelerator Laboratory（费米国家加速器实验室）；Enrico Fermi Institute, University of Chicago（芝加哥大学恩里科·费米研究所）；Argonne National Laboratory（阿贡国家实验室）；Boston University（波士顿大学）
SuMAC: On-sky demonstration of multi-pixel on-chip millimeter-wave spectroscopy at the Large Millimeter Telescope
Cardiff University（卡迪夫大学）；Jet Propulsion Laboratory（喷气推进实验室）；Dalhousie University（达尔豪斯大学）；Instituto Nacional de Astrofísica, Óptica y Electrónica（国家天体物理学、光学和电子学研究所）；California Institute of Technology（加州理工学院）；Boston University（波士顿大学）；The University of Chicago（芝加哥大学）；University of California Santa Barbara（加州大学圣巴巴拉分校）
High efficiency superconducting filterbank with impedance-defined resolution for millimeter-wave spectroscopy
CNRS-UCB International Research Laboratory, Centre Pierre Binétruy, IRL 2007, CPB-IN2P3（法国国家科学研究中心-巴黎第七大学国际研究实验室，皮埃尔·比内屈中心）；Lawrence Berkeley National Laboratory（劳伦斯伯克利国家实验室）；Université Paris Cité, CNRS, Astroparticule et Cosmologie（巴黎西岱大学，法国国家科学研究中心，亚原子粒子与宇宙学）
Concept integral field unit spectrometer instrument for the next-generation mm-wave cosmological surveys
Center for Astrophysics | Harvard & Smithsonian（哈佛-史密森天体物理中心）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；DTU-Space（丹麦技术大学空间研究所）；Dept. of Physics and Astronomy, University College London（伦敦大学学院物理与天文系）
DESHIMA 2.0: A 200-400 GHz Ultra-wideband Integrated Superconducting Spectrometer
SRON - Space Research Organisation Netherlands（荷兰空间研究所）；Delft University of Technology（代尔夫特理工大学）；Centro de Astrobiología (CAB), INTA-CSIC（西班牙国家航空航天技术研究所-西班牙高等科研理事会天体生物学中心）
FINER: development of the wideband millimeter-wave receiver system and preparations for first light on the Large Millimeter Telescope
Kitami Institute of Technology（北见工业大学）；Nagoya University（名古屋大学）；The University of Electro-Communications（电气通信大学）；University of Tsukuba（筑波大学）；Waseda University（早稻田大学）；National Astronomical Observatory of Japan（日本国立天文台）；The Graduate University for Advanced Studies (SOKENDAI)（综合研究大学院大学）；The University of Tokyo（东京大学）；Suwa University of Science（諏訪精密工科大学）；Keio University（庆应义塾大学）；National Institute of Information and Communications Technology（信息通信研究机构）；Chalmers University of Technology（查尔姆斯理工大学）；Chiba University（千叶大学）；Hokkaido University（北海道大学）；Instituto Nacional de Astrofísica, Óptica y Electrónica（墨西哥国家天体物理学、光学和电子研究所）；University of Yamanashi（山梨大学）；Osaka Metropolitan University（大阪公立大学）；Japan Aerospace Exploration Agency（日本宇宙航空研究开发机构）
A Wideband Millimeter-wave Receiver at 210-350 GHz for LMT-FINER
National Astronomical Observatory of Japan（日本国立天文台）；The University of Electro-Communications（电气通信大学）；Nagoya University（名古屋大学）；Kitami Institute of Technology（北见工业大学）；Suwa University of Science（诹访科学大学）；National Institute of Information and Communications Technology（信息通信研究机构）；The Graduate University for Advanced Studies (SOKENDAI)（综合研究大学院大学）
A High Efficiency Superconducting On-chip Filterbank with Directional Filters for Integral Field Units in the Sub-millimeter Regime
Delft University of Technology（代尔夫特理工大学）；Space Research Organization Netherlands (SRON)（荷兰空间研究所）；Centro de Astrobiología (CSIC-INTA)（天体生物学中心（西班牙国家航空航天技术研究所/西班牙国家研究委员会））；University of Cologne（科隆大学）
Millimeter Wave and Terahertz Spectra and Global Fit of Torsion-Rotation Transitions in the Ground, First and Second Excited Torsional States of 13CH3OH Methanol
Development of a planar cable-driven parallel robot for submillimeter and terahertz beam mapping measurements
University of Arizona（亚利桑那大学）；California Institute of Technology（加州理工学院）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）；Cornell University（康奈尔大学）
