Atmospheric phase characteristics of the ALMA long baseline-Reference-Cited by-同舟云学术

Atmospheric phase characteristics of the ALMA long baseline

Published:2016-07-27 Issue: Volume: Page:
ISSN:0277-786X
Container-title:SPIE Proceedings
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Author:

Matsushita Satoki¹,Asaki Yoshiharu²,Fomalont Edward B.²,Barkats Denis³,Corder Stuartt A.²,Hills Richard E.⁴,Kawabe Ryohei⁵,Maud Luke T.⁶,Morita Koh-Ichiro²,Nikolic Bojan⁴,Tilanus Remo P. J.⁷,Vlahakis Catherine²

Affiliation:

1. Academia Sinica Institute of Astronomy and Astrophysics (Taiwan)

2. Joint ALMA Observatory (Chile)

3. Harvard-Smithsonian Ctr. for Astrophysics (United States)

4. Cavendish Lab., Univ. of Cambridge (United Kingdom)

5. National Astronomical Observatory of Japan (Japan)

6. Leiden Observatory (Netherlands)

7. Leiden Observatory, Leiden Univ. (Netherlands)

Publisher

SPIE

Reference35 articles.

1. ALMA: status report on construction and early results from commissioning;Hills,July 2010

2. The 2014 ALMA Long Baseline Campaign: An Overview;Fomalont,July 2015

3. THE 2014 ALMA LONG BASELINE CAMPAIGN: OBSERVATIONS OF ASTEROID 3 JUNO AT 60 KILOMETER RESOLUTION

4. THE 2014 ALMA LONG BASELINE CAMPAIGN: FIRST RESULTS FROM HIGH ANGULAR RESOLUTION OBSERVATIONS TOWARD THE HL TAU REGION

5. THE 2014 ALMA LONG BASELINE CAMPAIGN: OBSERVATIONS OF THE STRONGLY LENSED SUBMILLIMETER GALAXY HATLAS J090311.6+003906 AT z = 3.042

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