Translator Disclaimer
Paper
25 July 2000 VLT science operations: the first year
Author Affiliations +
Abstract
On 31 March 2000, the ESO Very Large Telescope (VLT) will complete the first year of science operations. During this first year, Antu (UT1) was operated with two instruments: Focal Reducer/Low Resolution Spectrograph (FORS-1) and Infrared Spectrograph and Array Camera (ISAAC). Both Visitor and Service Mode operations were successfully supported, with roughly equal time spent in each mode. On 1 April 2000, Kueyen (UT2) will begin science operations with two new instruments: UV-Visible Echelle Spectrograph (UVES) and FORS-2. The VLT science operations concept revolves around a distributed operations model. Front-end (proposal, observation, and scheduling preparation support and management) and back-end (quality control, Service Mode data distribution, and archive) operations are executed at ESO headquarters in Garching bei Munchen, Germany. Observation execution and on-line quality control are managed on-site at the Paranal Observatory, Cerro Paranal, Chile. The VLT Data Flow System provides the backbone infrastructure for VLT operations. Here we present an overview of the VLT science operations concept, a summary of the results from Year 1, and a discussion of lessons learned and where the science operations concept had to be adapted to achieve the current level of operations.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David R. Silva, Roberto Gilmozzi, Bruno Leibundgut, and Gautier Mathys "VLT science operations: the first year", Proc. SPIE 4010, Observatory Operations to Optimize Scientific Return II, (25 July 2000); https://doi.org/10.1117/12.392478
PROCEEDINGS
8 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

The new Gemini Observatory archive a fast and low...
Proceedings of SPIE (August 08 2016)
Data interface control at the European Southern Observatory
Proceedings of SPIE (September 16 2004)
Quality control of VLT FLAMES/GIRAFFE data
Proceedings of SPIE (September 16 2004)
Tracking the processing status of Chandra observations
Proceedings of SPIE (January 02 2002)
VISTA data flow system: overview
Proceedings of SPIE (September 16 2004)
ESO data flow system in operations closing the data...
Proceedings of SPIE (July 25 2000)

Back to Top