We present results from the commissioning and early science programs of FIbre Dual Echelle Optical Spectrograph (FIDEOS), the new high- resolution echelle spectrograph developed at the Centre of Astro Engineering of Pontificia Universidad Catolica de Chile, and recently installed at the ESO 1-m telescope of La Silla. The instrument provides spectral resolution R ̃ 43 000 in the visible spectral range 420-800 nm, reaching a limiting magnitude of 11 in V band. Precision in the measurement of radial velocity is guaranteed by light feeding with an octagonal optical fibre, suitable mechanical isolation, thermal stabilization, and simultaneous wavelength calibration. Currently the instrument reaches radial velocity stability of ̃8 m s-1 over seve...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present results from the first two years of operations of the HARPS spectrograph installed on the...
"PUCHEROS (2012, UC observatory) and FIDEOS (2016, ESO-1m La Silla Observatory), are optical echelle...
The fibre–fed echelle spectrograph of Observatoire de Haute–Provence, ELODIE, is presented. This ins...
The current generation of astronomical spectrographs can measure radial velocity signals of exoplane...
The radial velocity method has been a key contributor to the search of exoplanets. Since the first c...
We present spectrograph design details and initial radial velocity results from the PRL optical fibe...
With the exception of the transit method employed by the Kepler Space Telescope, the radial velocity...
FEROS is a new fiber-fed bench-mounted prism-cross dispersed echelle spectrograph which has been rec...
The CHIRON optical high-resolution echelle spectrometer was commissioned at the 1.5 m telescope at C...
We present the first results of our precise radial velocity (RV) measurements of G and K giants....
Veloce is an ultra-stable fibre-fed R4 echelle spectrograph for the 3.9 m Anglo-Australian Telescope...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present results from the first two years of operations of the HARPS spectrograph installed on the...
"PUCHEROS (2012, UC observatory) and FIDEOS (2016, ESO-1m La Silla Observatory), are optical echelle...
The fibre–fed echelle spectrograph of Observatoire de Haute–Provence, ELODIE, is presented. This ins...
The current generation of astronomical spectrographs can measure radial velocity signals of exoplane...
The radial velocity method has been a key contributor to the search of exoplanets. Since the first c...
We present spectrograph design details and initial radial velocity results from the PRL optical fibe...
With the exception of the transit method employed by the Kepler Space Telescope, the radial velocity...
FEROS is a new fiber-fed bench-mounted prism-cross dispersed echelle spectrograph which has been rec...
The CHIRON optical high-resolution echelle spectrometer was commissioned at the 1.5 m telescope at C...
We present the first results of our precise radial velocity (RV) measurements of G and K giants....
Veloce is an ultra-stable fibre-fed R4 echelle spectrograph for the 3.9 m Anglo-Australian Telescope...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present the first data release of the Radial Velocity Experiment (RAVE), an ambitious spectroscop...
We present results from the first two years of operations of the HARPS spectrograph installed on the...