Atacama Compact Array Antennas
Masao Saito, Junji Inatani, Kouichiro Nakanishi, Takahiro Naoi, Masumi, Yamada, Hiro Saito, Bungo Ikenoue, Yoshihiro Kato, Kou-ichiro Morita,, Norikazu Mizuno, Satoru Iguchi

TL;DR
This paper presents comprehensive performance test results of the Atacama Compact Array antennas, demonstrating their high accuracy, stability, and speed, crucial for the ALMA observatory's scientific missions.
Contribution
It provides detailed performance metrics and validation results for the ACA antennas, highlighting their suitability for high-precision astronomical observations.
Findings
Pointing accuracy within 2.0 arcsec
Surface accuracy below 25 micrometers
Path-length stability of 15 micrometers over 3 minutes
Abstract
We report major performance test results of the Atacama Compact Array (ACA) 7-m and 12-m antennas of ALMA (Atacama Large Millimeter/submillimeter Array). The four major performances of the ACA antennas are all-sky pointing (to be not more than 2.0 arcsec), offset pointing (to be < 0.6 arcsec) surface accuracy (< 25(20) micrometer for 12(7)m-antenna), stability of path-length (15 micrometer over 3 min), and high servo capability (6 degrees/s for Azimuth and 3 degrees/s for Elevation). The high performance of the ACA antenna has been extensively evaluated at the Site Erection Facility area at an altitude of about 2900 meters. Test results of pointing performance, surface performance, and fast motion capability are demonstrated.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Radio Astronomy Observations and Technology · Astronomical Observations and Instrumentation
