CARMENES: data flow

DOI: 
10.1117/12.2233574
Publication date: 
01/07/2016
Main author: 
Caballero, J. A.
IAA authors: 
Amado, P. J.;Morales Muñoz, R.
Authors: 
Caballero, J. A.;Guàrdia, J.;López del Fresno, M.;Zechmeister, M.;de Juan, E.;Alonso-Floriano, F. J.;Amado, P. J.;Colomé, J.;Cortés-Contreras, M.;García-Piquer, Á.;Gesa, L.;de Guindos, E.;Hagen, H. -J.;Helmling, J.;Hernández Castaño, L.;Kürster, M.;López-Santiago, J.;Montes, D.;Morales Muñoz, R.;Pavlov, A.;Quirrenbach, A.;Reiners, A.;Ribas, I.;Seifert, W.;Solano, E.
Journal: 
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Publication type: 
Proceedings
Volume: 
9910
Pages: 
99100E
Abstract: 
<p>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.</p>
Database: 
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2016SPIE.9910E..0EC/abstract
ADS Bibcode: 
2016SPIE.9910E..0EC