Calibration of the Atacama Large Millimeter Array

被引：0

作者：

Mangum, J. G. ^{[1
]}

机构：

[1] Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA

来源：

CALIBRATION AND STANDARDIZATION OF MISSIONS AND LARGE SURVEYS IN ASTRONOMY AND ASTROPHYSICS | 2016年 / 503卷

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中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Atacama Large Millimeter Array (ALMA(1)), which began early science observations in October 2011, is an array of 66 antennas designed to study the universe at millimeter and submillimeter wavelengths. Critical to the quality of the science derived from ALMA is the calibration of its measurements. In the following I describe how the ALMA telescope is calibrated.

引用

页码：69 / 83

页数：15

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