CAFE2: an upgrade to the CAFE high-resolution spectrograph. Commissioning results and new public pipeline
arXiv:1906.04060 · doi:10.1093/mnras/stz3283
Abstract
The Calar Alto Fiber-fed Échelle spectrograph (CAFE) is a high-resolution spectrographs with high-precision radial velocity capabilities mounted in the 2.2m telescope of Calar Alto Observatory. It suffered from strong degradation after 4 years of operations and it has now been upgraded. The upgrades of the instrument (now named CAFE) aimed at improving the throughput and stability thanks to the inclusion of a new grating, an active temperature control in the isolated coudé room, and a new scrambling system among other minor changes. In this paper, we present the results of the re-commissioning of the instrument and a new pipeline (CAFExtractor) that provides the user with fully reduced data including radial velocity measurements of FGK dwarf stars. We have monitored the upgraded instrument for several months to characterize its main properties and test the new pipeline. It uses part of the CERES code, improves the wavelength calibration and radial velocity extraction (using the HARPS masks adapted), applies nightly drift corrections. The finally reduced spectra are presented in FITS files. The commissioning results show a clear improvement in the instrument performance with respect to the degraded status before the intervention. The room temperature is now stabilized down to 5 mK during one night and below 50 mK over two months. CAFE now provides 3 m/s precision on the reference ThAr frames and the on-sky tests provide a radial velocity precision of 8 m/s during one night (for S/N>50). The throughput of the instrument is now back to nominal values with an efficiency of around 15% at 550 nm. The limiting magnitude of the instrument for a 1h exposure and S/N=20 is V=15. With all these properties, CAFE enters into the small family of high-resolution spectrographs mounted on 2-4 meter-class telescopes capable of reaching radial velocity precisions below 10 m/s.
arXiv commentAccepted for publication in MNRAS. 15 pages, 14 figures and 4 tables. CAFExtractor is available through this Github link https://github.com/jlillo/cafextractor
References in corpus (14)
- ELODIE metallicity-biased search for transiting Hot Jupiters II. A very hot Jupiter transiting the bright K star HD189733
- CERES: A Set of Automated Routines for Echelle Spectra
- The CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems
- Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations
- The IACOB project. V. Spectroscopic parameters of the O-type stars in the modern grid of standards for spectral classification
- The SOPHIE search for northern extrasolar planets VIII. A warm Neptune orbiting HD164595
- CAFE: Calar Alto Fiber-fed Echelle spectrograph
- The OCCASO survey: Presentation and radial velocities of twelve Milky Way Open Clusters
- Radial velocity confirmation of Kepler-91 b. Additional evidence of its planetary nature using the Calar Alto/CAFE instrument
- EPIC211089792 b: an aligned and inflated hot jupiter in a young visual binary
- Searching for H emitting sources around MWC758: SPHERE/ZIMPOL high-contrast imaging
- A new look inside Planetary Nebula LoTr 5: A long-period binary with hints of a possible third component
- Eclipsing binaries and fast rotators in the Kepler sample. Characterization via radial velocity analysis from Calar Alto
- K2-30b and K2-34b: two inflated hot-Jupiters around Solar-type stars
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