The Atacama Large Millimeter/submillimeter Array (ALMA) Band 10 receiver covering 787 to 950 GHz is the highest frequency receiver of the ten bands envisioned for the ALMA Front End system. The Band 10 receivers have been undergoing installation and commissioning since 2012. After the Band 10 receiver tuning scripts (Josephson currents suppression, LO power optimization) and operation procedures had been developed and implemented, astronomical verification procedures (radio pointing, focus, beam squint, and end-to-end spectroscopic verification) were established in single dish mode at the ALMA Operations Support Facility (OSF; 2900 m elevation). Subsequently, the first Band 10 astronomical fringes were achieved at the Array Operations Site ...
The Atacama Large Millimeter/Submillimeter Array (ALMA) is now entering its 8th cycle of scientific ...
We present a set of compelling science cases for the 31–45 GHz Band 1 ALMA Receiver. The science ran...
The ALMA telescope will be an interferometer of 64 antennas, which will be situated in the Atacama d...
The Atacama Large Millimeter Array (ALMA) is a collaboration between Europe, North America, and Japa...
The Atacama Large Millimeter Array (ALMA) is an interferometer consisting of 64 antennae of 12 m dia...
Aims. We describe the design, construction, and characterization of the Band 9 heterodyne receivers ...
The Atacama Large Millimeter Array (ALMA) is a major ground-based telescope for millimeter and submi...
Artículo de publicación ISIAims. We describe the design, construction, and characterization of the B...
Aims. We describe the design, construction, and characterization of the Band 9 heterodyne receivers ...
This paper describes the design and development of the ALMA Band 9 receiver cartridges. The ALMA pro...
The Atacama Large Millimeter/submillimeter Array (ALMA) combines large collecting area and location ...
The Atacama Large Millimeter Array (ALMA) is a collaboration between Europe, North America, and Japa...
The Atacama Large Millimeter/Submillimeter Array (ALMA) is now entering its 8th cycle of scientific ...
We present a set of compelling science cases for the 31–45 GHz Band 1 ALMA Receiver. The science ran...
The ALMA telescope will be an interferometer of 64 antennas, which will be situated in the Atacama d...
The Atacama Large Millimeter Array (ALMA) is a collaboration between Europe, North America, and Japa...
The Atacama Large Millimeter Array (ALMA) is an interferometer consisting of 64 antennae of 12 m dia...
Aims. We describe the design, construction, and characterization of the Band 9 heterodyne receivers ...
The Atacama Large Millimeter Array (ALMA) is a major ground-based telescope for millimeter and submi...
Artículo de publicación ISIAims. We describe the design, construction, and characterization of the B...
Aims. We describe the design, construction, and characterization of the Band 9 heterodyne receivers ...
This paper describes the design and development of the ALMA Band 9 receiver cartridges. The ALMA pro...
The Atacama Large Millimeter/submillimeter Array (ALMA) combines large collecting area and location ...
The Atacama Large Millimeter Array (ALMA) is a collaboration between Europe, North America, and Japa...
The Atacama Large Millimeter/Submillimeter Array (ALMA) is now entering its 8th cycle of scientific ...
We present a set of compelling science cases for the 31–45 GHz Band 1 ALMA Receiver. The science ran...
The ALMA telescope will be an interferometer of 64 antennas, which will be situated in the Atacama d...