The ALMA Science Pipeline

被引：0

作者：

Geers, Vincent C. ^{[1
]}

Davis, Lindsey ^{[2
]}

Hales, Christopher A. ^{[2
]}

Kent, Brian R. ^{[3
]}

Kern, Jeff ^{[2
]}

Kosugi, George ^{[4
]}

Muders, Dirk ^{[5
]}

Nakazato, Takeshi ^{[4
]}

Sugimoto, Kanako ^{[4
]}

Williams, Stewart J. ^{[1
]}

Wyrowski, Friedrich ^{[5
]}

机构：

[1] UK Astron Technol Ctr, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[2] Natl Radio Astron Observ, POB 0,1003 Lopezville Rd, Socorro, NM 87801 USA

[3] Natl Radio Astron Observ, 520 Edgemt Rd, Charlottesville, VA 22903 USA

[4] Natl Astron Observ Japan, Osawa 2-21-1, Mitaka, Tokyo 1818588, Japan

[5] Max Planck Inst Radioastron, Huegel 69, D-53121 Bonn, Nrw, Germany

来源：

ASTRONOMICAL DATA ANALYSIS SOFTWARE AND SYSTEMS XXVI | 2019年 / 521卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Atacama Large Millimeter Array (ALMA) is a radio interferometer composed of 66 antennas located on the Chajnantor plateau at 5 km altitude in northern Chile. With baselines of up to 16 km, ALMA provides unprecedented spatial resolution and sensitivity in the mm/submm wavelength range for the study of star and galaxy formation. The ALMA project is designed to support the research interests of a broad and diverse astronomical community. As part of this support the ALMA science pipeline provides an automated calibration and imaging procedure which produces standard science quality data products for both radio expert and non-radio expert astronomers.

引用

页码：366 / 369

页数：4

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