Collaborative Research: Development of an enhanced CARMA for high-fidelity astronomical imaging from cm to mm wavelengths

合作研究：开发增强型 CARMA，用于从厘米到毫米波长的高保真天文成像

• 批准号: 1040504
• 负责人: Anthony C. Readhead
• 金额: $ 227.02万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2010
• 资助国家: 美国
• 起止时间: 2010-10-01 至 2016-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1040504&HistoricalAwards=false
• 关键词: Collaborative; Research; Development; enhanced; CARMA

The Combined Array for Research in Millimeter-wave Astronomy (CARMA) is an array of 23 radio telescopes located at Cedar Flat, in the Inyo Mountains of California. The array is heterogeneous, consisting of six 10-m telescopes belonging to Caltech, nine 6-m telescopes from the Berkeley-Illinois-Maryland Association, and eight 3.5-m telescopes of The University of Chicago. Not all telescopes currently have the capability to observe at the same wavelength or frequency bandpasses simultaneously. The goal of being able to outfit all telescopes with receivers capable of observing at the same bandpass at the same time will soon be realized. A collaboration between Dr. John Carpenter of the California Institute of Technology and Dr. John Carlstrom of The University of Chicago will develop the digital correlators and receivers to fully integrate the CARMA telescopes into a single array that cross-correlates the signals from all 23 antennas simultaneously over the full 8 GHz IF bandwidth of the CARMA receivers. This will provide significantly enhanced observing capability and will enable new discoveries in cosmology (especially the study of galaxy clusters and the Sunyaev-Zel'dovich effect) and star formation (through the study of the chemistry and kinematics of molecular gas in star-forming regions). This work is being funded by NSF's Major Research Instrumentation program though the Division of Astronomical Sciences.

毫米波天文学研究组合阵列（英语：Combined Array for Research in Millimeter-wave Astronomy，简称CARMA）是一个由23个射电望远镜组成的阵列，位于加州的因约山脉的雪松平原。 该阵列是异构的，包括六个属于加州理工学院的10米望远镜，九个来自伯克利-伊利诺伊州-马里兰州协会的6米望远镜，以及八个来自芝加哥大学的3.5米望远镜。 目前，并非所有望远镜都有能力同时在相同的波长或频带上进行观测。 能够为所有望远镜配备能够在同一时间以同一带通进行观测的接收器的目标将很快实现。 加州理工学院的John Carpenter博士和芝加哥大学的John Carlstrom博士将合作开发数字放大器和接收器，以将CARMA望远镜完全集成到一个阵列中，该阵列在CARMA接收器的整个8 GHz IF带宽上同时对来自所有23个天线的信号进行互相关。 这将大大提高观测能力，并将使人们能够在宇宙学（特别是星系团和Sunyaev-Zel'dovich效应的研究）和星星形成（通过研究恒星形成区分子气体的化学和运动学）方面有新的发现。 这项工作是由美国国家科学基金会的主要研究仪器计划通过天文科学部资助。