Use of RTS2 for LSST multiple channel CCD characterisation

0388510 - FZÚ 2013 RIV US eng C - Conference Paper (international conference)
Kubánek, Petr - Prouza, Michael - Kotov, I. - O´Connor, P. - Doherty, P. - Frank, J.
Use of RTS2 for LSST multiple channel CCD characterisation.
Software and Cyberinfrastructure for Astronomy II. Bellingham: SPIE, 2012 - (Radziwill, N.; Chiozzi, G.), 84512T/1-84512T/12. Proceedings of the SPIE, 8451. ISBN 9780819491527. ISSN 0277-786X.
[Software and Cyberinfrastructure for Astronomy II. Amsterdam (NL), 01.07.2012-04.07.2012]
R&D Projects: GA MŠMT ME09052; GA MŠMT 7E12064
EU Projects: European Commission(XE) 283783 - GLORIA
Institutional research plan: CEZ:AV0Z10100502
Keywords : observatory software * CCD testing * LSST
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

RTS2, or Remote Telescope System 2nd version, is a modular observatory control system. Development of RTS2 began in 2003 and since then it has been used at more than 20 observatories world-wide. Its main users are small, fully autonomous observatories, performing target of opportunity observations. This article focuses on the description of changes to the system which allow for the integration of LSST's multiple output CCD imagers.
Permanent Link: http://hdl.handle.net/11104/0217600