18 July 2014 Ten things we would do differently today: reflections on a decade of ALMA software development
Author Affiliations +
Abstract
The software for the Atacama Large Millimeter/submillimeter Array (ALMA) that has been developed in a collaboration of ESO, NRAO, NAOJ and the Joint ALMA Observatory for well over a decade is an integrated end-to-end software system of about six million lines of source code. As we enter the third cycle of science observations, we reflect on some of the decisions taken and call out ten topics where we could have taken a different approach at the time, or would take a different approach in today’s environment. We believe that these lessons learned should be helpful as the next generation of large telescope projects move into their construction phases.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Brian Glendenning, Brian Glendenning, Erich Schmid, Erich Schmid, George Kosugi, George Kosugi, Jeffrey S. Kern, Jeffrey S. Kern, Jorge Ibsen, Jorge Ibsen, Manabu Watanabe, Manabu Watanabe, Maurizio Chavan, Maurizio Chavan, Morgan Griffith, Morgan Griffith, Ruben Soto, Ruben Soto, "Ten things we would do differently today: reflections on a decade of ALMA software development", Proc. SPIE 9152, Software and Cyberinfrastructure for Astronomy III, 91521L (18 July 2014); doi: 10.1117/12.2054873; https://doi.org/10.1117/12.2054873
PROCEEDINGS
13 PAGES


SHARE
RELATED CONTENT

The LSST operations simulator
Proceedings of SPIE (August 03 2014)
Software design of the Gemini 8-m Telescopes
Proceedings of SPIE (March 20 1997)
RTS2 meta queues scheduling and its realisation for FLWO...
Proceedings of SPIE (September 12 2012)
Choosing a control system for CCAT
Proceedings of SPIE (July 19 2010)
Data Vault providing simple web access to NRAO data...
Proceedings of SPIE (July 14 2008)
Software for the EVLA: current status
Proceedings of SPIE (July 13 2008)
Software for the EVLA: an update
Proceedings of SPIE (June 26 2006)

Back to Top