An 8-mm diameter fibre robot positioner for massive spectroscopy surveys

DOI: 
10.1093/mnras/stv541
Publication date: 
11/06/2015
Main author: 
Fahim N.
IAA authors: 
Prada F.;Sánchez J.;Azzaro M.;Becerril S.
Authors: 
Fahim N., Prada F., Kneib J.P., Glez-de-Rivera G., Hörler P., Sánchez J., Azzaro M., Becerril S., Bleuler H., Bouri M., Castaño J., Garrido J., Gillet D., Gómez C., Gómez M.A., González-Arroyo A., Jenni L., Makarem L., Yepes G., Arrillaga X., Carrera M.A., Diego R., Charif M., Hug M., Lachat C.
Journal: 
Monthly Notices of the Royal Astronomical Society
Publication type: 
Article
Volume: 
450
Pages: 
794-806
Number: 
Abstract: 
Massive spectroscopic survey are becoming trendy in astrophysics and cosmology, as they can address new fundamental knowledge such as understanding the formation of the Milky Way and probing the nature of the mysterious dark energy. To enable massive spectroscopic surveys, new technology has been developed to place thousands of optical fibres at a given position on a focal plane. This technology needs to be: (1) accurate, with micrometer positional accuracy; (2) fast to minimize overhead; (3) robust to minimize failure; and (4) low cost. In this paper, we present the development, properties, and performance of a new single 8-mm in diameter fibre positioner robot, using two 4-mm DC-brushless gearmotors, that allows us to achieve accuracies up to 0.07 arcsec (5 μm). This device has been developed in the context of the Dark Energy Spectroscopic Instrument. © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.
Database: 
WOK
SCOPUS
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2015MNRAS.450..794F/abstract
ADS Bibcode: 
2015MNRAS.450..794F
Keywords: 
Instrumentation: spectrographs; Largescale structure of Universe; Surveys; Techniques: spectroscopic