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Proceedings Article

CARMENES: data flow

[+] Author Affiliations
J. A. Caballero, A. Quirrenbach, W. Seifert

Landessternwarte (Germany)

J. Guàrdia, J. Colomé, Á. García-Piquer, L. Gesa, I. Ribas

Institut de Ciències de l'Espai (Spain)

M. López del Fresno, E. Solano

Ctr. de Astrobiología (Spain)

M. Zechmeister, A. Reiners

Georg-August-Univ. Göttingen (Germany)

E. de Juan, E. de Guindos, J. Helmling, L. Hernández Castaño

Ctr. Astronómico Hispano-Alemán (Spain)

F. J. Alonso-Floriano, M. Cortés-Contreras, J. López-Santiago, D. Montes

Univ. Complutense de Madrid (Spain)

P. J. Amado, R. Morales Muñoz

Instituto de Astrofísica de Andalucía (Spain)

H.-J. Hagen

Hamburger Sternwarte (Germany)

M. Kürster, A. Pavlov

Max-Planck-Institut für Astronomie (Germany)

Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99100E (July 15, 2016); doi:10.1117/12.2233574
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From Conference Volume 9910

  • Observatory Operations: Strategies, Processes, and Systems VI
  • Alison B. Peck; Robert L. Seaman; Chris R. Benn
  • Edinburgh, United Kingdom | June 26, 2016

abstract

CARMENES, the new Calar Alto spectrograph especially built for radial-velocity surveys of exoearths around M dwarfs, is a very complicated system. For reaching the goal of 1 m/s radial-velocity accuracy, it is appropriate not only to monitor stars with the best observing procedure, but to monitor also the parameters of the CARMENES subsystems and safely store all the engineer and science data. Here we describe the CARMENES data flow from the different subsystems, through the instrument control system and pipeline, to the virtual-observatory data server and astronomers. © (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Citation

J. A. Caballero ; J. Guàrdia ; M. López del Fresno ; M. Zechmeister ; E. de Juan, et al.
" CARMENES: data flow ", Proc. SPIE 9910, Observatory Operations: Strategies, Processes, and Systems VI, 99100E (July 15, 2016); doi:10.1117/12.2233574; http://dx.doi.org/10.1117/12.2233574


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