30 September 2004 Instrument remote control project at TNG: SARG implementation
Author Affiliations +
Abstract
The high resolution spectrograph at TNG (SARG), mounted at the telescope in 2000, is based on the 'first generation CCD controller, transputers and VME real time computer that control the instrument and the detectors. The evolution of the CCD controller, with high performance in speed acquisition and transfer rate, has changed the architecture of the instrument control. Due to the high performances of modern LAN, it has become possible to have direct access to CCD controller and instruments features. The architecture is based on a remote system, connected to a local system through standard network facilities and communicating with it using an XML-like syntax. The remote system receives from the local system commands and, in turn, sends back telemetry and images. This control system will be tested for the first time with the SARG spectrograph, in the framework of the Instruments remote control project at the Telescopio Nazionale Galileo (TNG).
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rosario Cosentino, Rosario Cosentino, Pietro Bruno, Pietro Bruno, Manuel Gonzalez, Manuel Gonzalez, Manuel Huertas, Manuel Huertas, Salvatore Scuderi, Salvatore Scuderi, } "Instrument remote control project at TNG: SARG implementation", Proc. SPIE 5492, Ground-based Instrumentation for Astronomy, (30 September 2004); doi: 10.1117/12.551464; https://doi.org/10.1117/12.551464
PROCEEDINGS
9 PAGES


SHARE
RELATED CONTENT

The software for the AAT's HERMES instrument
Proceedings of SPIE (July 17 2014)
UVES instrument software in the VLT environment
Proceedings of SPIE (June 15 2000)
Harps-N: the new planet hunter at TNG
Proceedings of SPIE (September 23 2012)

Back to Top