ESPRESSO: the Echelle spectrograph for rocky exoplanets and stable spectroscopic observations

By F. Pepe, S. Cristiani, R. Rebolo Lopez, Nuno C. Santos, A. Amorim, G. Ávila, W. Benz, P. Bonifacio, A. Cabral, P. Carvas and 40 more. Astronomical Telescopes + Instrumentation, 2010

175 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The Occurrence and Architecture of Exoplanetary Systems (2014, background): “They include traditional optical spectrographs well suited for FGK dwarfs (e.g., ESPRESSO, Pepe et al. (2010); G-CLEF, Szentgyorgyi et al. (2012); CODEX, Pasquini et al. (2008) as well as new infrared spectrographs more appropriate for M dwarfs (IRD, Tamura et al. (2012); CARMENES, Quirrenbach et al”
The 4MOST instrument concept overview (2014, methodology): “lower resolut tion configur design with preferred LR 660-900nm, w ns were inves design([10]), ha 60μm; an ~f ed cable run f s mounted (b”
A Gaussian process framework for modelling stellar activity signals in radial velocity data (2015, background): “Third generation spectrographs, to come online in the next few years, are expected to have measurement errors below 10 cm s − 1 (Pasquini et al. 2008; Pepe et al. 2010).”