"PUCHEROS (2012, UC observatory) and FIDEOS (2016, ESO-1m La Silla Observatory), are optical echelle high-resolution spectrographs developed in the AIUC, Chile. A thorium-argon hollow-cathode emission-line lamp is used as wavelength calibration method in the two spectrographs. We show the results of the study in radial velocity stability of the instruments. Additionally, we identify the main factors that limit the performance of these spectrographs, and how we deal with them in order to achieve a better stability and precision in radial velocity measures."Contents of this collection: presentation slides, Q&A transcript
The objective of the dissertation is to investigate instrumental limitations of high-precision radia...
For precise measurement of the radial velocity change in a star, the precision of the wavelength sol...
We present a stable, inexpensive wavelength reference, based on a white-light interferometer for the...
We present results from the commissioning and early science programs of FIbre Dual Echelle Optical S...
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...
The radial velocity method has been used to discover hundreds of extrasolar planets in the past two ...
We report on the construction and testing of a vacuum-gap Fabry-Pérot etalon calibrator for high pre...
The design and construction of CARMENES has been presented at previous SPIE conferences. It is a nex...
The Second Workshop on Extreme Precision Radial Velocities defined circa 2015 the state of the art D...
International audienceThe Second Workshop on Extreme Precision Radial Velocities defined circa 2015 ...
The Second Workshop on Extreme Precision Radial Velocities defined circa 2015 the state of the art D...
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...
The objective of the dissertation is to investigate instrumental limitations of high-precision radia...
For precise measurement of the radial velocity change in a star, the precision of the wavelength sol...
We present a stable, inexpensive wavelength reference, based on a white-light interferometer for the...
We present results from the commissioning and early science programs of FIbre Dual Echelle Optical S...
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...
The radial velocity method has been used to discover hundreds of extrasolar planets in the past two ...
We report on the construction and testing of a vacuum-gap Fabry-Pérot etalon calibrator for high pre...
The design and construction of CARMENES has been presented at previous SPIE conferences. It is a nex...
The Second Workshop on Extreme Precision Radial Velocities defined circa 2015 the state of the art D...
International audienceThe Second Workshop on Extreme Precision Radial Velocities defined circa 2015 ...
The Second Workshop on Extreme Precision Radial Velocities defined circa 2015 the state of the art D...
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...
The objective of the dissertation is to investigate instrumental limitations of high-precision radia...
For precise measurement of the radial velocity change in a star, the precision of the wavelength sol...
We present a stable, inexpensive wavelength reference, based on a white-light interferometer for the...