6 August 2014 Translating PI observing proposals into ALMA observing scripts
Author Affiliations +
Abstract
The ALMA telescope is a complex 66-antenna array working in the specialized domain of mm- and sub-mm aperture synthesis imaging. To make ALMA accessible to technically inexperienced but scientifically expert users, the ALMA Observing Tool (OT) has been developed. Using the OT, scientifically oriented user input is formatted as observing proposals that are packaged for peer-review and assessment of technical feasibility. If accepted, the proposal’s scientifically oriented inputs are translated by the OT into scheduling blocks, which function as input to observing scripts for the telescope’s online control system. Here I describe the processes and practices by which this translation from PI scientific goals to online control input and schedule block execution actually occurs.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Harvey Steven Liszt, Harvey Steven Liszt, "Translating PI observing proposals into ALMA observing scripts", Proc. SPIE 9149, Observatory Operations: Strategies, Processes, and Systems V, 91490N (6 August 2014); doi: 10.1117/12.2055781; https://doi.org/10.1117/12.2055781
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

The SKA low frequency aperture array
Proceedings of SPIE (August 08 2016)
The ALMA OT in early science: supporting multiple customers
Proceedings of SPIE (September 23 2012)
Submillimeter array
Proceedings of SPIE (July 30 1998)
ALMA: the first year of observations
Proceedings of SPIE (September 12 2012)
Remote observing with the 30-m radiotelescope
Proceedings of SPIE (June 01 2000)

Back to Top