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.


Original document

The different versions of the original document can be found in:

https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9910/1/CARMENES-data-flow/10.1117/12.2233574.full,
https://academic.microsoft.com/#/detail/2470417756
Back to Top

Document information

Published on 01/01/2016

Volume 2016, 2016
DOI: 10.1117/12.2233574
Licence: CC BY-NC-SA license

Document Score

0

Views 0
Recommendations 0

Share this document

Keywords

claim authorship

Are you one of the authors of this document?