Bibcode
Pasquini, Luca; Cristiani, Stefano; García-López, R. J.; Haehnelt, Martin; Mayor, Michel; Liske, Jochen; Manescau, Antonio; Avila, Gerardo; Dekker, Hans; Iwert, Olaf; Delabre, Bernard; Lo Curto, Gaspare; D'Odorico, Valentina; Molaro, Paolo; Viel, Matteo; Vanzella, Eros; Bonifacio, Piercarlo; di Marcantonio, Paolo; Santin, Paolo; Comari, Maurizio; Cirami, Roberto; Coretti, Igor; Zerbi, Filippo Maria; Spanò, Paolo; Riva, Marco; Rebolo, R.; Israelian, G.; Herrero, A.; Zapatero Osorio, Maria Rosa; Tenegi, F.; Carswell, Bob; Becker, George; Udry, Stephane; Pepe, Francesco; Lovis, Christophe; Naef, Dominique; Dessauges, Miroslava; Mégevand, Denis
Bibliographical reference
Ground-based and Airborne Instrumentation for Astronomy III. Edited by McLean, Ian S.; Ramsay, Suzanne K.; Takami, Hideki. Proceedings of the SPIE, Volume 7735, pp. 77352F-77352F-12 (2010).
Advertised on:
7
2010
Citations
0
Refereed citations
0
Description
CODEX is the proposed ultra-stable optical high-resolution spectrograph
for the E-ELT, which will use novel Laser Comb calibration techniques
and an innovative design to open a new era for precision spectroscopy.
With its unique combination of light-collecting power and precision,
CODEX will make it possible to directly measure the acceleration of the
Universe by monitoring the cosmological redshift drift of spectroscopic
features at cosmological distances. CODEX will also allow the assembly
of the first sizeable sample of earth-like planets in the habitable
zones of their stars with the radial velocity technique. CODEX will take
this technique to the level of cm/sec radial velocity stability - a
factor of about 20 improvement compared to current instruments. These
are two of the scientific results anticipated for CODEX, which will be
complemented by a wide range of spectacular science in stellar, galactic
and extra-galactic Astronomy as well as Fundamental Physics. All the
critical technology items are available or (as for the Laser Frequency
Comb) are in an advanced state of testing. CODEX is located at the E-ELT
coudé focus that will cover the visible range from 370 to 710 nm
and provide a resolving power R~120000 with an aperture of 0.8
arcseconds in the sky.